<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2017.84045</article-id><article-id pub-id-type="publisher-id">JMP-75084</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Origin of Magnetic Fields of Stellar Objects in the Universe Based on the 5D Projection Theory
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Peter</surname><given-names>C. W. Fung</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>K.</surname><given-names>W. Wong</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Physics and Astronomy, University of Kansas, Kansas, USA</addr-line></aff><aff id="aff1"><addr-line>Department of Physics, University of Hong Kong, Hong Kong, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>peterallegro333@gmail.com(PCWF)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>03</month><year>2017</year></pub-date><volume>08</volume><issue>04</issue><fpage>668</fpage><lpage>746</lpage><history><date date-type="received"><day>February</day>	<month>23,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>March</month>	<year>28,</year>	</date><date date-type="accepted"><day>March</day>	<month>31,</month>	<year>2017</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Beginning with a 5D homogeneous universe [1], we have provided a plausible explanation of the self-rotation phenomenon of stellar objects previously with illustration of large number of star samples [2], via a 5D-4D projection. The origin of such rotation is the balance of the angular momenta of stars and that of positive and negative charged e-trino pairs, within a 
  3<em>D</em> &amp;otimes; 1<em>D </em>void of the stellar object, the existence of which is based on conservation/parity laws in physics if one starts with homogeneous 5D universe. While the in-phase e-trino pairs are proposed to be responsible for the generation of angular momentum, the anti-phase but oppositely charge pairs necessarily produce currents. In the 5D to 4D projection, one space variable in the 5D manifold was compacted to zero in most other 5D theories (including theories of Kaluza-Klein and Einstein [3] [4]). We have demonstrated, using the Fermat’s Last Theorem [5], that for validity of gauge invariance at the 4D-5D boundary, the 4
  <sup>th</sup> space variable in the 5D manifold is mapped into two current rings at both magnetic poles as required by Perelman entropy mapping; these loops are the origin of the dipolar magnetic field. One conclusion we draw is that there is no gravitational singularity, and hence no black holes in the universe, a result strongly supported by the recent discovery of many stars with masses well greater than 100 solar mass [6] [7] [8], without trace of phenomena observed (such as strong gamma and X ray emissions), which are supposed to be associated with black holes. We analyze the properties of such loop currents on the 4D-5D boundary, where Maxwell equations are valid. We derive explicit expressions for the dipolar fields over the whole temperature range. We then compare our prediction with measured surface magnetic fields of many stars. Since there is coupling in distribution between the in-phase and anti-phase pairs of e-trinos, the generated mag-netic field is directly related to the angular momentum, leading to the result that the magnetic field can be expressible in terms of only the mechanical variables (mass 
  <em>M</em>, radius 
  <em>R</em>, rotation period 
  <em>P</em>)of a star, as if Maxwell equations are “hidden”. An explanation for the occurrence of this “un-expected result” is provided in Section (7.6). Therefore we provide satisfactory answers to a number of “mysteries” of magnetism in astrophysics such as the “Magnetic Bode’s Relation/Law” [9] and the experimental finding that B-P graph in the log-log plot is linear. Moreover, we have developed a new method for studying the relations among the data (
  <em>M, R, P</em>) during stellar evolution. Ten groups of stellar objects, effectively over 2000 samples are used in various parts of the analysis. We also explain the emergence of huge magnetic field in very old stars like White Dwarfs in terms of formation of 2D Semion state on stellar surface and release of magnetic flux as magnetic storms upon changing the 2D state back to 3D structure. Moreover, we provide an explanation, on the ground of the 5D theory, for the detection of extremely weak fields in Venus and Mars and the asymmetric distribution of magnetic field on the Martian surface. We predict the equatorial fields B of the newly discovered Trappist-1 star and the 6 nearest planets. The log 
  <em>B &amp;minus;</em> log 
  <em>P</em> graph for the 6 planets is linear and they satisfy the Magnetic Bode’s relation. Based on the above analysis, we have discovered several new laws of stellar magnetism, which are summarized in Section (7.6).
 
</p></abstract><kwd-group><kwd>5D Projection Theory</kwd><kwd> Fermat’s Last Theorem</kwd><kwd> Perelman’s Mappings</kwd><kwd>  Self-Rotation</kwd><kwd> Dipolar Magnetic Field of Stars</kwd><kwd> Laws of Stellar Magnetism</kwd><kwd>  Laws of Stellar Angular Momentum</kwd><kwd> Magnetic Bode’s Law</kwd><kwd> Non-Existence  of Gravitational Singularity</kwd><kwd> Semion State of Atoms in Stellar Surface</kwd><kwd>  Magnetic Storm</kwd><kwd> Planetary Magnetic Field</kwd><kwd> Maxwell Equations at  4D-5D Boundary</kwd><kwd> Magnetic Fields of the Trappist-1 System</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction-Understanding Our Universe by Expanding the 4D Lorentz Manifold to the 5D Homogeneous Manifold and Project Back to the 4D Space-Time Structure via Two Projection Procedures</title><p>It is a very important step in physics to unify gravity with electrodynamics. Despite many trials, the past endeavors were unsuccessful. It is not correct to think that by adding another dimension to the Lorentz space-time, one can readily bridge gravity and electrodynamics. A unified theory along this line of thought therefore is not one that can be applied separately to a domain with masses in motion, and to another domain pertaining to dynamics of massless photons. The unified theory has to embrace both gravity and electrodynamics in an “inherent” manner. The general method we use is to analyze the physical properties of the universe via projection/mapping between the 4D and 5D space-time, with an analysis of the boundary conditions between the two domains.</p><p>In our model, after the absolute time<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x3.png" xlink:type="simple"/></inline-formula>, the universe is to be observed/ perceived. Since observation/measurement is realized after this absolute time instant, based on the uncertainty principle, the uncertainty of energy observed at</p><p>this time is specified by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x4.png" xlink:type="simple"/></inline-formula>. Thus there is an infinite amount of</p><p>energy generated at this instant in the 5D manifold. The 5D manifold has to be homogeneous the reasons of which have been discussed in [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] . There is another reason: no physical laws have yet to be enforced. Some laws appear when the energy is perceived to be associated with e-trinos (conservation of spin, etc.).Other laws are realized when matter is being generated in the 4D Lorentz manifold. This time instant may be considered to be corresponding to the time when a Big Bang occurs in a Big Bang model discussed in literature. The term “Big Bang” in this paper therefore refers to the definition above according to the 5D theory. Starting with the above defined Big Bang concept, energy is flowing “out” along the radial direction in 4D space, and due to the Maxwell 4D boundary imposed, and any radial vector direction can become the Ricci Flow axis and generate beyond a finite 5D void core with a 4D Lorentz doughnut manifold. Since the choice of the Ricci Flow axis is arbitrary, hence many such doughnut Lorentz manifolds can be simultaneously created, thus completing the Big Bang picture of universe creation in the context of the 5D projection theory.</p><p>We assume the universe began with a homogeneous 5D space-time structure described by the above metric equation. From the homogeneous 5D manifold, we can apply projection operations [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] back onto the 4D Lorentz manifold, and requiring all the basic laws of physics to satisfy the known gauge invariance properties, so that there is consistency of mathematical logic steps linking variables in the 5D and 4D domains. We can then analyze and interpret the mathematically -deduced consequence and compare some aspects when appropriate measurable data are available.</p><p>The above projection reduction approach was presented in [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] , leading to the topological reduction of the homogenous 5D into the group representation of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x5.png" xlink:type="simple"/></inline-formula>, where the L group represents the Lorentz 4D domain. It was emphasized that the resulting Poincare sphere, a “product” in projection, encloses an inhomogeneous 5D void in the center. Based on parity analysis, it has been remarked that massless spinors with equal amount of opposite charges must be present in such a void. In addition, vector potential, which gives rise to photons, must also exist inside the 5D void.</p><p>On the other hand, via the rigorous Perelman-Ricci Flow mapping [<xref ref-type="bibr" rid="scirp.75084-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref11">11</xref>] , a homogeneous 5D is mapped into an inhomogeneous 4D doughnut structure. The consequence carries the important implication that there is a Beginning of space-time from absolute Nothing, and time is unidirectional, i.e. irreversible and the law of causality follows. This mapping procedure is then followed by Perelman’s entropy mapping [<xref ref-type="bibr" rid="scirp.75084-ref12">12</xref>] , via which the doughnut structure becomes a matter sphere satisfying the Lorentz manifold, thus proving Poincare’s conjecture [<xref ref-type="bibr" rid="scirp.75084-ref13">13</xref>] .</p><p>It is our intention to show the mathematical connections between these two mapping/projection procedures, as well as to investigate the physical outcome from such investigation in this paper, with special focus on the origin of magnetic field in the universe. Note that whatever method we employ to analyze the space-time structure of the universe, we always come up with a boundary separating the 5D and 4D domains. We start with the Fermat’s Last Theorem to analyze the space structure in the void and 4D-5D boundary in Section (2).In particular, we show that that breaking of the homogeneity of the 5D space-time, due to the imposition of the lower dimension 4D boundary, would lead to a time-frozen, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x6.png" xlink:type="simple"/></inline-formula>space domain, with concurrent matter formation surrounding the void. The 1D space structure is interpreted, due to parity, as an entangled state of two loops at the void-4D boundary. The generation of matter is restricted by charge parity. When the lightest lepton is generated, there must be equal amount of positive charge generated also. The generation of neutron does not violate such parity. Modification of the size of the current loop when neutrons are generated is analyzed in Section (2.3), putting forth the notion that generation of heavy elements can achieved in a similar way.</p><p>We pay special attention to the meaning and mathematical representation of homogeneity. Since other theories relating to transformation between a 5D domain and 4D domain have been published, we give a very shot review on the Kaluza-Klein (K.K.) [<xref ref-type="bibr" rid="scirp.75084-ref4">4</xref>] theory in Section (3). Also, we shall pay a revisit to the issue of gravitational singularity there. Note that Einstein’s unified theory [<xref ref-type="bibr" rid="scirp.75084-ref3">3</xref>] also followed the consequence of the K.K theory. One crucial difference between the K.K. theory, hence Einstein’s, and the present one here is that the 5D manifold of these theories are not homogenous, and the 4<sup>th</sup> space coordinate in the 5D domain is compacted to reduce dimension. We need to review this issue also because the 4<sup>th</sup> space variable in our theory is rotated to the radial direction during dimension reduction, together with the emergence of a current loop, (as a consequence of the space-space transformation) in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x7.png" xlink:type="simple"/></inline-formula> boundary where Maxwell equations must satisfy. It is precisely the existence of this non- zero space variable, as a result of the Perelman entropy mapping (leading to a <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x8.png" xlink:type="simple"/></inline-formula> space structure) that provides the current loops that generate the intrinsic dipolar magnetic field in spherical stellar objects of the universe. Our analysis of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x9.png" xlink:type="simple"/></inline-formula> transformation leads us to conclude that there is no gravitational singularity in the universe.</p><p>Explicit expression for the dipolar magnetic field of a general stellar object is derived in Section (4). Though the classical Biot-Savart law is employed, the quantum signature of the charge current is incorporated. The Three Laws of Dipolar Magnetic Fields of stellar objects, similar to the three laws of Stellar Angular Momentum discovered in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] are also presented with numerical illustration in the same section there. Moreover, we have derived the ratio of the dipolar magnetic field strengths when the matter shell is composed of either (i) pure hydrogen ions, or (ii) purely Helium ions as two examples based on quark mass analysis during the generation of matter based on the dimension projection theory. As the mass density within the shell increases, the 3D space homogeneity of a shell near the surface is broken into<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x10.png" xlink:type="simple"/></inline-formula>. The variation of gravity is approximately only along a direction perpendicular to the local plane on the surface. It is this broken space that leads to the atomic binding from Bohr to Chern-Simons hydrogen solution. In the relativistic limit, the Chern-Simons solution is given by the Semion state in which the electron collapses into the proton environment, bringing with it the pinned magnetic flux. We explain in Section (5) how the consequence, qualitatively, of the formation of such Semion state could lead to the generation of huge sporadic magnetic field from the stellar surface when the 2D state changes back to the 3D state, as part of the stellar evolution process. To test the general validity of the dipolar field equation we have derived, we introduce in Section (6) a new method of graphical analysis using measured values of the basic set of data (mass, radius, rotation period), and compare the power indices of the relevant variables. Very satisfactory results has been obtained for 8 different star groups: (6.1) the pre-main-sequence stars in the Orion Nebula; (6.2) the NGC 6819 stars; (6.3) the mid-to-low mass stars of the main sequence; (6.4) the pre-dwarf M34 stars; (6.5) the NGC 2516 stars; (6.6) brown dwarfs; (6.7) white dwarfs and (6.8) magnetic white dwarfs. There are two features in astronomy related to stellar magnetic field which are like mysteries. One is the linear relation between surface magnetic field <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x11.png" xlink:type="simple"/></inline-formula> and equatorial rotation speed v in the log-log graph, and the other is the so-called “Magnetic Bode’s Law” which simply states that the parameter B<sub>s</sub>R<sup>3</sup> and Iω relation is also linear in a log-log plot, particular for cool stars; here<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x12.png" xlink:type="simple"/></inline-formula> is the angular momentum. Though we have carried out a very detailed analysis of the B-v relation in Section (6) for many star groups, no suitable complete measured data sets <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x13.png" xlink:type="simple"/></inline-formula> have been obtained for every star in these star groups in Section (6). Such a set of four variables for each individual star in the sun-like group with over 100 members have been published. We apply that in Section (7) to analyze the stated two mysteries. The study there is important because on face value, no parameters related to electric current are involved in the stated two relations. Where are the Maxwell equations “hidden” behind such Laws? Whereas other scientists have attempted to explain these features using various forms of dynamo theories, we find that our derived expression for the dipolar field can automatically explain such phenomena, implying that based on the 5D-4D projection theory, the co-existence of in-phase and anti-phase spinor pairs circulating in the stellar void can automatically explain the origin of angular momentum and the origin of dipolar magnetic field in stellar objects at the same time. Section (7.5) is devoted to compare the difference of the theoretical prediction and measured values of the dipole fields of some members of our planets. Section (7.6) is a summary of the laws and issues discovered in this paper. Section (7.7) concludes our endeavor. The numerical values of the relevant variables/parameters to be applied in our numerical study in this paper are all based on the fundamental well-established constants, such as electron mass, quark mass, electronic charge, the Planck constant, plus data measured only―there is no other input parameter and no parameterization process involved.</p></sec><sec id="s2"><title>2. The Meaning of Spatial Homogeneity &amp; Application of the Fermat’s Last Theorem to the Boundary of the 5D-4D Domains</title><sec id="s2_1"><title>2.1. Basics of the Special Properties of the 5D, 4D Domains and the 5D-4D Boundary</title><p>As we proceed through the paper, the physical properties of the 5D-4D boundary are of crucial importance; we therefore need to high-light some basics, which are consequence of the projection theory and fundamental physics.</p><p>a) From the 5D homogeneous metric, one can obtain a 5D second order energy-momentum differential operator without a term pertaining to mass. Solutions of such metric equation represent 5 vector potential fields (including charge-source terms, thus existence of e-trinos) traveling with speed c, similar to the fields associated with the Maxwell potentials in the 4D Lorentz manifold. In the 5D domain, a term pertaining to magnetic monopole exists. In 4D domain, the electric, magnetic symmetry is broken, so that there is no magnetic-mono- pole term in Maxwell equations.</p><p>b) In a 5D domain, a Dirac linearization process does not lead to mass creation via projection/mapping, implying the e-trinos must be massless, but charged. These spinor states are equivalent to magnetic monopole states in 5D. In 4D domain, a Dirac linearization process leads to solutions representing the state of massless, charge-neutral neutrino and the state of massive charged lepton (described by the SU(2) group) in pair form.</p><p>c) Based on (a) &amp; (b), the states of e-trinos and 4D Maxwell potentials must form the boundary between the 5D &amp; 4D homogeneous manifolds, implying that both classical and quantum representations are allowed in the boundary. A satisfactory quantum theory should also have such representations.</p><p>d) The void space is expressed as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x14.png" xlink:type="simple"/></inline-formula>, with time frozen, meaning that the pair spinor states in 3D are orthogonal to those in 1D structure. When a pair is charge neutral, it must be in 3D space, as the product <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x15.png" xlink:type="simple"/></inline-formula> gives the Maxwell potential after a Dirac linearization process; hence such spinor pairs generate a net angular momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x16.png" xlink:type="simple"/></inline-formula>. The remaining 1D space, being orthogonal to the 3D space, then must contain no net momentum. However, similar to the appearance of the monopole term in 5D Maxwell equations, the 1D space carries a current of magnitude 2ec, which results from<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x17.png" xlink:type="simple"/></inline-formula>. If such a current forms a ring or loop, with a single frequency<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x18.png" xlink:type="simple"/></inline-formula>, then these charges will produce a magnetic dipole field, but could annihilate, and cannot remain in a perpetual state. Because the 3D space is symmetric, such a current pair loop must be split into 2 parity states in two different magnetic latitudes, one in each hemisphere. Since the 2 parity loops produces the same in line magnetic field, they will give a pure dipolar field similar to a bar magnet. The general charge neutrality within the 1D domain implies that it is possible to break the neutral charge condition between hemispheres, as long as their sum neutrality is maintained. A more detail discussion later in relation to the conformal projection P1 of these spinor states on the creation of quarks and thus hadrons will be given.</p><p>e) According to the P1 projection, the 4th space coordinate of e-trinos in the 5D manifold is conformally mapped into quarks of fractional charges. In order to produce a proton (composed of (u, u, d) quarks) and a neutron (composed of (u, d, d) quarks), as an example, we need 3 up and 3 down quarks. Since the 3 up quarks have a total charge of 2e, they are projected via the P1 process from 2 e-trino loop states of one loop. As the 3 down quarks have a total net charge of -e, they can be produced by P1 from just 1 anti-e-trino state from the other loop. To balance the + e charge resulting from the stated P1 projection, the Po projection on an in-phase pair (on the void surface) gives a lepton, such as an electron (exists in Lorentz space L), due to SU(2) symmetry and the unidirectional nature of time in the 5D metric. Effectively, we say that the consequence of Po is specified by the group product<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x19.png" xlink:type="simple"/></inline-formula>. We have overall charge neutrality in the universe all the time.</p><p>f) After the entropy mapping, or equivalently the combined Po and P1 mapping, we have a spherically shaped mass stellar object model enclosing a <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x20.png" xlink:type="simple"/></inline-formula> void filled with charged massless spinors satisfying the Fermi-Dirac distribution. We can connect the physical quantities of the thermal bath of the Fermions in the void and the physical quantities of the matter shell, leading to the discovery of the 1st and 2nd Laws regions for these spinors stated in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . It has been shown that under the time independent situation, eigen states of massless spinors with opposite charges, together with vector potential exist inside the void. In fact, there are eight such eigen states:</p><disp-formula id="scirp.75084-formula253"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x21.png"  xlink:type="simple"/></disp-formula><p>where p, e ,s represent the momentum, charge, and spin respectively. The in phase circulation of the oppositely charged massless spinors (with spin degeneracy<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x22.png" xlink:type="simple"/></inline-formula>) gives rise a net total angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x23.png" xlink:type="simple"/></inline-formula> in the void. This angular momentum must be counter-balanced by an opposite angular momentum-<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x24.png" xlink:type="simple"/></inline-formula> generated in the Lorentz spherical mass shell, in order to preserve total zero angular momentum value. Thus, spherical stellar objects are found to be “self-ro- tating”. In the astronomical scale for stars, this <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x25.png" xlink:type="simple"/></inline-formula> leads to a repulsive potential within such a void, leading to the elimination of the gravitational singularity, similar to the action of the gluon repulsive potential within hadrons [<xref ref-type="bibr" rid="scirp.75084-ref14">14</xref>] . This aspect will be discussed in more details in Section (3).</p><p>g) In this paper, we analyze the consequence of the out of phase rotating of the spinor pairs specified by the following four state groups:</p><disp-formula id="scirp.75084-formula254"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x26.png"  xlink:type="simple"/></disp-formula><p>In the calculation of current, these four states lead to the spin degeneracy factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x27.png" xlink:type="simple"/></inline-formula> occurring in Section (4). These out of phase rotation states would generate a current of 2ec. For the 1D state to remain actually perpetual, such a 1D (pair) current state must be split into two loops, one near each magnetic pole, each carrying a current of e c (see (d) above).</p></sec><sec id="s2_2"><title>2.2. The Fermat’s Last Theorem and Space Time Metric</title><p>Detail of the 4D Maxwell boundary can be explicitly analyzed through Fermat's theorem, in terms of Abelian angles. The Fermat’s sum of quadratic coordinate components has been proved to be rigorous for any number of coordinate dimensions [<xref ref-type="bibr" rid="scirp.75084-ref5">5</xref>] .</p><p>Leonhard Euler in 1770 [<xref ref-type="bibr" rid="scirp.75084-ref15">15</xref>] was the first to prove that for all non-zero <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x28.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x29.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x30.png" xlink:type="simple"/></inline-formula> is the set of all positive integers, the equation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x31.png" xlink:type="simple"/></inline-formula> admits no solutions for n = 3. Fermat was the first to provide a proof that there is no solution for the case n = 4 (see [<xref ref-type="bibr" rid="scirp.75084-ref16">16</xref>] and also [<xref ref-type="bibr" rid="scirp.75084-ref17">17</xref>] ). It has been proved recently that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x32.png" xlink:type="simple"/></inline-formula> has solution, a result which is referred to as the Fermat’s Last Theorem for order 2.</p><p>In fact, we put forth the notion that n = 2 is the only condition that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x33.png" xlink:type="simple"/></inline-formula> has a solution. It is not surprising, therefore, to see that in relativity, manifold representation, equations of the form <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x34.png" xlink:type="simple"/></inline-formula> repeatedly appear.</p><p>By expanding the Lorentz manifold to the 5 space-time, we learn that the universe has a homogenous 5D space-time structure described by the metric</p><disp-formula id="scirp.75084-formula255"><label>(2.2.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x35.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x36.png" xlink:type="simple"/></inline-formula> are the spatial vector variables; in the usual representation,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x37.png" xlink:type="simple"/></inline-formula>.</p><p>In the homogeneous 5D space-time, all 4 orthogonal space axes are exactly equivalent. Thus each axis has a measure r' as represented in the complex phase angle O(1) group [<xref ref-type="bibr" rid="scirp.75084-ref18">18</xref>] . This group has three elements specified by angles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula> for the 4D orthogonal coordinates, reducing the Fermat's sum to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula>, together with the specification of angle elements in the O(1). For a 4D Maxwell space-time, this O(1) group has 2 angles:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula>, and the transformation is specified by the Euler angles, where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula>, is between 0 and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula>; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula>is between 0 and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula>. It is then easy to see that for a 3D space structure, the Little group O(1) is specified by the parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x45.png" xlink:type="simple"/></inline-formula>. For a 4D space, n has three values:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x46.png" xlink:type="simple"/></inline-formula>. When we fix the third angle <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x47.png" xlink:type="simple"/></inline-formula> to be a constant, the 5D homogeneous space-time splits into two Maxwell 4D of opposite parities. It is this explicit split that is revealed as 2 spherical gamma ray bubbles, one above and one below the Center of the Milky Way galactic core observed by NASA [<xref ref-type="bibr" rid="scirp.75084-ref19">19</xref>] . By this parity split, the vector potential field solutions of the 5D homogeneous metric equation with 2nd order operator breaks the 5D symmetry in the Maxwell sub-space-time, eliminating the magnetic mono-pole solution. It is also due precisely to this split, in the 5D Dirac linearized representation of the metric equation, that we have a set of e, and -e massless spinors. When these spinor fields couple to the Maxwell vector potentials, gauge transformation is satisfied. Such spinors exist only within a 5D manifold (see detailed discussion in [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] on this point). Application of projection Po on the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x48.png" xlink:type="simple"/></inline-formula> variable in the 4D Lorentz boundary creates a set of lepton masses (accompanied by neutrinos) described by the SU(2) group. We then arrive at a spinor differential operator which splits into two standard <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x49.png" xlink:type="simple"/></inline-formula> Dirac Gamma representations. On the other hand, the 5D spinor field equation also contains a set of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x50.png" xlink:type="simple"/></inline-formula> gamma matrices (Equation (7.9) of [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] ). The superposition of these 2 sets of gamma matrices in the Dirac equations in the Maxwell space-time description leads to Parity violation in weak interaction as discovered in Bethe decay. [<xref ref-type="bibr" rid="scirp.75084-ref20">20</xref>] .</p><p>Since the solutions of a differential equation is totally governed by the boundary conditions that are imposed, the vector and massless charged spinor solutions to the 5D homogeneous metric operator equation are dictated by the 4D Maxwell space-time boundary which forms the enclosure to (or embracing) the 5D manifold. At the absolute time t, the space volume of the homogeneous ND manifold must have a boundary enclosure of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x51.png" xlink:type="simple"/></inline-formula>, where N is an integer. Thus the homogeneous 5D manifold boundary is the Maxwell 4D. When the Fermat's sum is expressed in term of the rotation angles and the radius magnitude, it follows that the boundary condition must reduce the 3 independent angles in 5D by fixing any one as a constant, thus reducing this set to 2 independent angles in the Maxwell 4D domain. The result is that there is imposition in alignment between <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x52.png" xlink:type="simple"/></inline-formula> of the Fermat's sum in 5D, and r that of the Fermat's sum in 4D. This boundary continuity leads to the manifestation of a Ricci Flow direction, which will convert the homogeneous Maxwell 4D boundary through the two projections (Po &amp; P1) of the already broken symmetric property of the 4 space coordinates further into a 4D Lorentz manifold containing masses. In terms of topological mapping, this 4D Lorentz boundary manifold is precisely the doughnut structure proved by Perelman’s Ricci Flow mapping [<xref ref-type="bibr" rid="scirp.75084-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref11">11</xref>] . In terms of the reduced 5D domain, the space structure must still have a finite region, with a center core containing the axis z(in 3D space representation) perpendicular to the doughnut plane, which is an entangled coordinate composed of the 3D coordinate z and the 4th space dimension <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x53.png" xlink:type="simple"/></inline-formula> variable. The planer domain boundary in which 5D space structure still remains is then described by the Po projection of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x54.png" xlink:type="simple"/></inline-formula> to a 2D circle of radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x55.png" xlink:type="simple"/></inline-formula>. On the other hand, the 3D space volume of the Lorentz domain must be mapped by the remaining space variable <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x56.png" xlink:type="simple"/></inline-formula> to 3D space via the conformal P1 (space to space) projection. This mapping in turn would give us the created leptons and the Gell-Mann quarks enclosed in this covering Lorentz boundary. It is through these projection-mapping processes imposed by the boundary condition, and the gauge invariance property, on all the massive quantum field states in the Lorentz boundary manifold, that we have created a model for the formation of a Galaxy.</p><p>Since the determination of the Ricci Flow direction for the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x57.png" xlink:type="simple"/></inline-formula> vector such that we obtain an entangled 3D, the z axis has infinite multiple choices from the O(1) angle between 0 and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x58.png" xlink:type="simple"/></inline-formula>, it is then possible to simultaneously create many Lorentz doughnut 4D structures during the very beginning of the 5D space-time, when the absolute time is near 0, and through uncertainty, the initial energy is near infinite. In short the creation of many galaxies, near the beginning of the universe, according to the 5D projection theory, is a picture consistent with the general Big Bang theory in the literature. Furthermore, since the 5D metric of space-time implies the universe will expand continuously, in time course, expansion pushes all these created galaxies apart.</p><p>Our remaining problem is the general spherical shape of the massive stellar objects observed within each galaxy satisfying the Poincare Conjecture. To illustrate this topological mapping process, Perelman introduced an entropy mapping [<xref ref-type="bibr" rid="scirp.75084-ref12">12</xref>] , which basically closes the doughnut 5D core, into a void that contains a 3D spherical volume plus a 1D closed loop that is orthogonal to the 3D radius; this 1D loop must be on the surface of the spherical volume. Comparing projection theory and Perelman’s theory, the 3D radius of the void, is defined by the Po projection of the 4th space coordinate. This consequence is similar to that of the Ricci Flow mapping, except the matter domain totally encloses the 5D manifold. The physical state of this void is time frozen at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x59.png" xlink:type="simple"/></inline-formula>, a value specific to each stellar object. Electrons are thus created through Po outside of this void. However, overall charge neutrality must be maintained both within and outside the void in the mass shell of the stellar object. As such the measure of the 1D closed loop (hence the current density) on the spherical void surface cannot be 0, in opposition to that postulated by the KK and Einstein's theories. The measure of this 1D loop depends on the hadrons created through P1 in the Lorentz mass shell domain.</p></sec><sec id="s2_3"><title>2.3. Modification of the Size of the Current Loop When Neutrons Are Generated</title><p>We note again that in the 5D manifold, there are 5 vector potential components (instead of 4 in the Maxwell domain), and 2 massless spinors with charges e and -e. [Section 2.1]. In order that these solutions satisfy the boundary conditions imposed by the Maxwell domain, we need to transform the 5 component symmetric vector potentials into the 4 Maxwell vector potentials by breaking the symmetry of solution as carefully illustrated by Maxwell in his thesis, with the emergence of a magnetic mono-pole potential, which corresponds to the 5th component vector potential in the 5D manifold. [<xref ref-type="bibr" rid="scirp.75084-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref23">23</xref>] .</p><p>We will find an explicit expression for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x60.png" xlink:type="simple"/></inline-formula>. Now the Poincare void is given by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x61.png" xlink:type="simple"/></inline-formula>. According to Fermat's theorem, the 3D orthogonal representation is given by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x62.png" xlink:type="simple"/></inline-formula>; while <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x63.png" xlink:type="simple"/></inline-formula> is orthogonal to the 1D which must form a closed loop on the spherical surface. The quantum representations are given by photons along<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x64.png" xlink:type="simple"/></inline-formula>, thus the diameter 2r must satisfy integer multiple of the photon wave-length. The charged massless spinor pairs, is specified by the 1D space structure. As stated before, the current loop states, being perpetual, are split by parity into an upper and a lower hemisphere loops. The loops are therefore of radius &lt;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x62.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x65.png" xlink:type="simple"/></inline-formula>.There exists 2 parity representations all together. Thus according to the projection theory for the spinor states, the radius r, must be produced by Po, the time projection. Hence from the metric (2.2.1), with time frozen, we must have</p><disp-formula id="scirp.75084-formula256"><label>(2.3.1a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x66.png"  xlink:type="simple"/></disp-formula><p>While the current loop<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x67.png" xlink:type="simple"/></inline-formula>, split by north and south is given by</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x68.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x69.png" xlink:type="simple"/></inline-formula> (2.3.1b)</p><p>Combining these two representations, &amp; letting<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x70.png" xlink:type="simple"/></inline-formula>, with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x71.png" xlink:type="simple"/></inline-formula>, we arrive at</p><disp-formula id="scirp.75084-formula257"><label>(2.3.1c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x72.png"  xlink:type="simple"/></disp-formula><p>which determines the geometry of void boundary.</p><p>The rotation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula> to the radial direction is governed by the Projection Po, which takes time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula> to complete. At time<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula>, the lightest lepton, with rest mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula>, begins to be generated, and the void radius attains the perpetual value<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula>. We interpret P1 as the conformal projection where the residue of the variable<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x78.png" xlink:type="simple"/></inline-formula>, i.e. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x79.png" xlink:type="simple"/></inline-formula>(represented by c lτl, where τ is a three dimensional vector) is to be rotated to form the other orthogonal component (a ring with perimeter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x80.png" xlink:type="simple"/></inline-formula> in (2.3.1)), with gauge confinement imposed, so that a 5D domain can become a 4D domain, accompanying the generation of three quarks with total charge of + e to conserve the charge of the lightest lepton. Thus we can interpret lτl as the time at which these quarks are generated. Since the generation of these massive particles starts from nothing to reach a stationary state, we can apply the uncertainty principle with the energy-time conjugate pair. In other words, we can write<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x81.png" xlink:type="simple"/></inline-formula>, where n is a quantum number greater or equal to 1, with t representing the time of the stated generation of the masses, and E the total rest mass generated in each case. Note that the conformal projection of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x82.png" xlink:type="simple"/></inline-formula> gives the SU(3) quarks, with proton as its lightest positive charged spinor particle, composed of a set of u, u, d quarks, due to gauge confinement. The bare total mass of these three quarks is precisely<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x75.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x83.png" xlink:type="simple"/></inline-formula>.</p><p>Therefore, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x84.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x85.png" xlink:type="simple"/></inline-formula>. From the above two equations pertaining to uncertainty, we have the ratio<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x86.png" xlink:type="simple"/></inline-formula>. As<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x87.png" xlink:type="simple"/></inline-formula>, and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x85.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x88.png" xlink:type="simple"/></inline-formula>, stated above, we arrive at</p><disp-formula id="scirp.75084-formula258"><label>(2.3.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x89.png"  xlink:type="simple"/></disp-formula><p>This is the size of the current loop if a pair of electron and proton is generated simultaneously; in other words, hydrogen atom is generated.</p><p>Note that charge, linear momentum, angular momentum, and energy must each be conserved during the generation of matter. We have only the lightest lepton and quarks generated initially, before the gluon potential is in action to produce proton and neutron. A set of (u, u, d) of quarks must be generated (to build up eventually a proton) together with the generation of an electron, according to the 5D projection theory. The gauge requirement for the solution on quark spinors is the charge to mass ratio<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x90.png" xlink:type="simple"/></inline-formula>, a constant [<xref ref-type="bibr" rid="scirp.75084-ref24">24</xref>] , where j specifies the quark and its charge, we have<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x90.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x91.png" xlink:type="simple"/></inline-formula>, leading to</p><disp-formula id="scirp.75084-formula259"><label>(2.3.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x92.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x93.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x94.png" xlink:type="simple"/></inline-formula> are respectively the masses of the up and down quarks , and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x95.png" xlink:type="simple"/></inline-formula> is the bare quark mass of 34 MeV. Now the sum of the bare quark masses building the proton (u, u, d) satisfies the Lorentz sum rule. Therefore we can write</p><disp-formula id="scirp.75084-formula260"><label>(2.3.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x96.png"  xlink:type="simple"/></disp-formula><p>Since mass is generated from nothing, the uncertainty principle requires that</p><disp-formula id="scirp.75084-formula261"><label>(2.3.5a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x97.png"  xlink:type="simple"/></disp-formula><p>(as a minimum); where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x98.png" xlink:type="simple"/></inline-formula> measures the time taken to generate the set (u,u,d) of quarks for proton. Likewise, another similar equation can be written for neutron which is composed of the set (udd):</p><disp-formula id="scirp.75084-formula262"><label>(2.3.5b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x99.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x100.png" xlink:type="simple"/></inline-formula> is the total bare quark mass building up a neutron.</p><p>Using the data for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x101.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x102.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x103.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x104.png" xlink:type="simple"/></inline-formula>, Equation (2.3.5a) &amp; Equation (2.3.5b) give,</p><disp-formula id="scirp.75084-formula263"><label>(2.3.5c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x105.png"  xlink:type="simple"/></disp-formula><p>However, there is also the factor due to the reduced-mass effect of the proton-neutron pair, and the reduced mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x106.png" xlink:type="simple"/></inline-formula> becomes (chapter 8, [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] ):</p><disp-formula id="scirp.75084-formula264"><label>(2.3.6a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x107.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula265"><label>(2.3.6b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x108.png"  xlink:type="simple"/></disp-formula><p>Hence, effectively, the time to generate a proton-neutron pair is longer than generating two protons by a factor of 2.225. Now many electrons and protons are generated simultaneously, while the 5D void is expanding until the mass shell is generated. Thus, the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x109.png" xlink:type="simple"/></inline-formula> would be larger if the mass shell is built of proton-neutron pairs, or alpha particles, namely, helium nuclei. The size of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x110.png" xlink:type="simple"/></inline-formula> is reflected in the calculation of angular momentum as report in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] , leading to a larger absolute value of loop size measured by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x111.png" xlink:type="simple"/></inline-formula> in (2.3.2). In other words, the current element integral in calculating the current density generating the dipolar magnetic field in Equation (4.1.6) and hence (4.2.2a) should be multiplied by factor of</p><disp-formula id="scirp.75084-formula266"><label>(2.3.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x112.png"  xlink:type="simple"/></disp-formula><p>if the mass shell is composed of helium four. If the matter crust is composed of hydrogen and Helium 4, the factor b would be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x113.png" xlink:type="simple"/></inline-formula>. For more heavy elements, such as iron, the correction factor b will be different accordingly.</p><p>With expressions (2.3.2) &amp; (2.3.7), we can apply the magnitude of the current loop to calculate the magnetic field generated by such a loop. Before we do the application, we have to derive an explicit representation of the magnetic field generated such a current, one near each magnetic pole, when the particular element(s) is considered to be existing at the Lorentz space-time and void boundary. Such derivation will be carried out in Section (4). At the meantime, we need to analyze in the next Section about the origin of the “key” variable <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x114.png" xlink:type="simple"/></inline-formula> in the conformation mapping, which is also effectively involved in previous unified theories.</p></sec></sec><sec id="s3"><title>3. Proof of Non-Existence of Gravitational Singularity in the Universe</title><sec id="s3_1"><title>3.1. The Crucial Difference between the Kaluza-Klein 5D Theory, Einstein’s Unification Field Equation and Consequence of Perelman’s Two Mappings</title><p>The original Kaluza-Klein theory (KK theory, see e.g. review in [<xref ref-type="bibr" rid="scirp.75084-ref4">4</xref>] ) was an attempt to develop a field theory which could unify all the forces under one fundamental law. In the framework of the theory, distance squared between the two neighboring space points <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x115.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x116.png" xlink:type="simple"/></inline-formula>, the line element, in reference frame<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x117.png" xlink:type="simple"/></inline-formula>, is expressed as</p><disp-formula id="scirp.75084-formula267"><label>(3.1.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x118.png"  xlink:type="simple"/></disp-formula><p>where the usual summation rule is understood, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x119.png" xlink:type="simple"/></inline-formula> is the metric tensor. The space-time is uniform so far. Since the interval between P and Q is independent of the choice of reference frame, the line element (3.1.1) is invariant under the transformation between reference frames (such as from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x120.png" xlink:type="simple"/></inline-formula> to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x120.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x121.png" xlink:type="simple"/></inline-formula>), so that</p><disp-formula id="scirp.75084-formula268"><label>(3.1.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x122.png"  xlink:type="simple"/></disp-formula><p>Equating (3.1.1) to (3.1.2) gives</p><disp-formula id="scirp.75084-formula269"><label>(3.1.3a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x123.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.75084-formula270"><label>(3.1.3b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x124.png"  xlink:type="simple"/></disp-formula><p>is called the vielbein. For a non-uniform gravitational field, the KK theory introduces the notion that “At every point in a reference frame with an arbitrary gravitational field it is possible to choose a locally inertial (freely falling) reference frame.” In other words, like carrying operation using the concept of calculus, the flat Minkowski metric can be transformed into a curved space-time metric. However, we would remark that in Equations (3.1.3a) &amp; (3.1.3b), it was already assumed that a gravitational field is present due to the presence of the Riemannian tensor. This assumption implies that in the domain considered, mass exists. Thus the 4D is a Lorentz manifold, and by an extension to 5D space- time, such a 5D structure would not be a homogeneous 5D. Hence the Ricci- Flow mapping does not reduce this 5D back to 4D, except simply by closing the extra 4<sup>th</sup> space dimension into a closed loop.</p><p>Without going into further details, we would remark that both the KK theory and Einstein generalized field equations have difficulties to explain experimental data and interpret mathematical singularity: (i) In order to exclude the singularities in the equation set, both K.K. and Einstein introduced the method of compactness. Such an assumption leads to the models of black hole, and dark matter, which to us, are not necessary.; (ii) The electron charge e and mass m<sub>e</sub> are included in a certain constant κ in K.K. theory which bridges the electromagnetic potentials and some metric tensor components including the 5<sup>th</sup> dimension. The values of both e &amp; m<sub>e</sub><sub> </sub>deduced based on the KK theory (or Einstein’s field equations) were not consistent with the well-established experimental values then (see comments in [<xref ref-type="bibr" rid="scirp.75084-ref4">4</xref>] ); (iii) The KK theory (and Einstein unified field equations, [<xref ref-type="bibr" rid="scirp.75084-ref3">3</xref>] ) did not contain any of the nuclear forces; during that time there was lack of experimental data from accelerators and the corresponding concept in particle physics.</p><p>Concerning the key difference between their theories and projection theory developed in this series, we need to note that in KK theory, as well as Einstein's 5D metric, the proper time τ is not connected to the 4th space dimension variable. Therefore, the KK 5D is not homogeneous, neither is mass a result of space projection.</p></sec><sec id="s3_2"><title>3.2. Absence of Gravitational Singularity</title><p>As analyzed in Section (2), the 1D space within the Poincare matter sphere is a set of two closed loops that includes the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x125.png" xlink:type="simple"/></inline-formula> variable, one in each stellar hemisphere. This loop expression was employed by Einstein in his unified electrodynamic and gravity equation, as a compactization of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x126.png" xlink:type="simple"/></inline-formula><sub> </sub>variable. In his gravity solution, he then further assumed that the loop can be reduced to a structure with zero measure, and ignored the 5D space-time domain external to the doughnut domain by simply changing it to a simple Maxwell 4D space-time without the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x127.png" xlink:type="simple"/></inline-formula> variable. This definitely is an error, which would lead to singularities for the gravity field both within the doughnut domain as well as outside it. It is such mathematical errors that led to the appearance of singularities in the unified theory, and the suggestion of the existence of black holes in the universe. When <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x125.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x128.png" xlink:type="simple"/></inline-formula> is carefully retained in the space-time structure, black holes do not appear in the theory (see Wheeler’s early work [<xref ref-type="bibr" rid="scirp.75084-ref25">25</xref>] and a recent paper on the classical solutions of Maxwell equations [<xref ref-type="bibr" rid="scirp.75084-ref26">26</xref>] ). In fact, the mathematical/logical exclusion of the gravitation singularity based on simple classical physics can be realized by the following analysis. The important issue on the solutions of Maxwell equations in the 5D-4D boundary will be followed in the next section.</p><p>Assuming a uniform mass distribution in a plane with the 2D void region bounded by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x129.png" xlink:type="simple"/></inline-formula>. Then the gravitation force f in the region <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x129.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x130.png" xlink:type="simple"/></inline-formula> must vanish. However, for the region</p><disp-formula id="scirp.75084-formula271"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x131.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula>, with D representing the 2D mass density. If <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula> vanishes, according to Einstein, then f diverges as r goes to 0.This f divergence disappears when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula>, or equivalently<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula>. From another angle, we would remark that energy flow must be conserved into the Maxwell 4D boundary. Therefore the r of the Maxwell 4D as related to the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula> of that from the 5D, is scaled by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula> (see deduction leading to Equation (2.3.1b)). In quantum phase space representation, a spinor pair along r is an entangled state, and carries energy outward. It is precisely this physics that makes the doughnut core center of a galaxy, which remains in 5D, is not a black hole, since energy is radiating outward, not flowing into the center as suggested by some [<xref ref-type="bibr" rid="scirp.75084-ref27">27</xref>] . This is an absolutely clear reason against Einstein’s compacting<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><sub>.</sub>. If we follow the analysis of the metric equation pertaining to the 5D manifold and the 5D-4D boundary as above, the 4D Maxwell space-time does not allow outward flow of e, -e massless spinor pairs that carry outward energy of 2 hν. Then at the origin of the center of the universe, or the center of the galaxy, if a black hole should exist according to those theories, mathematical logic does not indicate there is any outward flow of energy and then becomes a black hole, as we transform 4D Lorentz space-time with mass into the covariant Riemannian curvature space-time to obtain the gravity equation, since energy density seeks for uniformity. On the contrary, according to the 5D projection picture, energy seeks for uniformity by flowing outward to fill the universe at all t. Hence the singularity in the gravity field solution due to mass distribution does not appear. The above statement is both mathematical precise as well as philosophical subtle. Recently, stars of huge masses have been detected by telescopes expositions. For examples, R13601 (M = 365<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula>), BAT99-98 (226<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x140.png" xlink:type="simple"/></inline-formula>), R136c (230<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x141.png" xlink:type="simple"/></inline-formula>), R136a2 (195<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x142.png" xlink:type="simple"/></inline-formula>), Melnick42 (189<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x142.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x143.png" xlink:type="simple"/></inline-formula>), WR101c (150<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x142.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x143.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x144.png" xlink:type="simple"/></inline-formula>), LBV 1806-20 (130 to 200<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x133.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x134.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x137.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x138.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x139.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x140.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x142.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x143.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x144.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x145.png" xlink:type="simple"/></inline-formula>) plus a long list have been detected with masses &gt; 100 solar mass (see e.g., [<xref ref-type="bibr" rid="scirp.75084-ref6">6</xref>] , [<xref ref-type="bibr" rid="scirp.75084-ref7">7</xref>] , [<xref ref-type="bibr" rid="scirp.75084-ref8">8</xref>] ). If gravitational singularity were to exist, they would long have become black holes already. Such undebatable experimental results give the strongest support to our proof sketched above.</p><p>Moreover, the finding of a <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x146.png" xlink:type="simple"/></inline-formula> two photon emission, together with neutrino obtained from the p-p collision experiment [<xref ref-type="bibr" rid="scirp.75084-ref28">28</xref>] and associated theoretical explanation [<xref ref-type="bibr" rid="scirp.75084-ref29">29</xref>] indicates that the generation of the lepton is accompanied by (neutral) neutrino. More precisely, it is shown in [<xref ref-type="bibr" rid="scirp.75084-ref29">29</xref>] that the spinor solution contains an oscillating phase, and the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x146.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x147.png" xlink:type="simple"/></inline-formula> resonance is shown to be predictable, without the necessity to introduce a Higgs vacuum. Since no anti-neutrinos have been detected so far, such negative result supports the notion that there is no anti-matter universe, and hence no black hole. Recently, a small distinctive X-ray signal (Photon~<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x146.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x147.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x148.png" xlink:type="simple"/></inline-formula>) from the Milky Way was observed by the Nasa’s chamber satellite and the result has been interpreted as indicative of the existence of dark matter [<xref ref-type="bibr" rid="scirp.75084-ref30">30</xref>] . According to the 5D theory, Perelman entropy mapping process on the creation of stellar objects necessarily will lead to a short period of gamma radiation (similar to gamma radiation out of a galactic center discussed in Section (2.2)) as the object becomes a Poincare sphere. That is our model of the birth of a pulsar [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . Therefore we do not agree to the interpretation of [<xref ref-type="bibr" rid="scirp.75084-ref30">30</xref>] because there are many pulsars in the region of the signal source.</p><p>Having analyzed the concrete role played by the space variable <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x149.png" xlink:type="simple"/></inline-formula><sub> </sub>in the conformal mapping, we can now proceed to derive the expression of the intrinsic dipolar magnetic fields appearing in stellar objects.</p></sec></sec><sec id="s4"><title>4. Explicit Expression of the Intrinsic Dipole Magnetic Field Generated by Current with Quantum Signature at the 5D-4D Interphase</title><sec id="s4_1"><title>4.1. Quantum Current Density of the Ring Current in the Void Boundary</title><p>During the deduction of the three laws of angular momentum in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] , we have not included those spinor pairs circulating out of phase. They do not produce a net angular momentum, but they produce a net electric current generated by the (e, p; -e, -p) massless spinor pairs within the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x150.png" xlink:type="simple"/></inline-formula> time frozen void.</p><p>As these charges build up a stationary/perpetual current state, the wave function of a spinor pair represented by the symbol <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x151.png" xlink:type="simple"/></inline-formula> can be written as a plane wave state,</p><disp-formula id="scirp.75084-formula272"><label>(4.1.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x152.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x153.png" xlink:type="simple"/></inline-formula> is a normalization constant, the dimension of which will be analyzed later in this section. The wave function squared gives the probability density. If there are N numbers of charges e, the charge density is defined simply as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x153.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x154.png" xlink:type="simple"/></inline-formula>. One can get the current density J (unit to be determined by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x153.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x154.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x155.png" xlink:type="simple"/></inline-formula> in (4.1.1)) via<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x153.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x154.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x155.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x156.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.75084-formula273"><label>(4.1.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x157.png"  xlink:type="simple"/></disp-formula><p>Now for non-relativistic particle with mass m moving along a circular orbit so that differentiation with respect to space variable is one-dimensional, we use the symbol <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x158.png" xlink:type="simple"/></inline-formula> to represent the momentum &amp;v is the velocity. It is elementary to show that</p><disp-formula id="scirp.75084-formula274"><label>(4.1.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x159.png"  xlink:type="simple"/></disp-formula><p>Since the spinor e and spinor?e are two distinguishable particles, in carrying the thermal averaging process later on, we need to calculate the number N for either type of spinors. The electric current, however, is doubled, because they are circulating out of phase in the classical sense. Therefore the overall current density in one ring is finally</p><disp-formula id="scirp.75084-formula275"><label>(4.1.4a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x160.png"  xlink:type="simple"/></disp-formula><p>We have left our sign convention in deciding the magnetic polarity, as the sign convention is very simple. We have fixed the “classical current” to be one dimensional, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x161.png" xlink:type="simple"/></inline-formula>, which is the track length of the current; namely, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x161.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x162.png" xlink:type="simple"/></inline-formula>and , where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x161.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x162.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x163.png" xlink:type="simple"/></inline-formula> is the void radius as defined in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] , whereas<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x161.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x162.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x163.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x164.png" xlink:type="simple"/></inline-formula>, is a proportionality constant which is determined in Section (2). There is another factor b to be multiplied to the current ring length to include the effects of presence of various elements (hydrogen, helium) at the 5D-4D boundary. This factor will be specified if we apply our theory to find the magnetic field of specific planet or star with fuel heavier than hydrogen. Therefore, before such specification,</p><disp-formula id="scirp.75084-formula276"><label>(4.1.4b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x165.png"  xlink:type="simple"/></disp-formula><p>Remark again that the subscript 2 signifies that the 1D space structure has an entangled structure of two loops, composed of both e &amp; -e spinors as explained in Section (2). Note that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x166.png" xlink:type="simple"/></inline-formula> is the probability of finding the spinor pair in a certain region of space. Within the space allowed to be traveled by the plane wave expressed in (4.1.1), the normalization of constant should take on a value such that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x166.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x167.png" xlink:type="simple"/></inline-formula> in this “normalized space”. If a material wire is present, the current can only circulate around this wire and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x166.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x167.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x168.png" xlink:type="simple"/></inline-formula> in (4.1.1) is the one D length l as stated above. But in quantum mechanics, a classical 1D current has a spread in space variable due to the uncertainty principle so that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x166.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x167.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x168.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x170.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x166.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x167.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x168.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x170.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x169.png" xlink:type="simple"/></inline-formula> where d is the spatial spread. The dimension of J is then ampere per meter, which is a physically realizable and a calculable quantity.</p><p>The electrodynamics of charged massless particles moving with velocity c is not at all explored much within the frame work of Maxwell equations and the frame work of quantum field theory. An insightful investigation of the exact solution of such particles in Maxwell equations has recently been published [<xref ref-type="bibr" rid="scirp.75084-ref26">26</xref>] . Explicit expressions for the vector potential and the electromagnetic field were derived under the following conditions of motion of the charged massless particles: (a) linear, (b) accelerated unbounded, (c) accelerated bounded. However, unless the model charge is attached to a string (as in string theory), usually there are singularities in those solutions.</p><p>First, we would emphasize that we proposed that the existence of the massless charged spinors are represented by solution(s) of the 5D metric, rather than the 4D Maxwell potentials generated from classical massless charged particle. In fact, if the spinor solution is obtained from the massless 4D Dirac equation, with the introduction of charge, such solution must be coupled to the Maxwell potentials, and the coupled equation(s) cannot satisfy the Lorentz gauge transformation without a string attachment. Yet when this hypothetical string is reduced to zero, singularities appear in the Maxwell solutions.</p><p>It might be simple to analyze the gauge invariance property for charged massless spinor in 4D by applying the projection of the metric from 4D onto 3D (as explained in [<xref ref-type="bibr" rid="scirp.75084-ref1">1</xref>] ). In this case the Lorentz gauge is changed to the Chern-Simons gauge [<xref ref-type="bibr" rid="scirp.75084-ref31">31</xref>] . To investigate whether a massless spinor moving with c can exist in the 4D metric, let us consider the hydrogen system, where the electron is assumed to be massless. This system has a Semion ground state [<xref ref-type="bibr" rid="scirp.75084-ref32">32</xref>] with binding energy equal to the reduced mass, which is then zero, implying such a ground state does not exist. In general, massless charged spinors cannot be bounded in 4D Maxwell space-time. The solutions found in [<xref ref-type="bibr" rid="scirp.75084-ref26">26</xref>] by attaching a string, is precisely found by addition of the 4th space dimension (making the system a 5D manifold), so that a finite confinement can occur in the (added) 4th space dimension. Hence if we extend the Maxwell 4D to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x171.png" xlink:type="simple"/></inline-formula>, then a confined state of such massless charged spinors within the Maxwell 4D, due to the entangled representation between the 1D string and the 4D manifold, could exist. One can proceed and follow step by step, with the same arguments in [<xref ref-type="bibr" rid="scirp.75084-ref26">26</xref>] but by introducing a finite string as the 5th dimension, then we expect none of the singularities would appear if only the scalar potential is involved. On the other hand, if the stated extra dimension also includes the vector potentials, then in place of the vanished Coulomb potential (a problem stated by the authors in that stated paper), a magnetic monopole potential is then created. This monopole can be removed only if we impose that such massless charged spinors can only exist in charge neutral pairs, and not in single entity. In fact, this is one reason for us to hypothesize that one system of the charge pairs is the origin of the angular momentum of the universe [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] , and another system of charged pairs is proposed in this paper to be the origin of the magnetic field in stellar, perhaps also in other objects. We would endorse particular credit to that paper for laying stone for researchers to stand on and think deeply about the inclusion of charge massless entities traveling with c in Maxwell’s equations. Under the updated research in quantum electrodynamics, we must admit that we cannot offer analytical solution to the magnetic field generated by the charged current composed by oppositely circulating spinors pairs strictly under the regime of quantum field theory. We could proceed with our analysis, however, based on the fact that the boundary condition of the 5D manifold is the 4D Lorentz space. We propose that Maxwell’s equations are satisfied at the 5D-4D interphase. We therefore propose to generalize the solution of charged current J<sub>2</sub> in (4.1.4b) to the relativistic case by simply replacing v by c, obtaining an estimation of the current density:</p><disp-formula id="scirp.75084-formula277"><label>(4.1.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x172.png"  xlink:type="simple"/></disp-formula><p>And the current over the ring is</p><disp-formula id="scirp.75084-formula278"><label>(4.1.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x173.png"  xlink:type="simple"/></disp-formula><p>In passing, we would note that even if there were e &amp; -e charges circulating in opposite directions along the 1D classical current ring, the chance of annihilation is non-zero. In general, the interaction cross-section of massive particles is larger than those of massless particles, such as photons. In fact, the strength of interaction of photons with massive particles depends strongly on the masses of the interacting particles. The cross-section area of a charge-neutral neutrino is well known to be extremely small, so that equipment to detect neutrinos is set in gold mine deep down underground. It has been estimated that there is only an upper limit on the mass of neutrino<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x174.png" xlink:type="simple"/></inline-formula>, but it has not been verified that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x174.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x175.png" xlink:type="simple"/></inline-formula> is zero. As in our model, the spinors are massless, we assume that their interaction cross-sections are extremely small, so that the annihilation rate of the oppositely circulating charges is practically zero, or extremely small over the life time of an stellar object. Moreover, we would remark that the interaction cross-section increases as the wavelengths of the spinor pairs are large; namely, those spinors with very low energy has a larger chance of annihilation. At temperature close to 0 K, the Fermi particles are confined mainly in the energy range of 0 to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x174.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x175.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x176.png" xlink:type="simple"/></inline-formula>. The result of [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] demonstrates that those spinor particles contributing to the total angular momentum have energies <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x174.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x175.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x176.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x177.png" xlink:type="simple"/></inline-formula> even under the Second Law condition<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x174.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x175.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x176.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x177.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x178.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s4_2"><title>4.2. Simple Representation of the Magnetic Dipolar Field Generated by the Classical Ring Current Model with Quantum Signature Incorporated</title><p>A charge current generates magnetic field in space. The Biot-Savart Law expresses the magnetic field in terms of the magnitude, spatial length, direction, and the distance from a reference point (such as the center of a ring current) of a current. According to this law, the magnetic induction field generated by a charge current density J at the space point x is</p><disp-formula id="scirp.75084-formula279"><label>(4.2.1a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x179.png"  xlink:type="simple"/></disp-formula><p>Using elementary vector analysis,</p><disp-formula id="scirp.75084-formula280"><label>(4.2.1b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x180.png"  xlink:type="simple"/></disp-formula><p>When the distance between the coordinate origin and the point of observation is much greater the radius of the model ring current, i.e. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x181.png" xlink:type="simple"/></inline-formula>in (4.2.1b),</p><disp-formula id="scirp.75084-formula281"><label>(4.2.2a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x182.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula282"><label>(4.2.2b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x183.png"  xlink:type="simple"/></disp-formula><p>Here <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x184.png" xlink:type="simple"/></inline-formula> is the current in units of Ampere, given by expression (4.1.6) above and θ is the polar angle in the usual polar coordinate system. We need to find the number of spinors in the loop, which is</p><disp-formula id="scirp.75084-formula283"><label>(4.2.3a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x185.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x186.png" xlink:type="simple"/></inline-formula> is the spin degeneracy, energy<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x186.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x187.png" xlink:type="simple"/></inline-formula>, F is the Fermi-Dirac distribution, &amp;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x186.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x187.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x188.png" xlink:type="simple"/></inline-formula>. Since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x186.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x187.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x188.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x189.png" xlink:type="simple"/></inline-formula>, and</p><p>the statistically averaged energy is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x190.png" xlink:type="simple"/></inline-formula>, so that from (4.2.3a)</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x191.png" xlink:type="simple"/></inline-formula>; (4.2.3b)</p><p>From (4.1.6),</p><disp-formula id="scirp.75084-formula284"><label>(4.2.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x192.png"  xlink:type="simple"/></disp-formula><p>In view of the derivation in Appendix A, we obtain</p><disp-formula id="scirp.75084-formula285"><label>(4.2.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x193.png"  xlink:type="simple"/></disp-formula><p>Then from (4.2.2b), the magnetic filed measured at the equator of the matter star <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x194.png" xlink:type="simple"/></inline-formula> becomes</p><disp-formula id="scirp.75084-formula286"><label>(4.2.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x195.png"  xlink:type="simple"/></disp-formula><p>This equation may be called the Law of Intrinsic Dipole Magnetic Field for Stellar Objects.</p><p>Before we proceed to obtain numerical values to illustrate the laws we discover related to the origin of the intrinsic dipolar magnetic field of stellar objects, we need to find explicit expression of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x196.png" xlink:type="simple"/></inline-formula>. The derivation of the analytical form of this integral is given in Appendix B:</p><disp-formula id="scirp.75084-formula287"><label>(4.2.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x197.png"  xlink:type="simple"/></disp-formula><p>Through computer program, using Simpson’s rule of integration, the integral <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula> at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula>. The approximate form in Equation (4.2.7) is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula>. So the approximation is very good for our estimation. Multiplied the area (as calculated via Simpson’s rule) by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula>, the energy squared of spinors as weighted by the Fermi distribution = <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula>. At<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula>, integration using Simpson’s rule, is 18.643. Multiplied 18.643 by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula>, the energy squared of spinors as weighted by the Fermi distribution =<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula>, not much different from the case with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x206.png" xlink:type="simple"/></inline-formula>. At<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x206.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x207.png" xlink:type="simple"/></inline-formula>, integration via Simpson’s rule, is 0.86332. The energy of spinors as weighted by the Fermi distribution <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x206.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x207.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x208.png" xlink:type="simple"/></inline-formula>, which is over two orders of magnitude higher than the case with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x206.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x207.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x208.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x209.png" xlink:type="simple"/></inline-formula>. Since the integral is directly proportional to the magnetic field, it means that there must be a sudden change in the integral <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x206.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x207.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x208.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x209.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x210.png" xlink:type="simple"/></inline-formula> over<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x198.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x199.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x200.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x201.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x202.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x203.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x204.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x205.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x206.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x207.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x208.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x209.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x210.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x211.png" xlink:type="simple"/></inline-formula>, similar to the Laws reported in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] .</p><p>We now plot the I versus T graph, since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x212.png" xlink:type="simple"/></inline-formula> Joule is a universal constant, considering it as the rest mass of the lightest lepton created. <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref> shows such a graph, indicating clearly that there is a rather sharp transition, in line with our numerical analysis just stated. The graph representing Equation (4.2.7) is composed of the green straight line, and the red horizontal line, plus the blue transition curve. In fact, let us consider the situation at very high temperature</p><p>Such that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x213.png" xlink:type="simple"/></inline-formula>. Take<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x213.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x214.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x213.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x214.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x215.png" xlink:type="simple"/></inline-formula>, the two summations in (4.2.7) cancel, so that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x213.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x214.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x215.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x216.png" xlink:type="simple"/></inline-formula> is approximated by</p><disp-formula id="scirp.75084-formula288"><label>(4.2.8a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x217.png"  xlink:type="simple"/></disp-formula><p>For even greater temperature such as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x218.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.75084-formula289"><label>(4.2.8b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x219.png"  xlink:type="simple"/></disp-formula><p>to good approximation. The straight green line in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref> with a constant positive slope represents such a line.</p><p>On the other hand, if the temperature is relatively low, such that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x220.png" xlink:type="simple"/></inline-formula>, the integral in (4.2.7) takes on a constant value of</p><disp-formula id="scirp.75084-formula290"><label>(4.2.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x221.png"  xlink:type="simple"/></disp-formula><p>In <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>, the integral in this region is represented approximately by a redhorizontal line. The intersection of the above two straight lines cross at the</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref></label><caption><title> The integrand, as depicted in expression (4.2.7), is a function of temperature T (K). The straight green line with a constant positive slope represents the approximate solution given by Equation (4.2.8b). The red horizontal line represents the approximate solution indicated by Equation (4.2.9). The two straight lines intersect at. T = 3.2 &#180; 10<sup>9</sup> K. We observe that the stated approximated solutions in the “low/cold” and “high/hot” temperature ranges are very good</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x222.png"/></fig><p>temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x223.png" xlink:type="simple"/></inline-formula>. This is the transition temperature, which is &gt; Bethe temperature of fusion.</p><p>We would emphasize that integral <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x224.png" xlink:type="simple"/></inline-formula> is not the only function that could be T-dependent in calculating magnetic field. In Equation (4.2.6),</p><disp-formula id="scirp.75084-formula291"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x225.png"  xlink:type="simple"/></disp-formula><p>can also be separated into two regions in temperature. Under the First Law of the angular momentum, i.e.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x226.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.75084-formula292"><label>(4.2.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x227.png"  xlink:type="simple"/></disp-formula><p>In view of Equations (4.2.8b) &amp; (4.2.10), we obtain the Law of Intrinsic Dipole Magnetic Field for Hot Stars below:</p><disp-formula id="scirp.75084-formula293"><label>(4.2.11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x228.png"  xlink:type="simple"/></disp-formula><p>As P&amp;R are dependent implicitly on T, when T is large, P is small, and one has to carry out detailed numerical analysis before one can learn how B(eq) varies with T in realistic samples. Moreover, all the equations for B(eq) hold under the condition of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x229.png" xlink:type="simple"/></inline-formula>. In case the matter shell is thin, a more complicated procedure is needed to study the angular momentum (and hence B) as demonstrated in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] on the analysis of Pulsar angular momentum. Due to limitation in space, we shall not study stars at very high temperature in this paper as it will be</p><p>equally complicated. Here we want to emphasize that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x230.png" xlink:type="simple"/></inline-formula></p><p>can be separated into two regions in T. At small T and large T, the asymptotic lines are respectively two straight lines (one horizontal, and one with positive slope) intersecting at <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x231.png" xlink:type="simple"/></inline-formula> several times of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x231.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x232.png" xlink:type="simple"/></inline-formula>, as demonstrated in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . The above integral is in the denominator of (4.2.11). The analysis of the property of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x231.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x232.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x233.png" xlink:type="simple"/></inline-formula> above, which is in the numerator, together with the result of [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] tells us</p><p>right away that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x234.png" xlink:type="simple"/></inline-formula> is a constant for a wide</p><p>cool region. Inspection of (4.2.11) reveals that therefore B(eq) depends explicitly only on the mechanical variables in front of the quotient of the state two integrals. This is a very crucial aspect of our discovery.</p><p>Under the regime of the Second Law of angular momentum, we present in Appendix B, the approximate expression of statistically weighted over<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x235.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.75084-formula294"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x236.png"  xlink:type="simple"/></disp-formula><p>and Equation (4.2.9) already gives the approximate expression for the integral<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x237.png" xlink:type="simple"/></inline-formula>. The equatorial magnetic field as depicted in (4.2.6) becomes</p><disp-formula id="scirp.75084-formula295"><label>(4.2.12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x238.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.75084-formula296"><label>(4.2.13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x239.png"  xlink:type="simple"/></disp-formula><p>Recalling that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x240.png" xlink:type="simple"/></inline-formula>. For convenience of computation,</p><disp-formula id="scirp.75084-formula297"><label>(4.2.14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x241.png"  xlink:type="simple"/></disp-formula><p>We may call Equation (4.2.12) as the Law of Intrinsic Dipole Magnetic Field for Cool Stellar Objects. This equation will be used throughout the numerical analysis in this paper.</p><p>We have deduced the magnetic expression understand the Second Law condition because we are interested in finding the dipole field when the matter shell has been formed and the temperature of the void-matter boundary is not too high <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x242.png" xlink:type="simple"/></inline-formula> in this paper. The huge magnetic field generated by quark current has been treated qualitatively in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . The intrinsic dipole field of pulsars where T is very high, will be treated elsewhere. It is important to note that according our theory, the dipole field intensity can be calculated if we know the “mechanical variables” (M, R, P). The very large magnetic field of stars near their end stage of evolution will be discussed in a later section.</p></sec></sec><sec id="s5"><title>5. On the Plausible Origin of Huge Non-Dipolar Strong Magnetic Fields of Many Stars, Including the Old/Dying Ones</title><p>It has been shown that the Maxwell and Chern-Simon gauge theories are coupled/compatible and the charge flux pinning phenomenon can be realized by the Maxwell-Chern-Simons gauge theory in a 2D system [<xref ref-type="bibr" rid="scirp.75084-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref32">32</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref33">33</xref>] .</p><p>Now the confinement of a 3D hydrogen to a 2D state is supported by the fact that exact analytical solutions for 2D hydrogen can be derived for the non-relati- vistic and the relativistic H-atom model [<xref ref-type="bibr" rid="scirp.75084-ref34">34</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref35">35</xref>] . From the view point of the Bohr’s model, the exact solutions for the relativistic ground state of the 2D-hy- drogen atom gives a binding energy as large as the reduced mass of the composite system [<xref ref-type="bibr" rid="scirp.75084-ref34">34</xref>] . The consequence is that the binding energy plus the rest energy of the system can become zero if the positive charge (the center of attraction) is much more massive than the electron. In other words, a 2D or collapsed hydrogen atom hydrogen atom can approach a Semion state, with magnetic flux attached to every electron [<xref ref-type="bibr" rid="scirp.75084-ref33">33</xref>] .</p><p>When a star has a large mass (such as the sun) and a small radius (such as the terrestrial radius), a large gravitation gradient exists along the radial direction, confining the motion of electrons from a 3D space to a <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x243.png" xlink:type="simple"/></inline-formula> space structure, considering the stellar surface to be a plane in a local region.</p><p>From the symmetry point of view, we say that the 3D space homogeneity is broken into<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula>, with gravity field along the 1D. It is this broken space homogeneity that leads to the atomic binding from Bohr to Chern-Simons hydrogen solution. In the relativistic limit, the Chern-Simons solution is given by the Semion state, where the electron collapses into the proton environment, bringing with it the pinned magnetic flux. Since the Semion state is applicable to all elements, and not just for the hydrogen, massive neutral objects including atomic structures, can be considered in such <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula> space manifold near the stellar surface. The atomic Coulomb binding between a nucleus and its outermost electron is no longer described by the homogeneous Coulomb potential alone, but must also include a difference in energy between the gravitation potential at the nucleus<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula>, and that of the electron<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula>; where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x248.png" xlink:type="simple"/></inline-formula> &amp; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x248.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x249.png" xlink:type="simple"/></inline-formula> are respectively the nucleus&amp; electron masses; <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x248.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x249.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x250.png" xlink:type="simple"/></inline-formula>are the (radial) distances between the center of the star to the nucleus and electron respectively. From the 5D theory <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x248.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x249.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x250.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x251.png" xlink:type="simple"/></inline-formula> are both greater than void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x248.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x249.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x250.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x251.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x252.png" xlink:type="simple"/></inline-formula><sub>. </sub>Setting<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x245.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x247.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x248.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x249.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x250.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x251.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x252.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x253.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.75084-formula298"><label>(5.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x254.png"  xlink:type="simple"/></disp-formula><p>via simple expansion of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x255.png" xlink:type="simple"/></inline-formula>. Now <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x255.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x256.png" xlink:type="simple"/></inline-formula> if the nucleus is proton. The ratio <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x255.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x256.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x257.png" xlink:type="simple"/></inline-formula> is of different scale and must be much smaller than that. Therefore</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x258.png" xlink:type="simple"/></inline-formula>.</p><p>Hence for non- zero h values, the gravitational potential difference <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula> is mainly modified by the (positive)factor<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula> and has a bigger absolute value; this modification effect is larger for larger h(which is atomic size), so far as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula>, a condition always satisfied . The physical consequence is that if the gravitation potential is mainly on the radial direction, the electrons tend to escape from the stellar surface, and away from the nucleus. Let us include the effect of the binding energy of a Semion state and Coulomb potential also. Now the exact binding energy of the Semion ground state energy is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.75084-ref35">35</xref>] , which is equal to?(kinetic energy + Coulombic potential energy+<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x263.png" xlink:type="simple"/></inline-formula>).Here the relativistic kinetic energy is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x263.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x264.png" xlink:type="simple"/></inline-formula>, and the Coulombic potential energy is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x263.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x264.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x265.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x263.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x264.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x265.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x266.png" xlink:type="simple"/></inline-formula> is the distance between the nucleus and the associated electron. In other words,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x263.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x264.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x265.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x266.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x267.png" xlink:type="simple"/></inline-formula>. On the stellar surface, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x259.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x260.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x263.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x264.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x265.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x266.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x267.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x268.png" xlink:type="simple"/></inline-formula>is small compared to V in magnitude. We can say that effectively the Coulomb potential under (Semionic) gauge constrain gives rise to the relativistic electron mass. Due to pressure fluctuation, and the fact that surface temperature is at least several thousand K, some of the Semions readily have enough kinetic energy to escape the Coulombic &amp;gravitation pull, and the pinned magnetic flux is released, together with relativistic electrons.</p><p>Let us take some concrete examples. It is well-known that magnetic storms are found to be periodic on the solar surface. We anticipate that the solar motion participates in the occurrence of periodicity. Thus if the gravitational potential difference (as a matter pressure) is the cause of Semion states formation, such states are likely to be formed slightly below the photosphere. Cyclic plasma turbulence could bring the Semion states to the surface, and the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x269.png" xlink:type="simple"/></inline-formula> structure could change back to a 3D structure, releasing magnetic flux in a cyclic manner, as explained in [<xref ref-type="bibr" rid="scirp.75084-ref36">36</xref>] . The consequence is the occurrence of flares and radio wave storms (emitted by the maser effect of relativistic electrons via cyclotron radiation). In fact, close to 100% circular polarized radio waves have been reported from Brown Dwarfs and the sun [<xref ref-type="bibr" rid="scirp.75084-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref38">38</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref39">39</xref>] . Based on the frequency of the emission, the magnetic field at the source is calculated, as will be discussed further in Section (7).</p><p>We would note also that the star will be positively charged and would attract negatively charged particles with low kinetic energy. Note for small stars such as Magnetic White Dwarfs<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x270.png" xlink:type="simple"/></inline-formula>, when gravity is strong enough to provide the necessary condition for Semion states to exist, but at relative higher temperature, Semions can escape, releasing huge magnetic field as stated. Electrons leave the star, leading to reduction of stellar mass. As the star further collapses, its gravity becomes far too strong for Semions to escape, and the surface magnetic storms cease. Many White Dwarfs have masses between<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x271.png" xlink:type="simple"/></inline-formula>, showing irregular or weak magnetic field. We speculate that White Dwarfs could well be the “older stage” of Magnetic White Dwarfs which have larger masses.</p><p>Let us “borrow” some result in condensed matter physics to estimate the magnitude of magnetic field generated by a group of Semions. The 2D number density of composite fermion system σ is related to the magnetic field B by (see e.g. [<xref ref-type="bibr" rid="scirp.75084-ref31">31</xref>] )</p><disp-formula id="scirp.75084-formula299"><label>(5.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x272.png"  xlink:type="simple"/></disp-formula><p>where n is the “level” of quantum flux and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x273.png" xlink:type="simple"/></inline-formula> is the unit quantum flux given by h/e. We should note that the magnetic field is pinned in the Semion layer. We propose during the evolution, a star could go through first the change in matter density leading to a situation that would favor the formation of 2D Semion state near its surface as sketched above.</p><p>Suppose for rough estimation, let us take a magnetic white dwarf WD0011134 associated with the set of data<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x274.png" xlink:type="simple"/></inline-formula>, giving mass density of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x275.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.75084-ref40">40</xref>] . Whereas helium plus other heavier elements are formed near the matter center region, suppose there are still Semion layers whose total area amounts to the whole surface area of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x276.png" xlink:type="simple"/></inline-formula>, as an upper limit estimation. Recalling the diameter of a hydrogen atom is 120 pm, mass of proton is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x276.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x277.png" xlink:type="simple"/></inline-formula>, the total number of hypothetical Semions there is</p><disp-formula id="scirp.75084-formula300"><label>(5.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x278.png"  xlink:type="simple"/></disp-formula><p>taking the level n = 1 as the upper limit of the magnetic field B estimation. The 2D density of Semion, from Equation (5.2), is therefore</p><disp-formula id="scirp.75084-formula301"><label>(5.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x279.png"  xlink:type="simple"/></disp-formula><p>If Semions in the whole surface layer have enough energy to overcome gravitational and Coulomb attractions, the average magnetic field (which is radial in directions) over the whole stellar surface, being hypothetical released is then</p><disp-formula id="scirp.75084-formula302"><label>(5.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x280.png"  xlink:type="simple"/></disp-formula><p>It is known that the magnetic fields of Magnetic White Dwarfs are non-dipo- lar and distributed irregularly [<xref ref-type="bibr" rid="scirp.75084-ref40">40</xref>] . Thus to produce a magnetic field of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x281.png" xlink:type="simple"/></inline-formula> in certain surface areas for the particular MWD as observed, it is necessary that only a small region of the hypothetical Semion layer with area <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x281.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x282.png" xlink:type="simple"/></inline-formula> of the stellar surface forms the Semion state. When those Semions covering only <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x281.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x282.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x283.png" xlink:type="simple"/></inline-formula> of the surface area change from 2D back to 3D structure, a magnetic field ~ <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x281.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x282.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x283.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x284.png" xlink:type="simple"/></inline-formula> will be released. Note that it is the flux that can be taken as the “absolute measure”, because when the magnetic flux lines are released and spread out to a certain area A, say, the magnetic field is flux/A. Without more observable information, we cannot compare the theoretical result and the detected magnitude of the sporadic magnetic field. The above rough order of magnitude estimation points to the fact that it is feasible that pressure wave oscillations in our model could explain qualitatively the huge magnetic field detected in MWD and other old stars.</p><p>Note that this final stage of the star still possess the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x285.png" xlink:type="simple"/></inline-formula> void center, which might or might not have enough massless charged spinors to maintain a self-rotation or dipolar magnetic field. In fact, according to our theory, the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x285.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x286.png" xlink:type="simple"/></inline-formula> for cool stars. As the radius of the stars becomes smaller, even though the mass can increase, the increase in P due to loss of energy from the void as the star cools down, can cause a reduction in<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x285.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x286.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x287.png" xlink:type="simple"/></inline-formula> of stars can vary in very complicated ways as shown by many examples in Section (6) later. In the limit when R<sub>o</sub> approaches zero, the explicit expression of B (equatorial) shows that it becomes zero, together with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x285.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x286.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x287.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x288.png" xlink:type="simple"/></inline-formula> too― this is how a star “dies” in our theory.</p></sec><sec id="s6"><title>6. Analysis of the Variation of the Theoretically Derived Dipole Magnetic Field with Respect to Change of the Basic Features of a Star</title><sec id="s6_1"><title>6.1. Introduction with a Set of Data of the Halo Stars in the Orion Nebula</title><p>We have derived the equatorial magnetic surface field in terms of the basic/“raw” data set (M, R, P):</p><disp-formula id="scirp.75084-formula303"><label>(6.1.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x289.png"  xlink:type="simple"/></disp-formula><p>We define the set of variables (M, R, P) as the basics/raw data variables. In some stars, all the three variables can be measured, but the number of such stars is small, and the accuracy of measurement is left with some high degree of uncertainty. In some star groups, the radius can only be theoretically deduced; a typical example is the application of the Hamada-Salpeter equation [<xref ref-type="bibr" rid="scirp.75084-ref41">41</xref>] to obtain the radii of (cool) dwarf stars with values of mass as input data. The above expression is valid only when the angular momentum is equal to that of a solid sphere with the same mass density, as a zero-order approximation. In stars, the matter sphere is built of magnetized plasma while fusion processes proceed to build up heavier elements. Eventually, we have neutron stars as briefly sketched in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . Essentially, therefore the three basic variables are inter-connected. We will leave the more detailed discussion on the laws we discover in the next section. As the rotation periods of pulsars have been observed to be slowed down continuously, and such an aspect is intuitively true from the consideration of energy conservation, obviously the B-P relation of different star groups would bring us useful information in stellar structure and stellar evolution. Therefore, we focus on the variation of the equatorial/polar field with respect to changing period of rotation first. We remark that the normalized void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x290.png" xlink:type="simple"/></inline-formula> is a function of mass density, as analyzed in our previous paper [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . In this paper, we have found theoretically that the surface dipole field is proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x290.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x291.png" xlink:type="simple"/></inline-formula>. Therefore, we have to take data for stars within a relatively close range of density as a subgroup in our investigation. We will introduce the methodology of our analysis as we follow a number of star groups.</p><p>So we begin with the pre-main ?sequence or hollow stars of the Orion Nebula. Data of these stars in the Milky Way are taken from [<xref ref-type="bibr" rid="scirp.75084-ref42">42</xref>] . Here the mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula>, radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x293.png" xlink:type="simple"/></inline-formula>, period of rotation P(days)are “basic data”. Only stars with density D greater than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x293.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x294.png" xlink:type="simple"/></inline-formula> are included. This number is arbitrary, but the choice is based on the idea that we analyze objects with a rather concrete spherical-like structure. Inclusion of the lower density ones does not affect the result. The surface equatorial magnetic field B (eq, theory, Gauss) has been derived in Section (4) to be expressible as a function of the basic parameters only. Under the condition of the Second Law of angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x293.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x294.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x295.png" xlink:type="simple"/></inline-formula> with Fermi energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x293.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x294.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x295.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x296.png" xlink:type="simple"/></inline-formula> (rest mass of electron), we calculate this B, the void radius R<sub>o</sub>, the magnetic parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x293.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x294.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x295.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x296.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x297.png" xlink:type="simple"/></inline-formula>, the angular momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x292.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x293.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x294.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x295.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x296.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x297.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x298.png" xlink:type="simple"/></inline-formula>, density and enter these values for each star in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>(a) and <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>(b) show the B(equatorial)-P graphs for the density ranges of 48 - 100, and 100 - 160 <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x299.png" xlink:type="simple"/></inline-formula> respectively. The average den-</p><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref></label><caption><title> (a) The surface equatorial magnetic field B (eq, Gauss) vs the period of rotation P(s) for stars in the Orion of the Milky Way with mass density between about 48 to 100 kg/m<sup>3</sup>. The one off star is reported to have a radius of 3.23 solar radii, and consider that is out of the group. The correlation is over 0.9 if we take off this “off-line” sample. We keep it there to show that when the density is too low, the B-P relation is deviated from linear in the log-log plot. The maximum of horizontal axis is 10<sup>6</sup> s. See data in <xref ref-type="table" rid="table1">Table 1</xref>; (b) The surface equatorial magnetic field B(eq, Gauss) vs the period of rotation P(s) for stars in the Orion of the Milky Way with mass density between about 100 to 160 kg/m<sup>3</sup>, using data in <xref ref-type="table" rid="table1">Table 1</xref>. The correlation is good and power index is −0.69. Though the correlation is good, further analysis as shown in the text indicates that the comparison between theory and experimental data is not simple, and several steps are needed, and the methodology becomes clearer as we go through the other sub-sections following.</title></caption><fig id ="fig2_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x300.png"/></fig><fig id ="fig2_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x301.png"/></fig></fig-group><table-wrap-group id="1"><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Data of the pre-main-sequence stars in the Orion Nebula in the Milky Way are taken from [<xref ref-type="bibr" rid="scirp.75084-ref42">42</xref>] . Here the mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula>, radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula>, period of rotation P(days)are “basic data”. Stars with density D greater than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x304.png" xlink:type="simple"/></inline-formula> are included. This number is arbitrary, but the choice is based on the idea that we analyze objects with a rather concrete spherical-like structure. Inclusion of the lower density ones does not affect the result. The surface equatorial magnetic field B (eq, theory, Gauss) has been derived in Section (5) to be expressible as a function of the basic parameters only. Under the condition of the Second Law of angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x304.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x305.png" xlink:type="simple"/></inline-formula> with Fermi energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x304.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x305.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x306.png" xlink:type="simple"/></inline-formula> (rest mass of electron), we calculate this B, the void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x304.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x305.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x306.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x307.png" xlink:type="simple"/></inline-formula>, the magnetic parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x304.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x305.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x306.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x307.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x308.png" xlink:type="simple"/></inline-formula>, the angular momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x302.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x303.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x304.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x305.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x306.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x307.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x308.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x309.png" xlink:type="simple"/></inline-formula>, density and enter these values for each star in the table</title></caption><table-wrap id="1_1"><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >Orion stars</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x310.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x311.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x312.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x313.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x314.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" >B (eq, theory, Gauss)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x315.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x316.png" xlink:type="simple"/></inline-formula></th></tr></thead><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1171</td><td align="center" valign="middle" >0.26</td><td align="center" valign="middle" >1.98</td><td align="center" valign="middle" >6.3936</td><td align="center" valign="middle" >2.611 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.497 &#215; 1027</td><td align="center" valign="middle" >3.857 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.5733</td><td align="center" valign="middle" >4.798 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.151 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >1219</td><td align="center" valign="middle" >0.40</td><td align="center" valign="middle" >1.96</td><td align="center" valign="middle" >1.1319</td><td align="center" valign="middle" >2.530 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.455 &#215; 1027</td><td align="center" valign="middle" >3.285 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.9430</td><td align="center" valign="middle" >7.502 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.967 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >1297</td><td align="center" valign="middle" >1.38</td><td align="center" valign="middle" >1.90</td><td align="center" valign="middle" >5.7280</td><td align="center" valign="middle" >2.308 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.347 &#215; 1027</td><td align="center" valign="middle" >2.104 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.3170</td><td align="center" valign="middle" >2.847 &#215; 102</td><td align="center" valign="middle" >1.761 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >1325</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >1.30</td><td align="center" valign="middle" >3.8360</td><td align="center" valign="middle" >7.391 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.594 &#215; 1026</td><td align="center" valign="middle" >2.132 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.2980</td><td align="center" valign="middle" >1.286 &#215; 102</td><td align="center" valign="middle" >9.930 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >1354</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.67</td><td align="center" valign="middle" >0.6912</td><td align="center" valign="middle" >1.567 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.613 &#215; 1027</td><td align="center" valign="middle" >2.245 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >3.5820</td><td align="center" valign="middle" >6.973 &#215; 101</td><td align="center" valign="middle" >1.789 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >1368</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.35</td><td align="center" valign="middle" >2.3846</td><td align="center" valign="middle" >8.277 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.612 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.137 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.9470</td><td align="center" valign="middle" >1.320 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.180 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >1396</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >2.03</td><td align="center" valign="middle" >1.6589</td><td align="center" valign="middle" >2.814 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.520 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.683 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >1.6060</td><td align="center" valign="middle" >4.727 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.665 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >1428</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >1.31</td><td align="center" valign="middle" >1.0022</td><td align="center" valign="middle" >7.563 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.352 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.042 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.1100</td><td align="center" valign="middle" >1.068 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.339 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >1440</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >1.47</td><td align="center" valign="middle" >1.1750</td><td align="center" valign="middle" >1.069 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.512 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.201 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >3.2860</td><td align="center" valign="middle" >1.200 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.530 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >1453</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.66</td><td align="center" valign="middle" >1.1750</td><td align="center" valign="middle" >1.539 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.740 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.305 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.4300</td><td align="center" valign="middle" >7.100 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.562 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >11</td><td align="center" valign="middle" >1465</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >1.85</td><td align="center" valign="middle" >1.1059</td><td align="center" valign="middle" >2.130 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.176 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.021 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.4300</td><td align="center" valign="middle" >6.000 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.742 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >12</td><td align="center" valign="middle" >1485</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.44</td><td align="center" valign="middle" >5.4778</td><td align="center" valign="middle" >1.005 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.513 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.106 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.9470</td><td align="center" valign="middle" >1.088 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >0.990 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >13</td><td align="center" valign="middle" >1500</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >1.90</td><td align="center" valign="middle" >7.6205</td><td align="center" valign="middle" >2.308 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.163 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.750 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.5040</td><td align="center" valign="middle" >4.940 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.058 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >14</td><td align="center" valign="middle" >1501</td><td align="center" valign="middle" >0.29</td><td align="center" valign="middle" >1.74</td><td align="center" valign="middle" >7.5427</td><td align="center" valign="middle" >1.772 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.183 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.816 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.6674</td><td align="center" valign="middle" >7.770 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.065 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >15</td><td align="center" valign="middle" >1511</td><td align="center" valign="middle" >0.38</td><td align="center" valign="middle" >1.89</td><td align="center" valign="middle" >1.3306</td><td align="center" valign="middle" >2.271 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >6.026 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.240 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.6530</td><td align="center" valign="middle" >7.948 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.832 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >16</td><td align="center" valign="middle" >1522</td><td align="center" valign="middle" >0.35</td><td align="center" valign="middle" >2.09</td><td align="center" valign="middle" >6.2986</td><td align="center" valign="middle" >3.071 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.053 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.872 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.6683</td><td align="center" valign="middle" >5.414 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.279 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >17</td><td align="center" valign="middle" >1545</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle" >1.79</td><td align="center" valign="middle" >4.5965</td><td align="center" valign="middle" >1.930 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.602 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.216 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.8300</td><td align="center" valign="middle" >6.155 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.178 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >18</td><td align="center" valign="middle" >1566</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.57</td><td align="center" valign="middle" >6.0480</td><td align="center" valign="middle" >1.302 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.006 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.268 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.7724</td><td align="center" valign="middle" >8.393 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.008 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >19</td><td align="center" valign="middle" >1627</td><td align="center" valign="middle" >0.26</td><td align="center" valign="middle" >1.93</td><td align="center" valign="middle" >8.7264</td><td align="center" valign="middle" >2.419 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.141 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.685 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.4719</td><td align="center" valign="middle" >5.107 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.052 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >1753</td><td align="center" valign="middle" >0.16</td><td align="center" valign="middle" >3.23</td><td align="center" valign="middle" >3.6288</td><td align="center" valign="middle" >1.134 &#215; 10<sup>28</sup></td><td align="center" valign="middle" >3.315 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.113 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >0.2924</td><td align="center" valign="middle" >6.582 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.500 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >21</td><td align="center" valign="middle" >1760</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >1.57</td><td align="center" valign="middle" >5.2963</td><td align="center" valign="middle" >1.302 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.000 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.252 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.7680</td><td align="center" valign="middle" >7.298 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.007 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >22</td><td align="center" valign="middle" >1805</td><td align="center" valign="middle" >0.30</td><td align="center" valign="middle" >2.03</td><td align="center" valign="middle" >4.5965</td><td align="center" valign="middle" >2.814 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.217 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >6.507 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.7880</td><td align="center" valign="middle" >5.064 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.312 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >23</td><td align="center" valign="middle" >1966</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >1.86</td><td align="center" valign="middle" >6.1430</td><td align="center" valign="middle" >2.165 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.240 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.000 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.5730</td><td align="center" valign="middle" >4.828 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.081 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >24</td><td align="center" valign="middle" >2037</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >1.73</td><td align="center" valign="middle" >1.8490</td><td align="center" valign="middle" >1.742 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.643 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >8.224 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.5170</td><td align="center" valign="middle" >5.727 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.392 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >25</td><td align="center" valign="middle" >2168</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >1.63</td><td align="center" valign="middle" >5.2877</td><td align="center" valign="middle" >1.457 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.099 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.550 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.7540</td><td align="center" valign="middle" >6.847 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.039 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >26</td><td align="center" valign="middle" >2246</td><td align="center" valign="middle" >0.33</td><td align="center" valign="middle" >1.63</td><td align="center" valign="middle" >8.1734</td><td align="center" valign="middle" >1.457 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.113 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.595 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.7636</td><td align="center" valign="middle" >1.076 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.043 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >27</td><td align="center" valign="middle" >2301</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >1.42</td><td align="center" valign="middle" >0.7344</td><td align="center" valign="middle" >9.633 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >3.051 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.964 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.1676</td><td align="center" valign="middle" >7.398 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.460 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >28</td><td align="center" valign="middle" >2425</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >1.44</td><td align="center" valign="middle" >1.4774</td><td align="center" valign="middle" >1.005 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.655 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.414 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.6472</td><td align="center" valign="middle" >6.148 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.191 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >29</td><td align="center" valign="middle" >2744</td><td align="center" valign="middle" >0.43</td><td align="center" valign="middle" >1.79</td><td align="center" valign="middle" >5.6419</td><td align="center" valign="middle" >1.930 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.063 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.910 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.0689</td><td align="center" valign="middle" >1.059 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.281 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >30</td><td align="center" valign="middle" >2784</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >1.26</td><td align="center" valign="middle" >3.4214</td><td align="center" valign="middle" >6.730 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.072 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.470 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.5930</td><td align="center" valign="middle" >1.553 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.030 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >31</td><td align="center" valign="middle" >2913</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >1.65</td><td align="center" valign="middle" >4.5014</td><td align="center" valign="middle" >1.511 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.263 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.073 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.8356</td><td align="center" valign="middle" >6.601 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.088 &#215; 10<sup>6</sup></td></tr></tbody></table></table-wrap><table-wrap id="1_2"><table><tbody><thead><tr><th align="center" valign="middle" >32</th><th align="center" valign="middle" >2470</th><th align="center" valign="middle" >0.23</th><th align="center" valign="middle" >1.55</th><th align="center" valign="middle" >2.4278</th><th align="center" valign="middle" >1.253 &#215; 10<sup>27</sup></th><th align="center" valign="middle" >1.956 &#215; 10<sup>27</sup></th><th align="center" valign="middle" >5.506 &#215; 10<sup>42</sup></th><th align="center" valign="middle" >1.5613</th><th align="center" valign="middle" >8.722 &#215; 10<sup>1</sup></th><th align="center" valign="middle" >1.259 &#215; 10<sup>6</sup></th></tr></thead><tr><td align="center" valign="middle" >33</td><td align="center" valign="middle" >3014</td><td align="center" valign="middle" >1.13</td><td align="center" valign="middle" >1.74</td><td align="center" valign="middle" >6.7565</td><td align="center" valign="middle" >1.772 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.562 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.225 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.0100</td><td align="center" valign="middle" >3.029 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.537 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >34</td><td align="center" valign="middle" >3115</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >1.91</td><td align="center" valign="middle" >5.8147</td><td align="center" valign="middle" >2.344 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.567 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.098 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.6686</td><td align="center" valign="middle" >5.472 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.169 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >35</td><td align="center" valign="middle" >3142</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.62</td><td align="center" valign="middle" >7.4650</td><td align="center" valign="middle" >1.430 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.001 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.956 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.6293</td><td align="center" valign="middle" >7.639 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >0.972 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >36</td><td align="center" valign="middle" >3161</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >1.89</td><td align="center" valign="middle" >0.7258</td><td align="center" valign="middle" >2.271 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.345 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.215 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >3.2344</td><td align="center" valign="middle" >5.647 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.957 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >37</td><td align="center" valign="middle" >3189</td><td align="center" valign="middle" >0.30</td><td align="center" valign="middle" >1.54</td><td align="center" valign="middle" >6.0480</td><td align="center" valign="middle" >1.229 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.158 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.846 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.9428</td><td align="center" valign="middle" >1.160 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.078 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >38</td><td align="center" valign="middle" >3217</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >1.35</td><td align="center" valign="middle" >3.2314</td><td align="center" valign="middle" >8.277 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.283 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.138 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.5500</td><td align="center" valign="middle" >1.320 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.094 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >39</td><td align="center" valign="middle" >3314</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >1.42</td><td align="center" valign="middle" >4.5446</td><td align="center" valign="middle" >9.633 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.652 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.147 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.0020</td><td align="center" valign="middle" >9.864 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >0.995 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >40</td><td align="center" valign="middle" >3341</td><td align="center" valign="middle" >1.12</td><td align="center" valign="middle" >1.80</td><td align="center" valign="middle" >1.4256</td><td align="center" valign="middle" >1.962 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.196 &#215; 10<sup>28</sup></td><td align="center" valign="middle" >6.158 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >6.0970</td><td align="center" valign="middle" >2.712 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >2.302 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >41</td><td align="center" valign="middle" >3406</td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >2.03</td><td align="center" valign="middle" >2.4106</td><td align="center" valign="middle" >2.814 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.589 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.233 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >1.9860</td><td align="center" valign="middle" >9.115 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.786 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >42</td><td align="center" valign="middle" >3438</td><td align="center" valign="middle" >0.14</td><td align="center" valign="middle" >1.55</td><td align="center" valign="middle" >2.2032</td><td align="center" valign="middle" >1.253 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.450 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.693 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.1572</td><td align="center" valign="middle" >5.309 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.139 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >43</td><td align="center" valign="middle" >3613</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >1.87</td><td align="center" valign="middle" >0.9763</td><td align="center" valign="middle" >2.200 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.965 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.906 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.2570</td><td align="center" valign="middle" >4.750 &#215; 10<sup>1</sup></td><td align="center" valign="middle" >1.717 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >45</td><td align="center" valign="middle" >3668</td><td align="center" valign="middle" >0.66</td><td align="center" valign="middle" >1.20</td><td align="center" valign="middle" >7.0675</td><td align="center" valign="middle" >5.813 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.318 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.253 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.2670</td><td align="center" valign="middle" >5.394 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.104 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >46</td><td align="center" valign="middle" >3672</td><td align="center" valign="middle" >0.30</td><td align="center" valign="middle" >1.27</td><td align="center" valign="middle" >6.4627</td><td align="center" valign="middle" >6.891 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.497 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.811 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.2330</td><td align="center" valign="middle" >2.068 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >0.953 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >47</td><td align="center" valign="middle" >3678</td><td align="center" valign="middle" >0.36</td><td align="center" valign="middle" >1.61</td><td align="center" valign="middle" >5.6419</td><td align="center" valign="middle" >1.404 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.539 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.001 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.0965</td><td align="center" valign="middle" >1.218 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.162 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >48</td><td align="center" valign="middle" >3756</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >1.76</td><td align="center" valign="middle" >4.2422</td><td align="center" valign="middle" >1.834 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.197 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.060 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >1.7430</td><td align="center" valign="middle" >1.554 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.483 &#215; 10<sup>6</sup></td></tr></tbody></table></table-wrap></table-wrap-group><p>sity of the stars in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>(a) is very low, and we neglect the mathematical analysis. The B-P plot in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>(b) for stars with density in the range of about 1.0 - 1.6 <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x317.png" xlink:type="simple"/></inline-formula> gives an expression</p><disp-formula id="scirp.75084-formula304"><label>(6.1.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x318.png"  xlink:type="simple"/></disp-formula><p>Substituting (6.1.2) into (6.1.1), we arrive at</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x319.png" xlink:type="simple"/></inline-formula>,</p><p>Or</p><disp-formula id="scirp.75084-formula305"><label>(6.1.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x320.png"  xlink:type="simple"/></disp-formula><p>Further analysis shows that there is no clear mathematical relation of the P-R plot, nor the P-M plot, using the raw data. In other words, we cannot compare the theoretical prediction and experimental relations for this group of stars. Such a result is to be expected, because they are halo stars and the theory assumes that the angular momentum expression to be represented by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x321.png" xlink:type="simple"/></inline-formula>. The average density of this pre-main sequence stars is one order smaller than the sun, which is a lump of plasma, and is several hundred times smaller than that of the earth. As we proceed to analyze different groups with greater density, the comparison between theory and raw data becomes valid.</p></sec><sec id="s6_2"><title>6.2. NGC 6819 Stars</title><p>We proceed with another group of stars with larger density, since the magnitude of B is sensitive to density values. Parameters include mass M in units of solar mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x322.png" xlink:type="simple"/></inline-formula>, radius R (in units of solar radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x322.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x323.png" xlink:type="simple"/></inline-formula>), the period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x322.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x323.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x324.png" xlink:type="simple"/></inline-formula> of 30 stars in NGC 6819 according to [<xref ref-type="bibr" rid="scirp.75084-ref43">43</xref>] . The masses are read approximately from the data points of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x322.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x323.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x324.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x325.png" xlink:type="simple"/></inline-formula> graph of [<xref ref-type="bibr" rid="scirp.75084-ref43">43</xref>] . The radius is deduced according to the following equation:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x322.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x323.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x324.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x325.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x326.png" xlink:type="simple"/></inline-formula>, for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x322.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x323.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x324.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x325.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x326.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x327.png" xlink:type="simple"/></inline-formula> as in reference [<xref ref-type="bibr" rid="scirp.75084-ref44">44</xref>] . The other variables are calculated and entered into <xref ref-type="table" rid="table2">Table 2</xref>, with the same setting of <xref ref-type="table" rid="table1">Table 1</xref>.</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Some parameters of stars in NGC 6819. Parameters mass M in units of solar mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula>, radius R (in units of solar radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula>), period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula> of 30 stars in NGC 6819 according to [<xref ref-type="bibr" rid="scirp.75084-ref43">43</xref>] and the deduced void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula>, the equatorial surface magnetic field B(equatorial, Gauss) are calculated, under the condition of the Second Law <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula> according to Section (5) of this paper. The Fermi energy of the spinorpairs is taken to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x333.png" xlink:type="simple"/></inline-formula>. The masses are read approximately from the data points of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x333.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x334.png" xlink:type="simple"/></inline-formula> graph of [<xref ref-type="bibr" rid="scirp.75084-ref43">43</xref>] . The radius is deduced according to the following equation:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x333.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x334.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x335.png" xlink:type="simple"/></inline-formula>, for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x333.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x334.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x335.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x336.png" xlink:type="simple"/></inline-formula>, as in reference [<xref ref-type="bibr" rid="scirp.75084-ref44">44</xref>] . The magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x333.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x334.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x335.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x336.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x337.png" xlink:type="simple"/></inline-formula> and the angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x330.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x331.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x332.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x333.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x334.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x335.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x336.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x337.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x338.png" xlink:type="simple"/></inline-formula> are also entered into the table</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >No.</th><th align="center" valign="middle" >NGC 6819 stars</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >R(m)</th><th align="center" valign="middle" >P(s)</th><th align="center" valign="middle" >R<sup>3</sup> (10<sup>26</sup>m<sup>3</sup>)</th><th align="center" valign="middle" >G-R<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >Iω (J-s)</th><th align="center" valign="middle" >B (eq, G)</th><th align="center" valign="middle" >D (10<sup>2</sup> kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub>(m)</th></tr></thead><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >5,111,207</td><td align="center" valign="middle" >1.405</td><td align="center" valign="middle" >1.0166 &#215; 10<sup>9</sup></td><td align="center" valign="middle" >4.568 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >10.507</td><td align="center" valign="middle" >4.33 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.59 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >4.123</td><td align="center" valign="middle" >6.19</td><td align="center" valign="middle" >1.64 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >5,023,899</td><td align="center" valign="middle" >1.37</td><td align="center" valign="middle" >9.9267 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >4.156 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >9.7820</td><td align="center" valign="middle" >4.40 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.62 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >4.500</td><td align="center" valign="middle" >6.52</td><td align="center" valign="middle" >1.65 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >5,023,760</td><td align="center" valign="middle" >1.355</td><td align="center" valign="middle" >9.8239 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >4.130 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >9.4810</td><td align="center" valign="middle" >4.32 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.58 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >4.556</td><td align="center" valign="middle" >6.79</td><td align="center" valign="middle" >1.64 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >5,024,227</td><td align="center" valign="middle" >1.355</td><td align="center" valign="middle" >9.8239 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >4.370 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >9.4810</td><td align="center" valign="middle" >4.14 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.52 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >4.366</td><td align="center" valign="middle" >6.79</td><td align="center" valign="middle" >1.62 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >5,024,122</td><td align="center" valign="middle" >1.3</td><td align="center" valign="middle" >9.4470 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >5.500 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >8.4300</td><td align="center" valign="middle" >3.19 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.06 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >3.781</td><td align="center" valign="middle" >7.33</td><td align="center" valign="middle" >1.48 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >5,112,499</td><td align="center" valign="middle" >1.28</td><td align="center" valign="middle" >9.3093 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >3.840 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >8.0680</td><td align="center" valign="middle" >4.04 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.45 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >5.003</td><td align="center" valign="middle" >7.54</td><td align="center" valign="middle" >1.60 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >5,113,601</td><td align="center" valign="middle" >1.28</td><td align="center" valign="middle" >9.3093 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >6.060 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >8.0680</td><td align="center" valign="middle" >2.87 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.16 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.552</td><td align="center" valign="middle" >7.54</td><td align="center" valign="middle" >1.43 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >5,026,583</td><td align="center" valign="middle" >1.228</td><td align="center" valign="middle" >8.9520 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >4.230 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >7.1730</td><td align="center" valign="middle" >3.43 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.16 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >4.776</td><td align="center" valign="middle" >8.13</td><td align="center" valign="middle" >1.52 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >4,938,993</td><td align="center" valign="middle" >1.21</td><td align="center" valign="middle" >8.8273 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.030 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >6.8787</td><td align="center" valign="middle" >1.71 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.60 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.484</td><td align="center" valign="middle" >8.36</td><td align="center" valign="middle" >1.20 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >5,111,834</td><td align="center" valign="middle" >1.101</td><td align="center" valign="middle" >8.0740 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.200 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >5.2635</td><td align="center" valign="middle" >1.08 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.99 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.051</td><td align="center" valign="middle" >9.94</td><td align="center" valign="middle" >1.03 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >11</td><td align="center" valign="middle" >5,111,908</td><td align="center" valign="middle" >1.09</td><td align="center" valign="middle" >7.9975 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.500 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >5.1160</td><td align="center" valign="middle" >1.02 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.32 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.998</td><td align="center" valign="middle" >10.1</td><td align="center" valign="middle" >1.01 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >12</td><td align="center" valign="middle" >5,024,856</td><td align="center" valign="middle" >1.037</td><td align="center" valign="middle" >7.6296 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.570 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >4.4420</td><td align="center" valign="middle" >8.88 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.92 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.999</td><td align="center" valign="middle" >11.1</td><td align="center" valign="middle" >9.67 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >13</td><td align="center" valign="middle" >5,024,280</td><td align="center" valign="middle" >1.026</td><td align="center" valign="middle" >7.5531 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.500 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >4.3100</td><td align="center" valign="middle" >8.99 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.95 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.085</td><td align="center" valign="middle" >11.3</td><td align="center" valign="middle" >9.71 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >14</td><td align="center" valign="middle" >5,112,507</td><td align="center" valign="middle" >1.026</td><td align="center" valign="middle" >7.5531 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.570 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >4.3093</td><td align="center" valign="middle" >8.68 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.86 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.013</td><td align="center" valign="middle" >11.3</td><td align="center" valign="middle" >9.60 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >15</td><td align="center" valign="middle" >5,023,796</td><td align="center" valign="middle" >1.012</td><td align="center" valign="middle" >7.4558 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.580 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >4.1450</td><td align="center" valign="middle" >8.38 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.78 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.023</td><td align="center" valign="middle" >11.6</td><td align="center" valign="middle" >9.49 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >16</td><td align="center" valign="middle" >5,024,008</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >7.3723 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.590 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >4.0070</td><td align="center" valign="middle" >8.13 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.71 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.030</td><td align="center" valign="middle" >11.9</td><td align="center" valign="middle" >9.40 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >17</td><td align="center" valign="middle" >5,023,724</td><td align="center" valign="middle" >0.99</td><td align="center" valign="middle" >7.3030 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.560 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.8943</td><td align="center" valign="middle" >8.09 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.70 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.078</td><td align="center" valign="middle" >12.1</td><td align="center" valign="middle" >9.38 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >18</td><td align="center" valign="middle" >5,023,875</td><td align="center" valign="middle" >0.978</td><td align="center" valign="middle" >7.2193 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.580 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.7620</td><td align="center" valign="middle" >7.77 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.61 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.066</td><td align="center" valign="middle" >12.4</td><td align="center" valign="middle" >9.26 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >19</td><td align="center" valign="middle" >5,112,268</td><td align="center" valign="middle" >0.972</td><td align="center" valign="middle" >7.1775 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.620 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.6970</td><td align="center" valign="middle" >7.56 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.55 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.045</td><td align="center" valign="middle" >12.5</td><td align="center" valign="middle" >9.17 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >4,937,169</td><td align="center" valign="middle" >0.952</td><td align="center" valign="middle" >7.0870 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.700 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.4853</td><td align="center" valign="middle" >6.97 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.39 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.000</td><td align="center" valign="middle" >13.0</td><td align="center" valign="middle" >8.92 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >21</td><td align="center" valign="middle" >5,025,271</td><td align="center" valign="middle" >0.952</td><td align="center" valign="middle" >7.0871 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.840 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.4853</td><td align="center" valign="middle" >6.55 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.28 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.880</td><td align="center" valign="middle" >13.0</td><td align="center" valign="middle" >8.74 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >22</td><td align="center" valign="middle" >5,111,939</td><td align="center" valign="middle" >0.952</td><td align="center" valign="middle" >7.0871 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.880 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.4853</td><td align="center" valign="middle" >6.45 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.26 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.850</td><td align="center" valign="middle" >13.0</td><td align="center" valign="middle" >8.70 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >23</td><td align="center" valign="middle" >5,112,871</td><td align="center" valign="middle" >0.946</td><td align="center" valign="middle" >6.9953 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.840 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.4234</td><td align="center" valign="middle" >6.47 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.26 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.890</td><td align="center" valign="middle" >13.1</td><td align="center" valign="middle" >8.71 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >24</td><td align="center" valign="middle" >5,023,666</td><td align="center" valign="middle" >0.93</td><td align="center" valign="middle" >6.8834 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.860 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.2620</td><td align="center" valign="middle" >6.18 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.18 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.894</td><td align="center" valign="middle" >13.5</td><td align="center" valign="middle" >8.57 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >25</td><td align="center" valign="middle" >5,024,182</td><td align="center" valign="middle" >0.916</td><td align="center" valign="middle" >6.7860 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.840 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.1245</td><td align="center" valign="middle" >6.03 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.15 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.930</td><td align="center" valign="middle" >13.9</td><td align="center" valign="middle" >8.50 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >26</td><td align="center" valign="middle" >5,023,926</td><td align="center" valign="middle" >0.903</td><td align="center" valign="middle" >6.6949 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.800 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.0000</td><td align="center" valign="middle" >5.94 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.13 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.980</td><td align="center" valign="middle" >14.3</td><td align="center" valign="middle" >8.46 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >27</td><td align="center" valign="middle" >4,937,149</td><td align="center" valign="middle" >0.883</td><td align="center" valign="middle" >6.5544 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.870 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.8160</td><td align="center" valign="middle" >5.49 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.01 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.950</td><td align="center" valign="middle" >14.9</td><td align="center" valign="middle" >8.24 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >28</td><td align="center" valign="middle" >4,936,891</td><td align="center" valign="middle" >0.862</td><td align="center" valign="middle" >6.4069 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.900 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.6300</td><td align="center" valign="middle" >5.16 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.32 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.960</td><td align="center" valign="middle" >15.6</td><td align="center" valign="middle" >8.07 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >29</td><td align="center" valign="middle" >4,937,119</td><td align="center" valign="middle" >0.852</td><td align="center" valign="middle" >6.3367 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >2.010 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.5445</td><td align="center" valign="middle" >4.81 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.51 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.890</td><td align="center" valign="middle" >15.9</td><td align="center" valign="middle" >7.89 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >30</td><td align="center" valign="middle" >4,937,356</td><td align="center" valign="middle" >0.847</td><td align="center" valign="middle" >6.3019 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.830 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.5024</td><td align="center" valign="middle" >5.10 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.17 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.038</td><td align="center" valign="middle" >16.1</td><td align="center" valign="middle" >8.04 &#215; 10<sup>5</sup></td></tr></tbody></table></table-wrap><p>First, we plot the B − P graph in log scale using the measured basic variables (established expression like mass-radius relation for dwarfs). <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref> gives such a graph with a negative slope of −0.584. Equation (6.1.1) can then be written as</p><disp-formula id="scirp.75084-formula306"><label>(6.2.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x339.png"  xlink:type="simple"/></disp-formula><p>Since the correlation is very good, we can assume that</p><disp-formula id="scirp.75084-formula307"><label>(6.2.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x340.png"  xlink:type="simple"/></disp-formula><p>is valid, and Equation (6.2.1) becomes</p><disp-formula id="scirp.75084-formula308"><label>(6.2.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x341.png"  xlink:type="simple"/></disp-formula><p>Since the stars are associated with various values of the sets (M, R, P), if Equation (6.2.2) is to be approximately true, these variables must vary in such a way that the function F<sub>1</sub> is approximately a constant. We plot in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref> the values of F<sub>1 </sub>for these 30 stars using the raw data from <xref ref-type="table" rid="table2">Table 2</xref>. There are some fluctuations, but in a rough way, we can proceed to analyze Equation (6.2.3), taking F<sub>1</sub> as a constant.</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref></label><caption><title> The variation of the theoretical surface magnetic fields B (eq, theory, Gauss) of NGC 6819 stars with changing period of rotation P(s), according to the 5D theory. The data are taken from numbers entered into <xref ref-type="table" rid="table2">Table 2</xref>. The slope of the log-log plot is about minus 0.584</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x342.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref></label><caption><title> Values of the function F<sub>1</sub> for 30 stars in NGC 6819. The upper horizontal line represents the value 3.0 &#180; 10<sup>8</sup>. The average of these 30 numbers is about 2.5 &#180; 10<sup>8</sup> (SI units)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x343.png"/></fig><p>Equation (6.2.2) can then be approximated by:</p><disp-formula id="scirp.75084-formula309"><label>(6.2.4a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x344.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula310"><label>(6.2.4b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x345.png"  xlink:type="simple"/></disp-formula><p>Employing raw data from <xref ref-type="table" rid="table2">Table 2</xref> for different star members of the NGC 6819 group, the graph of log P against log R is linear with a slope of -3.76 (see <xref ref-type="fig" rid="fig5"><xref ref-type="fig" rid="fig">Figure </xref>5</xref>), so that Equation (6.2.4b) can be expressed as</p><disp-formula id="scirp.75084-formula311"><label>(6.2.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x346.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula312"><label>(6.2.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x347.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula313"><label>(6.2.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x348.png"  xlink:type="simple"/></disp-formula><p>Note that the above equation is the consequence of the theoretically derived Equation (6.2.1), with the use of the P-R relation from measured data. To test the validity of the theory, we now use the raw data sets (M, R) from <xref ref-type="table" rid="table2">Table 2</xref>, and plot their relation in <xref ref-type="fig" rid="fig6"><xref ref-type="fig" rid="fig">Figure </xref>6</xref> below. This graph gives a power index of 1.0612. Observing that there are variations of data of this group of stars with density several hundred of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x349.png" xlink:type="simple"/></inline-formula>, the comparison can be considered to give satisfactory result. Recollecting no such comparison is possible for pre-main sequence stars with mass density up to 160<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x349.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x350.png" xlink:type="simple"/></inline-formula>, we observe that we might arrive at better results with other star groups with larger mass density (and/or more accurate data) in later sub-sections.</p><p>Following, <xref ref-type="fig" rid="fig7"><xref ref-type="fig" rid="fig">Figure </xref>7</xref> shows the variation of the theoretical surface magnetic fields B (eq, theory, G) of NGC 6819 stars with changing values of the void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x351.png" xlink:type="simple"/></inline-formula>. The result indicates that for larger void size, the surface magnetic field is larger because the effective number of spinor pairs rotating in opposite direction is also larger. The variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x351.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x352.png" xlink:type="simple"/></inline-formula> vs density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x351.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x352.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x353.png" xlink:type="simple"/></inline-formula> is shown in <xref ref-type="fig" rid="fig8"><xref ref-type="fig" rid="fig">Figure </xref>8</xref>, giving slope of −0.867. Such a result suggests that those</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5"><xref ref-type="fig" rid="fig">Figure </xref>5</xref></label><caption><title> Employing raw data values in <xref ref-type="table" rid="table2">Table 2</xref>, this graph shows the variation of the period P with different values of the radius R for different star members. The slope of the above graph is −3.761. The maximum of horizontal axis is 2 &#180; 10<sup>9</sup> m</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x354.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6"><xref ref-type="fig" rid="fig">Figure </xref>6</xref></label><caption><title> The Mass?radius relation using raw data from <xref ref-type="table" rid="table2">Table 2</xref>. The slope of the power relation is 1.0612. As a very rough estimation, we predict from theory that the slope of the log M-log R plot is 1.168. The maximum value on the horizontal axis is 2.0 &#180; 10<sup>9</sup> m</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x355.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7"><xref ref-type="fig" rid="fig">Figure </xref>7</xref></label><caption><title> The variation of the theoretical surface magnetic fields B (eq, Gauss) of NGC 6819 stars with changing void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x357.png" xlink:type="simple"/></inline-formula> indicates that for larger void size, the surface magnetic field is larger because the effective number of spinor pairs rotating in opposite direction is also larger. For other basic parameters and calculated variables, refer to <xref ref-type="table" rid="table2">Table 2</xref>. The slope of this log-log plot is about 1.3. The maximum of the horizontal axis is 2.0 &#180; 10<sup>6</sup> m</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x356.png"/></fig><p>stars have larger void radius R<sub>o</sub> when the mass density is low, suggesting that gravity contraction causes the void size to decrease, but at a very slow rate because the value of the slope is not far from unity. We would investigate whether such effect is similar to other star groups, and the power index should in principle, indicative of the mass of the stars involved. As suggested by the crowing of data points in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref> and <xref ref-type="fig" rid="fig8"><xref ref-type="fig" rid="fig">Figure </xref>8</xref>, we could have divided these 30 stars into two sub-groups according to density. Since the NGC 6819 stars have density up to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x358.png" xlink:type="simple"/></inline-formula> as a maximum value, we will not do such sub-divi- sion analysis, but would proceed to analyze other groups with different densities in the following sub-sections. Using the “raw data” in <xref ref-type="table" rid="table2">Table 2</xref>, we show the M- R relation in a log-log plot, giving a power index of 1.0612. The deduction is not very accurate, as expected, since the model is rather crude; however the analysis provides a modality to analyze stellar properties.</p><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8"><xref ref-type="fig" rid="fig">Figure </xref>8</xref></label><caption><title> Void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x360.png" xlink:type="simple"/></inline-formula> against the mass density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x360.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x361.png" xlink:type="simple"/></inline-formula> for the 30 NGC 6819 stars. The limit of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x360.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x361.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x362.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x359.png"/></fig></sec><sec id="s6_3"><title>6.3. Low to-Mid Mass Main Sequence Stars</title><p>We follow up to study the B - P graph for Low-to-Mid mass main sequence stars. Parameters mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x363.png" xlink:type="simple"/></inline-formula>, period of rotation P are obtained from the data published in [<xref ref-type="bibr" rid="scirp.75084-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref46">46</xref>] , with radius deduced using the equation in [<xref ref-type="bibr" rid="scirp.75084-ref44">44</xref>] . Other relevant data calculated are entered into <xref ref-type="table" rid="table3">Table 3</xref>. <xref ref-type="fig" rid="fig9"><xref ref-type="fig" rid="fig">Figure </xref>9</xref> gives us the power index is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x363.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x364.png" xlink:type="simple"/></inline-formula>, and Equation (6.1.1) for this group becomes</p><disp-formula id="scirp.75084-formula314"><label>(6.3.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x365.png"  xlink:type="simple"/></disp-formula><p>Following the argument of the previous sub-section, we can take that the function</p><disp-formula id="scirp.75084-formula315"><label>(6.3.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x366.png"  xlink:type="simple"/></disp-formula><p>is approximately constant, and the above equation gives <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x367.png" xlink:type="simple"/></inline-formula>, resulting</p><disp-formula id="scirp.75084-formula316"><label>(6.3.3a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x368.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula317"><label>(6.3.3b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x369.png"  xlink:type="simple"/></disp-formula><p>Since the M vs R plot is a good straight line with positive slope β = 1.0985(<xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>0), we can write (6.3.3b) as</p><disp-formula id="scirp.75084-formula318"><label>(6.3.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x370.png"  xlink:type="simple"/></disp-formula><p>We require</p><disp-formula id="scirp.75084-formula319"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x371.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula320"><label>(6.3.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x372.png"  xlink:type="simple"/></disp-formula><p>If one plots the P-R graph (not shown here), the line of best fit has a very large positive slope(specified by angle<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x373.png" xlink:type="simple"/></inline-formula>), in line with our theoretical result of tan <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x373.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x374.png" xlink:type="simple"/></inline-formula> in our text above. We calculate, using experimental raw data from <xref ref-type="table" rid="table3">Table 3</xref>, the quantity A of (6.3.5) and plot it against the number of stars in this</p><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9"><xref ref-type="fig" rid="fig">Figure </xref>9</xref></label><caption><title> Employing values in <xref ref-type="table" rid="table3">Table 3</xref>, theoretically deduced equatorial dipolar magnetic field B (eq, Gauss) against rotation period <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x376.png" xlink:type="simple"/></inline-formula> of twelve Low-to-Mid Mass main sequence stars. The power index is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x376.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x377.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x375.png"/></fig><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>0</label><caption><title> The measured variation of mass M (kg) with respect to change of radius R of some members of the Low-to-Mid Mass main sequence stars (see <xref ref-type="table" rid="table3">Table 3</xref>). The power index is about 1.0985 here, as compared to the theoretical prediction value of 1.1; see details in Section (5). The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x379.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x378.png"/></fig><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Low-to-mid mass main sequence stars. Parameters mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x380.png" xlink:type="simple"/></inline-formula>, period of rotation P are obtained from the data published in [<xref ref-type="bibr" rid="scirp.75084-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref46">46</xref>] , with radius deduced using the equation in [<xref ref-type="bibr" rid="scirp.75084-ref44">44</xref>] . The intrinsic dipolar magnetic fields B(equatorial, theory, Gauss), the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x380.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x381.png" xlink:type="simple"/></inline-formula> are calculated according to the theory presented in Section (4) of this paper under the condition of the Second Law of angular momentum, with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x380.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x381.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x382.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x380.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x381.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x382.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x383.png" xlink:type="simple"/></inline-formula> is taken to be the rest mass of electron</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Star</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >R (10<sup>8</sup> m)</th><th align="center" valign="middle" >P(s)</th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" >B-R<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >Iω (J-s)</th><th align="center" valign="middle" >B (eq, theory, G)</th><th align="center" valign="middle" >D (10<sup>3</sup> kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (10<sup>6</sup> m)</th></tr></thead><tr><td align="center" valign="middle" >Sun</td><td align="center" valign="middle" >1.0000</td><td align="center" valign="middle" >6.9550</td><td align="center" valign="middle" >2.1600 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.364 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.9211 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.120 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.760</td><td align="center" valign="middle" >1.3880</td><td align="center" valign="middle" >0.8453</td></tr><tr><td align="center" valign="middle" >KIC892376</td><td align="center" valign="middle" >0.4699</td><td align="center" valign="middle" >3.6112</td><td align="center" valign="middle" >1.3237 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.709 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.0214 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.300 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >21.690</td><td align="center" valign="middle" >4.7400</td><td align="center" valign="middle" >1.0133</td></tr><tr><td align="center" valign="middle" >1026474</td><td align="center" valign="middle" >0.5914</td><td align="center" valign="middle" >4.4878</td><td align="center" valign="middle" >1.3556 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >9.038 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.6540 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.394 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >18.300</td><td align="center" valign="middle" >3.1090</td><td align="center" valign="middle" >1.1897</td></tr><tr><td align="center" valign="middle" >1026146</td><td align="center" valign="middle" >0.6472</td><td align="center" valign="middle" >4.8869</td><td align="center" valign="middle" >1.2866 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.167 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >3.7140 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >6.008 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.182</td><td align="center" valign="middle" >2.6344</td><td align="center" valign="middle" >0.7234</td></tr><tr><td align="center" valign="middle" >1162635</td><td align="center" valign="middle" >0.4497</td><td align="center" valign="middle" >3.4643</td><td align="center" valign="middle" >1.3546 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >4.158 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.6210 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.993 &#215; 10<sup>4</sup><sup>1</sup></td><td align="center" valign="middle" >3.900</td><td align="center" valign="middle" >5.1385</td><td align="center" valign="middle" >0.5490</td></tr><tr><td align="center" valign="middle" >1164102</td><td align="center" valign="middle" >0.5606</td><td align="center" valign="middle" >4.2220</td><td align="center" valign="middle" >2.7210 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >7.529 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.5270 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.837 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.028</td><td align="center" valign="middle" >3.5400</td><td align="center" valign="middle" >0.5379</td></tr><tr><td align="center" valign="middle" >1027110</td><td align="center" valign="middle" >0.6046</td><td align="center" valign="middle" >4.5824</td><td align="center" valign="middle" >1.4697 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >9.622 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.6310 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.320 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >16.950</td><td align="center" valign="middle" >2.9850</td><td align="center" valign="middle" >1.1850</td></tr><tr><td align="center" valign="middle" >1160684</td><td align="center" valign="middle" >0.5239</td><td align="center" valign="middle" >4.0021</td><td align="center" valign="middle" >3.6200 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >6.410 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >3.4186 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.159 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >53.330</td><td align="center" valign="middle" >3.8826</td><td align="center" valign="middle" >1.5163</td></tr><tr><td align="center" valign="middle" >1027277</td><td align="center" valign="middle" >0.6735</td><td align="center" valign="middle" >5.0744</td><td align="center" valign="middle" >5.1960 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.307 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.4210 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.669 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.088</td><td align="center" valign="middle" >2.4488</td><td align="center" valign="middle" >0.5253</td></tr><tr><td align="center" valign="middle" >IM VirB</td><td align="center" valign="middle" >0.6644</td><td align="center" valign="middle" >4.7363</td><td align="center" valign="middle" >1.1320 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >1.063 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.2365 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >6.585 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >21.050</td><td align="center" valign="middle" >2.9710</td><td align="center" valign="middle" >1.3166</td></tr><tr><td align="center" valign="middle" >GU BooA</td><td align="center" valign="middle" >0.6101</td><td align="center" valign="middle" >4.3608</td><td align="center" valign="middle" >4.2336 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >8.293 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >3.8760 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.371 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >46.740</td><td align="center" valign="middle" >3.4950</td><td align="center" valign="middle" >1.5810</td></tr><tr><td align="center" valign="middle" >UV PscB</td><td align="center" valign="middle" >0.7644</td><td align="center" valign="middle" >5.8074</td><td align="center" valign="middle" >6.9120 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.959 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.8855 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.865 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >24.944</td><td align="center" valign="middle" >1.8540</td><td align="center" valign="middle" >1.7080</td></tr><tr><td align="center" valign="middle" >YY GemA</td><td align="center" valign="middle" >0.5992</td><td align="center" valign="middle" >4.3079</td><td align="center" valign="middle" >7.5168 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >7.995 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >2.4030 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.399 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >30.054</td><td align="center" valign="middle" >3.5600</td><td align="center" valign="middle" >1.3554</td></tr></tbody></table></table-wrap><p>group in the following <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>1. The constant A for 12 stars with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x384.png" xlink:type="simple"/></inline-formula>. Thus, with the power index having the units of s/m, we have deduced an explicit relation between R and P for the Low-to-Mid mass main sequence stars:</p><disp-formula id="scirp.75084-formula321"><label>(6.3.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x385.png"  xlink:type="simple"/></disp-formula><p>With the establishment of (6.3.6), we also deduce that</p><disp-formula id="scirp.75084-formula322"><label>(6.3.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x386.png"  xlink:type="simple"/></disp-formula><p>Likewise, we obtain</p><disp-formula id="scirp.75084-formula323"><label>(6.3.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x387.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula324"><label>(6.3.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x388.png"  xlink:type="simple"/></disp-formula><p>The result of Equation (6.3.9) is shown in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>2. Note that as explained in Section (2.3), the void radius R<sub>o</sub> and hence current loop size depends also the type of elements generated in the matter shell at the time of observation.</p><fig id="fig11"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>1</label><caption><title> According to our theory, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x390.png" xlink:type="simple"/></inline-formula>, a constant. Using raw data from <xref ref-type="table" rid="table3">Table 3</xref>, we plot these values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x390.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x391.png" xlink:type="simple"/></inline-formula> for 12 Low-to-Mid Mass main sequence stars <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x390.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x391.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x392.png" xlink:type="simple"/></inline-formula> and are found, in this figure, to be close to constant, with an average of 404.83 s</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x389.png"/></fig><fig id="fig12"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>2</label><caption><title> Employing values in <xref ref-type="table" rid="table3">Table 3</xref>, theoretically deduced equatorial dipolar magnetic field B (Gauss) against void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x394.png" xlink:type="simple"/></inline-formula> of twelve Low-to-Mid Mass main sequence stars, with relatively good correlation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x393.png"/></fig><p>Among this group of stars, we cannot expect all the star samples are built of hydrogen only. Thus the correlation of 0.83 in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>2 refelects the stated variation, and in our opinion, such correlation is already high in astronomy studies.</p></sec><sec id="s6_4"><title>6.4. M34 Stars</title><p>M34 stars are pre-dwarfs having mass density slightly greater than that discussed in the last sub-section. Basic data are taken from [<xref ref-type="bibr" rid="scirp.75084-ref47">47</xref>] and other relevant variables are calculated and listed in <xref ref-type="table" rid="table4">Table 4</xref>. Taking M34 stars within a mass density range of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x395.png" xlink:type="simple"/></inline-formula> from <xref ref-type="table" rid="table4">Table 4</xref>, we plot the B-P graph in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>3. The slope is −0.915. Putting the equation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x395.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x396.png" xlink:type="simple"/></inline-formula> into Equation (6.1.1), we arrive at</p><disp-formula id="scirp.75084-formula325"><label>(6.4.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x397.png"  xlink:type="simple"/></disp-formula><p>Using raw data from <xref ref-type="table" rid="table4">Table 4</xref>, the M-R relation is shown in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>4, giving a slope of 0.9169. Substituting equation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x398.png" xlink:type="simple"/></inline-formula> into Equation (6.4.1), we get</p><disp-formula id="scirp.75084-formula326"><label>(6.4.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x399.png"  xlink:type="simple"/></disp-formula><p>So far, we can say that Equation (6.4.2) is a consequence of the derived Equation (6.1.1) with input of raw data. The P-R plot in log scale (<xref ref-type="fig" rid="fig">Figure </xref>not shown) from raw data shows a slope of ~5, supporting Equation (6.4.2) though the</p><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Stars of the M34 group [<xref ref-type="bibr" rid="scirp.75084-ref47">47</xref>] . The equatorial magnetic fields B (Gauss) are calculated according to the theory of Section (5) of this paper. The deduced values of the magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x400.png" xlink:type="simple"/></inline-formula> and the void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x400.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x401.png" xlink:type="simple"/></inline-formula>, together with the mass density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x400.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x401.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x402.png" xlink:type="simple"/></inline-formula> are calculated and entered into the table. Numerically, B and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x400.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x401.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x402.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x403.png" xlink:type="simple"/></inline-formula> can be found by using the following equations derived in this paper.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x400.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x401.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x402.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x403.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x404.png" xlink:type="simple"/></inline-formula></title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Star no.</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >R/R<sub>?</sub></th><th align="center" valign="middle" >P (s)</th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >Iω (J-s)</th><th align="center" valign="middle" >B (Gauss)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (m)</th></tr></thead><tr><td align="center" valign="middle" >M34-1-304</td><td align="center" valign="middle" >0.90</td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" >5.250 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >2.2150 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.2830 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.1390 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >5.792</td><td align="center" valign="middle" >1.930 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.0940 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-1-459</td><td align="center" valign="middle" >0.58</td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >1.2476 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >5.2970 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.326 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.4820 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >25.03</td><td align="center" valign="middle" >5.200 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.1060 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-1-654</td><td align="center" valign="middle" >0.82</td><td align="center" valign="middle" >0.77</td><td align="center" valign="middle" >8.0836 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >1.5360 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >7.209 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.4550 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >4.694</td><td align="center" valign="middle" >2.540 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.0247 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1015</td><td align="center" valign="middle" >0.53</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >9.5472 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.9580 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.3094 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.2250 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >33.082</td><td align="center" valign="middle" >6.361 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.1010 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1017</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >3.1389 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.0657 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >4.4500 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.4435 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >14.52</td><td align="center" valign="middle" >7.593 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.6845 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1054</td><td align="center" valign="middle" >0.53</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >*1.0637 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.9580 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >2.1472 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >3.9555 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >5.425</td><td align="center" valign="middle" >6.361 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.0271 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1178</td><td align="center" valign="middle" >0.74</td><td align="center" valign="middle" >0.69</td><td align="center" valign="middle" >9.3226 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.1050 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.8605 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.1428 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >25.90</td><td align="center" valign="middle" >3.182 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.4290 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1540</td><td align="center" valign="middle" >0.95</td><td align="center" valign="middle" >0.92</td><td align="center" valign="middle" >5.9072 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >2.6200 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.3300 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.2930 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >5.078</td><td align="center" valign="middle" >1.850 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.1070 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1719</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >0.41</td><td align="center" valign="middle" >7.5514 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.3190 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.0570 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.4235 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >45.58</td><td align="center" valign="middle" >9.220 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.0253 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-1-1906</td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >0.50</td><td align="center" valign="middle" >2.0805 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.2053 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >7.6310 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.5700 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >18.145</td><td align="center" valign="middle" >6.100 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.1980 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-1-2324</td><td align="center" valign="middle" >0.36</td><td align="center" valign="middle" >0.34</td><td align="center" valign="middle" >5.3654 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.3220 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >8.7230 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.8760 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >65.984</td><td align="center" valign="middle" >1.294 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >9.6164 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-1-2370</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >5.3309 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >7.3850 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >5.4260 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.9620 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >73.47</td><td align="center" valign="middle" >1.800 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >8.2094 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-2-599</td><td align="center" valign="middle" >0.67</td><td align="center" valign="middle" >0.63</td><td align="center" valign="middle" >8.6400 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >8.4123 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >4.3610 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >7.4460 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >5.185</td><td align="center" valign="middle" >3.784 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >5.1850 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >M34-2-2676</td><td align="center" valign="middle" >0.47</td><td align="center" valign="middle" >0.43</td><td align="center" valign="middle" >3.9053 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.6750 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.9230 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.3840 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >71.90</td><td align="center" valign="middle" >8.347 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.2510 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >M34-2-3071</td><td align="center" valign="middle" >0.91</td><td align="center" valign="middle" >0.88</td><td align="center" valign="middle" >6.7262 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >2.2930 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.0934 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >3.4640 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >4.768</td><td align="center" valign="middle" >1.885 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.0368 &#215; 10<sup>6</sup></td></tr></tbody></table></table-wrap><p>*this datum was observed under poor condition.</p><fig id="fig13"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>3</label><caption><title> The equatorial magnetic field B (eq, Gauss) vs <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x406.png" xlink:type="simple"/></inline-formula> for 12 examples of M34 stars (within the density range of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x406.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x407.png" xlink:type="simple"/></inline-formula>) using data in <xref ref-type="table" rid="table4">Table 4</xref> [<xref ref-type="bibr" rid="scirp.75084-ref47">47</xref>] . The slope is-0.915 for these pre-dwarf stars</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x405.png"/></fig><fig id="fig14"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>4</label><caption><title> Mass vs radius of 12 pre-Dwarfs of the M34 group within a rather wide mass density of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x409.png" xlink:type="simple"/></inline-formula>. The slope is 0.9169. The limit of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x409.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x410.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x408.png"/></fig><p>points are relatively scattered, due to large variation of the mass density among these samples. Just as that demonstrated in the last sub-section, if we have enough samples of narrow density range, the agreement between theory and measured result would be much better. Following, we plot the D-R graph in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>5. The negative slope indicates that the smaller the star, the higher the density, implying that in the star group more elements are formed in smaller sized stars, increasing the gravity force which leads to a smaller radius. This feature is characteristic of pre-Dwarfs and Dwarfs.</p></sec><sec id="s6_5"><title>6.5. Averages of 254 Stars in the NGC 2516 Group</title><p>NGC 2516 is an open star cluster in the southern sky, also called Southern Beehive [<xref ref-type="bibr" rid="scirp.75084-ref48">48</xref>] . Following the same method as in other groups, basic data are taken from [<xref ref-type="bibr" rid="scirp.75084-ref49">49</xref>] and other variables are calculated, listed in <xref ref-type="table" rid="table5">Table 5</xref>. The B-P graph indicated in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>6 can be represented by the equation</p><disp-formula id="scirp.75084-formula327"><label>(6.5.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x411.png"  xlink:type="simple"/></disp-formula><p>Substituting Equation (6.5.1) into (6.1.1), we have,</p><disp-formula id="scirp.75084-formula328"><label>(6.5.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x412.png"  xlink:type="simple"/></disp-formula><p>This function F<sub>5</sub> has been found numerically to be <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x413.png" xlink:type="simple"/></inline-formula> (SI units) for the five sets of averages of totally 254 stars, and we assume F<sub>5 </sub>to be a constant in our rough estimation, so that</p><disp-formula id="scirp.75084-formula329"><label>(6.5.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x414.png"  xlink:type="simple"/></disp-formula><p>which becomes</p><disp-formula id="scirp.75084-formula330"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x415.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula331"><label>(6.5.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x416.png"  xlink:type="simple"/></disp-formula><p>From (6.5.3) &amp; (6.5.4), we obtain an equation relating M and P resulting from theory (with information from basic data only):</p><disp-formula id="scirp.75084-formula332"><label>(6.5.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x417.png"  xlink:type="simple"/></disp-formula><fig-group id="fig15"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>5</label><caption><title> Mass density vs radius of the same 12 pre-dwarfs M34 (as in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>4) within a wide range of density. The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x419.png" xlink:type="simple"/></inline-formula>.</title></caption><fig id ="fig15_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x418.png"/></fig></fig-group><table-wrap id="table5" ><label><xref ref-type="table" rid="table5">Table 5</xref></label><caption><title> Five data set representing 254 Low massstars in NGC 2516.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x420.png" xlink:type="simple"/></inline-formula>, R, P values are all taken from [<xref ref-type="bibr" rid="scirp.75084-ref49">49</xref>] . The equatorial magnetic fields B (Gauss) are calculated according to the theory of Section (5) of this paper. The deduced values of the magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x420.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x421.png" xlink:type="simple"/></inline-formula> and the void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x420.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x421.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x422.png" xlink:type="simple"/></inline-formula>, together with the mass density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x420.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x421.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x422.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x423.png" xlink:type="simple"/></inline-formula> are calculated and entered into the table. Numerically, B and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x420.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x421.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x422.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x423.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x424.png" xlink:type="simple"/></inline-formula> can be found by using the following equations derived in this paper.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x420.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x421.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x422.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x423.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x424.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x425.png" xlink:type="simple"/></inline-formula></title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Star no.</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >Radius (m)</th><th align="center" valign="middle" >P(s)</th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >Iω(J-s)</th><th align="center" valign="middle" >B (Gauss)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub>(m)</th></tr></thead><tr><td align="center" valign="middle" >N2516-1-1-784</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >5.61 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.6508 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >3.220 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.9700 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >69.254</td><td align="center" valign="middle" >2.430 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.230 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >N2516-1-1-351</td><td align="center" valign="middle" >0.44</td><td align="center" valign="middle" >0.41</td><td align="center" valign="middle" >2.00 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >2.3187 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >5.000 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.9345 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >21.570</td><td align="center" valign="middle" >9.020 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.000 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >N2516-1-1-958</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >5.44 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.0660 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >2.950 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.416 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >9.615</td><td align="center" valign="middle" >7.593 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.700 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >N2516-1-1-881</td><td align="center" valign="middle" >0.55</td><td align="center" valign="middle" >0.51</td><td align="center" valign="middle" >6.63 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.4630 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >3.341 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.2200 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >7.487</td><td align="center" valign="middle" >5.855 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.980 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >N2516-1-1-1470</td><td align="center" valign="middle" >0.56</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >7.61 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.7300 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >3.147 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.8166 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >6.652</td><td align="center" valign="middle" >5.624 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.850 &#215; 10<sup>5</sup></td></tr></tbody></table></table-wrap><fig id="fig16"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>6</label><caption><title> 254 Low massstars in NGC 2516. The equatorial magnetic fields B (eq, Gauss) is plotted against the period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x427.png" xlink:type="simple"/></inline-formula> using the data in <xref ref-type="table" rid="table5">Table 5</xref> (from [<xref ref-type="bibr" rid="scirp.75084-ref49">49</xref>] ). The slope is minus 0.89</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x426.png"/></fig><p>We use the basic data from <xref ref-type="table" rid="table5">Table 5</xref> to plot the P-R graph &amp;M-R relation in <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>7 and <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>8 respectively; these graphs have power indices of 3.3721 &amp;1.349 respectively. The agreement of the M-R relation between theory and experiment (1.37 vs 1.349) is amazingly close, noting that only three significant figures have been used in computation.</p><p>In the following <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>9, we show the dependence of B (eq, theory, Gauss) on void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x428.png" xlink:type="simple"/></inline-formula>, showing a slope of 3.718 in the log-log plot. In <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>0 we show the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x428.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x429.png" xlink:type="simple"/></inline-formula> graph. Note that within this D range, when D increases <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x428.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x429.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x430.png" xlink:type="simple"/></inline-formula> still increases with it, implying that gravity contraction has not been effective in these 254 stars. We also see that the power index in the M-R plot in</p><p><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>8 is relatively large, being 1.3487, suggesting material is being added on the star with M&amp; R increasing at the same time. It is interesting to note that the power index is only 0.4123. We expect for Dwarfs, such an index in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x431.png" xlink:type="simple"/></inline-formula> would turn over to negative values.</p></sec><sec id="s6_6"><title>6.6. Brown Dwarfs with Effectively 1353 Star Data</title><p>Nine sets of raw data, each representing an average of 150 stars are entered into <xref ref-type="table" rid="table6">Table 6</xref>. Effectively we have averages of 1350 brown dwarfs. In addition, we add another three sets of data for three brown dwarfs with relative fast rotation speeds according to ref [<xref ref-type="bibr" rid="scirp.75084-ref50">50</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref52">52</xref>] and [<xref ref-type="bibr" rid="scirp.75084-ref36">36</xref>] .</p><p>As shown in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>1, the power index <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x432.png" xlink:type="simple"/></inline-formula> is −0.96, and following the same procedure in analysis, we arrive at an equation for these brown dwarf samples:</p><disp-formula id="scirp.75084-formula333"><label>(6.6.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x433.png"  xlink:type="simple"/></disp-formula><p>This constant F is found to be about <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x434.png" xlink:type="simple"/></inline-formula> (SI units).Similarly, we write (6.6.1) as</p><disp-formula id="scirp.75084-formula334"><label>(6.6.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x435.png"  xlink:type="simple"/></disp-formula><p>which becomes</p><fig id="fig17"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>7</label><caption><title> The period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x437.png" xlink:type="simple"/></inline-formula> of the averages of 254 low mass stars in the NGC 2516 versus the radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x437.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x438.png" xlink:type="simple"/></inline-formula> in a log-log plot. The slope is 3.3721 and correlation is good. See <xref ref-type="table" rid="table5">Table 5</xref> for other data values. The maximum value of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x437.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x438.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x439.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x436.png"/></fig><fig id="fig18"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>8</label><caption><title> Mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x441.png" xlink:type="simple"/></inline-formula> versus Radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x441.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x442.png" xlink:type="simple"/></inline-formula> of 254 low mass stars in the NGC 2516 based on “raw data” listed in <xref ref-type="table" rid="table5">Table 5</xref>. The slope is 1.3487 with excellent correlation. The theoretically predicted value is 1.37 (see Equation (6.5.5))</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x440.png"/></fig><fig id="fig19"  position="float"><label><xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>9</label><caption><title> 254 Low massstars in NGC 2516. The equatorial magnetic fields B (eq, Gauss) is plotted against the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x444.png" xlink:type="simple"/></inline-formula> using the data in <xref ref-type="table" rid="table5">Table 5</xref> (from [<xref ref-type="bibr" rid="scirp.75084-ref49">49</xref>] ). The slope is about 3.72. The maximum of the horizontal axis is 2 &#180; 10<sup>6</sup> m</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x443.png"/></fig><fig id="fig20"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>0</label><caption><title> The void radius R<sub>o</sub> is plotted against the mass density D for the 254 stars in NGC 2516, represented by five averaged sets. Note that within this D range, when D increases R<sub>o</sub> still increases with it, implying that gravity contraction has not been effective in these 254 stars. It is interesting to note that the power index is only 0.4123. We expect for Dwarfs, such an index in the<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x446.png" xlink:type="simple"/></inline-formula> would turn over to negative values. The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x446.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x447.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x445.png"/></fig><fig id="fig21"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>1</label><caption><title> Employing values in <xref ref-type="table" rid="table6">Table 6</xref>, theoretically deduced equatorial dipolar magnetic field B (Gauss) against rotation period <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x449.png" xlink:type="simple"/></inline-formula> of 1350 Brown Dwarfs. Each of the set of 9 data points labelled BDL in <xref ref-type="table" rid="table6">Table 6</xref> represents the average of 150 stars. The last three members in the same table, i.e. TVLM, J0036, J1835 are individual dwarfs as reported in [<xref ref-type="bibr" rid="scirp.75084-ref36">36</xref>] . B = 3.0 &#215; 10<sup>6</sup> P<sup>−0.96</sup></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x448.png"/></fig><table-wrap id="table6" ><label><xref ref-type="table" rid="table6">Table 6</xref></label><caption><title> Data of 1350 Brown dwarfs in the Pleiades [<xref ref-type="bibr" rid="scirp.75084-ref50">50</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref52">52</xref>] . The data of the last three brown dwarfs are taken from [<xref ref-type="bibr" rid="scirp.75084-ref36">36</xref>] . Parameters include mass M, radius R, period of rotation P, mass density D are entered into this table. Here, the radius is assumed to follow the Hamada-Salpeter model [<xref ref-type="bibr" rid="scirp.75084-ref41">41</xref>] for dwarfs. The intrinsic dipolar magnetic field along the equator <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x450.png" xlink:type="simple"/></inline-formula> and the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x450.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x451.png" xlink:type="simple"/></inline-formula> are deduced based on the theory of this paper. The magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x450.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x451.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x452.png" xlink:type="simple"/></inline-formula> (based on our theory) and angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x450.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x451.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x452.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x453.png" xlink:type="simple"/></inline-formula> are also entered. Note that the log-log plot of these two variables follow a straight line. The dependent variables are deduced based on the Second Law of angular momentum [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x450.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x451.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x452.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x453.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x454.png" xlink:type="simple"/></inline-formula>taking the Fermi energy of the spinor pairs to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x450.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x451.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x452.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x453.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x454.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x455.png" xlink:type="simple"/></inline-formula>. We would also remark that each representative datum point from BPL102-BPL190 published is the average of slightly over150 members</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Star no.</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >R/R<sub>?</sub></th><th align="center" valign="middle" >P (s)</th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" >Iω(J-s)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >B(eq, G)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (m)</th></tr></thead><tr><td align="center" valign="middle" >BPL102</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle" >0.26981</td><td align="center" valign="middle" >7.7040 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >6.608 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >5.720 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >3.577 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >54.13</td><td align="center" valign="middle" >1.800 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >7.145 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL106</td><td align="center" valign="middle" >0.08</td><td align="center" valign="middle" >0.09744</td><td align="center" valign="middle" >1.4688 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.112 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >1.250 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.145 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >367.8</td><td align="center" valign="middle" >1.220 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.887 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL115</td><td align="center" valign="middle" >0.10</td><td align="center" valign="middle" >0.12031</td><td align="center" valign="middle" >1.0476 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.859 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >3.343 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.392 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >408.3</td><td align="center" valign="middle" >8.100 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >6.248 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL125</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >0.17649</td><td align="center" valign="middle" >6.9660 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.850 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >1.623 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.428 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >77.22</td><td align="center" valign="middle" >3.850 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.216 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL129</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >0.15416</td><td align="center" valign="middle" >3.4700 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.233 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >2.154 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.721 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >139.62</td><td align="center" valign="middle" >5.000 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.600 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL138</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle" >0.28600</td><td align="center" valign="middle" >9.2916 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >7.870 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >5.324 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >3.392 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >43.1</td><td align="center" valign="middle" >5.970 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >7.020 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL150</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.20967</td><td align="center" valign="middle" >6.6456 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.100 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >2.880 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.140 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >69.00</td><td align="center" valign="middle" >2.760 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >6.020 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL164</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >0.15416</td><td align="center" valign="middle" >7.2576 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.233 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >1.030 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >9.894 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >80.27</td><td align="center" valign="middle" >5.000 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.641 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >BPL190</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >0.17649</td><td align="center" valign="middle" >1.4497 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >1.850 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >7.800 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >8.030 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >43.42</td><td align="center" valign="middle" >3.850 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.343 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >TVLM</td><td align="center" valign="middle" >0.07</td><td align="center" valign="middle" >0.10300</td><td align="center" valign="middle" >7.0490 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.676 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >2.550 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.952 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >530.94</td><td align="center" valign="middle" >9.047 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.840 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >J0036</td><td align="center" valign="middle" >0.067</td><td align="center" valign="middle" >0.09500</td><td align="center" valign="middle" >1.1088 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.884 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >1.320 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.191 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >413.0</td><td align="center" valign="middle" >1.104 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.952 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >J1835</td><td align="center" valign="middle" >0.083</td><td align="center" valign="middle" >0.10700</td><td align="center" valign="middle" >1.0224 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.120 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >2.250 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.777 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >431.13</td><td align="center" valign="middle" >9.568 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.659 &#215; 10<sup>5</sup></td></tr></tbody></table></table-wrap><disp-formula id="scirp.75084-formula335"><label>(6.6.3a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x456.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula336"><label>(6.6.3b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x457.png"  xlink:type="simple"/></disp-formula><p>Since the graph of log P against log R is linear with a slope of +2.4462 (see <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>2), Equation (6.6.3b) can be expressed as</p><disp-formula id="scirp.75084-formula337"><label>(6.6.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x458.png"  xlink:type="simple"/></disp-formula><p>under the constrain</p><disp-formula id="scirp.75084-formula338"><label>(6.6.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x459.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula339"><label>(6.6.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x460.png"  xlink:type="simple"/></disp-formula><p>The log M versus log R plot in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>3 shows a slope of 1.185. The discrepancy is rather expected as the data points in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x461.png" xlink:type="simple"/></inline-formula> graphs are rather scattered, with only moderate correlation<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x461.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x462.png" xlink:type="simple"/></inline-formula>, implying the functional dependence among (M, R, P) is rather complicated. A relatively slight increase of the slope from 2.4462 to 2.91125 in the P―R graph would bring out a theoretical prediction of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x461.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x462.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x463.png" xlink:type="simple"/></inline-formula>, identical to that obtained from basic data. The B (eq, theory, G) vs R<sub>o</sub>/R graph is shown in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>4, as an illustration of the Law of Intrinsic Dipole Magnetic Field for Cool Stellar Objects, namely, expression (4.2.14). Note also that the theoretical pole field is twice the equatorial field, so the maximum surface field of Brown Dwarfs is within the kGauss range, as observed.</p><fig id="fig22"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>2</label><caption><title> Each of the set of 9 data points labelled BDL in <xref ref-type="table" rid="table6">Table 6</xref> represents the average of 150 stars. Using these data, together with other three members in the same table, (i.e., TVLM, J0036, J1835) the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x465.png" xlink:type="simple"/></inline-formula> vs radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x465.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x466.png" xlink:type="simple"/></inline-formula> graph in log scale is shown above. The slope of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x465.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x466.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x467.png" xlink:type="simple"/></inline-formula> plot is 2.4462. The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x465.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x466.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x467.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x468.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x464.png"/></fig><fig id="fig23"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>3</label><caption><title> Using data in <xref ref-type="table" rid="table6">Table 6</xref>, we show the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x470.png" xlink:type="simple"/></inline-formula> relation for 1350 Brown Dwarfs (represented by averages of 9 groups) plus three other individual ones. The slope is 1.1849</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x469.png"/></fig><fig id="fig24"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>4</label><caption><title> Surface equatorial field B (eq, theory, Gauss) vs the normalized void radius R<sub>o</sub>/R for averages of 1353 Brown Dwarfs thin a rather wide range mass density as specified. This is an illustration of the Law of Intrinsic Dipole Magnetic Field for Cool Stellar Objects. The maximum value on the horizontal axis is 10<sup>−2</sup>. The slope is 3.0 as depicted in expression (4.2.14)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x471.png"/></fig></sec><sec id="s6_7"><title>6.7. White Dwarfs</title><p>Basic data for a number of White Dwarfs are obtained from [<xref ref-type="bibr" rid="scirp.75084-ref53">53</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref54">54</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref55">55</xref>] . Other variables are calculated and entered into <xref ref-type="table" rid="table7">Table 7</xref>. Using sets of (B, P) values, we show in the usual way the B-P graph in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>5, finding the slope to be by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x472.png" xlink:type="simple"/></inline-formula>, and expression (6.1.1) becomes</p><disp-formula id="scirp.75084-formula340"><label>(6.7.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x473.png"  xlink:type="simple"/></disp-formula><p>We have found that numerically, as in other star groups the LHS of the following equation is an approximate constant:</p><disp-formula id="scirp.75084-formula341"><label>(6.7.2a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x474.png"  xlink:type="simple"/></disp-formula><p>leading to</p><disp-formula id="scirp.75084-formula342"><label>(6.7.2b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x475.png"  xlink:type="simple"/></disp-formula><p>Equation (6.7.2b) indicates that our theory predicts a large negative slope</p><table-wrap id="table7" ><label><xref ref-type="table" rid="table7">Table 7</xref></label><caption><title> White dwarfs. This table lists Mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula>, radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula>, period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula> of some white dwarfs with low mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula> based on [<xref ref-type="bibr" rid="scirp.75084-ref53">53</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref54">54</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref55">55</xref>] . Here, the radius is assumed to follow the Hamada-Salpeter model [<xref ref-type="bibr" rid="scirp.75084-ref41">41</xref>] for dwarfs. The intrinsic dipolar magnetic field along the equator <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x480.png" xlink:type="simple"/></inline-formula> and the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x480.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x481.png" xlink:type="simple"/></inline-formula> are deduced based on the theory of this paper. The magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x480.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x481.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x482.png" xlink:type="simple"/></inline-formula> and angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x480.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x481.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x482.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x483.png" xlink:type="simple"/></inline-formula> are also entered. Note that the log-log relation of these two variables follow a straight line. The dependent variables are deduced based on the Second Law of angular momentum [<xref ref-type="bibr" rid="scirp.75084-ref6">6</xref>] <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x480.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x481.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x482.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x483.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x484.png" xlink:type="simple"/></inline-formula>taking the Fermi energy of the spinor pairs to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x476.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x477.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x478.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x479.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x480.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x481.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x482.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x483.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x484.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x485.png" xlink:type="simple"/></inline-formula></title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Star no.</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >R/R<sub>⊙</sub></th><th align="center" valign="middle" >P (s)</th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" >BR<sup>3</sup> (G.m<sup>3</sup>)</th><th align="center" valign="middle" >Iω (J.s)</th><th align="center" valign="middle" >B (eq, theory G)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (m)</th></tr></thead><tr><td align="center" valign="middle" >GD140</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.0132</td><td align="center" valign="middle" >1.037 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.738 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >1.697 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.114 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.193 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.92 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >5.585 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >Grw+73 8031</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.0132</td><td align="center" valign="middle" >1.296 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.738 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >1.436 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.691 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.856 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.92 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >5.280 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >WD1337+70</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.0132</td><td align="center" valign="middle" >1.728 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.738 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >1.157 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.269 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.495 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.92 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >4.914 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >LB253</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.0132</td><td align="center" valign="middle" >2.592 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.738 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >8.535 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >9.211 &#215; 10<sup>4</sup><sup>0</sup></td><td align="center" valign="middle" >1.103 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.92 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >4.440 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >W1346</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.0132</td><td align="center" valign="middle" >5.184 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.738 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >5.077 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >4.230 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >6.561 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.92 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >3.734 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >G1423−B2B</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.0132</td><td align="center" valign="middle" >6.998 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.738 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >4.054 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >3.132 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >5.239 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.92 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >3.464 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >PG2131+066</td><td align="center" valign="middle" >0.62</td><td align="center" valign="middle" >0.0119</td><td align="center" valign="middle" >1.814 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.669 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >1.937 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.171 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >3.417 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >5.95 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >2.707 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >L19-2</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >0.0122</td><td align="center" valign="middle" >9.504 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >6.109 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >5.663 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >2.273 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >9.270 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >4.65 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.798 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >NGC1501</td><td align="center" valign="middle" >0.55</td><td align="center" valign="middle" >0.0128</td><td align="center" valign="middle" >1.011 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >7.0554 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >5.447 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >2.156 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >7.720 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.03 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >1.775 &#215; 10<sup>5</sup></td></tr></tbody></table></table-wrap><fig id="fig25"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>5</label><caption><title> Employing values in <xref ref-type="table" rid="table7">Table 7</xref>, theoretically deduced surface equatorial dipolar magnetic field B (eq, theory, Gauss) against rotation period <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x487.png" xlink:type="simple"/></inline-formula> of nine white dwarfs is shown above. The slope of this log-log plot is −0.705, with excellent correlation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x486.png"/></fig><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x488.png" xlink:type="simple"/></inline-formula>. Referring to <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>6, the P-R plot based on “raw observational data” gives a very large magnitude of negative slope around −35. We have emphasized previously that the slopes of the P-R plot of some other star groups are positive. This “turning over” result is important in the stellar evolution process. When the mass density is high (in White dwarfs,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x488.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x489.png" xlink:type="simple"/></inline-formula>), and the gravity force is much larger than those stars in all the groups discussed in Sections (6.1 - 6.6). Fusion proceeds slowly and the radius shrinks while rotation slows down with P increasing at a fast rate, like an aging organism, leading to a large negative slope in the P-R plot, as observed. Due to the inaccuracy of the measured values of R, the radius of a dwarf is usually calculated via the Hamada-</p><fig id="fig26"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>6</label><caption><title> Refer to <xref ref-type="table" rid="table7">Table 7</xref>. The period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x491.png" xlink:type="simple"/></inline-formula> versus the radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x491.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x492.png" xlink:type="simple"/></inline-formula> in the log-log plot gives a very large magnitude of negative slope using the data for the 9 members collected. Note that the slopes of the P-R plot of some other star groups are positive. This “turning over” result is important in the stellar evolution process. When the mass density is high (such as in the White dwarfs, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x491.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x492.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x493.png" xlink:type="simple"/></inline-formula>, and the gravity force is much larger than those stars in all the groups discussed in Sections (6.1 - 6.6)). Fusion proceeds slowly and the radius shrinks while rotation slows down with P increasing at a fast rate, like an aging organism, leading to a large negative slope in the P-R plot, as observed. Due to the inaccuracy of the measured values of R, it is difficult at this stage to obtain well defined power law relation. For stars at younger age, fusion processes bring in heavier elements, but the density is low so that the gravitation contraction cannot overcome centrifugal force, and positive slopes should result in the P-R plots, as observed experimentally. More detailed discussion requires the analysis of the variation of mass density mathematically as a function of R</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x490.png"/></fig><p>Salpeter relation for dwarfs for decades [<xref ref-type="bibr" rid="scirp.75084-ref41">41</xref>] . It is difficult at this stage to obtain well defined power law relation for the P-R relation with sample masses within a narrow range of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x494.png" xlink:type="simple"/></inline-formula>. Equation (6.7.2b) gives the rough estimation that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x494.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x495.png" xlink:type="simple"/></inline-formula>constant, which is quite true approximately (see <xref ref-type="table" rid="table7">Table 7</xref>).</p><p>In other words, expression (6.7.2b) becomes</p><disp-formula id="scirp.75084-formula343"><label>(6.7.2c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x496.png"  xlink:type="simple"/></disp-formula><p>For stars at younger age, fusion processes bring in heavier elements, but the density is low so that the gravitation contraction cannot overcome centrifugal force, and positive slopes should result in the P-R plots, as observed experimentally. More detailed discussion requires the analysis of the variation of mass density mathematically as a function of R.</p><p>Employing data values in <xref ref-type="table" rid="table7">Table 7</xref>, theoretically deduced equatorial dipolar magnetic field B (eq, theory, G) vs the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x497.png" xlink:type="simple"/></inline-formula> under conditions governed by the Second law of Angular Momentum is shown in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>7. The slope is 2.81, with excellent correlation. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x497.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x498.png" xlink:type="simple"/></inline-formula>values are within a very narrow range. The magnetic dipole fields are within <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x497.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x498.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x499.png" xlink:type="simple"/></inline-formula> Gauss. The order of magnitude of white dwarfs’ surface field is much of a debate even up to</p><fig id="fig27"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>7</label><caption><title>Employing data values in <xref ref-type="table" rid="table7">Table 7</xref>, theoretically deduced equatorial dipolar magnetic field B (Gauss) against the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x501.png" xlink:type="simple"/></inline-formula> under conditions governed by the Second law of Angular Momentum. The slope is 2.81, with excellent correlation. We consider that the measured magnetic fields of white dwarfs are affected by the change in dynamics of the spinors inside the void during stellar evolution. The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x501.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x502.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x500.png"/></fig><p>now. Some detect field~Tesla or more, and some measurements lead to the suggestion that while there are two types of White Dwarfs-one with negligible magnetic field and another type with huge magnetic field. We have devoted one short section on the plausible origin of the sporadic fields, explained in terms of Chern-Simon potential in Secction (5) already. Equations 6.7.2(a) &amp; 6.7.2 (c) might be considered to be the two laws consequential to the new Equation (6.7.1) for White Dwarfs of low masses as stated.</p></sec><sec id="s6_8"><title>6.8. Magnetic White Dwarfs</title><p>Taking 7 Magnetic Whit Dwarf (MWD) samples [<xref ref-type="bibr" rid="scirp.75084-ref40">40</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref55">55</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref56">56</xref>] with close mass density values, we plot the B-P graph in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>8, using data in <xref ref-type="table" rid="table8">Table 8</xref>. Now the slope of <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>8 is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x503.png" xlink:type="simple"/></inline-formula>, and expression (6.1.1) becomes</p><disp-formula id="scirp.75084-formula344"><label>(6.8.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x504.png"  xlink:type="simple"/></disp-formula><p>Leading to;</p><disp-formula id="scirp.75084-formula345"><label>(6.8.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x505.png"  xlink:type="simple"/></disp-formula><p>The function C<sub>1</sub> for the seven members are respectively 319.864, 318.5664, 319.917, 318.75, 319.635, 319.16, 319.40. The average K<sub>1</sub> is about 319.33 (see <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>9).</p><p>Therefore (6.8.2) becomes</p><disp-formula id="scirp.75084-formula346"><label>(6.8.3a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x506.png"  xlink:type="simple"/></disp-formula><p>Or</p><disp-formula id="scirp.75084-formula347"><label>(6.8.3b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x507.png"  xlink:type="simple"/></disp-formula><p>Now the relation between Mass and radius is assumed to follow the model of Hamada and Salpeter. Using data in <xref ref-type="table" rid="table8">Table 8</xref>, we show the M-R graph in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>0 giving a slope of −1.159. Substituting therefore the following equation</p><disp-formula id="scirp.75084-formula348"><label>(6.8.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x508.png"  xlink:type="simple"/></disp-formula><fig id="fig28"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>8</label><caption><title> Employing values in <xref ref-type="table" rid="table8">Table 8</xref>, theoretically deduced equatorial dipolar magnetic field B (eq, theory, Gauss) against rotation period <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x510.png" xlink:type="simple"/></inline-formula> of seven magnetic white dwarfs of close mass density values. The slope of this log-log plot is −0.712, with excellent correlation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x509.png"/></fig><fig id="fig29"  position="float"><label><xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>9</label><caption><title> The values of the function C<sub>1</sub> in Equation (6.8.2) are very close to a constant with a mean of 319.33 (SI units)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x511.png"/></fig><table-wrap id="table8" ><label><xref ref-type="table" rid="table8">Table 8</xref></label><caption><title> Magnetic White Dwarfs. Parameters include mass M, radius R, period of rotation P, mass density D, the deduced void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x512.png" xlink:type="simple"/></inline-formula>, intrinsic equatorial dipole magnetic field magnetic B (Gauss), magnetic parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x512.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x513.png" xlink:type="simple"/></inline-formula>, angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x512.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x513.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x514.png" xlink:type="simple"/></inline-formula> are entered into the table. The basic parameters are taken from [<xref ref-type="bibr" rid="scirp.75084-ref55">55</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref56">56</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref40">40</xref>] and the star’s radius is assumed to follow the Hamada &amp; Salpeter’s relation [<xref ref-type="bibr" rid="scirp.75084-ref41">41</xref>] for dwarfs. The theoretical results are calculated under the condition of the Second Law<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x512.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x513.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x514.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x515.png" xlink:type="simple"/></inline-formula>, taking the Fermi energy of the spinor pairs to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x512.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x513.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x514.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x515.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x516.png" xlink:type="simple"/></inline-formula></title></caption><table><tbody><thead><tr><th align="center" valign="middle" >MWD</th><th align="center" valign="middle" >M/M<sub>?</sub></th><th align="center" valign="middle" >R/R<sub>⊙</sub></th><th align="center" valign="middle" >P(s)</th><th align="center" valign="middle" >R<sup>3</sup> (10<sup>20</sup>m<sup>3</sup>)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >Iω (J-s )</th><th align="center" valign="middle" >B (eq, theory, Gauss)</th><th align="center" valign="middle" >D (10<sup>9</sup> kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (10<sup>5</sup> m)</th></tr></thead><tr><td align="center" valign="middle" >WD0533+053</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >0.0110</td><td align="center" valign="middle" >3.600 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >4.478</td><td align="center" valign="middle" >6.410 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >5.773 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >1.431 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >0.7532</td><td align="center" valign="middle" >4.028</td></tr><tr><td align="center" valign="middle" >WD1031+234</td><td align="center" valign="middle" >0.93</td><td align="center" valign="middle" >0.0088</td><td align="center" valign="middle" >1.224 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.293</td><td align="center" valign="middle" >2.243 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.42 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >9.783 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.9270</td><td align="center" valign="middle" >2.839</td></tr><tr><td align="center" valign="middle" >WD0548−001</td><td align="center" valign="middle" >0.69</td><td align="center" valign="middle" >0.0113</td><td align="center" valign="middle" >1.482 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.854</td><td align="center" valign="middle" >2.260 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >1.438 &#215; 10<sup>40</sup></td><td align="center" valign="middle" >4.656 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >0.6752</td><td align="center" valign="middle" >2.846</td></tr><tr><td align="center" valign="middle" >WD0009+501</td><td align="center" valign="middle" >0.74</td><td align="center" valign="middle" >0.0107</td><td align="center" valign="middle" >2.160 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.121</td><td align="center" valign="middle" >1.655 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >9.489 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >4.015 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >0.8530</td><td align="center" valign="middle" >2.564</td></tr><tr><td align="center" valign="middle" >WD0011−134</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >0.0110</td><td align="center" valign="middle" >4.680 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.478</td><td align="center" valign="middle" >9.364 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >4.441 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >2.091 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >0.7530</td><td align="center" valign="middle" >2.121</td></tr><tr><td align="center" valign="middle" >WD1533−057</td><td align="center" valign="middle" >0.94</td><td align="center" valign="middle" >0.0086</td><td align="center" valign="middle" >8.640 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.140</td><td align="center" valign="middle" >5.041 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >1.947 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >2.356 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.0870</td><td align="center" valign="middle" >1.726</td></tr><tr><td align="center" valign="middle" >WD0912+536</td><td align="center" valign="middle" >0.75</td><td align="center" valign="middle" >0.0105</td><td align="center" valign="middle" >1.149 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.895</td><td align="center" valign="middle" >4.638 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >1.741 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >1.191 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >0.9150</td><td align="center" valign="middle" >1.678</td></tr><tr><td align="center" valign="middle" >WD1953−011</td><td align="center" valign="middle" >0.74</td><td align="center" valign="middle" >0.0107</td><td align="center" valign="middle" >1.246 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.121</td><td align="center" valign="middle" >4.445 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >1.645 &#215; 10<sup>39</sup></td><td align="center" valign="middle" >1.079 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >0.8530</td><td align="center" valign="middle" >1.655</td></tr><tr><td align="center" valign="middle" >WD1829+547</td><td align="center" valign="middle" >0.90</td><td align="center" valign="middle" >0.0090</td><td align="center" valign="middle" >3.154 &#215; 10<sup>9</sup></td><td align="center" valign="middle" >2.453</td><td align="center" valign="middle" >1.979 &#215; 10<sup>21</sup></td><td align="center" valign="middle" >5.593 &#215; 10<sup>34</sup></td><td align="center" valign="middle" >8.0693 &#215; 10</td><td align="center" valign="middle" >1.7433</td><td align="center" valign="middle" >0.126</td></tr></tbody></table></table-wrap><p>Into Equation (6.8.3b), we arrive at</p><disp-formula id="scirp.75084-formula349"><label>(6.8.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x517.png"  xlink:type="simple"/></disp-formula><p>So far, we can consider that the theoretical Equation (6.8.1) leads to (6.8.5) using only the stated M-R relation, with input of “raw data”. When we plot <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x518.png" xlink:type="simple"/></inline-formula> vs <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x518.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x519.png" xlink:type="simple"/></inline-formula> based on measured data (<xref ref-type="fig" rid="fig">Figure </xref>not shown), the slope is negative and the magnitude is rather large, within a range −58 to −62, being consistent to Equation (6.8.5), though the data points are rather scattered.</p><p>We show the relation between the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x520.png" xlink:type="simple"/></inline-formula> and mass density D in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>1. Clearly, we theorize that if the mass densities of some MWD are larger, the gravitation forces are larger in these stars, leading to smaller void sizes.</p><fig id="fig30"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>0</label><caption><title> Mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x522.png" xlink:type="simple"/></inline-formula> vs radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x522.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x523.png" xlink:type="simple"/></inline-formula> for 7 magnetic white dwarfs. Linear scaling gives a better presentation, giving a power index of −1.159</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x521.png"/></fig><fig id="fig31"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>1</label><caption><title> The relation between the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x525.png" xlink:type="simple"/></inline-formula> and mass density D. We theorize that if the mass densities of some MWD are larger, the gravitation forces are larger in these stars, leading to smaller void sizes. The slope of the graph is −3.547. The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x525.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x526.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x524.png"/></fig></sec></sec><sec id="s7"><title>7. General Discussion and Summary</title><sec id="s7_1"><title>7.1. The Mystery of the Relationship between Surface Magnetic Field and Equatorial Rotational Speed of Stars</title><p>It is well known that the three groups of Zeeman components, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x527.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x527.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x528.png" xlink:type="simple"/></inline-formula> of spectral lines (such as a Calcium line), are characterized by different magnetic moments, leading to three distinctive polarization states of these components. The polarization states of electromagnetic waves can be determined by measuring all the four Stokes parameters I, Q, U, V of these waves received. Here Stokes parameter I represents the integrated light intensity (unpolarized light), Stokes parameters Q and U measure the two orthogonal directions of li- near polarization, and Stokes parameter V measures circular polarization(for practical detection of polarization of radio waves from a star, see [<xref ref-type="bibr" rid="scirp.75084-ref57">57</xref>] ). The “longitudinal magnetic field<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x527.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x528.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x529.png" xlink:type="simple"/></inline-formula>”or the “mean line-of-sight magnetic field” is a line intensity weighted average (over the visible hemisphere of a star) of the magnetic field component directed along the line of-sight. In practice, it is obtained from measuring the separation between the positions of the spectral line profiles in the detected left and right circularly polarized light. However, the angle i between the line of sight and the magnetic axis of a star is usually unknown unless under very special circumstances (see e.g. Techniques for stellar magnetic field measurements, [<xref ref-type="bibr" rid="scirp.75084-ref58">58</xref>] and [<xref ref-type="bibr" rid="scirp.75084-ref59">59</xref>] ). Moreover, the polarization states (or the Stokes parameters) are transferred and are changed during the passage of the waves through the intervening plasma between the star and the point of observation [<xref ref-type="bibr" rid="scirp.75084-ref60">60</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref61">61</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref62">62</xref>] . The characteristics of the plasma are generally not known for a distant star and another source of errors can be introduced in the interpretation.</p><p>On the other hand, measuring directly the features of Zeeman splitting in stellar spectral lines offers another method of detection of surface magnetic field strength of a star. However, such method, which in principle, should give more accurate surface magnetic fields, is limited to field strength greater than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x530.png" xlink:type="simple"/></inline-formula> kG, and rotation period smaller than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x530.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x531.png" xlink:type="simple"/></inline-formula> based on discussion in [<xref ref-type="bibr" rid="scirp.75084-ref63">63</xref>] and our estimation. We would also remark that in addition to a dipole field, stars (such as the sun) could have flares which carry magnetic fields much stronger than the “intrinsic” dipole field, though the total area of the flare regions in the photosphere is much smaller than the surface of the visible disc. Thus during the quiescent time period, or in older stars, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x530.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x531.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x532.png" xlink:type="simple"/></inline-formula>or mean surface B has a value close to the equatorial dipole field of a star. During the magnetically active periods, or in younger stars which might have less magnetic activities, the measured average field might fall between the equatorial and the polar field (which is simply twice the equatorial field)or close to the polar field. Moreover, If cyclotron radiation is observed in the emission from a target star/stellar object (see e.g. application of such radiation mechanism, including the maser effect, to explain the radio emissions from the sun and planet Jupiter already half a century ago [<xref ref-type="bibr" rid="scirp.75084-ref64">64</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref65">65</xref>] ), and if the polarization is close to circular, one can calculate the magnetic field at the source readily. Such a method has been applied to estimate the surface magnetic field of some Brown Dwarfs recently [<xref ref-type="bibr" rid="scirp.75084-ref36">36</xref>] . However, the maser effect of such emissions does not tell us which harmonic(s) carries the dominant radiative power and there could be a difference of factor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x530.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x531.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x532.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x533.png" xlink:type="simple"/></inline-formula> in the estimation. Since the star is moving with respect to the observer, in general, there is error due to Doppler broadening. Therefore the “measured <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x530.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x531.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x532.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x533.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x534.png" xlink:type="simple"/></inline-formula> value” or mean surface magnetic field can only be taken to be an order of magnetic field estimation when compared with the theory. In general, the measured field is larger than the predicted dipole field. Nevertheless, the measured magnetic fields reported in literature provide certain trends, relative variation among star groups which are important for our understanding of stellar evolution. Note that the rotational period of a star is commonly taken to be represented by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x530.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x531.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x532.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x533.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x534.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x535.png" xlink:type="simple"/></inline-formula>.</p><p>We have analyzed the B (equatorial, theory) ?P relation for 8 groups of stars in the last section. Experimentally, it has long been discovered that the mean projected rotational velocity <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x536.png" xlink:type="simple"/></inline-formula> of main-sequence stars increases slowly with type, reaching a maximum of about <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x536.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x537.png" xlink:type="simple"/></inline-formula> in the late-B star class (see [<xref ref-type="bibr" rid="scirp.75084-ref66">66</xref>] or earlier works of Abt &amp; Hunter). Reiners [<xref ref-type="bibr" rid="scirp.75084-ref67">67</xref>] found out that there was a linear relation between the averaged magnetic field and rotation speed in log scale (see <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>1 of that paper). A rough estimation shows the slope to be around <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x536.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x537.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x538.png" xlink:type="simple"/></inline-formula> Note that the inverse of the rotational speed v is proportional to the rotational period P. As demonstrated there, such a B-P relation is sensitive to change of mass density. We therefore attempt to compare the theoretical consequence and the measured magnetic field in one group of stars with relative larger star number (than we have employed in Section (6) for various stellar groups), particularly when age information is available. Before we do that, let us introduce some relevant background for further analysis.</p><p>Blackett found a positive correlation between the magnetic moment <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula> and angular momentum of the Earth, Sun and an A2p star 78 Virgins, and proposed that such a relation might be a fundamental a law (see discussion in [<xref ref-type="bibr" rid="scirp.75084-ref68">68</xref>] ). Later studies coined this correlation as the “Magnetic Bode’s Law” (see e.g. [<xref ref-type="bibr" rid="scirp.75084-ref69">69</xref>] ). This law can be stated as log (magnetic moment as represented by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula>) vs log (angular momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula>) has an approximate linear relation for many stars; here B is the equatorial magnetic. Though we consider the application of this law to planets is unconvincing, such investigation opens up an interesting and important issue. First we would note that a magnet experiences a torque <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula> in the presence of a magnetic field B and the magnetic moment <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula> is defined as the maximum torque <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula> experienced by the magnet, satisfying<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula>. The SI unit is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula>. When a current I flows around a plane coil of (vector) area A, this coil also experiences a torque<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula>. The unit is Ampere<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula>. In the study of stellar magnetism, consider the magnetic field to be produced by a current loop. Measured at a far distance r, as in our case, the magnetic moment of the star is related to the magnetic field by<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x549.png" xlink:type="simple"/></inline-formula>. Thus the magnetic moment is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x549.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x550.png" xlink:type="simple"/></inline-formula>. Hence, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x549.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x550.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x551.png" xlink:type="simple"/></inline-formula>with a unit of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x549.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x550.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x551.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x552.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x549.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x550.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x551.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x552.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x553.png" xlink:type="simple"/></inline-formula> does not have the right unit as magnetic moment and might be mis-interpreted when physical concept is involved in our series of works. We would therefore call “<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x540.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x541.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x542.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x543.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x544.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x545.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x546.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x547.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x548.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x549.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x550.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x551.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x552.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x553.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x554.png" xlink:type="simple"/></inline-formula>” as a magnetic parameter in our analysis to follow.</p><p>Now if the “magnetic Bode’s Law” is established, two important issues emerge: (i) Since an electric current or permanent magnet must exist to generate a magnetic field, it is of fundamental interest in physics to know how the Maxwell equations are “hidden behind”/within the magnetic Bode’s law; (ii) On the application side, variables in magnetism (magnetic field, flux) can be calculated from variables of mechanics (period of rotation, radius, mass) and vice versa if only one is unknown; (iii) Various models of dynamo theories have been proposed to explain the source of dipolar field and sporadic fields of stars. We note that long ago, using over ten thousand spot samples, it has been shown, using rather stringent statistics (the Maximum-likelihood analysis) that there is no statistical evidence that sunspots in the northern hemisphere and southern hemisphere are correlated [<xref ref-type="bibr" rid="scirp.75084-ref70">70</xref>] . This result supports the theory that the solar flare phenomenon is more likely to be associated with local variations.</p><p>In 1996, Baliunas, et al. reported the values of measured magnetic fields of 112 low main sequence stars (type F to late K with one M) [<xref ref-type="bibr" rid="scirp.75084-ref71">71</xref>] by analyzing features of the spectral lines arising from Zeeman splitting mentioned earlier, carried over 25 years at Mount Wilson Observatory. The rotation periods of 80 stars were inferred from periodic fluctuations with the stated Ca II records; for the other 32 stars, rotation was computed from the close relation between Ca II flux and the Rossby number (see details of Rossby number in [<xref ref-type="bibr" rid="scirp.75084-ref72">72</xref>] ) in order to reduce the errors due to the unknown values of the angle i between the magnetic axis of rotation and the line of sight. The authors employ a quantity R<sub>HK</sub>’ (called magnetic heating parameter) to approximate the magnetic moment &#181;<sub>m</sub> and presented the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x555.png" xlink:type="simple"/></inline-formula> graph, indicating a linear relation with a slope of about 0.6 (see <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref> of [<xref ref-type="bibr" rid="scirp.75084-ref66">66</xref>] ) with rather narrow spread in astronomical sale. Among the 112 stars under studied, the surface magnetic fields <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x555.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x556.png" xlink:type="simple"/></inline-formula> of 13 members were published in [<xref ref-type="bibr" rid="scirp.75084-ref73">73</xref>] . Defining <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x555.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x556.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x557.png" xlink:type="simple"/></inline-formula> as magnetic moment of a star, it was reported that the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x555.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x556.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x557.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x558.png" xlink:type="simple"/></inline-formula> graph also shows a linear relationship with a slope of 0.54.The above review and analysis indicates that in order to explain the Magnetic Bode’s Law, one has to assume that there is no need to have information about the current in the matter star; in that case one has to look for the “missing electric current” (or the hidden Maxwell equations) which generates the magnetic field. If one assumes dynamo models do exist in reality to explain the emergence of magnetic field, it is hard to believe that with so many variable conditions occurring in the matter structures of different stars, a rather general <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x555.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x556.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x557.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x558.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x559.png" xlink:type="simple"/></inline-formula> and B-P relations in the log-log plot occurs for a large number of cool stars. In this paper, we have already derived an explicit expression for the dipolar magnetic field of stellar objects in terms of only the basic data set (M, R, P).</p><p>It is therefore fruitful to compare our theoretical prediction with measured data within one main star type with more samples than in the last section.</p><p>Incidentally, more recently, Marsden et al. [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] compiled a rather comprehensive survey of the data of 170 sun-like stars, providing the measured “longitudinal surface magnetic field<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x560.png" xlink:type="simple"/></inline-formula>” as defined above, mass, radius, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x560.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x561.png" xlink:type="simple"/></inline-formula>, age of these stars. Though limited by the methodology of measurement as mentioned above in Stokes parameter analysis and the error involved in the angle of sight i (and hence the period of rotation P), so that the uncertainties of B(we will use the symbol B to replace<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x560.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x561.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x562.png" xlink:type="simple"/></inline-formula>) field and P can be 100 % or more in practical cases, yet we can still take these data to investigate the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x560.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x561.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x562.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x563.png" xlink:type="simple"/></inline-formula> relation based on our 5D theory and compared with the measured data, as a beginning step for comparison of theoretical result and experimental data. In <xref ref-type="table" rid="table9">Table 9</xref>, we list the data relevant to this study with examples taken from [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] . The mass density is calculated based on the simple model of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x560.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x561.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x562.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x563.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x564.png" xlink:type="simple"/></inline-formula>. This is a rough estimation because in a sun-like star, most of the matter is in a plasma state, and at different depth, the rotation rates are different for any single star, so that the D is the average, and the angular momentum thus calculated, based on the “solid” model will inevitably introduce significant errors in magnitudes in the next step of our analysis.</p></sec><sec id="s7_2"><title>7.2. Comparison between Theoretical Deduced Surface Magnetic Fields and Measured Values for Sun-Like Stars with Age Smaller Than about 3 Gyr</title><p>Since the magnetic field measured is the average surface “longitudinal” field, we use the polar magnetic field derived from our theory in Section (5), which is simply twice the equatorial field, and plot the dependent variable B (polar, theory, G) in Gauss against the measured <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x565.png" xlink:type="simple"/></inline-formula> for two ranges of density (points in red are within the density range of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x565.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x566.png" xlink:type="simple"/></inline-formula>; points in light red are within the density range of 900 to ~<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x565.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x566.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x567.png" xlink:type="simple"/></inline-formula>) in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>2 below. We used polar rather than equatorial fields because we expect more extra-dipole magnetic activity in younger stars, as explained above in this section. The power indices are respectively 0.5506 &amp; 0.5563 in this graph. Note that in <xref ref-type="fig" rid="fig2"><xref ref-type="fig" rid="fig">Figure </xref>2</xref>1 of [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] the power index is around 1.0; the magnetic fields of those stars are in general one order of magnitude higher. We anticipate that those stars have higher mass densities than the ones in this diagram, and conclude that the slope of the log-log lot gradual increases as the mass density enlarges. Putting the measured data (represented by triangles points in <xref ref-type="table" rid="table9">Table 9</xref>(a)) into <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>2, we have <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>3, demonstrating that the experimental and theoretical results are consistent within an order of magnitude.</p><p>One can use the “raw data” and plot the mass vs radius graph, for sun-like stars with density in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x568.png" xlink:type="simple"/></inline-formula> (deep blue) and in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x568.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x569.png" xlink:type="simple"/></inline-formula> (light blue). These stars are young ones with ages<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x568.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x569.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x570.png" xlink:type="simple"/></inline-formula>. The relation is not simple- roughly power law for the higher density ones and a polynomial for the lower density stars. We do not show this graph but note that with changing density, the M-R relation varies.</p><p>In <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>4, the theoretically derived polar magnetic field is plotted against the period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x571.png" xlink:type="simple"/></inline-formula> for a group of sun-like stars within the density range of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x571.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x572.png" xlink:type="simple"/></inline-formula>, in red color. The other sub-group in light red represents those within the density range of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x571.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x572.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x573.png" xlink:type="simple"/></inline-formula>. The power indices are respectively −0.741 and −0.716, close to the values deduced in</p><table-wrap-group id="9"><label><xref ref-type="table" rid="table9">Table 9</xref></label><caption><title> (a) Young Sun-like stars. Entry numbers in columns 1, 2, 3, 4, 5, 7 are taken directly from [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] and entries of other columns are deduced or calculated based on the present theory. When the age information is not available (N), raw data are still used if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x574.png" xlink:type="simple"/></inline-formula> is greater than or around<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x574.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x575.png" xlink:type="simple"/></inline-formula>; (b) Old sun-like stars. Entry numbers in columns 1, 2, 3, 4, 5, 7 are taken directly from [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] and entries of other columns are deduced or calculated based on the present theory. If the age information is not available (N), raw data are still used (as transition stars) if <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x574.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x575.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x576.png" xlink:type="simple"/></inline-formula> is smaller than or around<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x574.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x575.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x576.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x577.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x574.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x575.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x576.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x577.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x578.png" xlink:type="simple"/></inline-formula>about equals to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x574.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x575.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x576.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x577.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x578.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x579.png" xlink:type="simple"/></inline-formula> is taken as the boundary between young and old sun-like stars</title></caption><table-wrap id="9_1"><caption><title> (b)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >HIP no.</th><th align="center" valign="middle" >Age (Gyr)</th><th align="center" valign="middle" >M/M<sub>⊙</sub></th><th align="center" valign="middle" >R/R<sub>⊙</sub></th><th align="center" valign="middle" >v sin i (m·s<sup>−1</sup>)</th><th align="center" valign="middle" >P (s)</th><th align="center" valign="middle" >B (measure, G)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>, measure)</th><th align="center" valign="middle" >Iω (J-s)</th><th align="center" valign="middle" >B (eq, theory, G)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (m)</th></tr></thead><tr><td align="center" valign="middle" >42,333</td><td align="center" valign="middle" >1.88</td><td align="center" valign="middle" >1.038</td><td align="center" valign="middle" >0.98</td><td align="center" valign="middle" >4.00 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.0706 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >7.7</td><td align="center" valign="middle" >2.438 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.253 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.160</td><td align="center" valign="middle" >1.560 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.007 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >42,403</td><td align="center" valign="middle" >1.04</td><td align="center" valign="middle" >1.189</td><td align="center" valign="middle" >1.17</td><td align="center" valign="middle" >6.30 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.1157 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.2</td><td align="center" valign="middle" >2.262 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.850 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.300</td><td align="center" valign="middle" >1.000 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.220 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >43,410</td><td align="center" valign="middle" >1.88</td><td align="center" valign="middle" >1.211</td><td align="center" valign="middle" >1.24</td><td align="center" valign="middle" >9.00 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.021 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >8.1</td><td align="center" valign="middle" >5.196 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.482 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.840</td><td align="center" valign="middle" >8.970 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.359 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >43,726</td><td align="center" valign="middle" >1.32</td><td align="center" valign="middle" >1.056</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >1.20 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.6416 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.7</td><td align="center" valign="middle" >1.245 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.015 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.240</td><td align="center" valign="middle" >1.490 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.520 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >44,897</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" >1.133</td><td align="center" valign="middle" >1.06</td><td align="center" valign="middle" >3.70 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.1877 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >6.6</td><td align="center" valign="middle" >2.645 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.593 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.775</td><td align="center" valign="middle" >1.340 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.043 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >46,580</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" >0.786</td><td align="center" valign="middle" >0.73</td><td align="center" valign="middle" >3.10 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.0291 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >13.5</td><td align="center" valign="middle" >1.767 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.847 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >4.110</td><td align="center" valign="middle" >2.850 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.186 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >49,908</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.600</td><td align="center" valign="middle" >0.64</td><td align="center" valign="middle" >1.90 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.4715 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.4</td><td align="center" valign="middle" >2.996 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.601 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >3.128</td><td align="center" valign="middle" >3.240 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.551 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >56,242</td><td align="center" valign="middle" >3.8</td><td align="center" valign="middle" >1.0069</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >3.30 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.4567 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.7</td><td align="center" valign="middle" >7.612 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.024 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.061</td><td align="center" valign="middle" >1.070 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.800 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >56,997</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.850</td><td align="center" valign="middle" >0.90</td><td align="center" valign="middle" >2.40 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.6387 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >14.6</td><td align="center" valign="middle" >3.580 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.016 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.246</td><td align="center" valign="middle" >1.650 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.251 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >57,939</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.661</td><td align="center" valign="middle" >0.66</td><td align="center" valign="middle" >5.00 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >5.7684 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >6.6</td><td align="center" valign="middle" >6.384 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.208 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.153</td><td align="center" valign="middle" >3.250 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >4.844 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >62,523</td><td align="center" valign="middle" >1.40</td><td align="center" valign="middle" >1.004</td><td align="center" valign="middle" >0.93</td><td align="center" valign="middle" >2.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.4515 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.0</td><td align="center" valign="middle" >8.118 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.4474 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.653</td><td align="center" valign="middle" >1.763 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.013 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >66,147</td><td align="center" valign="middle" >0.00</td><td align="center" valign="middle" >0.805</td><td align="center" valign="middle" >0.94</td><td align="center" valign="middle" >1.4 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.3098 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >7.3</td><td align="center" valign="middle" >9.952 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.6173 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >12.570</td><td align="center" valign="middle" >2.805 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.205 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >66,275</td><td align="center" valign="middle" >1.64</td><td align="center" valign="middle" >1.341</td><td align="center" valign="middle" >1.46</td><td align="center" valign="middle" >1.5 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.2535 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >3.2</td><td align="center" valign="middle" >3.350 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.6259 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >4.210</td><td align="center" valign="middle" >2.549 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.650 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >68,184</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >0.78</td><td align="center" valign="middle" >1.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.622 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.7</td><td align="center" valign="middle" >5.907 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.491 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.869</td><td align="center" valign="middle" >2.380 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.730 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >71,181</td><td align="center" valign="middle" >1.96</td><td align="center" valign="middle" >0.78</td><td align="center" valign="middle" >0.74</td><td align="center" valign="middle" >1.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.7965 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >5.1</td><td align="center" valign="middle" >6.953 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.752 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.636</td><td align="center" valign="middle" >2.718 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.156 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >113,829</td><td align="center" valign="middle" >1.20</td><td align="center" valign="middle" >1.066</td><td align="center" valign="middle" >1.01</td><td align="center" valign="middle" >3.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.3793 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.7</td><td align="center" valign="middle" >9.359 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.9074 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.548</td><td align="center" valign="middle" >1.461 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.656 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >116,613</td><td align="center" valign="middle" >1.16</td><td align="center" valign="middle" >1.075</td><td align="center" valign="middle" >1.01</td><td align="center" valign="middle" >3.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.4712 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >5.2</td><td align="center" valign="middle" >1.802 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.8033 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.443</td><td align="center" valign="middle" >1.473 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.522 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >544</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.977</td><td align="center" valign="middle" >0.88</td><td align="center" valign="middle" >4.1 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.4000 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >2.70</td><td align="center" valign="middle" >4.564 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.763 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >4.930</td><td align="center" valign="middle" >2.750 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.470 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >3203</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >1.011</td><td align="center" valign="middle" >0.95</td><td align="center" valign="middle" >4.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.6546 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >7.2</td><td align="center" valign="middle" >2.077 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.2864 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.510</td><td align="center" valign="middle" >1.665 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.011 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >3765</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.756</td><td align="center" valign="middle" >0.76</td><td align="center" valign="middle" >2.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.6606 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.6</td><td align="center" valign="middle" >5.317 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >6.362 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.625</td><td align="center" valign="middle" >2.432 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.339 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >3979</td><td align="center" valign="middle" >0.76</td><td align="center" valign="middle" >0.939</td><td align="center" valign="middle" >0.88</td><td align="center" valign="middle" >1.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.9300 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.2</td><td align="center" valign="middle" >5.044 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.115 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.579</td><td align="center" valign="middle" >2.639 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.632 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >7244</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >1.037</td><td align="center" valign="middle" >0.95</td><td align="center" valign="middle" >2.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.8870 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.5</td><td align="center" valign="middle" >1.010 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.1999 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.163</td><td align="center" valign="middle" >1.708 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.600 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >7981</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.816</td><td align="center" valign="middle" >0.82</td><td align="center" valign="middle" >1.7 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.1079 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.3</td><td align="center" valign="middle" >6.122 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >6.297 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.074</td><td align="center" valign="middle" >2.090 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.320 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >10,339</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.957</td><td align="center" valign="middle" >0.89</td><td align="center" valign="middle" >6.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.4821 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >10.9</td><td align="center" valign="middle" >2.585 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.829 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >5.005</td><td align="center" valign="middle" >1.917 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.066 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >12,114</td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >0.809</td><td align="center" valign="middle" >0.76</td><td align="center" valign="middle" >2.9 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.1452 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >1.772 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.871 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >3.649</td><td align="center" valign="middle" >2.602 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.191 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >15,457</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >1.034</td><td align="center" valign="middle" >0.95</td><td align="center" valign="middle" >5.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.9836 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >7.7</td><td align="center" valign="middle" >2.221 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.828 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >4.114</td><td align="center" valign="middle" >1.703 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.066 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >16,537</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.856</td><td align="center" valign="middle" >0.77</td><td align="center" valign="middle" >2.4 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.4020 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >10.9</td><td align="center" valign="middle" >1.536 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.758 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >3.207</td><td align="center" valign="middle" >2.650 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.950 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >71,631</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >1.044</td><td align="center" valign="middle" >0.97</td><td align="center" valign="middle" >1.68 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.5230 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >45.3</td><td align="center" valign="middle" >1.391 &#215; 10<sup>28</sup></td><td align="center" valign="middle" >9.419 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >9.530</td><td align="center" valign="middle" >1.615 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.440 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >72,848</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.926</td><td align="center" valign="middle" >0.84</td><td align="center" valign="middle" >4.5 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.1573 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >7.6</td><td align="center" valign="middle" >1.515 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.9378 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >4.482</td><td align="center" valign="middle" >2.200 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.696 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >79,578</td><td align="center" valign="middle" >1.92</td><td align="center" valign="middle" >1.042</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >1.4 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.1214 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.4</td><td align="center" valign="middle" >1.144 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >8.0778 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.377</td><td align="center" valign="middle" >1.472 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.789 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >81,300</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.892</td><td align="center" valign="middle" >0.82</td><td align="center" valign="middle" >2.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.6290 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >1.113 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.9076 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.690</td><td align="center" valign="middle" >1.280 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.983 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >82,588</td><td align="center" valign="middle" >0.72</td><td align="center" valign="middle" >0.927</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >3.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.7749 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >8.5</td><td align="center" valign="middle" >1.7561 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.6576 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.847</td><td align="center" valign="middle" >2.130 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.324 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >88,945</td><td align="center" valign="middle" >2.04</td><td align="center" valign="middle" >1.039</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >7.9 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >5.4763 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >11.2</td><td align="center" valign="middle" >3.656 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.499 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >5.149</td><td align="center" valign="middle" >1.510 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.197 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >88,972</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.791</td><td align="center" valign="middle" >0.79</td><td align="center" valign="middle" >2.1 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.6439 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.5</td><td align="center" valign="middle" >2.488 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >7.265 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >2.580</td><td align="center" valign="middle" >2.270 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.586 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >91,043</td><td align="center" valign="middle" >0.03</td><td align="center" valign="middle" >1.06</td><td align="center" valign="middle" >1.09</td><td align="center" valign="middle" >39.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.2214 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >89.7</td><td align="center" valign="middle" >3.908 &#215; 10<sup>28</sup></td><td align="center" valign="middle" >2.4947 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >13.940</td><td align="center" valign="middle" >1.160 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.837 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >92,984</td><td align="center" valign="middle" >2.72</td><td align="center" valign="middle" >1.058</td><td align="center" valign="middle" >1.06</td><td align="center" valign="middle" >1.23 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.7660 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >11.3</td><td align="center" valign="middle" >4.528 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >7.637 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >6.239</td><td align="center" valign="middle" >1.250 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.366 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >96,085</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >0.831</td><td align="center" valign="middle" >0.77</td><td align="center" valign="middle" >3.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.1216 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.8</td><td align="center" valign="middle" >2.765 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.063 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.708</td><td align="center" valign="middle" >2.570 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.343 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >98,921</td><td align="center" valign="middle" >1.76</td><td align="center" valign="middle" >1.065</td><td align="center" valign="middle" >1.01</td><td align="center" valign="middle" >4.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.0264 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >9.8</td><td align="center" valign="middle" >3.397 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.561 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >3.178</td><td align="center" valign="middle" >1.460 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.049 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >107,350</td><td align="center" valign="middle" >0.0</td><td align="center" valign="middle" >1.103</td><td align="center" valign="middle" >1.04</td><td align="center" valign="middle" >1.06 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.2875 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >14.8</td><td align="center" valign="middle" >5.601 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >6.732 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >6.009</td><td align="center" valign="middle" >1.390 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.324 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >109,572</td><td align="center" valign="middle" >2.44</td><td align="center" valign="middle" >1.51</td><td align="center" valign="middle" >2.52</td><td align="center" valign="middle" >1.16 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >9.4934 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >4.307 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.444 &#215; 10<sup>41 </sup></td><td align="center" valign="middle" >0.200</td><td align="center" valign="middle" >1.330 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.027 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >113,829</td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >1.066</td><td align="center" valign="middle" >1.01</td><td align="center" valign="middle" >3.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.3793 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.7</td><td align="center" valign="middle" >9.359 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.962 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.550</td><td align="center" valign="middle" >1.460 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.657 &#215; 10<sup>5</sup></td></tr></tbody></table></table-wrap><table-wrap id="9_2"><caption><title></title></caption><table><tbody><thead><tr><th align="center" valign="middle" >HIP no.</th><th align="center" valign="middle" >Age (Gyr)</th><th align="center" valign="middle" >M/M<sub>⊙</sub></th><th align="center" valign="middle" >R/R<sub>⊙</sub></th><th align="center" valign="middle" >v sin i (m·s<sup>−1</sup>)</th><th align="center" valign="middle" >P(s)</th><th align="center" valign="middle" >B (measure, G)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>, measure)</th><th align="center" valign="middle" >Iω (J-s)</th><th align="center" valign="middle" >B (eq, theory, G)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (m)</th></tr></thead><tr><td align="center" valign="middle" >49,081</td><td align="center" valign="middle" >9.52</td><td align="center" valign="middle" >0.960</td><td align="center" valign="middle" >1.06</td><td align="center" valign="middle" >3.4 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.362 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >3.2055 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.915 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.210</td><td align="center" valign="middle" >1.138 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.667 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >9350</td><td align="center" valign="middle" >5.44</td><td align="center" valign="middle" >0.979</td><td align="center" valign="middle" >0.97</td><td align="center" valign="middle" >1.9 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.231 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >1.5352 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.990 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.770</td><td align="center" valign="middle" >1.515 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.215 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >49,756</td><td align="center" valign="middle" >8.28</td><td align="center" valign="middle" >0.975</td><td align="center" valign="middle" >1.07</td><td align="center" valign="middle" >1.5 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.117 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.1</td><td align="center" valign="middle" >8.6550 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.663 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.186</td><td align="center" valign="middle" >1.972 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.928 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >50,316</td><td align="center" valign="middle" >8.00</td><td align="center" valign="middle" >1.070</td><td align="center" valign="middle" >1,46</td><td align="center" valign="middle" >2.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.454 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.1</td><td align="center" valign="middle" >3.2460 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.248 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.954</td><td align="center" valign="middle" >4.855 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.006 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >55,459</td><td align="center" valign="middle" >5.64</td><td align="center" valign="middle" >1.009</td><td align="center" valign="middle" >1.04</td><td align="center" valign="middle" >2.1 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >4.545 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.6</td><td align="center" valign="middle" >6.0550 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.809 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >0.957</td><td align="center" valign="middle" >1.270 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.174 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >56,242</td><td align="center" valign="middle" >3.80</td><td align="center" valign="middle" >1.007</td><td align="center" valign="middle" >1.10</td><td align="center" valign="middle" >3.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.457 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.7</td><td align="center" valign="middle" >7.6123 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.024 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.061</td><td align="center" valign="middle" >1.125 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.800 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >67,422</td><td align="center" valign="middle" >N</td><td align="center" valign="middle" >0.870</td><td align="center" valign="middle" >1.01</td><td align="center" valign="middle" >0.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.471 &#215; 10<sup>7</sup></td><td align="center" valign="middle" >4.8</td><td align="center" valign="middle" >1.6640 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.594 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >0.371</td><td align="center" valign="middle" >1.192 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >5.078 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >111,274</td><td align="center" valign="middle" >11.4</td><td align="center" valign="middle" >0.979</td><td align="center" valign="middle" >1.38</td><td align="center" valign="middle" >2.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.015 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >1.0610 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.496 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.833</td><td align="center" valign="middle" >5.260 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >9.509 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >113,896</td><td align="center" valign="middle" >6.88</td><td align="center" valign="middle" >1.036</td><td align="center" valign="middle" >1.24</td><td align="center" valign="middle" >2.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.935 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >1.6040 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.991 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.422</td><td align="center" valign="middle" >7.673 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >9.760 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >114,378</td><td align="center" valign="middle" >6.72</td><td align="center" valign="middle" >1.009</td><td align="center" valign="middle" >1.13</td><td align="center" valign="middle" >1.0 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >4.794 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >1.11</td><td align="center" valign="middle" >5.3880 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >6.502 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >4.564</td><td align="center" valign="middle" >9.875 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.312 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >114,456</td><td align="center" valign="middle" >9.16</td><td align="center" valign="middle" >0.939</td><td align="center" valign="middle" >0.97</td><td align="center" valign="middle" >2.1 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.019 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >3.6846 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.059 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.850</td><td align="center" valign="middle" >1.453 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.336 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >114,622</td><td align="center" valign="middle" >12.5</td><td align="center" valign="middle" >0.794</td><td align="center" valign="middle" >0.77</td><td align="center" valign="middle" >1.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.365 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.1</td><td align="center" valign="middle" >1.5350 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >3.385 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.572</td><td align="center" valign="middle" >2.456 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.268 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >115,951</td><td align="center" valign="middle" >6.76</td><td align="center" valign="middle" >1.098</td><td align="center" valign="middle" >1.39</td><td align="center" valign="middle" >2.9 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.074 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.1</td><td align="center" valign="middle" >9.9387 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.449 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >0.531</td><td align="center" valign="middle" >5.773 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >7.880 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >116,106</td><td align="center" valign="middle" >6.28</td><td align="center" valign="middle" >1.015</td><td align="center" valign="middle" >1.15</td><td align="center" valign="middle" >3.7 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.358 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.0</td><td align="center" valign="middle" >1.0233 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >2.391 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.045</td><td align="center" valign="middle" >9.424 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.022 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >116,421</td><td align="center" valign="middle" >11.5</td><td align="center" valign="middle" >0.947</td><td align="center" valign="middle" >1.27</td><td align="center" valign="middle" >1.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >5.550 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.0</td><td align="center" valign="middle" >6.8913 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >7.330 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >0.582</td><td align="center" valign="middle" >6.530 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >7.423 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >682</td><td align="center" valign="middle" >612</td><td align="center" valign="middle" >1.045</td><td align="center" valign="middle" >1.12</td><td align="center" valign="middle" >1.5 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.352 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >4.4</td><td align="center" valign="middle" >2.0797 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >9.440 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.621</td><td align="center" valign="middle" >1.050 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.441 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >1499</td><td align="center" valign="middle" >7.12</td><td align="center" valign="middle" >1.026</td><td align="center" valign="middle" >1.11</td><td align="center" valign="middle" >1.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.032 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >6.6</td><td align="center" valign="middle" >3.0370 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.009 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.190</td><td align="center" valign="middle" >1.059 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.235 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >1813</td><td align="center" valign="middle" >10.9</td><td align="center" valign="middle" >0.965</td><td align="center" valign="middle" >1.18</td><td align="center" valign="middle" >2.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.842 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.4</td><td align="center" valign="middle" >1.3266 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.765 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.510</td><td align="center" valign="middle" >8.294 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >9.472 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >4127</td><td align="center" valign="middle" >6.64</td><td align="center" valign="middle" >1.108</td><td align="center" valign="middle" >1.60</td><td align="center" valign="middle" >4.1 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.705 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.5</td><td align="center" valign="middle" >4.8230 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.018 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.122</td><td align="center" valign="middle" >1.600 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.164 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >5985</td><td align="center" valign="middle" >5.12</td><td align="center" valign="middle" >1.101</td><td align="center" valign="middle" >1.25</td><td align="center" valign="middle" >5.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.093 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.4</td><td align="center" valign="middle" >9.1991 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >3.811 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.250</td><td align="center" valign="middle" >7.960 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.148 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >6405</td><td align="center" valign="middle" >5.88</td><td align="center" valign="middle" >0.953</td><td align="center" valign="middle" >0.98</td><td align="center" valign="middle" >1.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.677 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >2.5331 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >8.273 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.420</td><td align="center" valign="middle" >1.430 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.837 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >7276</td><td align="center" valign="middle" >5.04</td><td align="center" valign="middle" >1.242</td><td align="center" valign="middle" >1.80</td><td align="center" valign="middle" >4.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.873 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >1.5696 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >5.198 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.955</td><td align="center" valign="middle" >3.007 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.241 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >7513</td><td align="center" valign="middle" >3.12</td><td align="center" valign="middle" >1.310</td><td align="center" valign="middle" >1.64</td><td align="center" valign="middle" >9.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.465 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >3.7100 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.142 &#215; 10<sup>43</sup></td><td align="center" valign="middle" >2.280</td><td align="center" valign="middle" >4.194 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.511 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >7585</td><td align="center" valign="middle" >5.08</td><td align="center" valign="middle" >1.022</td><td align="center" valign="middle" >1.04</td><td align="center" valign="middle" >2.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.748 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >9.4610 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.530 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.980</td><td align="center" valign="middle" >1.283 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.139 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >7734</td><td align="center" valign="middle" >3.76</td><td align="center" valign="middle" >1.010</td><td align="center" valign="middle" >0.98</td><td align="center" valign="middle" >2.4 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.784 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >6.6</td><td align="center" valign="middle" >2.0898 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >1.315 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.110</td><td align="center" valign="middle" >1.515 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.800 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >8159</td><td align="center" valign="middle" >7.84</td><td align="center" valign="middle" >1.112</td><td align="center" valign="middle" >1.73</td><td align="center" valign="middle" >2.5 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.024 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >6.9680 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.663 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.651</td><td align="center" valign="middle" >3.033 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.050 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >8362</td><td align="center" valign="middle" >10.1</td><td align="center" valign="middle" >0.836</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >1.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.857 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >1.8594 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.175 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.600</td><td align="center" valign="middle" >1.945 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.970 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >9829</td><td align="center" valign="middle" >11.3</td><td align="center" valign="middle" >0.877</td><td align="center" valign="middle" >0.97</td><td align="center" valign="middle" >2.2 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.927 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.3</td><td align="center" valign="middle" >7.0622 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.036 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.820</td><td align="center" valign="middle" >1.357 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.291 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >10,505</td><td align="center" valign="middle" >7.88</td><td align="center" valign="middle" >1.011</td><td align="center" valign="middle" >1.09</td><td align="center" valign="middle" >1.5 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.176 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >3.4854 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >9.151 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >1.170</td><td align="center" valign="middle" >1.102 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.037 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >14,150</td><td align="center" valign="middle" >7.60</td><td align="center" valign="middle" >0.962</td><td align="center" valign="middle" >0.99</td><td align="center" valign="middle" >0.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >5.408 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >2.9380 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.218 &#215; 10<sup>41</sup></td><td align="center" valign="middle" >0.873</td><td align="center" valign="middle" >1.400 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >6.622 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >9911</td><td align="center" valign="middle" >7.16</td><td align="center" valign="middle" >1.080</td><td align="center" valign="middle" >1.36</td><td align="center" valign="middle" >2.7 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.201 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >6.7704 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.196 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.160</td><td align="center" valign="middle" >6.060 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.000 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >12,048</td><td align="center" valign="middle" >8.68</td><td align="center" valign="middle" >1.052</td><td align="center" valign="middle" >1.39</td><td align="center" valign="middle" >1.9 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.197 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.0</td><td align="center" valign="middle" >9.0352 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.538 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.832</td><td align="center" valign="middle" >5.530 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >9.151 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >113,357</td><td align="center" valign="middle" >6.76</td><td align="center" valign="middle" >1.054</td><td align="center" valign="middle" >1.15</td><td align="center" valign="middle" >2.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.933 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >3.0700 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.745 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.614</td><td align="center" valign="middle" >9.780 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >9.444 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >11,548</td><td align="center" valign="middle" >6.76</td><td align="center" valign="middle" >1.101</td><td align="center" valign="middle" >1.81</td><td align="center" valign="middle" >4.3 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.839 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.3</td><td align="center" valign="middle" >5.9850 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >4.744 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.877</td><td align="center" valign="middle" >2.620 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.213 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >60,353</td><td align="center" valign="middle" >3.28</td><td align="center" valign="middle" >1.163</td><td align="center" valign="middle" >1.23</td><td align="center" valign="middle" >6.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.530 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >1.8168 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >4.976 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >2.902</td><td align="center" valign="middle" >8.810 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >1.228 &#215; 10<sup>6</sup></td></tr><tr><td align="center" valign="middle" >74,432</td><td align="center" valign="middle" >10.2</td><td align="center" valign="middle" >0.992</td><td align="center" valign="middle" >1.19</td><td align="center" valign="middle" >1.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.889 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >3.9740 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.176 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.082</td><td align="center" valign="middle" >8.280 &#215; 10<sup>2</sup></td><td align="center" valign="middle" >8.555 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >76,114</td><td align="center" valign="middle" >8.44</td><td align="center" valign="middle" >0.957</td><td align="center" valign="middle" >1.05</td><td align="center" valign="middle" >1.0 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >4.589 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.9</td><td align="center" valign="middle" >2.7230 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.553 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >0.899</td><td align="center" valign="middle" >1.660 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.091 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >79,672</td><td align="center" valign="middle" >5.84</td><td align="center" valign="middle" >1.005</td><td align="center" valign="middle" >1.04</td><td align="center" valign="middle" >2.6 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.748 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.3</td><td align="center" valign="middle" >8.6924 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.504 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.608</td><td align="center" valign="middle" >1.260 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >9.705 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >109,378</td><td align="center" valign="middle" >10.6</td><td align="center" valign="middle" >0.986</td><td align="center" valign="middle" >1.06</td><td align="center" valign="middle" >1.8 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >2.563 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >3.2055 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.046 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.404</td><td align="center" valign="middle" >1.169 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.310 &#215; 10<sup>5</sup></td></tr></tbody></table></table-wrap></table-wrap-group><fig id="fig32"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>2</label><caption><title> The surface dipole field at the pole vs the parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x581.png" xlink:type="simple"/></inline-formula>; here v is the speed of rotation of the equator and i the angle between the magnetic axis and the line of sight. The density of this groups of stars in red ranges from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x581.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x582.png" xlink:type="simple"/></inline-formula> (power index = 0.5506). The other group of stars in light red have densities in the range of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x581.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x582.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x583.png" xlink:type="simple"/></inline-formula> (power index = 0.5563, practically the same as the other one). The age of all the stars in this diagram are below about 3.0 Gyr</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x580.png"/></fig><fig id="fig33"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>3</label><caption><title> Putting the measured data based on <xref ref-type="table" rid="table9">Table 9</xref>(a) into <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>2, we have <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>3 above, showing that the experimental result (triangles; the deep/light blue ones pertain to the higher/lower density groups respective) and theoretical prediction (circles) are rather close in astronomical estimation. The power indices of the two straight lines are respectively 0.5506(deep reed) &amp; 0.5563 (light red). The correlation coefficients are already specified in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>2</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x584.png"/></fig><fig id="fig34"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>4</label><caption><title> The theoretically derived polar magnetic field vs the period of rotation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x586.png" xlink:type="simple"/></inline-formula> for a group of sun-like stars within the density range of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x586.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x587.png" xlink:type="simple"/></inline-formula>, in red color. The other sub-group of circles in light red indicates those within the density range of 900 to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x586.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x587.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x588.png" xlink:type="simple"/></inline-formula>. The power indices are respectively −0.741 and −0.716. The ages of these stars are below ~3 Gyr</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x585.png"/></fig><p>the last section for other star groups. Putting the measured data listed in <xref ref-type="table" rid="table9">Table 9</xref>(a) into <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>4, we arrive at <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>5, and we observe that both the measured (triangles) and theoretical (circles) magnetic fields decrease with increasing P with the same general trend.</p><p>The only parameter value we have assumed, based on the argument explained twice before, is the Fermi energy of the spinor to be equal to the rest mass of electron. The cool stars considered in this sub-section and the next is similar to the regime of the Second Law of angular momentum we derived in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] and this paper.</p><p>Now we proceed to analyze the relation between the magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x589.png" xlink:type="simple"/></inline-formula> and the angular momentum. In <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>6 we present the graph with the magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x589.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x590.png" xlink:type="simple"/></inline-formula> vs the angular momentum of a group of sun-like stars with age around and below 3 Gyr. The triangles are the measured values (deeper blue for density greater than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x589.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x590.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x591.png" xlink:type="simple"/></inline-formula>, and light blue ones pertain to density below<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x589.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x590.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x591.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x592.png" xlink:type="simple"/></inline-formula>. The circles represent points that are derived and calculated from the theory of Section (4), using the measured values of (M, R, P). Deep red ones have densities in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x589.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x590.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x591.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x592.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x593.png" xlink:type="simple"/></inline-formula> and the light red ones have densities between<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x589.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x590.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x591.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x592.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x593.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x594.png" xlink:type="simple"/></inline-formula>, as in other figures. The straight line threads through the theoretical equatorial field “calculated points”, and the upper circular points pertain to the polar fields of the same stars. From the graph, the average of the measured data falls in between these two trends, having about the same slope of 0.75.</p><fig id="fig35"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>5</label><caption><title> Putting the measured data as listed in <xref ref-type="table" rid="table9">Table 9</xref>(a) into <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>4, we obtain the above graph, showing that both the measured (triangles; the deep/light blue ones pertain to the higher/lower density groups respective) and theoretical polar magnetic fields (circles) decrease with increasing P. The power indices of the two straight lines are respectively-0.741 (deep reed) &amp;−0.716 (light red). The correlation coefficients are already specified in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>4</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x595.png"/></fig><fig id="fig36"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>6</label><caption><title> The magnetic parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x597.png" xlink:type="simple"/></inline-formula> vs the angular momentum of a group of sun-like stars with age around and below 3 Gyr. The triangles are the measured values (deeper blue for density greater than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x597.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x598.png" xlink:type="simple"/></inline-formula>, and light blue ones pertain to density below<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x597.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x598.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x599.png" xlink:type="simple"/></inline-formula>). The circles represent points that are derived and calculated from the theory of Section (4), using the measured values of (M, R, P). Deep red ones have densities in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x597.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x598.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x599.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x600.png" xlink:type="simple"/></inline-formula> and the light red ones have densities between<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x597.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x598.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x599.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x600.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x601.png" xlink:type="simple"/></inline-formula>, as in other figures. Many light red and deep red circles overlap; the light ones cover up the deep red ones. The straight line threads through the theoretically predicted equatorial magnetic field data, and the upper points (follow a straight line), pertain to the polar fields. From the graph, the average of the measured data falls in between these two trends, having about the same slope of ~0.75</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x596.png"/></fig></sec><sec id="s7_3"><title>7.3. Comparison between Theoretical Deduced Surface Magnetic Fields and Measured Values for Old Sun-Like Stars with Age Greater Than about 3 Gyr</title><p>We will not take too much space to indicate all graphs above for the older sun- like stars, because there is high similarity in some. Based on data listed in <xref ref-type="table" rid="table9">Table 9</xref>(b), in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>7, we present the relevant graphs that are related to our discussion--Mass vs radius of sun-like stars with age between ~3 and 13 Gyr. The red triangles represent those with mass density between 1.0 to 2.5 times <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x602.png" xlink:type="simple"/></inline-formula> and the purple ones have densities below<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x602.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x603.png" xlink:type="simple"/></inline-formula>. The definition of young and old is arbitrary; therefore there is one star appearing both the old and young graphs for the transition. The data are all experimentally measured with various methodologies for different variables of the data set (M,R,P).The power index is 0.4649 for the high density ones, where it is 0.3391 for the low density ones; the correlation is not excellent, but good enough to show an important natural aspect in stellar evolution: as this group of stars ages, the mass does not decrease, implying that matter is being continuously generated, with increase in size of the star, but keeping a lower mass density. Note that the sun has been predicted to become a red giant.</p><fig id="fig37"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>7</label><caption><title> Mass vs radius of sun-like stars with age between ~3 and 13 Gyr. The red triangles represent those with mass density between 1.0 to 2.5 times <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x605.png" xlink:type="simple"/></inline-formula> and the purple ones have densities below<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x605.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x606.png" xlink:type="simple"/></inline-formula>. The definition of young and old is arbitrary; therefore there is one star appearing in both the old and young graphs for the transition. The data are all experimental measured with various methodologies for different variables of the data set (M, R, P). The power index is 0.4649 for the high density ones, where it is 0.3391 for the low density ones; the correlation is not excellent, but good enough to show an important natural aspect in stellar evolution: as this group of stars ages, the mass does not decrease, implying matter is being continuously generated, with increase in size of star, but keeping a lower mass density. We cannot follow the stellar evolution as the data are associated with different groups in location. There are forty star samples there, but many are overlapping in the middle. The trend is obvious from Physics, because the mass is around one solar mass, below the Chandrasekhar limit, and the gravitational attraction cannot overcome the centrifugal force, though the rotation speed is slowing down. The upper limit of the vertical axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x605.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x606.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x607.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x604.png"/></fig><p>The variation of the theoretical equatorial fields of old sun-like stars with changing P is demonstrated in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>8(a). The red circles represent those stars with mass density in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x608.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x608.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x609.png" xlink:type="simple"/></inline-formula>. The pink ones pertain to density in the range from several hundred <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x608.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x609.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x610.png" xlink:type="simple"/></inline-formula> to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x608.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x609.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x610.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x611.png" xlink:type="simple"/></inline-formula>. Notice that for the young star group, the slopes are very close, but the slopes for the old stars are sensitive to change in density. This is expected as there is a significant change in star radius as a star evolves in its old age, in this sun-like group. Having identified the slopes for the relatively high and low density subgroups of the old stars, we can put the theoretical equatorial fields together in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>8(b). The pink circles now represent the old stars with mass density in the whole range from several hundred <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x608.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x609.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x610.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x611.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x612.png" xlink:type="simple"/></inline-formula> to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x608.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x609.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x610.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x611.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x612.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x613.png" xlink:type="simple"/></inline-formula>. The averaged slope obtained here is in line with the B-P plots of other groups such as NGC 6819, low-to-mid mass main sequence stars plus others, showing slopes around −0.75, as analyzed earlier in the previous section.</p><fig-group id="fig38"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>8</label><caption><title> (a) The theoretical equatorial fields of old sun-like stars change with variation of rotation period P. The red circles represent those stars with mass density in the range<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x616.png" xlink:type="simple"/></inline-formula>. The pink ones pertain to densities in the range from several hundred<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x616.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x617.png" xlink:type="simple"/></inline-formula>. Notice that for the young star group, the slopes are very close, but the slopes for the old stars are sensitive to change in density. This is expected as there is a significant change in star radius as a star evolves in its old age, in this sun-like group; (b) The theoretical equatorial fields of old sun-like stars change with variation of rotation period P. These pink circles represent those stars with mass density in the whole range from several hundred<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x616.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x617.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x618.png" xlink:type="simple"/></inline-formula>. The averaged slope obtained here is in line with the B-P plots of other groups such as NGC 6819, low-to-mid mass main sequence stars plus others, showing slopes around?0.75, as analyzed earlier. The relative low correlation is due to the presence of samples with very low mass density ~ several hundred kg/m<sup>3</sup> only.</title></caption><fig id ="fig38_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x614.png"/></fig><fig id ="fig38_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x615.png"/></fig></fig-group><p>Using raw data in [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] , the magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x619.png" xlink:type="simple"/></inline-formula> and angular momentum relations of the old star samples are shown in <xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>9, with triangle representing the measured values and the circles representing the theoretical equatorial magnetic fields, with no distinction between density ranges here.</p></sec><sec id="s7_4"><title>7.4. Explanation of the Magnetic Bode’s Law and the Law of Intrinsic Dipolar Field for Stellar Objects</title><p>We have provided names “young” &amp; “old” for sun-like stars. The separation is not arbitrary. If we go through the data in <xref ref-type="table" rid="table9">Table 9</xref>(a) and <xref ref-type="table" rid="table9">Table 9</xref>(b), we will notice that most of the young stars have masses and radii satisfying roughly<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x620.png" xlink:type="simple"/></inline-formula>. The reverse is true for old stars. In other words, we may roughly take a critical value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x620.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x621.png" xlink:type="simple"/></inline-formula> (i.e. the value<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x620.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x621.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x622.png" xlink:type="simple"/></inline-formula>) as an age boundary, which is gradual. The magnetic fields of the young ones are larger by almost an order of magnitude. Before we explain the magnetic Bode’s Law, let us put the measured surface fields for the young and old stars together in the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x620.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x621.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x622.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x623.png" xlink:type="simple"/></inline-formula> graph, covering a mass density range of several hundred to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x620.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x621.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x622.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x623.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x624.png" xlink:type="simple"/></inline-formula> (<xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>0). Triangles (darker ones are young, and the lighter blue ones are young) are data reported by measurement.</p><p>Now let us recollect that we have derived an explicit expression for the equatorial field, represented by</p><disp-formula id="scirp.75084-formula350"><label>(7.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x625.png"  xlink:type="simple"/></disp-formula><p>And the magnetic parameter is</p><disp-formula id="scirp.75084-formula351"><label>(7.2a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x626.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula352"><label>(7.2b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x627.png"  xlink:type="simple"/></disp-formula><fig id="fig39"  position="float"><label><xref ref-type="fig" rid="fig3"><xref ref-type="fig" rid="fig">Figure </xref>3</xref>9</label><caption><title> The magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x629.png" xlink:type="simple"/></inline-formula> vs angular momentum of the solid star model for sun-like stars with age between around 3 Gyr and 13 Gyr, as density ranging from several hundred to about 2.5 &#215; 10<sup>3</sup> kg/m<sup>3</sup>.. Triangles are the measured data, and circles are equatorial dipolar fields predicted from the theory of Section (4) using raw data in [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] . The line of best fit for the measured points is roughly estimated to be between the lines pertaining to the equatorial and polar fields respectively</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x628.png"/></fig><fig id="fig40"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>0</label><caption><title> The magnetic parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x631.png" xlink:type="simple"/></inline-formula> (B is the equatorial field) is plotted against the angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x631.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x632.png" xlink:type="simple"/></inline-formula> for both young and old sun-like stars within the range of 0.0 to 13 Gyr and mass density ranging from several hundred to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x631.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x632.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x633.png" xlink:type="simple"/></inline-formula>. Triangles (darker ones are young, and the lighter blue ones are old stars) are measured data reported, and the red and pink ones are results of theoretical prediction according to the derivation in Section (4). Many pink-red ones overlap. In fact the red/pink circles represent the result of proving one is equal to one, because the linear relationship of the above two variables satisfy an equation (derived in this paper) which precisely states such relation. The limit of the vertical scale is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x631.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x632.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x633.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x634.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x630.png"/></fig><p>where C<sub>1</sub>, C<sub>2</sub> are constants. So our theoretical derivation tells us that if we plot <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x635.png" xlink:type="simple"/></inline-formula> against<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x635.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x636.png" xlink:type="simple"/></inline-formula>, we should see a straight line with slope 0.75. The red &amp; pink circles are points using the “raw data” from [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] , as listed in <xref ref-type="table" rid="table9">Table 9</xref>(a) and <xref ref-type="table" rid="table9">Table 9</xref>(b). The line of best does give a slope of 0.75 with perfect correlation. Many pink-red ones overlap. In fact, the red/pink circles represent the result of proving one is equal to one, because the linear relationship of the above two variables satisfy an equation which precisely state such relation. Note that Maxwell equation does not explicitly appear in our equation. According to the 5D projection theory, it is the structure of the spinors inside the void core that provides the origin (i.e. the electric current) of the magnetic field. Therefore, the mystery of the “hidden Maxwell equation” or the Magnetic Bode’s Relation/Law in astronomy can be explained by this model. We would remark also that such a law is satisfied by cool stars only-- precisely the condition of our Second Law of angular momentum [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . The solid sphere model is very rough for a lump of plasma, as explained before. Therefore, we should expect there are some deviations in the slope of 0.75 in experimental findings.</p><p>Let us finally proceed to obtain demonstration of the Law of Intrinsic Dipolar Magnetic Field for Stellar Objects. When the equatorial field <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x637.png" xlink:type="simple"/></inline-formula> is plotted against<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x637.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x638.png" xlink:type="simple"/></inline-formula>, the relation is strictly linear in the log-log plot, as demonstrated by the track of the pink circles for old stars in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>1. The power index is about 3.0 according to our theory. In other words, this general Law of Intrinsic Magnetic Dipole Field for stellar objects derived in this paper can simply be stated as</p><fig id="fig41"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>1</label><caption><title> The theoretically deduced equatorial magnetic fields of sun-like stars with age &gt; about 3 Gyr vs the normalized void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x640.png" xlink:type="simple"/></inline-formula>, using the “raw data” from [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] . The power index is 3.0 according to our theory. This is the general Law of Intrinsic Magnetic Dipole Field for stellar objects derived in this paper. For comparison, the measured surface magnetic fields published in [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] are plotted against <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x640.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x641.png" xlink:type="simple"/></inline-formula> also in the same figure, with blue triangles as data points. We have shown only samples of one star group as an illustration. Other measured data points of the young stars behave in the same way. This law has been applied to analyze all the 8 star groups in Sections (6) &amp; (7). Incidentally, there are 40 (circles) stars along the linear line here, with lots of overlapping of star points. As in other graphs, the theoretical line goes through the midst of the experimental data; in this case, R<sub>o</sub><sub> </sub>is deduced from theory and the range of R<sub>o</sub><sub> </sub>for each star group is rather narrow. The upper limit of the vertical scale is 20 Gauss. The measured surface fields of the old sun-like stars fall into the range of a fraction of a Gauss to about ten Gauss. The maximum of the horizontal axis is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x640.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x641.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x642.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x639.png"/></fig><disp-formula id="scirp.75084-formula353"><label>(7.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x643.png"  xlink:type="simple"/></disp-formula><p>For comparison, the measured surface magnetic fields published in [<xref ref-type="bibr" rid="scirp.75084-ref74">74</xref>] are plotted against <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x644.png" xlink:type="simple"/></inline-formula> also in the same figure, with blue triangles as data points.</p><p>We have shown only samples of one star group as an illustration. Other measured data points of the young stars behave in the same way. This law has been applied to analyze all the 8 star groups in Sections (6) &amp; (7). We shall not repeat to show such similar graphs for other star groups. The reader can test this law readily. Such results show that once the “mechanical” data set (M, R, P) is obtained, the magnetic field can be calculated, without the explicit use of the Maxwell equations. This law is in line with the Law specified in Equation (7.2b) and the linear relation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x645.png" xlink:type="simple"/></inline-formula> studied in details in Section (6). Incidentally, there are 40 (circles) stars along the linear line in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>1, with lots of overlapping of star points. As in other graphs, the theoretical line goes through the midst of the experimental data; in this case, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x645.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x646.png" xlink:type="simple"/></inline-formula>is deduced from theory and the range of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x645.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x646.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x647.png" xlink:type="simple"/></inline-formula> for each star group is rather narrow. The upper limit of the vertical scale is 20 Gauss. The measured surface fields of the old sun-like stars fall into the range of a fraction of a Gauss to about ten Gauss.</p></sec><sec id="s7_5"><title>7.5. On Dipolar Magnetic Fields of the Solar Planets and the Planets of the Trappist-1 System</title><p>There are some mysteries in the properties of the magnetic fields of our planets. Before we analyze them, let us list the relevant data/variables in <xref ref-type="table" rid="table1">Table 1</xref>0 based on data from [<xref ref-type="bibr" rid="scirp.75084-ref75">75</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref76">76</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref77">77</xref>] . We plot the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x648.png" xlink:type="simple"/></inline-formula> graph, treating them like stars. The densities of the 9 planets known have averaged densities ranging from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x648.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x649.png" xlink:type="simple"/></inline-formula> (Saturn) to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x648.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x649.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x650.png" xlink:type="simple"/></inline-formula> (Earth), not too wide a range, and we show the B-P relation (dark green circles) as one group in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>2. The power index is −0.871. The circle in the middle of the figure indicates the B-P data set of the Pluto-binary.</p><p>The reported measured equatorial fields of 7 planets are indicated by the orange triangles. According to rotation periods and their distances from the sun, it appears that five pairs appear-(i) Mercury (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula>, large;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula>) &amp; Venus<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula>; (ii) Earth <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula> &amp; Mars<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x655.png" xlink:type="simple"/></inline-formula>; (iii) Jupiter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x655.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x656.png" xlink:type="simple"/></inline-formula> &amp; Saturn<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x655.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x656.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x657.png" xlink:type="simple"/></inline-formula>; (iv) Uranus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x655.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x656.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x657.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x658.png" xlink:type="simple"/></inline-formula> &amp; Neptune <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x655.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x656.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x657.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x658.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x659.png" xlink:type="simple"/></inline-formula>; (v) Pluto as a binary system <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x651.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x652.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x653.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x654.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x655.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x656.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x657.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x658.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x659.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x660.png" xlink:type="simple"/></inline-formula>.</p><p>In our model, the conformal projection of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x661.png" xlink:type="simple"/></inline-formula> generates the SU (3) quarks. A proton is composed of a set of u, u, d quarks, due to gauge confinement. The bare total mass of these three quarks is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x661.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x662.png" xlink:type="simple"/></inline-formula>. Upon complete generation of electrons, we have a certain void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x661.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x662.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x663.png" xlink:type="simple"/></inline-formula>. We have derived, based on the uncertainty principle, when equal number of electrons and protons (i.e. hydrogen atoms) are generated, the size of the current loop in the 5D void is fixed:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x661.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x662.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x663.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x664.png" xlink:type="simple"/></inline-formula>. The types and number of the quarks generated by P1 are determined by the principle of charge conservation and uni-direction nature of time. Since negative charges are generated by Po, only massive particles with positive or zero charges (forming hadrons), which satisfy gauge invariance in Lorentz space-time, can come to exist from this conformal projection P1. The lowest</p><table-wrap id="table10" ><label><xref ref-type="table" rid="table1">Table 1</xref>0</label><caption><title> The solar system. Parameters include mass M, radius R, period of rotation P, mass density D and the deduced void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x665.png" xlink:type="simple"/></inline-formula> governed by the Second Law <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x665.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x666.png" xlink:type="simple"/></inline-formula> taking the Fermi energy of the spinor pairs to be<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x665.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x666.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x667.png" xlink:type="simple"/></inline-formula>. The angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x665.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x666.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x667.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x668.png" xlink:type="simple"/></inline-formula> and the magnetic parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x665.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x666.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x667.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x668.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x669.png" xlink:type="simple"/></inline-formula>, mass density are also entered (see [<xref ref-type="bibr" rid="scirp.75084-ref75">75</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref76">76</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref77">77</xref>] [<xref ref-type="bibr" rid="scirp.75084-ref78">78</xref>] )</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Planet</th><th align="center" valign="middle" >Mass (kg)</th><th align="center" valign="middle" >Radius (m)</th><th align="center" valign="middle" >P(s)</th><th align="center" valign="middle" >R<sup>3</sup> (m<sup>3</sup>)</th><th align="center" valign="middle" >BR<sup>3</sup> (G-m<sup>3</sup>)</th><th align="center" valign="middle" >Iω (J-s)</th><th align="center" valign="middle" >B (eq, theory, G)</th><th align="center" valign="middle" >D (kg/m<sup>3</sup>)</th><th align="center" valign="middle" >R<sub>o</sub> (m)</th></tr></thead><tr><td align="center" valign="middle" >Sun</td><td align="center" valign="middle" >1.990 &#215; 10<sup>30</sup></td><td align="center" valign="middle" >6.955 &#215; 10<sup>8</sup></td><td align="center" valign="middle" >2.160 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >3.364 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.921 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >1.100 &#215; 10<sup>42</sup></td><td align="center" valign="middle" >1.7600</td><td align="center" valign="middle" >1.410 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.453 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >Mercury</td><td align="center" valign="middle" >3.300 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >2.440 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >5.067 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >1.453 &#215; 10<sup>19</sup></td><td align="center" valign="middle" >5.343 &#215; 10<sup>17</sup></td><td align="center" valign="middle" >9.745 &#215; 10<sup>29</sup></td><td align="center" valign="middle" >0.0368</td><td align="center" valign="middle" >5.427 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.164 &#215; 10<sup>2</sup></td></tr><tr><td align="center" valign="middle" >Venus</td><td align="center" valign="middle" >4.867 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >6.050 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >2.100 &#215; 10<sup>7</sup></td><td align="center" valign="middle" >2.214 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >5.400 &#215; 10<sup>18</sup></td><td align="center" valign="middle" >2.133 &#215; 10<sup>31</sup></td><td align="center" valign="middle" >0.0244</td><td align="center" valign="middle" >5.204 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.766 &#215; 10<sup>3</sup></td></tr><tr><td align="center" valign="middle" >Earth</td><td align="center" valign="middle" >5.972 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >6.370 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >8.640 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >2.585 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >4.136 &#215; 10<sup>20</sup></td><td align="center" valign="middle" >6.800 &#215; 10<sup>33</sup></td><td align="center" valign="middle" >1.6000</td><td align="center" valign="middle" >5.510 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >7.530 &#215; 10<sup>3</sup></td></tr><tr><td align="center" valign="middle" >Mars</td><td align="center" valign="middle" >6.417 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >3.390 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >8.864 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.894 &#215; 10<sup>19</sup></td><td align="center" valign="middle" >2.992 &#215; 10<sup>19</sup></td><td align="center" valign="middle" >2.087 &#215; 10<sup>32</sup></td><td align="center" valign="middle" >0.7680</td><td align="center" valign="middle" >3.940 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.124 &#215; 10<sup>3</sup></td></tr><tr><td align="center" valign="middle" >Jupiter</td><td align="center" valign="middle" >1.898 &#215; 10<sup>27</sup></td><td align="center" valign="middle" >6.991 &#215; 10<sup>7</sup></td><td align="center" valign="middle" >3.573 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >3.417 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >2.224 &#215; 10<sup>24</sup></td><td align="center" valign="middle" >6.780 &#215; 10<sup>38</sup></td><td align="center" valign="middle" >6.5100</td><td align="center" valign="middle" >1.330 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >1.313 &#215; 10<sup>5</sup></td></tr><tr><td align="center" valign="middle" >Saturn</td><td align="center" valign="middle" >5.684 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >5.823 &#215; 10<sup>7</sup></td><td align="center" valign="middle" >3.836 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.975 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >6.481 &#215; 10<sup>23</sup></td><td align="center" valign="middle" >1.374 &#215; 10<sup>38</sup></td><td align="center" valign="middle" >3.2820</td><td align="center" valign="middle" >0.687 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >8.714 &#215; 10<sup>4</sup></td></tr><tr><td align="center" valign="middle" >Uranus</td><td align="center" valign="middle" >8.682 &#215; 10<sup>25</sup></td><td align="center" valign="middle" >2.540 &#215; 10<sup>7</sup></td><td align="center" valign="middle" >6.120 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.639 &#215; 10<sup>22</sup></td><td align="center" valign="middle" >3.214 &#215; 10<sup>22</sup></td><td align="center" valign="middle" >2.300 &#215; 10<sup>36</sup></td><td align="center" valign="middle" >1.9610</td><td align="center" valign="middle" >1.270 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.200 &#215; 10<sup>4</sup></td></tr><tr><td align="center" valign="middle" >Neptune</td><td align="center" valign="middle" >1.024 &#215; 10<sup>26</sup></td><td align="center" valign="middle" >2.460 &#215; 10<sup>7</sup></td><td align="center" valign="middle" >5.800 &#215; 10<sup>4</sup></td><td align="center" valign="middle" >1.489 &#215; 10<sup>22</sup></td><td align="center" valign="middle" >3.610 &#215; 10<sup>22</sup></td><td align="center" valign="middle" >2.400 &#215; 10<sup>36</sup></td><td align="center" valign="middle" >2.4250</td><td align="center" valign="middle" >1.638 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >3.327 &#215; 10<sup>4</sup></td></tr><tr><td align="center" valign="middle" >Pluto</td><td align="center" valign="middle" >1.471 &#215; 10<sup>22</sup></td><td align="center" valign="middle" >1.184 &#215; 10<sup>6</sup></td><td align="center" valign="middle" >5.520 &#215; 10<sup>5</sup></td><td align="center" valign="middle" >1.660 &#215; 10<sup>18</sup></td><td align="center" valign="middle" >9.225 &#215; 10<sup>16</sup></td><td align="center" valign="middle" >9.380 &#215; 10<sup>28</sup></td><td align="center" valign="middle" >0.0556</td><td align="center" valign="middle" >1.880 &#215; 10<sup>3</sup></td><td align="center" valign="middle" >4.550 &#215; 10<sup>2</sup></td></tr></tbody></table></table-wrap><fig id="fig42"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>2</label><caption><title> Theoretical equatorial magnetic fields of the 9 planets, treating them as stars, are indicated by the deep green circles. Taking into the consideration of the planets being appearing as 5 pairs and theoretically from Perelman entropy mapping as discussed in Section (7.5), B (eq, theory, G)/5 for the 9 planets are represented by the bright green circles―the B-P plot shows good correlation with a power index of −0.871. The reported measured fields are represented by orange triangles, and appear to be much closer to the bright green circles</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x670.png"/></fig><p>energy and thus rest mass of hadrons are the protons (composed of (u, u, d) quarks) and neutrons (composed of (u, d, d) quarks), meaning that the Lorentz mass shell contains only u and d quarks of charges (2/3)e, and -(1.3)e. To create a proton (u, u, d) and a neutron (u, d, d) from P1, it requires 2 e massless spinors states, but just 1-e massless spinor state. When all the possible electron-proton pairs are created, the system can only generate neutrons, or the sets of (u, d, d) quarks. The quark mass for neutron is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x671.png" xlink:type="simple"/></inline-formula>. Hence, the reduced quark mass for a (p, n) pair is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x671.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x672.png" xlink:type="simple"/></inline-formula>, and the loop radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x671.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x672.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x673.png" xlink:type="simple"/></inline-formula> increases by about 10%. As more matter is effectively “deposited” on the matter surface, R increases essentially, and there is a decrease of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x671.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x672.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x673.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x674.png" xlink:type="simple"/></inline-formula>. Thus, according to Equations (4.2.5) &amp; (4.2.6), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x671.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x672.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x673.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x674.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x675.png" xlink:type="simple"/></inline-formula>and it could decrease, despite there is increase of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x671.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x672.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x673.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x674.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x675.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x676.png" xlink:type="simple"/></inline-formula>.</p><p>We plot the average surface temperature against distance from the sun in log- log scale (<xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>3), showing a straight line with power index of −0.593. If the planets were “materials” thrown out from the sun whose age is 4.6 Gyr, the heat energy of the planets would have been dissipated as thermal radiation, and the slope would be much steeper. We speculate that the solar system evolved from a Perelman entropy mapping. The angular momenta of the planets and the sun</p><fig id="fig43"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>3</label><caption><title> Average surface temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x678.png" xlink:type="simple"/></inline-formula> vs distance from the sun for the planets starting with mercury on the left, ending with Pluto on the right</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x677.png"/></fig><p>contribute to the total angular momentum of the Milky Way during the initial epoch. The rotation rate could have been deduced from the temperature if one were to observe these objects passed through a wide temperature range. Now these objects are already in the “cool range”, i.e. under the Second Law regime. Due to different processes of evolution and the fact that these stellar objects have very small masses as compared to the sun, the cooling process is very effective (so that the core temperature of the sun is &gt;&gt; than of the planets), and the mass density is in general much larger than that of the sun for the inner two pairs of planets.</p><p>In deriving the angular momentum of the e-trinos states in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] , the normalized void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x679.png" xlink:type="simple"/></inline-formula> is a function of T and even on cooling down to the Second Law region with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x679.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x680.png" xlink:type="simple"/></inline-formula>, we have assumed that the temperature of the core is much greater than that on the surface, so that a large T gradient is established. Hence, the spinor state energy of the in-phase e-trinos depends on the core temperature and these spin states generate a certain amount of angular momentum. Such angular momentum is balanced by the angular momentum of the stellar object as we observe it. This balance is true for stars and most planets. However, the said T gradient is greatly reduced in Mercury and Venus because they are close to the solar surface, and their surface temperatures are high on receiving photons from the sun. Thus the spin state energies of the voids of Mercury and Venus are much lower than those of other planets. Moreover, there is coupling between the planet’s spin and its orbital angular momentum around the Sun. These two factors lead to the observed large P values of the Mercury and Venus (the same argument applies to the moon).If there were a planet existing almost on the solar surface, that planet would have practically zero spin (i.e.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x679.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x680.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x681.png" xlink:type="simple"/></inline-formula>) and an observer on the Sun sees only one half of the surface.</p><p>Thus, we consider that the generation of planets via the existence of the star sun is represented by the same group symmetry, and the 9 planets can be counted as 5 twins (with Pluto with its binary as a pair, but lying in the asteroid zone of the solar system). The arrangement of these planets shows Lie Group symmetry, due to SU(3) symmetry. There are two parity of choices in each element of the five (pairs) representation. In other words, there is a(p, n) duplet at the mass level, and the stellar object would split into two in view of, effectively, the SU(3) symmetry. Since the observed data suggests there are 5 pairs, similar to correct for spin multiplicity in a Fermi gas, the possible quantum states need to be divided by 5 when we do the averaging process for the loop current in calculating the dipole magnetic field. Thus we divide the dipole field strength by 5, and show the B-P graph in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>2 also (bright green circles). It is interesting to note that the measured values are then close to the theorized ones; the theoretical and measured values of the Earth overlap. Field of Mars is far off. We will provide an explanation of this abnormality below.</p><p>Let us first come back to the process of generation of mass in an individual planet, after splitting into pairs. Normally the ec current states of different energy E, and opposite charge and velocity signs, are statistically random, and therefore the parity bias in surface mass creation by P1, is not favored, but non-zero. If such abnormal distribution occurs, the equal number of states within each hemisphere can then be broken. Let us propose a simple scenario for P1 projection in Mars. Suppose the 2 e states came from Northern hemisphere, while the -e state, came from 1 loop in the Southern hemisphere. If that had happened, then the remaining e spinors in the north loop was less than the remaining -e spinors in the south. Such a repeated P1 projection, during Mars cooling (note that there are many volcanoes detected), will result in the magnetic field strength at the South Pole much greater than that at the North Pole [<xref ref-type="bibr" rid="scirp.75084-ref78">78</xref>] . For a similar reason but to a less degree in the stated parity bias property during the P1 projection, Venus could have a very weak magnetic field.</p><p>The dipolar planetary magnetic field shields the stellar particles radiation from impacting the planet’s surface without much energy lost; the magnetic field also serves to sustain the planetary atmosphere and to reduce possible material ejection from the planet’s surface. Thus Mars with an uneven dipole field and a thin atmosphere is known to have sent rocks that hit the earth.</p><p>In passing, we would remark that projection Po of the in-phase spinor states on the 3D surface of the void generate electrons in the Lorentz manifold, but leaving behind net positive massless spinor states on the void surface. A net current resulting from such states would generate magnetic field. Similarly, projection P1 of the out- of-phase spinor states in the 1D loops of the void generate quarks in the Lorentz manifold, but leaving behind net negative massless spinor states in the current loops of the void surface. Both events would lead to variation of the surface magnetic fields. Whether this model could explain the reversal of dipole polarity is outside the scope of this paper. We would also emphasize that most quarks and electrons were created when Perelman mappings were being implemented. The number of in-phase and anti-phase spinor states left over within the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x682.png" xlink:type="simple"/></inline-formula> structure represents only a very small amount of the original number at the initial instant when there is infinite amount of energy in the universe.</p><p>According to [<xref ref-type="bibr" rid="scirp.75084-ref79">79</xref>] , the basic data sets of the six planets nearest to the newly discovered Trappist-1 system are</p><disp-formula id="scirp.75084-formula354"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x683.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula355"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x684.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula356"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x685.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula357"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x686.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula358"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x687.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula359"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x688.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x689.png" xlink:type="simple"/></inline-formula> are respectively the mass and radius of the Earth. The equatorial dipole magnetic fields of these planets according to Equation (4.2.12) are respectively 0.925 Gauss; 0.974 Gauss; 0.43 Gauss; 0.33 Gauss; 0.216 Gauss; 0.255 Gauss, and the Trappist-1 star has a equatorial field of 59.8 Gauss. These planets have dipole fields of the same order of magnitude as that of Earth, while the star’s dipole field is many times that of the Sun. In our solar system, the solar wind, magnetic fields associated with sun’s spots are however much greater than the dipole field and causes deformation of the field line patterns creating the radiation belts in the magneto-spheres of the earth. As the planets in the Trappist-1 system are closer to their star than earth to the Sun, we need to know more about the sporadic fields, if any, from Trappist-1 before we can tell whether the dipole fields of these 6/7 planets can provide enough shielding from the star high energy particles radiation (for living organisms to survive). If oceans are present on these planets, at least deep water living organisms may have chance to survive even if the stated shielding is not strong enough, because the radiation energy released from this cool dwarf star is much weaker than that of the Sun. Thus knowledge of the magnetic fields is one decisive factor for us to consider in our search for living organisms there, and in what form. Before we get more information on such research, we show the B-P relation in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>4. Moreover, the magnetic parameter B-R<sup>3</sup> is plotted vs angular momentum <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x689.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x690.png" xlink:type="simple"/></inline-formula> in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>5. The good correlations indicate that these planets, like cool stars satisfy the linear B-P relation (log-log plot) and the Magnetic Bode’s law.</p></sec><sec id="s7_6"><title>7.6. Summary of the Discoveries Reported in This Paper</title><p>We have sketched the steps that during the mapping from 5D to 4D manifold, the 4<sup>th</sup> spatial variable in the 5D space-time structure would become the (non- zero) current loop with radius x’ at the 5D-4D boundary (one around each magnetic pole). In the unified 5D theories of Kaluza-Klein and Einstein, this space variable is compacted to zero, leading to gravitational singularity and hence black holes. Our deduction shows that such gravitational singularity does not exist, and the conclusion is well sup-</p><fig id="fig44"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>4</label><caption><title> The theoretical equatorial dipole magnetic field of the six planets nearest to the newly discovered Trappist-1 system against the period of rotation<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x692.png" xlink:type="simple"/></inline-formula>. The slope is ?0.764; values of the magnetic fields are stated in the text</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x691.png"/></fig><fig id="fig45"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>5</label><caption><title> Change of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x694.png" xlink:type="simple"/></inline-formula> with respect to variation of angular momentum is indicated, giving a power index of 0.86 for the 6 planets of the Trappist-1 system</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x693.png"/></fig><p>ported by the numerous detections of stars with masses &gt; 100 M<sub>⊙</sub> (the largest one reported so far has a mass of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x695.png" xlink:type="simple"/></inline-formula>) during the past two years.</p><p>Comparing the time intervals after the Big Bang when the lightest lepton (electron) is generated and that when the three quarks (building up a proton) join to form a proton, we obtain the radius of the loop current x’ in terms of the void radius R<sub>o</sub>:</p><disp-formula id="scirp.75084-formula360"><label>(7.6.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x696.png"  xlink:type="simple"/></disp-formula><p>for all stellar objects with hydrogen as fuel. The modification on x’ when the next heavier element (Helium) becomes the fuel of the star is also derived.</p><p>Analyzing the early stage of formation of a galaxy based on the 5D projection theory, we have provided an answer to the detection of unexpected gamma ray bubbles, one above, and one below a galaxy.</p><p>Since Maxwell equations are classical and valid in both the 5D and 4D manifolds, we have derived an explicit expression of the number density of the spinor pairs (which satisfies the Fermi-Dirac distribution but also form the current loop with radius x’ in the classical sense) at the 4D-5D boundary, with quantum signature based on (i) the uncertainty principle &amp; (ii) quantum statistics. Viewed in a 4D Lorentz manifold, this current loop must produce a magnetic field in the classical sense. Therefore we simply apply the Biot-Savart law, with quantum nature incorporated in the number density of the e-trinos, to derive the expression of a distant magnetic field as observed on the matter surface of a stellar object. The surface magnetic field is found to be</p><disp-formula id="scirp.75084-formula361"><label>(7.6.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x697.png"  xlink:type="simple"/></disp-formula><p>The variables are only M, R, P as the Fermi energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x698.png" xlink:type="simple"/></inline-formula> is taken to be the rest mass of electron because it is the lightest lepton generated, as explained in details in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] and this paper. We call (7.6.2) as the Law of Intrinsic Dipole Magnetic Field (for stellar objects).</p><p>Expanding <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x699.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x699.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x700.png" xlink:type="simple"/></inline-formula></p><p>as convergent series, we discover that the approximate expression for B can be separated into three regions in temperature domain. In the high temperature domain where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x701.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.75084-formula362"><label>(7.6.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x702.png"  xlink:type="simple"/></disp-formula><p>We call Equation (7.6.3) the Law of Intrinsic Dipole Magnetic Field for Hot Stars. This law is applicable to fast rotating pulsars at very high temperature.</p><p>On the other hand, if<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x703.png" xlink:type="simple"/></inline-formula>, Equation (7.6.2) becomes approximately</p><disp-formula id="scirp.75084-formula363"><label>(7.6.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x704.png"  xlink:type="simple"/></disp-formula><p>Thus under the low temperature domain, B is independent of T. We call Equation (7.6.4) as the Law of Intrinsic Dipole Magnetic Field for Cool Stellar Objects. Such an interesting result is obvious because the angular momentum of the object is a function of the void radius R<sub>o</sub> and the amount of current generated (hence the dipole field strength) near the magnetic poles in the 4D-5D boundary is also a function of R<sub>o</sub>. The current density, which usually appears in Maxwell equations, is illuminated, giving the “un-ex- pected result” as specified in Equation (7.6.4). The transition temperature between the two domains is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x705.png" xlink:type="simple"/></inline-formula>, which is &gt; the Bethe fusion temperature as discovered for angular momentum in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] . We call such a temperature domain as the Law of Transition between Hot and Cool Stars.</p><p>Taking a cool star as a solid sphere as an approximation, it is elementary to show from Equation (7.6.4) that</p><disp-formula id="scirp.75084-formula364"><label>(7.6.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x706.png"  xlink:type="simple"/></disp-formula><p>which is simply the “mysterious Magnetic Bode’s Law” found experimentally for cool stars.</p><p>We have found that for samples within a range of mass density, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x707.png" xlink:type="simple"/></inline-formula> plot is a straight line. Since for a star, P is inversely proportional to the rotation speed of the equator v, our analysis of nine star groups in Sections (6) &amp; (7) explains why experimentally the relation between log (B) and log (v) (or log P) is found to be linear for many stars. Such a graph for all the star samples involved in this paper is presented in <xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>6.</p><p>Moreover, based on the numerical analysis in Sections (6) &amp; (7) for nine star groups, we have found that once the power index of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x708.png" xlink:type="simple"/></inline-formula> for a number of samples is determined in graphing, we can write down explicit expression relating the variables (M, R, P) of this star group. We can use that expression to find out other crucial properties of that star group theoretically (such as M-R relation); such properties can be compared with experimental data directly. This (novel) method is useful to study stellar evolution, as experienced in our study on the young and old sun-like stars in Section (7.2) &amp; (7.3).</p><p>We have proposed that electrons of the elements (atoms), starting with hydrogen could form 2D Semion states, with pinning of magnetic flux. Due to pressure wave or, in fact fluctuations during the natural cooling process, Semion state can be formed on/near the stellar surface when the gravitational force is</p><fig id="fig46"  position="float"><label><xref ref-type="fig" rid="fig4"><xref ref-type="fig" rid="fig">Figure </xref>4</xref>6</label><caption><title> Predicted equatorial magnetic fields against period of rotation P for the following star groups: (1) Pre-main sequences stars of the Orion (light purple); (2) NGC 6819(orange); (3) Low-to Mid-Mass main sequence stars (bright red); (4) Sun-like young stars (red slightly deeper than that of group (3)) &amp; sun-like old stars (deep red). Notice that the young ones are close to groups (2) &amp; (3), whereas the old ones are close group (1) instead.(5) Pre-dwarfs M34 (bright green); (6) NGC 2516 (pink); (7) Brown Dwarfs (brown); (8) White Dwarfs (blue); (9) Magnetic White Dwarfs (light bright blue). Note that the line of best fit is drawn through each group except the sun-like group (4). Since each group covers a relatively wide mass density, the slopes of the 8 lines above are slightly different from the values analyzed in Section (6). Many points of stars are overlapping. As data for some stars are averaged over a much larger number of stars, the total effective number of stars analyzed is well over 2000. Power indices and correlation coefficients have already been specified in the analysis of each star group</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/18-7503096x709.png"/></fig><p>very large and the void radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x710.png" xlink:type="simple"/></inline-formula> is relatively small. The Semion quasi-particles could get back to the 3D states due to fluctuation in thermo dynamical balance, releasing huge magnetic field, such as that observed in slowly rotating, high density White Dwarfs. Thus, we have provided a plausible explanation for the emergence of huge magnetic field in many stars, including very old ones.</p><p>We have provided an explanation of the asymmetry of magnetic field on the Martian surface and compared the measured and theoretically deduced dipolar magnetic fields of the planets. For the different star groups we studied in Section (6), we cannot compare directly the theoretical magnetic field values with all the stars because we it is difficult to find the published complete set of data for most of these stars. Group comparison (such as Brown Dwarfs group) indicates that our predicted results are in line, in fact, within the same order of magnitude, with observational data and in general trends. For the sun-like group where the whole set of data (B, M, R, P) are available, theoretical predicted values agrees quite well with data (within an order of magnitude), considering the uncertainty and limitation in measurements discussed in details in Section (7.1).</p><p>We predict the equatorial fields B of the newly discovered Trappist-1 star and the 6 nearest planets. The B − P graph, and the B R<sup>3</sup> ? Iω graph in the log-log plots for the 6 planets are both linear.</p></sec><sec id="s7_7"><title>7.7. Conclusion</title><p>Based on the homogeneous 5D model of the universe, we have developed explicit expressions to explain quite a number of unanswered queries or mysteries in astrophysics, as outlined in Section (7.6). One step further, we hope that similar study can serve someway in building a part of the bridge to embrace Maxwell electro-magnetism and quantum mechanics in the future.</p></sec></sec><sec id="s8"><title>Acknowledgements</title><p>We wish to express our gratitude to the various types of assistance of Mr. Benjamin Fung and Dr. Junling Gao, Mr. Vincent Wan during the preparation of this manuscript. We appreciate Mr. Cressidy Fan for plotting <xref ref-type="fig" rid="fig1"><xref ref-type="fig" rid="fig">Figure </xref>1</xref>. We would also wish to express our thanks to Dr. Gisela Dreschhoff, and Dr. Hogne Jungner for their critically reading of the manuscript, plus Dr. Wilson Wong for discussion on issues related to this paper. Last but not least, we thank Professor W. K. Chow for his help when in need for this long project. Both authors declare that there is no conflict of interests in this academic project.</p></sec><sec id="s9"><title>Cite this paper</title><p>Fung, P.C.W. and Wong, K.W. (2017) Origin of Magnetic Fields of Stellar Objects in the Universe Based on the 5D Projection Theory. Journal of Modern Physics, 8, 668-746. https://doi.org/10.4236/jmp.2017.84045</p></sec><sec id="s10"><title>Appendix A: Explicit Expression of the Void Radius</title><p>To calculate the void radius<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x711.png" xlink:type="simple"/></inline-formula>, we need to review a few steps of angular momentum of the in-phase spinor pairs inside the void</p><disp-formula id="scirp.75084-formula365"><label>(A.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x712.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x713.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x713.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x714.png" xlink:type="simple"/></inline-formula>is the spin degeneracy, p the momentum, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x713.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x714.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x715.png" xlink:type="simple"/></inline-formula>is the Fermi-Dirac distribution and the other symbols are standard polar coordinate variables.</p><p>If we treat s pair of in-phase spinors of opposite charge as a bound state, the energy is taken to be the additive energy in the pair. We have already noted in [<xref ref-type="bibr" rid="scirp.75084-ref6">6</xref>] that e,-e are two different types of Fermi particles, and the total angular momentum is then twice of that pertains to either one type―the above expression is then multiplied by a factor of two. The resulting total angular momentum deduced from these two types of treatment different by a numerical constant of several times only. For astronomical estimation, we have considered the loop current based on the Biot-Savart Law to be the additive sum of two currents due to oppositely rotating spinor charges in section (4). Here we also take that the total angular momentum of the system to be twice that in the above equation. Integrating over<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x716.png" xlink:type="simple"/></inline-formula>, with the spin degeneracy to be 4, the total angular momentum</p><disp-formula id="scirp.75084-formula366"><label>(A.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x717.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula367"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x718.png"  xlink:type="simple"/></disp-formula><p>The constant D is found to be:</p><disp-formula id="scirp.75084-formula368"><label>(A.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x719.png"  xlink:type="simple"/></disp-formula><p>Under the region satisfied by the Second Law of Angular Momentum, it has been shown in [<xref ref-type="bibr" rid="scirp.75084-ref2">2</xref>] that</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x720.png" xlink:type="simple"/></inline-formula>approximately. (A.4)</p><p>Considering a stellar object to be a solid sphere with mass M, radius R, period of rotation P, conservation of angular momentum among the 5D void and the 4D matter shell requires that</p><disp-formula id="scirp.75084-formula369"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x721.png"  xlink:type="simple"/></disp-formula><p>Giving</p><disp-formula id="scirp.75084-formula370"><label>(A.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x722.png"  xlink:type="simple"/></disp-formula><p>Numerically,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x723.png" xlink:type="simple"/></inline-formula>.</p><disp-formula id="scirp.75084-formula371"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x724.png"  xlink:type="simple"/></disp-formula><p>The dimension of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x725.png" xlink:type="simple"/></inline-formula>, thus the dimension of R.H.S. of (A.5) is m. Therefore,</p><disp-formula id="scirp.75084-formula372"><label>(A.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x726.png"  xlink:type="simple"/></disp-formula></sec><sec id="s11"><title>Appendix B: Converging Series of the Integral <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x727.png" xlink:type="simple"/></inline-formula></title><disp-formula id="scirp.75084-formula373"><label>(B1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x728.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.75084-formula374"><label>(B.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x729.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula375"><label>(B.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x730.png"  xlink:type="simple"/></disp-formula><p>With<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x731.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x731.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x732.png" xlink:type="simple"/></inline-formula>, k = Boltzmann constant and T is the temperature. In<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x731.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x732.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x733.png" xlink:type="simple"/></inline-formula>, the Fermi-Dirac distribution function</p><disp-formula id="scirp.75084-formula376"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x734.png"  xlink:type="simple"/></disp-formula><p>is bounded for a wide range of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x735.png" xlink:type="simple"/></inline-formula> in our study, and F varies between ⋍ 1/2 and 1.0. We can therefore expand <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x735.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x736.png" xlink:type="simple"/></inline-formula> as a series:</p><disp-formula id="scirp.75084-formula377"><label>(B.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x737.png"  xlink:type="simple"/></disp-formula><p>Now <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x738.png" xlink:type="simple"/></inline-formula> (B.5)</p><p>Integration by parts gives,</p><disp-formula id="scirp.75084-formula378"><label>(B.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x739.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula379"><label>(B.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x740.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula380"><label>(B.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x741.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula381"><label>(B.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x742.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula382"><label>(B.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x743.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula383"><label>(B.11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x744.png"  xlink:type="simple"/></disp-formula><p>Summing all the series, we arrive at</p><disp-formula id="scirp.75084-formula384"><label>(B.12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x745.png"  xlink:type="simple"/></disp-formula><p>Transforming<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x746.png" xlink:type="simple"/></inline-formula>, Equation (B.3) becomes the sum of two definite integrals with explicit forms:</p><disp-formula id="scirp.75084-formula385"><label>(B.13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x747.png"  xlink:type="simple"/></disp-formula><p>From (B.1), (B.12),(B.13),</p><disp-formula id="scirp.75084-formula386"><label>(B.14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x748.png"  xlink:type="simple"/></disp-formula><p>When<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x749.png" xlink:type="simple"/></inline-formula>, the two converging series cancel, and</p><disp-formula id="scirp.75084-formula387"><label>(B.15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x750.png"  xlink:type="simple"/></disp-formula><p>When<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/18-7503096x751.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.75084-formula388"><label>(B.16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/18-7503096x752.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.75084-formula389"><graphic  xlink:href="http://html.scirp.org/file/18-7503096x753.png"  xlink:type="simple"/></disp-formula><p>Submit or recommend next manuscript to SCIRP and we will provide best service for you:</p><p>Accepting pre-submission inquiries through Email, Facebook, LinkedIn, Twitter, etc.</p><p>A wide selection of journals (inclusive of 9 subjects, more than 200 journals)</p><p>Providing 24-hour high-quality service</p><p>User-friendly online submission system</p><p>Fair and swift peer-review system</p><p>Efficient typesetting and proofreading procedure</p><p>Display of the result of downloads and visits, as well as the number of cited articles</p><p>Maximum dissemination of your research work</p><p>Submit your manuscript at: http://papersubmission.scirp.org/</p><p>Or contact jmp@scirp.org</p></sec></body><back><ref-list><title>References</title><ref id="scirp.75084-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Wong, K.W., Dreschhoff, G.A.M. and Jungner, H. 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