<?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">JHEPGC</journal-id><journal-title-group><journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title></journal-title-group><issn pub-type="epub">2380-4327</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2017.33033</article-id><article-id pub-id-type="publisher-id">JHEPGC-76778</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>
 
 
  Mathematical Overview of Hypersphere World-Universe Model
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Vladimir</surname><given-names>S. Netchitailo</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Biolase Inc., Irvine CA, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>v.netchitailo@sbcglobal.net</email></corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>06</month><year>2017</year></pub-date><volume>03</volume><issue>03</issue><fpage>415</fpage><lpage>437</lpage><history><date date-type="received"><day>March</day>	<month>30,</month>	<year>2016</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>June</month>	<year>6,</year>	</date><date date-type="accepted"><day>June</day>	<month>9,</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>
 
 
  The Hypersphere World-Universe Model (WUM) provides a mathematical framework that allows calculating the primary cosmological parameters of the World which are in good agreement with the most recent measurements and observations. WUM explains the experimental data accumulated in the field of Cosmology and Astroparticle Physics over the last decades: the age of the World and critical energy density; the gravitational parameter and Hubble’s parameter; temperatures of the cosmic microwave background radiation and the peak of the far-infrared background radiation; the concentration of intergalactic plasma and time delay of Fast Radio Bursts. Additionally, the model predicts masses of dark matter particles, photons, and neutrinos; proposes new types of particle interactions (Super Weak and Extremely Weak); shows inter-connectivity of primary cosmological parameters of the World. WUM proposes to introduce a new fundamental parameter Q in the CODATA internationally recommended values. This paper is the summary of the mathematical results obtained in [1]-[4].
 
</p></abstract><kwd-group><kwd>Hypersphere World-Universe Model</kwd><kwd> Primary Cosmological Parameters</kwd><kwd> Medium of the World</kwd><kwd> Macroobjects Structure</kwd><kwd> Gravitoelectromagnetism</kwd><kwd> Dark Matter Particles</kwd><kwd> Intergalactic Plasma</kwd><kwd> Microwave Background Radiation</kwd><kwd> Far-Infrared Background Radiation</kwd><kwd> Fast Radio Bursts</kwd><kwd> Emergent Phenomena</kwd><kwd> CODATA</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Hypersphere World-Universe Model (WUM) views the World as a 3-dimen- sional hypersphere that expands along the fourth spatial dimension in the Universe. A hypersphere is an example of a 3-manifold which locally behaves like regular euclidean 3-dimensional space: just as a sphere looks like a plane to small enough observers. WUM is based on Maxwell’s equations (ME) that form the foundation of Electromagnetism and Gravitoelectromagnetism. According to ME, there exist two measurable physical characteristics: energy density and energy flux density.</p><p>WUM makes reasonable assumptions in the main areas of cosmology. The remarkable agreement of the calculated values of the primary cosmological parameters with the observational data gives us considerable confidence in the model.</p><p>The principal idea of WUM is that the energy density of the World <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x2.png" xlink:type="simple"/></inline-formula> equals to the critical energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x3.png" xlink:type="simple"/></inline-formula> necessary for 3-manifold at any cosmological time. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x4.png" xlink:type="simple"/></inline-formula>can be found by considering a sphere of radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x5.png" xlink:type="simple"/></inline-formula> and enclosed mass M, with a small test mass m on the periphery of the sphere. Mass M can be calculated by multiplication of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x6.png" xlink:type="simple"/></inline-formula> by the volume of the sphere. The equation for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x7.png" xlink:type="simple"/></inline-formula> can be found from the escape speed calculation for test mass m:</p><disp-formula id="scirp.76778-formula42"><label>(1.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x8.png"  xlink:type="simple"/></disp-formula><p>where G is the gravitational constant, H is Hubble’s parameter, and c is the gravitoelectrodynamic constant that is identical to the electrodynamic constant c in Maxwell’s equations.</p><p>WUM introduces a fundamental dimensionless time-varying parameter Q that is the measure of the curvature of the Hypersphere. Q can be calculated from the average value of the gravitational constant and in present epoch equals to (see Section 2):</p><disp-formula id="scirp.76778-formula43"><label>(1.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x9.png"  xlink:type="simple"/></disp-formula><p>WUM develops a mathematical framework that allows for direct calculation of a number of cosmological parameters through Q. The precision of such parameters increases by orders of magnitude (see Section 2). Below we will use the following fundamental constants:</p><p>・ Basic unit of length<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x10.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x11.png" xlink:type="simple"/></inline-formula>being the classical electron radius;</p><p>・ Planck constant h;</p><p>・ Basic unit of energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x12.png" xlink:type="simple"/></inline-formula> that is the basic gravitoelectrodynamic charge;</p><p>・ Basic unit of energy density<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x13.png" xlink:type="simple"/></inline-formula>;</p><p>・ Basic unit or surface energy density<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x14.png" xlink:type="simple"/></inline-formula>;</p><p>・ Basic unit of mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x15.png" xlink:type="simple"/></inline-formula>;</p><p>・ Basic unit of frequency<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x16.png" xlink:type="simple"/></inline-formula>;</p><p>・ Fine-structure constant<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x17.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2"><title>2. Primary Cosmological Parameters</title><p>Equation (1.1) can be rewritten as</p><disp-formula id="scirp.76778-formula44"><label>(2.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x18.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x19.png" xlink:type="simple"/></inline-formula> is the gravitomagnetic parameter and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x19.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x20.png" xlink:type="simple"/></inline-formula> is the energy density of</p><p>the Medium. Hubble’s parameter H can be expressed:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x21.png" xlink:type="simple"/></inline-formula>, where R is the</p><p>Hubble’s radius and is the radius of the Hypersphere in WUM. Introducing the dimensionless parameter Q:</p><disp-formula id="scirp.76778-formula45"><label>(2.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x22.png"  xlink:type="simple"/></disp-formula><p>we can rewrite (2.1)</p><disp-formula id="scirp.76778-formula46"><label>(2.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x23.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x24.png" xlink:type="simple"/></inline-formula> is the energy density of Macroobjects of the World. Assuming that</p><disp-formula id="scirp.76778-formula47"><label>(2.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x25.png"  xlink:type="simple"/></disp-formula><p>we can find the equation for the critical energy density:</p><disp-formula id="scirp.76778-formula48"><label>(2.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x26.png"  xlink:type="simple"/></disp-formula><p>and for the gravitational constant:</p><disp-formula id="scirp.76778-formula49"><label>(2.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x27.png"  xlink:type="simple"/></disp-formula><p>We can calculate the value of G based on the value of H. Conversely, we can find the value of the Hubble’s parameter based on the value of the gravitational parameter. H and G are interchangeable! Knowing value of one, it is possible to calculate the other.</p><p>According to (2.2) we can find the value of dimensionless parameter Q based on the value of H, but the accuracy of its measurements is very poor. We have obtained the value of Q in (1.2) based on the Equation (2.6), and value of G that is measured with much better accuracy. Then we can calculate the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x28.png" xlink:type="simple"/></inline-formula> in present epoch:</p><disp-formula id="scirp.76778-formula50"><label>(2.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x29.png"  xlink:type="simple"/></disp-formula><p>Thus calculated value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x30.png" xlink:type="simple"/></inline-formula> is in excellent agreement with experimentally measured value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x31.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref5">5</xref>] and proves assumption (2.4).</p></sec><sec id="s3"><title>3. Gravitation</title><p>In frames of WUM the parameter G can be calculated based on the value of the energy density of the Medium <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x32.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref2">2</xref>] :</p><disp-formula id="scirp.76778-formula51"><label>(3.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x33.png"  xlink:type="simple"/></disp-formula><p>where a dimension-transposing parameter P equals to:</p><disp-formula id="scirp.76778-formula52"><label>(3.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x34.png"  xlink:type="simple"/></disp-formula><p>Then the Newton’s law of universal gravitation can be rewritten in the following way:</p><disp-formula id="scirp.76778-formula53"><label>(3.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x35.png"  xlink:type="simple"/></disp-formula><p>where we introduced the measurable parameter of the Medium <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x36.png" xlink:type="simple"/></inline-formula> instead of</p><p>the phenomenological coefficient G ; and gravitoelectromagnetic charges <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x37.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x38.png" xlink:type="simple"/></inline-formula> instead of macroobjects masses m and M (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x39.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x38.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x39.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x40.png" xlink:type="simple"/></inline-formula> are</p><p>Compton length of mass m and M respectively). The gravitoelectromagnetic charges in (3.3) have a dimension of “Area”, which is equivalent to “Energy”, with the constant that equals to the basic unit of surface energy density<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x41.png" xlink:type="simple"/></inline-formula>.</p><p>Following the approach developed in [<xref ref-type="bibr" rid="scirp.76778-ref2">2</xref>] we can find the gravitomagnetic parameter of the Medium<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x42.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula54"><label>(3.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x43.png"  xlink:type="simple"/></disp-formula><p>and the impedance of the Medium<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x44.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula55"><label>(3.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x45.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x46.png" xlink:type="simple"/></inline-formula> is a cosmological time. These parameters are analogous to the per-</p><p>meability <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x47.png" xlink:type="simple"/></inline-formula> and impedance of electromagnetic field<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x48.png" xlink:type="simple"/></inline-formula>, where</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x49.png" xlink:type="simple"/></inline-formula>is the permittivity of electromagnetic field and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x50.png" xlink:type="simple"/></inline-formula>.</p><p>It follows that measuring the value of Hubble’s parameter anywhere in the World and taking its inverse value allows us to calculate the absolute Age of the World. The Hubble’s parameter is then the most important characteristic of the World, as it defines the Worlds’ Age. While in our Model Hubble’s parameter</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x51.png" xlink:type="simple"/></inline-formula>has a clear physical meaning, the gravitational parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x52.png" xlink:type="simple"/></inline-formula> is a</p><p>phenomenological coefficient in the Newton’s law of universal gravitation.</p><p>The second important characteristic of the World is the gravitomagnetic parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x53.png" xlink:type="simple"/></inline-formula>. Taking its inverse value, we can find the absolute radius of curvature of the World in the fourth spatial dimension. We emphasize that the above two parameters (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x54.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x55.png" xlink:type="simple"/></inline-formula>) are principally different physical characteristics of the Medium that are connected through the gravitoelectrodynamic constant<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x56.png" xlink:type="simple"/></inline-formula>. It means that Time is not a physical dimension and is absolutely different entity than Space. Time is a factor of the World.</p><p>It follows that Gravity, Space and Time itself can be introduced only for a World filled with Matter consisting of elementary particles which take part in simple interactions at a microscopic level. The collective result of their interactions can be observed at a macroscopic level. Gravity, Space and Time are then emergent phenomena [<xref ref-type="bibr" rid="scirp.76778-ref3">3</xref>] .</p></sec><sec id="s4"><title>4. Intergalactic Plasma</title><p>In our Model, the World consists of stable massive elementary particles with lifetimes longer than the age of the World. Protons with mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x57.png" xlink:type="simple"/></inline-formula> and energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x58.png" xlink:type="simple"/></inline-formula> and electrons with mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x59.png" xlink:type="simple"/></inline-formula> and energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x60.png" xlink:type="simple"/></inline-formula> have identical concentrations in the World:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x61.png" xlink:type="simple"/></inline-formula>.</p><p>Low density intergalactic plasma consisting of protons and electrons has plasma frequency<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x62.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula56"><label>(4.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x63.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x64.png" xlink:type="simple"/></inline-formula> is the elementary charge. Since the formula calculating the potential energy of interaction of protons and electrons contains the same parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x65.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula57"><label>(4.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x66.png"  xlink:type="simple"/></disp-formula><p>where we assume that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x67.png" xlink:type="simple"/></inline-formula> is proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x68.png" xlink:type="simple"/></inline-formula>, then <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x69.png" xlink:type="simple"/></inline-formula> is proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x70.png" xlink:type="simple"/></inline-formula>. Energy densities of protons and electrons are then proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x71.png" xlink:type="simple"/></inline-formula>, similar to the critical energy density<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x69.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x70.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x72.png" xlink:type="simple"/></inline-formula>.</p><p>We substitute <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x73.png" xlink:type="simple"/></inline-formula> into (4.1) and calculate concentra-</p><p>tion of protons and electrons:</p><disp-formula id="scirp.76778-formula58"><label>(4.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x74.png"  xlink:type="simple"/></disp-formula><p>A. Mirizzi, et al. found that the mean diffuse intergalactic plasma density is bounded by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x75.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref6">6</xref>] corresponding to the WMAP measurement of the baryon density [<xref ref-type="bibr" rid="scirp.76778-ref7">7</xref>] . The Mediums’ plasma density (4.3) is in good agreement with the estimated value [<xref ref-type="bibr" rid="scirp.76778-ref6">6</xref>] .</p><p>From Equation (4.2) we obtain the value of the lowest frequency<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x76.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula59"><label>(4.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x77.png"  xlink:type="simple"/></disp-formula><p>Photons with energy smaller than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x78.png" xlink:type="simple"/></inline-formula> cannot propagate in plasma, thus <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x79.png" xlink:type="simple"/></inline-formula> is the smallest amount of energy a photon may possess. Following the authors of [<xref ref-type="bibr" rid="scirp.76778-ref8">8</xref>] we can call this amount of energy the rest energy of photons that equals to</p><disp-formula id="scirp.76778-formula60"><label>(4.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x80.png"  xlink:type="simple"/></disp-formula><p>The above value is in good agreement with the value <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x81.png" xlink:type="simple"/></inline-formula> estimated in [<xref ref-type="bibr" rid="scirp.76778-ref8">8</xref>] . It is more relevant to call <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x82.png" xlink:type="simple"/></inline-formula> the minimum energy of photons which can pass through the Intergalactic plasma.</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x83.png" xlink:type="simple"/></inline-formula>is the energy density of protons in the Medium. The relative energy density of protons <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x84.png" xlink:type="simple"/></inline-formula> is then the ratio of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x84.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x85.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula61"><label>(4.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x86.png"  xlink:type="simple"/></disp-formula><p>This value is in good agreement with experimentally found value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x87.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref9">9</xref>] . The results obtained in [<xref ref-type="bibr" rid="scirp.76778-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref8">8</xref>] and [<xref ref-type="bibr" rid="scirp.76778-ref9">9</xref>] prove assumption (4.2).</p><p>According to WUM, the black body spectrum of Microwave Background Radiation (MBR) is due to thermodynamic equilibrium of photons with low density intergalactic plasma consisting of protons and electrons. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x88.png" xlink:type="simple"/></inline-formula>is the energy density of electrons in the Medium. We assume that the energy density of MBR <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x89.png" xlink:type="simple"/></inline-formula> equals to twice the value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x88.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x90.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula62"><label>(4.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x91.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x92.png" xlink:type="simple"/></inline-formula> is the Boltzmann constant and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x93.png" xlink:type="simple"/></inline-formula> is MBR temperature. We can now calculate the value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x94.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula63"><label>(4.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x95.png"  xlink:type="simple"/></disp-formula><p>Thus calculated value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x96.png" xlink:type="simple"/></inline-formula> is in excellent agreement with experimentally measured value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x97.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref10">10</xref>] and proves assumption (4.7).</p></sec><sec id="s5"><title>5. Fast Radio Bursts</title><p>Fast Radio Burst (FRB) is a high-energy astrophysical phenomenon manifested as a transient radio pulse lasting only a few milliseconds. These are bright, unresolved, broadband, millisecond flashes found in parts of the sky outside the Milky Way. The component frequencies of each burst are delayed by different amounts of time depending on the wavelength. This delay is described by a value referred to as a Dispersion Measure (DM) which is the total column density of free electrons between the observer and the source of FRB. Fast radio bursts have DMs which are: much larger than expected for a source inside the Milky Way [<xref ref-type="bibr" rid="scirp.76778-ref11">11</xref>] ; and consistent with propagation through ionized plasma [<xref ref-type="bibr" rid="scirp.76778-ref12">12</xref>] . In this Section we calculate a time delay of FRB based on the characteristics of the Intergalactic Plasma discussed in [<xref ref-type="bibr" rid="scirp.76778-ref4">4</xref>] (see Section 4).</p><p>Consider a photon with initial frequency <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula> and energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula> emitted at time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x100.png" xlink:type="simple"/></inline-formula> when the radius of the hypersphere World in the fourth spatial dimension was<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x101.png" xlink:type="simple"/></inline-formula>. The photon is continuously losing kinetic energy as it moves from galaxy to the Earth until time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x102.png" xlink:type="simple"/></inline-formula> when the radius is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x103.png" xlink:type="simple"/></inline-formula>. The observer will measure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x104.png" xlink:type="simple"/></inline-formula> and energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x100.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x101.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x104.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x105.png" xlink:type="simple"/></inline-formula> and calculate a redshift:</p><disp-formula id="scirp.76778-formula64"><label>(5.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x106.png"  xlink:type="simple"/></disp-formula><p>Recall that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x107.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x108.png" xlink:type="simple"/></inline-formula> are cosmological times (ages of the World at the moments of emitting and observing). A light-travel time distance to a galaxy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x107.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x108.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x109.png" xlink:type="simple"/></inline-formula> equals to</p><disp-formula id="scirp.76778-formula65"><label>(5.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x110.png"  xlink:type="simple"/></disp-formula><p>Let’s calculate photons’ traveling time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x111.png" xlink:type="simple"/></inline-formula> from a galaxy to the Earth taking into account that the rest energy of photons <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x112.png" xlink:type="simple"/></inline-formula> is much smaller than the energy of photons<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x113.png" xlink:type="simple"/></inline-formula>.</p><disp-formula id="scirp.76778-formula66"><label>(5.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x114.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x115.png" xlink:type="simple"/></inline-formula> is photons’ time delay relative to the light-travel time <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x116.png" xlink:type="simple"/></inline-formula> that equals to:</p><disp-formula id="scirp.76778-formula67"><label>(5.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x117.png"  xlink:type="simple"/></disp-formula><p>All observed FRBs have redshifts<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x118.png" xlink:type="simple"/></inline-formula>. It means that we can use the Hubble’s law:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x118.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x119.png" xlink:type="simple"/></inline-formula>. Then</p><disp-formula id="scirp.76778-formula68"><label>(5.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x120.png"  xlink:type="simple"/></disp-formula><p>Photons’ rest energy squared at radius r between <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x121.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x122.png" xlink:type="simple"/></inline-formula> equals to (3.5):</p><disp-formula id="scirp.76778-formula69"><label>(5.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x123.png"  xlink:type="simple"/></disp-formula><p>According to WUM, photons’ energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x124.png" xlink:type="simple"/></inline-formula> on the way from galaxy to an observer can be expressed by the following equation:</p><disp-formula id="scirp.76778-formula70"><label>(5.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x125.png"  xlink:type="simple"/></disp-formula><p>which reduces to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x126.png" xlink:type="simple"/></inline-formula> at (5.5) and to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x127.png" xlink:type="simple"/></inline-formula> at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x126.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x127.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x128.png" xlink:type="simple"/></inline-formula>. Placing the values of the parameters (5.5), (5.6), (5.7) into (5.4), we have for photons’ time delay:</p><disp-formula id="scirp.76778-formula71"><label>(5.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x129.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x130.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x131.png" xlink:type="simple"/></inline-formula>. Taking <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x132.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref12">12</xref>] we get the calcu-</p><p>lated value of photons’ time delay</p><disp-formula id="scirp.76778-formula72"><label>(5.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x133.png"  xlink:type="simple"/></disp-formula><p>which is in good agreement with experimentally measured value [<xref ref-type="bibr" rid="scirp.76778-ref12">12</xref>]</p><disp-formula id="scirp.76778-formula73"><label>(5.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x134.png"  xlink:type="simple"/></disp-formula><p>It is worth to note that in our calculations there is no need in the dispersion measure.</p></sec><sec id="s6"><title>6. Neutrinos</title><p>It is now established that there are three different types of neutrino: electronic<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x135.png" xlink:type="simple"/></inline-formula>, muonic<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x136.png" xlink:type="simple"/></inline-formula>, and tauonic<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x135.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x136.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x137.png" xlink:type="simple"/></inline-formula>, and their antiparticles. Neutrino oscillations imply that neutrinos have non-zero masses [<xref ref-type="bibr" rid="scirp.76778-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref14">14</xref>] .</p><p>Let’s take neutrino masses <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x138.png" xlink:type="simple"/></inline-formula> that are near [<xref ref-type="bibr" rid="scirp.76778-ref15">15</xref>]</p><disp-formula id="scirp.76778-formula74"><label>(6.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x139.png"  xlink:type="simple"/></disp-formula><p>Their concentrations n<sub>v</sub> are then proportional to</p><disp-formula id="scirp.76778-formula75"><label>(6.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x140.png"  xlink:type="simple"/></disp-formula><p>and energy densities of neutrinos are proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x141.png" xlink:type="simple"/></inline-formula>, since critical energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x142.png" xlink:type="simple"/></inline-formula> is proportional to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x142.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x143.png" xlink:type="simple"/></inline-formula> (see Section 2).</p><p>Experimental results obtained by M. Sanchez [<xref ref-type="bibr" rid="scirp.76778-ref16">16</xref>] show <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x144.png" xlink:type="simple"/></inline-formula> neutrino oscillations with parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x144.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x145.png" xlink:type="simple"/></inline-formula> given by</p><disp-formula id="scirp.76778-formula76"><label>(6.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x146.png"  xlink:type="simple"/></disp-formula><p>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x147.png" xlink:type="simple"/></inline-formula> neutrino oscillations with parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x147.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x148.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula77"><label>(6.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x149.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x150.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x150.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x151.png" xlink:type="simple"/></inline-formula> are mass splitting for solar and atmospheric neutrinos respectively. Significantly more accurate result was obtained by P. Kaus, et al. [<xref ref-type="bibr" rid="scirp.76778-ref17">17</xref>] for the ratio of the mass splitting:</p><disp-formula id="scirp.76778-formula78"><label>(6.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x152.png"  xlink:type="simple"/></disp-formula><p>Let’s assume that muonic neutrino’s mass indeed equals to</p><disp-formula id="scirp.76778-formula79"><label>(6.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x153.png"  xlink:type="simple"/></disp-formula><p>From equation (6.5) it then follows that</p><disp-formula id="scirp.76778-formula80"><label>(6.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x154.png"  xlink:type="simple"/></disp-formula><p>Then the squared values of the muonic and tauonic neutrino masses fall into ranges (6.3) and (6.4):</p><disp-formula id="scirp.76778-formula81"><label>(6.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x155.png"  xlink:type="simple"/></disp-formula><p>Let’s assume that electronic neutrino mass equals to</p><disp-formula id="scirp.76778-formula82"><label>(6.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x156.png"  xlink:type="simple"/></disp-formula><p>The sum of the calculated neutrino masses</p><disp-formula id="scirp.76778-formula83"><label>(6.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x157.png"  xlink:type="simple"/></disp-formula><p>is also in a good agreement with the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x158.png" xlink:type="simple"/></inline-formula> discussed in literature [<xref ref-type="bibr" rid="scirp.76778-ref18">18</xref>] .</p><p>Considering that all elementary particles, including neutrinos, are fully cha-</p><p>racterized by their four-momentum<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x159.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula84"><label>(6.11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x160.png"  xlink:type="simple"/></disp-formula><p>we obtain the following neutrino energy densities <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x161.png" xlink:type="simple"/></inline-formula> in accordance with theoretical calculations made by L. D. Landau and E. M. Lifshitz [<xref ref-type="bibr" rid="scirp.76778-ref19">19</xref>] :</p><disp-formula id="scirp.76778-formula85"><label>(6.12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x162.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x163.png" xlink:type="simple"/></inline-formula> is Fermi momentum,</p><disp-formula id="scirp.76778-formula86"><label>(6.13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x164.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula87"><label>(6.14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x165.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula88"><label>(6.15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x166.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula89"><label>(6.16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x167.png"  xlink:type="simple"/></disp-formula><p>Let’s take the following value for Fermi momentum p<sub>F</sub>:</p><disp-formula id="scirp.76778-formula90"><label>(6.17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x168.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x169.png" xlink:type="simple"/></inline-formula> is the extrapolated value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x169.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x170.png" xlink:type="simple"/></inline-formula> at the Beginning when</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x171.png" xlink:type="simple"/></inline-formula>. Using (6.13), we obtain neutrinos relative energy densities <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x171.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x172.png" xlink:type="simple"/></inline-formula> in the Medium in terms of the critical energy density<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x171.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x172.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x173.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula91"><label>(6.18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x174.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.76778-formula92"><label>(6.19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x175.png"  xlink:type="simple"/></disp-formula><p>It’s commonly accepted that concentrations of all types of neutrinos are equal. This assumption allows us to calculate the total neutrinos relative energy density in the Medium:</p><disp-formula id="scirp.76778-formula93"><label>(6.20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x176.png"  xlink:type="simple"/></disp-formula><p>One of the principal ideas of WUM holds that energy densities of Medium particles are proportional to proton energy density in the World’s Medium [<xref ref-type="bibr" rid="scirp.76778-ref2">2</xref>] :</p><disp-formula id="scirp.76778-formula94"><label>(6.21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x177.png"  xlink:type="simple"/></disp-formula><p>which depends on the Fine-structure constant<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x178.png" xlink:type="simple"/></inline-formula>. We take the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x178.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x179.png" xlink:type="simple"/></inline-formula> to equal</p><disp-formula id="scirp.76778-formula95"><label>(6.22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x180.png"  xlink:type="simple"/></disp-formula><p>which is remarkably close to its value calculated in (6.20).</p><p>The assumptions made in (6.6), (6.9), (6.17) and (6.22) are further supported by the excellent numerical agreement of calculated and measured value of Fine-structure constant α discussed in Section 11.</p></sec><sec id="s7"><title>7. Cosmic Far-Infrared Background</title><p>The cosmic Far-Infrared Background (FIRB), which was announced in January 1998, is part of the Cosmic Infrared Background, with wavelengths near 100 microns that is the peak power wavelength of the black body radiation at temperature 29 K. In this Section we introduce Bose-Einstein Condensate (BEC) drops of dineutrinos whose mass is about Planck mass, and their temperature is around 29 K. These drops are responsible for the FIRB [<xref ref-type="bibr" rid="scirp.76778-ref15">15</xref>] .</p><p>According to [<xref ref-type="bibr" rid="scirp.76778-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref22">22</xref>] , the size of large cosmic grains <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x181.png" xlink:type="simple"/></inline-formula> is roughly equal to the length<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x181.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x182.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula96"><label>(7.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x183.png"  xlink:type="simple"/></disp-formula><p>and their mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x184.png" xlink:type="simple"/></inline-formula> is close to the Planck mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x184.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x185.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula97"><label>(7.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x186.png"  xlink:type="simple"/></disp-formula><p>The density of grains <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x187.png" xlink:type="simple"/></inline-formula> is about</p><disp-formula id="scirp.76778-formula98"><label>(7.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x188.png"  xlink:type="simple"/></disp-formula><p>According to WUM, Planck mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x189.png" xlink:type="simple"/></inline-formula> equals to [<xref ref-type="bibr" rid="scirp.76778-ref15">15</xref>]</p><disp-formula id="scirp.76778-formula99"><label>(7.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x190.png"  xlink:type="simple"/></disp-formula><p>Note that the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x191.png" xlink:type="simple"/></inline-formula> is increasing with cosmological time, and is proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x191.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x192.png" xlink:type="simple"/></inline-formula>. Then,</p><disp-formula id="scirp.76778-formula100"><label>(7.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x193.png"  xlink:type="simple"/></disp-formula><p>A grain of mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x194.png" xlink:type="simple"/></inline-formula> and radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x194.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x195.png" xlink:type="simple"/></inline-formula> is receiving energy from the Medium of the World as the result of dineutrinos Bose-Einstein Condensation (see Section 8) at the following rate:</p><disp-formula id="scirp.76778-formula101"><label>(7.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x196.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x197.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x197.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x198.png" xlink:type="simple"/></inline-formula> are parameters.</p><p>The received energy will increase the grain’s temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x199.png" xlink:type="simple"/></inline-formula>, until equilibrium is achieved: power received equals to the power irradiated by the surface of a grain in accordance with the Stefan-Boltzmann law</p><disp-formula id="scirp.76778-formula102"><label>(7.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x200.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x201.png" xlink:type="simple"/></inline-formula> is Stefan-Boltzmann constant:</p><disp-formula id="scirp.76778-formula103"><label>(7.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x202.png"  xlink:type="simple"/></disp-formula><p>With Nikola Tesla’s principle at heart-There is no energy in matter other than that received from the environment-we apply the World equation [<xref ref-type="bibr" rid="scirp.76778-ref23">23</xref>] to a grain:</p><disp-formula id="scirp.76778-formula104"><label>(7.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x203.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x204.png" xlink:type="simple"/></inline-formula> is a basic unit of surface energy density:</p><disp-formula id="scirp.76778-formula105"><label>(7.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x205.png"  xlink:type="simple"/></disp-formula><p>We then calculate the grain’s stationary temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x206.png" xlink:type="simple"/></inline-formula> to be</p><disp-formula id="scirp.76778-formula106"><label>(7.11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x207.png"  xlink:type="simple"/></disp-formula><p>This result is in an excellent agreement with experimentally measured value of 29 K [<xref ref-type="bibr" rid="scirp.76778-ref24">24</xref>] - [<xref ref-type="bibr" rid="scirp.76778-ref35">35</xref>] and proves the assumptions (7.1), (7.2) and (7.9).</p><p>Cosmic FIRB radiation is not a black body radiation. Otherwise, its energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x208.png" xlink:type="simple"/></inline-formula> at temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x208.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x209.png" xlink:type="simple"/></inline-formula> would be too high and equal to the energy density of the Medium of the World:</p><disp-formula id="scirp.76778-formula107"><label>(7.12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x210.png"  xlink:type="simple"/></disp-formula><p>The total flux of the FIRB radiation is the sum of the contributions of all individual grains. Comparing Equations (7.11) and (4.8), we can find the relation between the grains’ temperature and the temperature of the MBR:</p><disp-formula id="scirp.76778-formula108"><label>(7.13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x211.png"  xlink:type="simple"/></disp-formula><p>where electron relative energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x212.png" xlink:type="simple"/></inline-formula> in terms of the critical energy density equals to</p><disp-formula id="scirp.76778-formula109"><label>(7.14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x213.png"  xlink:type="simple"/></disp-formula></sec><sec id="s8"><title>8. Bose-Einstein Condensate</title><p>New cosmological models employing the Bose-Einstein Condensates (BEC) have been actively discussed in literature in recent years [<xref ref-type="bibr" rid="scirp.76778-ref36">36</xref>] - [<xref ref-type="bibr" rid="scirp.76778-ref50">50</xref>] . The transition to BEC occurs below a critical temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x214.png" xlink:type="simple"/></inline-formula>, which for a uniform three-di- mensional gas consisting of non-interacting particles with no apparent internal degrees of freedom is given by</p><disp-formula id="scirp.76778-formula110"><label>(8.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x215.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x216.png" xlink:type="simple"/></inline-formula> is the particle concentration, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x216.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x217.png" xlink:type="simple"/></inline-formula>is the mass per boson, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x216.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x217.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x218.png" xlink:type="simple"/></inline-formula>is the Riemann zeta function:</p><disp-formula id="scirp.76778-formula111"><label>(8.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x219.png"  xlink:type="simple"/></disp-formula><p>According to our Model, we can take the value of the critical temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x220.png" xlink:type="simple"/></inline-formula> to equal the stationary temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x220.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x221.png" xlink:type="simple"/></inline-formula> of Large Grains (see Equation (7.11)). Let’s assume that the energy density of boson particles <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x220.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x221.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x222.png" xlink:type="simple"/></inline-formula> equals to the MBR energy density (see (4.7)):</p><disp-formula id="scirp.76778-formula112"><label>(8.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x223.png"  xlink:type="simple"/></disp-formula><p>Taking into account Equations (7.11), (8.1) and (8.3), we can calculate the value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x224.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula113"><label>(8.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x225.png"  xlink:type="simple"/></disp-formula><p>and the value of the mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x226.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula114"><label>(8.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x227.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x228.png" xlink:type="simple"/></inline-formula>is about 10 orders of magnitude larger than the rest mass of photon’s (see (4.5)) and is in the range of neutrinos masses (see Section 6).</p><p>The calculated values of mass and concentration of dineutrinos satisfy the conditions for their Bose-Einstein condensation. Consequently, BEC drops whose masses are about Planck mass can be created. The stability of such drops is provided by the detailed equilibrium between the energy absorption from the Medium of the World (provided by dineutrinos as a result of their Bose-Einstein condensation) and re-emission of this energy in FIRB at the stationary temperature <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x229.png" xlink:type="simple"/></inline-formula> (see Section 7).</p><p>In WUM the FIRB energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x230.png" xlink:type="simple"/></inline-formula> equals to [<xref ref-type="bibr" rid="scirp.76778-ref15">15</xref>]</p><disp-formula id="scirp.76778-formula115"><label>(8.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x231.png"  xlink:type="simple"/></disp-formula><p>which is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x232.png" xlink:type="simple"/></inline-formula> times smaller than the energy density of MBR and dineutrinos:</p><disp-formula id="scirp.76778-formula116"><label>(8.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x233.png"  xlink:type="simple"/></disp-formula><p>The ratio between FIRB and MBR corresponds to the value of 3.4% calculated by E. L. Wright [<xref ref-type="bibr" rid="scirp.76778-ref51">51</xref>] .</p></sec><sec id="s9"><title>9. Multicomponent Dark Matter</title><p>Dark Matter (DM) is among the most important open problems in both cosmology and particle physics. Dark Matter problem can be, in principle, achieved through extended theories of gravity, as it is discussed, for example, in [<xref ref-type="bibr" rid="scirp.76778-ref52">52</xref>] .</p><p>There are three prominent hypotheses on nonbaryonic DM, namely Hot Dark Matter (HDM), Warm Dark Matter (WDM), and Cold Dark Matter (CDM). A neutralino with mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x234.png" xlink:type="simple"/></inline-formula> in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x235.png" xlink:type="simple"/></inline-formula> range is the leading CDM candidate. Light DMP is heavier than WDM and HDM but lighter than neutralinos are DM candidates too. Subsequently, we will refer to the light DMP as WIMPs. Their mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x236.png" xlink:type="simple"/></inline-formula> falls into <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x236.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x237.png" xlink:type="simple"/></inline-formula> range. It is known that a sterile neutrino with mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x236.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x237.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x238.png" xlink:type="simple"/></inline-formula> in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x234.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x235.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x236.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x237.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x238.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x239.png" xlink:type="simple"/></inline-formula> range is a good WDM candidate. In our opinion, a tauonic neutrino is a good HDM candidate.</p><p>In addition to fermions discussed above, we offer another type of DMP-bo- sons, consisting of two fermions each. There exist two types of DM bosons which we called DIRACs and ELOPs [<xref ref-type="bibr" rid="scirp.76778-ref23">23</xref>] . DIRACs are magnetic dipoles with</p><p>mass<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x240.png" xlink:type="simple"/></inline-formula>, consisting of two Dirac monopoles with mass about <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x240.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x241.png" xlink:type="simple"/></inline-formula> and charge<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x240.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x241.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x242.png" xlink:type="simple"/></inline-formula>. Dissociated DIRACs can only exist at nuclear densities or at high tem-</p><p>peratures. In our opinion, Dirac monopoles are the smallest building blocks of constituent quarks and hadrons (mesons and baryons).</p><p>The second boson is the ELOP (named by analogy to an ELectron-nortisOP</p><p>dipole). ELOP weighs <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x243.png" xlink:type="simple"/></inline-formula> and consists of two preons with mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x243.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x244.png" xlink:type="simple"/></inline-formula> and charge <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x243.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x244.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x245.png" xlink:type="simple"/></inline-formula> which we took to match the Quark Model. ELOPs break</p><p>into two preons at nuclear densities or at high temperatures. In particle physics, preons are postulated to be “point-like” particles, conceived to be subcomponents of quarks and leptons [<xref ref-type="bibr" rid="scirp.76778-ref53">53</xref>] .</p><p>WUM postulates that masses of DMP are proportional to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x246.png" xlink:type="simple"/></inline-formula> multiplied by different exponents of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x246.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x247.png" xlink:type="simple"/></inline-formula> and can be expressed with the following formulae:</p><p>CDM particles (neutralinos and WIMPs):</p><disp-formula id="scirp.76778-formula117"><label>(9.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x248.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula118"><label>(9.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x249.png"  xlink:type="simple"/></disp-formula><p>DIRACs:</p><disp-formula id="scirp.76778-formula119"><label>(9.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x250.png"  xlink:type="simple"/></disp-formula><p>ELOPs:</p><disp-formula id="scirp.76778-formula120"><label>(9.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x251.png"  xlink:type="simple"/></disp-formula><p>WDM particles (sterile neutrinos):</p><disp-formula id="scirp.76778-formula121"><label>(9.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x252.png"  xlink:type="simple"/></disp-formula><p>These values fall into the ranges estimated in literature. The role of those particles in macroobject cores built up from fermionic dark matter will be discussed in Section 10.</p><p>Our Model holds that the energy densities of all types of DMP are proportional to the proton energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x253.png" xlink:type="simple"/></inline-formula> in the World’s Medium (see (4.6)). In all, there are 5 different types of DMP. Then the total energy density of DMP is</p><disp-formula id="scirp.76778-formula122"><label>(9.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x254.png"  xlink:type="simple"/></disp-formula><p>which is close to the measured DM energy density: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x255.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref54">54</xref>] . Note that one of outstanding puzzles in particle physics and cosmology relates to so-called cosmic coincidence: the ratio of dark matter density in the World to baryonic matter density in the Medium of the World <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x255.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x256.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.76778-ref55">55</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref56">56</xref>] .</p><p>Neutralinos, WIMPs, and sterile neutrinos are Majorana fermions, which partake in the annihilation interaction with strength equals to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x257.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x257.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x258.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x257.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x258.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x259.png" xlink:type="simple"/></inline-formula> respectively (see Section 10). The signatures of DMP annihilation with expected masses of 1.3 TeV, 9.6 GeV, 70 MeV, 340 keV, and 3.7 keV are found in spectra of the diffuse gamma-ray background and the emission of various macroobjects in the World [<xref ref-type="bibr" rid="scirp.76778-ref23">23</xref>] .</p><p>The assumptions made in (8.3) and (8.6) are further supported by the excellent numerical agreement of calculated and measured value of fine-structure constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x260.png" xlink:type="simple"/></inline-formula> discussed in Section 11.</p></sec><sec id="s10"><title>10. Macroobject Cores Built up from Fermionic Dark Matter</title><p>In this section, we discuss the possibility of all macroobject cores consisting of DMP introduced in Section 9. The first phase of stellar evolution in the history of the World may be dark stars, powered by Dark Matter heating rather than fusion. Neutralinos and WIMPs, which are their own antiparticles, can annihilate and provide an important heat source for the stars and planets in the World.</p><p>In our view, all macroobjects of the World (including galaxy clusters, galaxies, star clusters, extrasolar systems, and planets) possess the following properties:</p><p>・ Macroobject cores are made up of DMP;</p><p>・ Macroobjects consist of all particles under consideration, in the same proportion as they exist in the World’s Medium;</p><p>・ Macroobjects contain other particles, including DM and baryonic matter, in shells surrounding the cores.</p><p>Taking into account the main principle of the World-Universe Model (all physical parameters can be expressed in terms of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x261.png" xlink:type="simple"/></inline-formula>, small integer numbers, and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x262.png" xlink:type="simple"/></inline-formula>) we modify the published theory of Fermionic Compact Stars (FCS) developed by G. Narain, et al. [<xref ref-type="bibr" rid="scirp.76778-ref57">57</xref>] as follows. We take a scaling solution for a free Fermi gas consisting of fermions with mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x261.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x262.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x263.png" xlink:type="simple"/></inline-formula> in accordance with following equations:</p><p>Maximum mass:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x264.png" xlink:type="simple"/></inline-formula>; (10.1)</p><p>Minimum radius:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x265.png" xlink:type="simple"/></inline-formula>; (10.2)</p><p>Maximum density:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x266.png" xlink:type="simple"/></inline-formula> (10.3)</p><p>where</p><disp-formula id="scirp.76778-formula123"><label>(10.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x267.png"  xlink:type="simple"/></disp-formula><p>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula> is Planck mass, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula>is a Compton length of the fermion.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula>, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula> are parameters. Let us choose <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula> as the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula> (instead of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x275.png" xlink:type="simple"/></inline-formula> taken by G. Narain, et al. [<xref ref-type="bibr" rid="scirp.76778-ref57">57</xref>] ). Then diameter of FCS is proportional to the fermion Compton length<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x276.png" xlink:type="simple"/></inline-formula>. We use <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x276.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x277.png" xlink:type="simple"/></inline-formula> as the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x276.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x277.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x278.png" xlink:type="simple"/></inline-formula> (instead of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x276.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x277.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x278.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x279.png" xlink:type="simple"/></inline-formula> taken by G. Narain, et al. [<xref ref-type="bibr" rid="scirp.76778-ref57">57</xref>] ). Then <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x268.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x269.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x270.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x271.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x272.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x273.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x274.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x275.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x276.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x277.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x278.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x279.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x280.png" xlink:type="simple"/></inline-formula> will equal to</p><disp-formula id="scirp.76778-formula124"><label>(10.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x281.png"  xlink:type="simple"/></disp-formula><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Parameter values for FCS made up of various fermions</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Fermion</th><th align="center" valign="middle" >Fermion relative mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x282.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" >Macroobject relative mass <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x283.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" >Macroobject relative radius <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x284.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" >Macroobject relative density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x285.png" xlink:type="simple"/></inline-formula></th></tr></thead><tr><td align="center" valign="middle" >Sterile neutrino</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x286.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x287.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x288.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x289.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Preon</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x290.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x291.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x292.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x293.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Electron-proton (white dwarf)</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x294.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x295.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x296.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x297.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Monopole</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x298.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x299.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x300.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x301.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >WIMP</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x302.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x303.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x304.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x305.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Neutralino</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x306.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x307.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x308.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x309.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Interacting WIMPs</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x310.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x311.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x312.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x313.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Interacting neutralinos</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x314.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x315.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x316.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x317.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >Neutron (star)</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x318.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x319.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x320.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x321.png" xlink:type="simple"/></inline-formula></td></tr></tbody></table></table-wrap><p><xref ref-type="table" rid="table1">Table 1</xref> summarizes the parameter values for FCS made up of various fermions:</p><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x322.png" xlink:type="simple"/></inline-formula> (10.6)</p><disp-formula id="scirp.76778-formula125"><label>(10.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x323.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula126"><label>(10.8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x324.png"  xlink:type="simple"/></disp-formula><p>A maximum density of neutron stars equals to the nuclear density:</p><disp-formula id="scirp.76778-formula127"><label>(10.9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x325.png"  xlink:type="simple"/></disp-formula><p>which is the maximum possible density of any macroobject in the World.</p><p>A Compact Star made up of heavier particles, WIMPs and neutralinos, could in principle have a much higher density. In order for such a star to remain stable and not exceed the nuclear density, WIMPs and neutralinos must partake in an annihilation interaction whose strength equals to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x326.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x326.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x327.png" xlink:type="simple"/></inline-formula> respectively.</p><p>Scaling solution for interacting WIMPs can also be described with equations (10.1), (10.2), (10.3) and the following values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x328.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x329.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x328.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x329.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x330.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula128"><label>(10.10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x331.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula129"><label>(10.11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x332.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula130"><label>(10.12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x333.png"  xlink:type="simple"/></disp-formula><p>The maximum mass and minimum radius increase about two orders of magnitude each and the maximum density equals to the nuclear density. Note that parameters of a FCS made up of strongly interacting WIMPs are identical to those of neutron stars.</p><p>In accordance with the paper by G. Narain, et al. [<xref ref-type="bibr" rid="scirp.76778-ref57">57</xref>] , the most attractive</p><p>feature of the strongly interacting Fermi gas of WIMPs is practically constant value of FCS minimum radius in the large range of masses <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x334.png" xlink:type="simple"/></inline-formula> from</p><disp-formula id="scirp.76778-formula131"><label>(10.13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x335.png"  xlink:type="simple"/></disp-formula><p>down to</p><disp-formula id="scirp.76778-formula132"><label>(10.14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x336.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x337.png" xlink:type="simple"/></inline-formula>is more than eight orders of magnitude smaller than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x337.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x338.png" xlink:type="simple"/></inline-formula>. It makes strongly interacting WIMPs good candidates for stellar and planetary cores of extrasolar systems with Red stars [<xref ref-type="bibr" rid="scirp.76778-ref23">23</xref>] .</p><p>When the mass of a FCS made up of WIMPs is much smaller than the maximum mass, the scaling solution yields the following equation for parameters <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x339.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x339.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x340.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula133"><label>(10.15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x341.png"  xlink:type="simple"/></disp-formula><p>Compare <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x342.png" xlink:type="simple"/></inline-formula> with the value of 91 used by G. Narain, et al. [<xref ref-type="bibr" rid="scirp.76778-ref57">57</xref>] .</p><p>Minimum mass and maximum radius take on the following values:</p><disp-formula id="scirp.76778-formula134"><label>(10.16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x343.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula135"><label>(10.17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x344.png"  xlink:type="simple"/></disp-formula><p>It follows that the range of FCS masses (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x345.png" xlink:type="simple"/></inline-formula>) spans about three orders of magnitude, and the range of FCS core radii (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x345.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x346.png" xlink:type="simple"/></inline-formula>)-one order of magnitude. It makes WIMPs good candidates for brown dwarf cores too [<xref ref-type="bibr" rid="scirp.76778-ref23">23</xref>] .</p><p>Scaling solution for interacting neutralinos can be described with the same equations (10.1), (10.2), (10.3) and the following values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x347.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x347.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x348.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x347.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x348.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x349.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula136"><label>(10.18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x350.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula137"><label>(10.19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x351.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula138"><label>(10.20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x352.png"  xlink:type="simple"/></disp-formula><p>In this case, the maximum mass and minimum radius increase about four orders of magnitude each and the maximum density equals to the nuclear density. Note that parameters of a FCS made up of strongly interacting neutralinos are identical to those of neutron stars.</p><p>Practically constant value of FCS minimum radius takes place in the huge range of masses <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x353.png" xlink:type="simple"/></inline-formula> from</p><disp-formula id="scirp.76778-formula139"><label>(10.21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x354.png"  xlink:type="simple"/></disp-formula><p>down to</p><disp-formula id="scirp.76778-formula140"><label>(10.22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x355.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x356.png" xlink:type="simple"/></inline-formula>is more than seventeen orders of magnitude smaller than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x356.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x357.png" xlink:type="simple"/></inline-formula>. It makes strongly interacting neutralinos good candidates for stellar and planetary cores of extrasolar systems with Main-sequence stars [<xref ref-type="bibr" rid="scirp.76778-ref23">23</xref>] .</p><p>When the mass of a FCS made up of neutralinos is much smaller than the maximum mass, the scaling solution yields the following equation for parameters <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x358.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x358.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x359.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.76778-formula141"><label>(10.23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x360.png"  xlink:type="simple"/></disp-formula><p>Minimum mass and maximum radius take on the following values:</p><disp-formula id="scirp.76778-formula142"><label>(10.24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x361.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula143"><label>(10.25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x362.png"  xlink:type="simple"/></disp-formula><p>It means that the range of FCS masses (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x363.png" xlink:type="simple"/></inline-formula>) is about twelve orders of magnitude, and the range of FCS core radiuses (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x363.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x364.png" xlink:type="simple"/></inline-formula>) is about four orders of magnitude.</p><p>Fermionic Compact Stars have the following properties:</p><p>・ The maximum potential of interaction <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x365.png" xlink:type="simple"/></inline-formula> between any particle or macroobject and FCS made up of any fermions</p><disp-formula id="scirp.76778-formula144"><label>(10.26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x366.png"  xlink:type="simple"/></disp-formula><p>does not depend on the nature of fermions;</p><p>・ The minimum radius of FCS made of any fermion</p><disp-formula id="scirp.76778-formula145"><label>(10.27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x367.png"  xlink:type="simple"/></disp-formula><p>equals to three Schwarzschild radii and does not depend on the nature of the fermion;</p><p>・ FCS density does not depend on <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x368.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x368.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x369.png" xlink:type="simple"/></inline-formula> and does not change in time while <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x368.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x369.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x370.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x368.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x369.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x370.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x371.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s11"><title>11. Energy Density of Dineutrinos, FIRB and the World</title><p>Our Model holds that the energy densities of all types of Dark Matter particles (DMP) are proportional to the proton energy density in the World’s Medium. In all, there are 5 different types of DMP (see Section 9). Then the total energy density of Dark Matter (DM) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x372.png" xlink:type="simple"/></inline-formula>is</p><disp-formula id="scirp.76778-formula146"><label>(11.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x373.png"  xlink:type="simple"/></disp-formula><p>The total electron energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x374.png" xlink:type="simple"/></inline-formula> is:</p><disp-formula id="scirp.76778-formula147"><label>(11.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x375.png"  xlink:type="simple"/></disp-formula><p>The MBR energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x376.png" xlink:type="simple"/></inline-formula> equals to [<xref ref-type="bibr" rid="scirp.76778-ref1">1</xref>] :</p><disp-formula id="scirp.76778-formula148"><label>(11.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x377.png"  xlink:type="simple"/></disp-formula><p>We took energy density of dineutrinos <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x378.png" xlink:type="simple"/></inline-formula> and FIRB <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x378.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x379.png" xlink:type="simple"/></inline-formula> (see Section 8):</p><disp-formula id="scirp.76778-formula149"><label>(11.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x380.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula150"><label>(11.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x381.png"  xlink:type="simple"/></disp-formula><p>Then the energy density of the World <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x382.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.76778-formula151"><label>(11.6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x383.png"  xlink:type="simple"/></disp-formula><p>Equation (11.6) contains such exact terms as the result of the Models’ predictions and demonstrates consistency of WUM. From (11.6) we can calculate the</p><p>value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x384.png" xlink:type="simple"/></inline-formula>, using electron-to-proton mass ratio <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x384.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x385.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.76778-formula152"><label>(11.7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x386.png"  xlink:type="simple"/></disp-formula><p>which is in an excellent agreement with the commonly adopted value of 137.035999074 (44). It follows that there exists a direct correlation between con-</p><p>stants α and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x387.png" xlink:type="simple"/></inline-formula> expressed by Equation (11.6). As shown above, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x387.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x388.png" xlink:type="simple"/></inline-formula>is not</p><p>an independent constant, but is instead derived from<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x389.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s12"><title>12. Grand Unified Theory</title><p>At the very Beginning (Q = 1) all extrapolated fundamental interactions of the World-strong, electromagnetic, weak, Super Weak and Extremely Weak (pro-</p><p>posed in WUM), and gravitational-had the same cross-section of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x390.png" xlink:type="simple"/></inline-formula>, and</p><p>could be characterized by the Unified coupling constant:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x391.png" xlink:type="simple"/></inline-formula>. The extrapolated energy density of the World was four orders of magnitude smaller than the nuclear energy density [<xref ref-type="bibr" rid="scirp.76778-ref1">1</xref>] . The average energy density of the World has since been decreasing in time<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x391.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x392.png" xlink:type="simple"/></inline-formula>.</p><p>The gravitational coupling parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x393.png" xlink:type="simple"/></inline-formula> is similarly decreasing:</p><disp-formula id="scirp.76778-formula153"><label>(12.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x394.png"  xlink:type="simple"/></disp-formula><p>The weak coupling parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x395.png" xlink:type="simple"/></inline-formula> is decreasing as follows:</p><disp-formula id="scirp.76778-formula154"><label>(12.2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x396.png"  xlink:type="simple"/></disp-formula><p>The strong <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x397.png" xlink:type="simple"/></inline-formula> and electromagnetic <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x397.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x398.png" xlink:type="simple"/></inline-formula> coupling parameters remain con- stant in time:</p><disp-formula id="scirp.76778-formula155"><label>(12.3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x399.png"  xlink:type="simple"/></disp-formula><p>The difference in the strong and the electromagnetic interactions is not in the coupling parameters but in the strength of these interactions depending on the</p><p>particles involved: electrons with charge <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x400.png" xlink:type="simple"/></inline-formula> and monopoles with charge <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x400.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x401.png" xlink:type="simple"/></inline-formula></p><p>in electromagnetic and strong interactions respectively.</p><p>The super weak coupling parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x402.png" xlink:type="simple"/></inline-formula> and the extremely weak coupling parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x402.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x403.png" xlink:type="simple"/></inline-formula> proposed in WUM are decreasing as follows:</p><disp-formula id="scirp.76778-formula156"><label>(12.4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x404.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.76778-formula157"><label>(12.5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x405.png"  xlink:type="simple"/></disp-formula><p>According to WUM, the coupling strength of super-weak interaction is <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x406.png" xlink:type="simple"/></inline-formula> times weaker than that of weak interaction. The possibility of such ratio of interactions was discussed in the developed theoretical models explaining CP and Strangeness violation [<xref ref-type="bibr" rid="scirp.76778-ref58">58</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref59">59</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref60">60</xref>] [<xref ref-type="bibr" rid="scirp.76778-ref61">61</xref>] . Super-weak and Extremely-weak interactions provide an important clue to Physics beyond the Standard Model.</p></sec><sec id="s13"><title>13. Conclusions</title><p>WUM holds that there exist relations between all Q-dependent parameters: Newtonian parameter of gravitation and Hubble’s parameter; critical energy density and Fermi coupling parameter; temperatures of the microwave background radiation and far-infrared background radiation peak. The calculated values of these parameters are in good agreement with the latest results of their measurements.</p><p>Today, Fermi coupling parameter <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-2180210x407.png" xlink:type="simple"/></inline-formula> is known with the highest precision [<xref ref-type="bibr" rid="scirp.76778-ref1">1</xref>] :</p><disp-formula id="scirp.76778-formula158"><label>(13.1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-2180210x408.png"  xlink:type="simple"/></disp-formula><p>Based on its average value, we can calculate and significantly increase the precision of all Q-dependent parameters. We propose to introduce Q as a new fundamental parameter tracked by CODATA, and use its value in calculation of all Q-dependent parameters.</p></sec><sec id="s14"><title>Acknowledgements</title><p>I am grateful to anonymous referees for valuable comments and important remarks that helped me to improve the understanding of the Model. Special thanks to my son Ilya Netchitailo who helped shape the manuscript to its present form.</p></sec><sec id="s15"><title>Cite this paper</title><p>Netchitailo, V.S. (2017) Mathematical Overview of Hypersphere World-Universe Model. Journal of High Energy Physics, Gravitation and Cos- mology, 3, 415-437. https://doi.org/10.4236/jhepgc.2017.33033</p></sec></body><back><ref-list><title>References</title><ref id="scirp.76778-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Netchitailo, V.S. (2016) Overview of Hypersphere World-Universe Model. Journal of High Energy Physics, Gravitation and Cosmology, 2, 593.  
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