<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2014.511101</article-id><article-id pub-id-type="publisher-id">JMP-47484</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>Baryon Magnetic Moment in the Scalar Strong Interaction Hadron Theory</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>F.</surname><given-names>C. Hoh</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>Dragarbrunnsg, 55C, 75320 Uppsala, Sweden</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>hoh@telia.com</email></corresp></author-notes><pub-date pub-type="epub"><day>30</day><month>06</month><year>2014</year></pub-date><volume>05</volume><issue>11</issue><fpage>995</fpage><lpage>1000</lpage><history><date date-type="received"><day>21</day>	<month>March</month>	<year>2014</year></date><date date-type="rev-recd"><day>15</day>	<month>April</month>	<year>2014</year>	</date><date date-type="accepted"><day>8</day>	<month>May</month>	<year>2014</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 magnetic moments of the baryon octet are derived from a first
principle’s theory, the scalar strong interaction hadron theory, and are in
approximate agreement with data. It is conjectured that this agreement may be
improved by including the “spin-orbit coupling” term not evaluated here. 
</p></abstract><kwd-group><kwd>Baryon Magnetic Moment</kwd><kwd> First Principle’s Theory</kwd><kwd> Internal Coordinates</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The existing treatments of baryon magnetic moment are all phenomenological and based upon models [<xref ref-type="bibr" rid="scirp.47484-ref1">1</xref>] . The predicted results depend upon free parameters introduced and lack theoretical foundation, unlike the derivation of electron’s magnetic and anomalous magnetic moments from the established Dirac equation and QED. Here, the main stream first principle’s theory, Quantum Chromodynamics [<xref ref-type="bibr" rid="scirp.47484-ref2">2</xref>] , cannot be applied to this problem; it does not work at low energies. Therefore, the scalar strong interaction hadron theory, a first principle’s theory which has proven to be rather successful in accounting for low energy, so far mainly mesonic phenomena, has been applied to this problem</p></sec><sec id="s2"><title>2. Baryon Wave Equations in Electromagnetic Field</title><p>The baryon magnetic moment has been treated [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] using a first principle’s theory, the scalar strong interaction hadron theory [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] . In [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] , however, the quark coordinates in the electromagnetic potential were approximated by those of the baryon. The quarks were also assumed to be static. The results of [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] are about 1/3 of the measured ones [<xref ref-type="bibr" rid="scirp.47484-ref2">2</xref>] .</p><p>These two approximations are removed here and the factor 1/3 drops out; the results are now in approximate agreement with data. This paper is thus nearly the same as the 1994 paper [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] without these two approximations and relies on the book [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] . The total equations of motion for the octet baryons ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (9.3.9)) have been generalaized to include U(1) gauge fields A to become [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (5.1),</p><disp-formula id="scirp.47484-formula1723"><label>(1a)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\d79e6230-dbfb-43c6-9608-4b9209f37ff1.png"/></disp-formula><disp-formula id="scirp.47484-formula1724"><label>(1b)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\75fffa44-8aa4-40dc-829f-708ae98130d2.png"/></disp-formula><p>Here, I, II and III refer to the three quarks, x stands for the 4 vector x<sup>m</sup>, c and y the baryon wave functions in space time where the undotted and dotted spinor indices run from 1 to 2, F<sub>b</sub> the interquark scalar strong interacton ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (9.2.11)) producing confinememt, and analogous to [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (3.1.4).</p><disp-formula id="scirp.47484-formula1725"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\a552ded8-826a-480d-bfbd-aa22823c3b28.png"/></disp-formula><p>The d function is not a Lorentz invariant. Further, z, u, and v stand for the internal coordinates z<sub>I</sub>, z<sub>II</sub> and z<sub>III</sub>, respectively, x the internal baryon function, p, s, q the flavors of the three quarks, m<sub>3op</sub> the quark mass operator ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (9.3.8, 12, 13)), and q<sub>op</sub><sub> </sub>the quarks charge operator ([<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (2.8)), ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (2.3.14)),</p><disp-formula id="scirp.47484-formula1726"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\8051355b-ea34-4679-ad63-3e1d0604cb10.png"/></disp-formula></sec><sec id="s3"><title>3. Internal Baryon Wave Functions</title><p>The normalized internal functions for the octet baryons reads ([<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (8.1)),</p><disp-formula id="scirp.47484-formula1727"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\20e55903-f043-4037-aa97-ad310727a5d4.png"/></disp-formula><p>In passing, it is pointed out that these internal functions [<xref ref-type="bibr" rid="scirp.47484-ref5">5</xref>] are essential to the present theory. By exploiting a symmetry among z, v and u, the QCD Lagrangian [<xref ref-type="bibr" rid="scirp.47484-ref2">2</xref>] has been derived from this theory [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] in the high energy limit [<xref ref-type="bibr" rid="scirp.47484-ref6">6</xref>] . These x’s can be removed by multiplying (1) by x<sub>psq</sub> = (x<sup>psq</sup>)<sup>*</sup> via [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (2.5a),</p><disp-formula id="scirp.47484-formula1728"><label>(5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\eda7b452-f8ee-4911-95b5-545ca7d5362f.png"/></disp-formula><p>These q’s are given on lines 2 and 3 of <xref ref-type="table" rid="table1">Table 1</xref> below.</p><p>Gauge invariance of (1) is shown in the same way as that for mesons in ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (6.3.1, 2)) extended to include a third quark. The external electromagnetic field is static and has no time component,</p><disp-formula id="scirp.47484-formula1729"><label>(6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\29ae5248-a5e4-4a3d-81f8-f85f13bb2b82.png"/></disp-formula><table-wrap id="table1"  position="float"><object-id pub-id-type="pii">Table 1</object-id><label>Table 1</label><caption><p>. Octet baryon magnetic moments from (17) using the q’s from (5). There are no data for S<sup>0</sup>, only the transition magnetic moment S<sup>0</sup> &#174; L</p></caption><table><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >proton</th><th align="center" valign="middle" >neutron</th><th align="center" valign="middle" >L</th><th align="center" valign="middle" >S<sup>+</sup><sup></sup></th><th align="center" valign="middle" >S<sup>0</sup></th><th align="center" valign="middle" >S<sup>-</sup><sup></sup></th><th align="center" valign="middle" >X<sup>0</sup><sup></sup></th><th align="center" valign="middle" >X<sup>-</sup><sup></sup></th></tr></thead><tbody><tr><td align="center" valign="middle" >q<sub>I</sub>/e = q<sub>III</sub>/e</td><td align="center" valign="middle" >1/2</td><td align="center" valign="middle" >-1/6</td><td align="center" valign="middle" >-1/12</td><td align="center" valign="middle" >1/2</td><td align="center" valign="middle" >1/12</td><td align="center" valign="middle" >-1/3</td><td align="center" valign="middle" >-1/6</td><td align="center" valign="middle" >-1/3<sup></sup></td></tr><tr><td align="center" valign="middle" >q<sub>II</sub>/e from (5)</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >1/3</td><td align="center" valign="middle" >1/6</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >-1/6</td><td align="center" valign="middle" >-1/3</td><td align="center" valign="middle" >1/3</td><td align="center" valign="middle" >-1/3</td></tr><tr><td align="center" valign="middle" >m<sub>b</sub> (17)</td><td align="center" valign="middle" >3</td><td align="center" valign="middle" >-1.997</td><td align="center" valign="middle" >-0.841</td><td align="center" valign="middle" >2.367</td><td align="center" valign="middle" >0.787</td><td align="center" valign="middle" >-0.783</td><td align="center" valign="middle" >-1.427</td><td align="center" valign="middle" >-0.71</td></tr><tr><td align="center" valign="middle" >m<sub>b</sub> data [2] </td><td align="center" valign="middle" >2.793</td><td align="center" valign="middle" >-1.913</td><td align="center" valign="middle" >-0.613</td><td align="center" valign="middle" >2.458</td><td align="center" valign="middle" >1.61(S<sup>0</sup>&#174;L)</td><td align="center" valign="middle" >-1.16</td><td align="center" valign="middle" >-1.25</td><td align="center" valign="middle" >-0.6507</td></tr></tbody></table></table-wrap></sec><sec id="s4"><title>4. Transformation into Laboratory and Relative Coordinates</title><p>Taking the left operator of (1b) and operating it on (1a) and making use of (1b, 3-6) leads to [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (5.4),</p><disp-formula id="scirp.47484-formula1730"><label>(7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\8a6e831c-8ffd-4e2f-8aa3-6369137d6de5.png"/></disp-formula><disp-formula id="scirp.47484-formula1731"><label>(8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\c5f38041-8b94-4872-b394-307d4ebe1a0d.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\831c8803-824e-45a0-ad0d-0f8be30167cf.png" xlink:type="simple"/></inline-formula> is the eigenvalue of m<sub>3op</sub> ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (9.3.15, 17, 19)), [A, B]=AB-BA. A sister pair of equations are obtained for y and R<sub>B</sub>(c,q) by reversing the roles of (1a) and (1b). Note that the three braced operators refer to different coordinates and therefore commute with each other.</p><p>Following [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (6.1, 4), let</p><disp-formula id="scirp.47484-formula1732"><label>(9a)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\2745c709-ea7c-4c12-bb2c-95c939d06e73.png"/></disp-formula><p>so that by relations of the type of (2),</p><disp-formula id="scirp.47484-formula1733"><label>(9b)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\29c59666-825d-40e9-8117-a71b2a86898b.png"/></disp-formula><p>The relative energies in [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (6.4) has been put to 0 in accordance with [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (3.5.6). Alternatively, [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (3.1.10a) type of relations can be used to remove them to arrive at [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (10.1.2). Here X is the laboratory coordinate of the baryon and x and y are the relative coordinates of the quarks shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>(a).</p></sec><sec id="s5"><title>5. First Order Relations and Magnetic Moment</title><p>In the the absence of electromagnetic perturbation or putting the A&#180;s to zero, (1) reduces to the zeroth order equations ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (9.3.9)). A in (7, 8) will now produce a pertubation of c and y in (7) so that, in terms of (9),</p><fig-group id="fig1"><caption><title>Figure 1</title><p> (a) illustrates the general (9a), (b) the zeroth order quark-diquark configuration with x<sub>I</sub> = x<sub>III</sub> = x<sub>I</sub><sub>,III</sub>, d = 1/2 in (9a), ([4] (10.1.1)), X<sub>0</sub> denotes the zeroth order laboratory coordinates, (c) special case of (a) with c = 1/2 and d = 1/3, giving a maximally allowed E<sub>1b</sub> in (16)</p></caption><fig id ="fig1_1"><label>(a) (b) (c)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\010fa677-e9ce-4d26-9022-828df61db0f0.png"/></fig></fig-group><p></p><disp-formula id="scirp.47484-formula1734"><label>(10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\7eadef5a-b011-4493-b220-888eeacfb8eb.png"/></disp-formula><p>where the subscript 1 denotes first order pertubation, E<sub>0</sub> denotes the baryon mass and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\9912d3b0-3574-4b81-a365-53c5da82e6c3.png" xlink:type="simple"/></inline-formula> is that in <xref ref-type="fig" rid="fig1">Figure 1</xref>(b), as does x in c which enters the zeroth order ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (10.1.2)). The first line beneath (9b) is noted.</p><p>Let the external magnetic field be</p><disp-formula id="scirp.47484-formula1735"><label>(11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\3dbececb-d42e-4657-8215-968c5e556d48.png"/></disp-formula><p>where j<sub>g</sub>(X) is a gauge functon. With (9), we find</p><disp-formula id="scirp.47484-formula1736"><label>(12)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\5db8df32-bb0c-4286-94c8-2710fe950455.png"/></disp-formula><p>The apparoximation made beneath (4.1) in [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] keeps only the first term on the right of (12). This turns out to be the reason that the results in (7.10) and <xref ref-type="table" rid="table1">Table 1</xref> there are three times too small.</p><p>After inserting (10) into (7), we wish to obtain the perturbed baryon energy E<sub>1b</sub> as a function of the first order q&#180;s there. With (2), (9), (11), and <xref ref-type="fig" rid="fig1">Figure 1</xref>(a), the first order part of the first braces in (7) reads</p><disp-formula id="scirp.47484-formula1737"><label>(13)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\3a21fec1-83f9-4026-a6eb-8cb012b72e4d.png"/></disp-formula><p>The zeroth order part of the remaining two braces in (7) is found from (9) and <xref ref-type="fig" rid="fig1">Figure 1</xref>(b) and is</p><disp-formula id="scirp.47484-formula1738"><label>(14)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\497d7b8f-c991-4c7c-b437-1db148556802.png"/></disp-formula><p>The first order parts of the second and third braces in (7) are analogously found; the associated zeroth order parts are of the same form as the last of (14). The first order part of (7) now reads</p><disp-formula id="scirp.47484-formula1739"><label>(15)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\eee3866e-1f9d-4fce-9221-cfae8aa1eb50.png"/></disp-formula><p>Here, it has been noted that <xref ref-type="fig" rid="fig1">Figure 1</xref>(a) and <xref ref-type="fig" rid="fig1">Figure 1</xref>(b) show that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\cce1ea08-e1a4-4e06-a0d1-91aecf6793b5.png" xlink:type="simple"/></inline-formula> and X<sub>0 </sub>differ by a quantity independent of each of them so that<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\3ac06293-f1c3-4432-8b29-a4e142cdc4a0.png" xlink:type="simple"/></inline-formula>. Note that the strong interaction F<sub>b</sub> for a free baryon and m<sub>3op</sub> are not affected by the perturbative A fields and operate only on zeroth order wave functions. The argument of c and F<sub>b</sub> has thus been changed to reflect that <xref ref-type="fig" rid="fig1">Figure 1</xref>(b) applies. R<sub>B</sub><sub>1</sub> denotes the first order part of (8).</p><p>The dominating contributions to the energy shift E<sub>1b</sub> in the first term of (15) comes from the three qs<sub>3</sub> terms on the left of (15) which contribute equally, but of opposite signs, to E<sub>1b</sub> for spin up and spin down wave function components shown in (16b) below. The second and third terms on the right of (15) are just the zeroth order part of (7, 8) and can be absorbed into it. The first and last terms on the right of (15) do not contain s<sub>3</sub> splitting term and their contributions to E<sub>1b </sub>are of the same sign for the spin up and down components. These contributions, to the degree that they are of equal magnitude, cancel out in the evaluation of the magnetic moment. These two terms will be ignored here to arrive at an approximate expression of the magnetic moment.</p><p>The zeroth order c on the remaining left of (15) for the spinor index c = 1, 2 are eigenfunctions of the qs<sub>3</sub> operators; we obatin the equivalent of [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (7.3),</p><disp-formula id="scirp.47484-formula1740"><label>(16a)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\ad64dac6-f26b-4c51-994a-c76a9fbd9b2a.png"/></disp-formula><disp-formula id="scirp.47484-formula1741"><label>(16b)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\f6f15ba3-5141-4ee6-ae31-1f875ff7513a.png"/></disp-formula><p>The doublet wave functions ([<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (7.4)] are reproduced in (16b) and are the spin up m = 1/2 part ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (10.3.8a)). The corresponding spin down m = -1/2 part ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (10.3.8b)) is basically (16b) with the both expressions interchanged. The radial wave functions g<sub>0</sub>(r) and f<sub>0</sub>(r) have been plotted in ([<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] <xref ref-type="fig" rid="fig11">Figure 11</xref>.1).</p><p>The space dependent part associated with O<sub>b</sub> in (16a) drops out, just like that in [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (4.5b) or [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (6.3.12) for vector meson. The maximally allowed stationary energy shift E<sub>1b</sub> is found for c = 1/2 and d = 1/3, same as [<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (7.9). Let E<sub>p</sub> be the proton massn magnetic moment reads</p><disp-formula id="scirp.47484-formula1742"><label>(17)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501781x\32760bd5-66be-4887-a7db-b4fe68f40bdb.png"/></disp-formula><p>which is 3 times the 1994 result ([<xref ref-type="bibr" rid="scirp.47484-ref3">3</xref>] (7.10)) without neglect of quark motion beneath (8.3) there. The results are shown on line 4 in <xref ref-type="table" rid="table1">Table 1</xref> and are in approximate agreement with data [<xref ref-type="bibr" rid="scirp.47484-ref2">2</xref>] on line 5.</p></sec><sec id="s6"><title>6. Conclusion</title><p>The baryon magnetic moment has been treated for the first time starting from a first principle’s theory, the scalar strong interaction hadron theory, that the predicted results are in approximate agreement with data which lends further support to the fact that this theory is basically viable and can replace QCD at low energies.</p><p>It is conjectured that the difference between the last two lines in <xref ref-type="table" rid="table1">Table 1</xref> may be due to the first term R<sub>B1</sub> on the right of (15). This “rest” term arises from the strong quark-diquark interaction F(r); its effect resembles spin-orbit coupling in atomic physics. Its inclusion calls for numerical integration. The last term of (15) can be balanced off by including the equally probable spin down m = -1/2 wave functions of [<xref ref-type="bibr" rid="scirp.47484-ref4">4</xref>] (10.3.8b) mentioned beneath (16b). An additional degree of freedom is the choice of the gauge function j<sub>g</sub>(X) in (11); the simplest form is a constant which does not contribute to (11).</p></sec></body><back><ref-list><title>References</title><ref id="scirp.47484-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">LICHTENBERG, D.B. (1978) UNITARY SYMMETRY AND ELEMENTARY PARTICLES. ACADEMIC PRESS, WALTHAM.</mixed-citation></ref><ref id="scirp.47484-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">BERINGER, J., ET AL. (2012) PHYSICAL REVIEW D, 86, ARTICLE ID: 010001. HTTP://DX.DOI.ORG/10.1103/PHYSREVD.86.010001</mixed-citation></ref><ref id="scirp.47484-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">HOH, F.C. (1994) INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 33, 2351-2363.</mixed-citation></ref><ref id="scirp.47484-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">HOH, F.C. (2011) SCALAR STRONG INTERACTION HADRON THEORY. NOVA SCIENCE PUBLISHERS, NEW YORK.HTTPS://WWW.NOVAPUBLISHERS.COM/CATALOG/PRODUCT_INFO.PHP?PRODUCTS_ID=27069</mixed-citation></ref><ref id="scirp.47484-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">BEG, M.A.B. AND RUEGG, H. (1965) JOURNAL OF MATHEMATICAL PHYSICS, 6, 677-682.HTTP://DX.DOI.ORG/10.1063/1.1704325</mixed-citation></ref><ref id="scirp.47484-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">HOH, F.C. (2013) JOURNAL OF MODERN PHYSICS, 4, 1171-1175. HTTP://DX.DOI.ORG/10.4236/JMP.2013.49157</mixed-citation></ref></ref-list></back></article>