<?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>
   <issn publication-format="print">
    2380-4335
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jhepgc.2025.112038
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-142321
   </article-id>
   <article-categories>
    <subj-group subj-group-type="heading">
     <subject>
      Articles
     </subject>
    </subj-group>
    <subj-group subj-group-type="Discipline-v2">
     <subject>
      Physics 
     </subject>
     <subject>
       Mathematics
     </subject>
    </subj-group>
   </article-categories>
   <title-group>
    The Unification of Gravity with Electromagnetism in the Classical Newtonian Region, with an Explanation of the Crookes Radiometer, and a Model for “Dark Matter”
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Stephen Joseph
      </surname>
      <given-names>
       Kennedy
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aUniversity of Massachusetts at Dartmouth, Dartmouth, MA, USA
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     18
    </day> 
    <month>
     03
    </month>
    <year>
     2025
    </year>
   </pub-date> 
   <volume>
    11
   </volume> 
   <issue>
    02
   </issue>
   <fpage>
    554
   </fpage>
   <lpage>
    566
   </lpage>
   <history>
    <date date-type="received">
     <day>
      8,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      25,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      25,
     </day>
     <month>
      April
     </month>
     <year>
      2025
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © 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>
    Maxwell wrote that he wanted to “leaven” his Treatise on Electromagnetism with Quaternions. Maxwell died before doing this. Silberstein and Conway accomplished this partially. This presentation claims the Lorenz condition field is proportional to the gravitational potential. This results in a gravitic-electromagnetic unification in the classical Newtonian region. An explanation of the Crookes radiometer is given and a model for dark matter is presented.
   </abstract>
   <kwd-group> 
    <kwd>
     Unified Field
    </kwd> 
    <kwd>
      Dark Matter
    </kwd> 
    <kwd>
      Gravity
    </kwd> 
    <kwd>
      Quaternion
    </kwd> 
    <kwd>
      Pauli Algebra
    </kwd> 
    <kwd>
      Crookes Radiometer
    </kwd> 
    <kwd>
      Photo-Graviton
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <p>Michael Faraday met W.R. Hamilton in 1834, in Dublin <xref ref-type="bibr" rid="scirp.142321-1">
     [1]
    </xref>. It is speculated that Faraday told Hamilton of the weird electromagnetism experimental results he and others were getting. Electromagnetism needed some sort of geometric algebra to organize it. Hamilton, after much effort <xref ref-type="bibr" rid="scirp.142321-2">
     [2]
    </xref>, in 1843, finally found, a generalization of complex numbers 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mi>
         Q 
       </mi> 
       <mo>
         ↔ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        w 
      </mi> 
      <mo>
        + 
      </mo> 
      <mi>
        x 
      </mi> 
      <mover accent="true"> 
       <mi>
         i 
       </mi> 
       <mo>
         ^ 
       </mo> 
      </mover> 
      <mo>
        + 
      </mo> 
      <mi>
        y 
      </mi> 
      <mover accent="true"> 
       <mi>
         j 
       </mi> 
       <mo>
         ^ 
       </mo> 
      </mover> 
      <mo>
        + 
      </mo> 
      <mi>
        z 
      </mi> 
      <mover accent="true"> 
       <mi>
         k 
       </mi> 
       <mo>
         ^ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        w 
      </mi> 
      <mo>
        + 
      </mo> 
      <mover accent="true"> 
       <mi>
         r 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </mrow> 
    </math> ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mo>
       ↔ 
     </mo> 
    </math> double arrow denotes a quaternion, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mo>
       → 
     </mo> 
    </math> right arrow denotes a vector, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mo>
       ˆ 
     </mo> 
    </math> a caret denotes a unit vector, plain symbol denotes a scalar ) that he called Quaternions, then in 1844 complex component quaternions calling them biquaternions. Complex quaternions can be represented as 2 × 2 matrices (Pauli matrices) <xref ref-type="bibr" rid="scirp.142321-3">
     [3]
    </xref> 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         σ 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        i 
      </mi> 
      <mover accent="true"> 
       <mi>
         i 
       </mi> 
       <mo>
         ^ 
       </mo> 
      </mover> 
     </mrow> 
    </math> 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          σ 
        </mi> 
        <mo>
          ^ 
        </mo> 
       </mover> 
       <mn>
         2 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        i 
      </mi> 
      <mover accent="true"> 
       <mi>
         j 
       </mi> 
       <mo>
         ^ 
       </mo> 
      </mover> 
     </mrow> 
    </math> 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          σ 
        </mi> 
        <mo>
          ^ 
        </mo> 
       </mover> 
       <mn>
         3 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        i 
      </mi> 
      <mover accent="true"> 
       <mi>
         k 
       </mi> 
       <mo>
         ^ 
       </mo> 
      </mover> 
     </mrow> 
    </math> with all the properties of complex numbers except they are not commutative and division by a small class of quaternions that do not have an inverse, called zero divisors, are not allowed. Complex quaternions or Pauli quaternions can be represented by vector analysis notation, vector analysis being a truncated form of quaternions <xref ref-type="bibr" rid="scirp.142321-4">
     [4]
    </xref>. Hamilton’s real quaternions have been used by computer scientists since the 1980’s for 3 dimensional rotations.<sup>1</sup></p>
   <p>In 1854 Peter Guthrie Tait, a boyhood friend of Maxwell, went to Ireland from his native Scotland to study Quaternions. He informed Maxwell of quaternions in a series of letters <xref ref-type="bibr" rid="scirp.142321-5">
     [5]
    </xref>. Maxwell used the quaternion in his researches on how to make sense of the electromagnetism experiments of Faraday and others. In the 1870’s Maxwell came up with 4 equations; 2 scalar equations and 2 vector equations now known as “Maxwell’s Equations” that summarized the known electromagnetism experiments. He used quaternions to deduce that electromagnetic waves that traveled at the speed of light existed. This was later confirmed H. Hertz. Maxwell wrote to Tait <xref ref-type="bibr" rid="scirp.142321-5">
     [5]
    </xref> that he wanted to “leaven” his work on electromagnetism with quaternions. Maxwell’s early death, due to cancer, prevented this from happening.</p>
   <p>Quaternions fell out of favor in mainstream physics in the early 20th century. However, some quaternion research was still going on by some people such as, L. Silberstein and A. Conway. Conway <xref ref-type="bibr" rid="scirp.142321-6">
     [6]
    </xref> and Silberstein <xref ref-type="bibr" rid="scirp.142321-7">
     [7]
    </xref> <xref ref-type="bibr" rid="scirp.142321-8">
     [8]
    </xref> both apparently knew that all four Maxwell’s equations could be written as one complex quaternion equation. However, when the equations were written in terms of Scalar and Vector Potentials, the equations had a troubling loose end. The quantity 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <msub> 
         <mi>
           A 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        + 
      </mo> 
      <mover accent="true"> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ⋅ 
      </mo> 
      <mover accent="true"> 
       <mi>
         A 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ≡ 
      </mo> 
      <mi>
        G 
      </mi> 
     </mrow> 
    </math>, the scalar part of the field generated by the potentials, was not associated with anything in observed reality so that most treatments set 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <msub> 
         <mi>
           A 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        + 
      </mo> 
      <mover accent="true"> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ⋅ 
      </mo> 
      <mover accent="true"> 
       <mi>
         A 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>, known as the “Lorenz condition”<sup>2</sup>. Both Silberstein and Conway seem to have followed this convention, with their quaternion electric field-Magnetic flux density fields being, the complex vector 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        − 
      </mo> 
      <mover accent="true"> 
       <mi>
         E 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        + 
      </mo> 
      <mi>
        i 
      </mi> 
      <mover accent="true"> 
       <mi>
         B 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </mrow> 
    </math>. The quantity 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mo>
         ∂ 
       </mo> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msub> 
       <mi>
         A 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mover accent="true"> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ⋅ 
      </mo> 
      <mover accent="true"> 
       <mi>
         A 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ≡ 
      </mo> 
      <mi>
        G 
      </mi> 
     </mrow> 
    </math> with the short hand ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mo>
         ∂ 
       </mo> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        → 
      </mo> 
      <msub> 
       <mo>
         ∂ 
       </mo> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>) when left as the scalar part of the electromagnetic</p>
   <p>field denoted as, the quaternion 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        G 
      </mi> 
      <mo>
        − 
      </mo> 
      <mover accent="true"> 
       <mi>
         E 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        + 
      </mo> 
      <mi>
        i 
      </mi> 
      <mover accent="true"> 
       <mi>
         B 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </mrow> 
    </math> which will be called the classical quaternion electromagnetic field. Maxwell’s equations are slightly modified but the effects after interpreting G as being proportional to the gravitational potential are so small as to be undetectable in terrestrial experiments. The full treatment below Equations (10) and (11) gives a one step derivation of the electromagnetic wave equation in which in the time independent angular independent case, the Laplacian operator on the G field being set equal to what is called the continuity Equation (12), which equals zero, with a static solution of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mi>
         k 
       </mi> 
       <mi>
         r 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> equation, where r is a distance from an appropriate origin. When k = 0 the standard Lorenz condition 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        ∂ 
      </mo> 
      <msub> 
       <mi>
         A 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mover accent="true"> 
       <mo>
         ∇ 
       </mo> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ⋅ 
      </mo> 
      <mover accent="true"> 
       <mi>
         A 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
      <mo>
        ≡ 
      </mo> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math> is obtained, however, if 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        k 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mi>
        κ 
      </mi> 
      <mi mathvariant="script">
        G 
      </mi> 
      <mi>
        m 
      </mi> 
      <mi>
        M 
      </mi> 
     </mrow> 
    </math> where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi mathvariant="script">
       G 
     </mi> 
    </math> is Newton’s gravitational constant with a proportionality constant 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       κ 
     </mi> 
    </math> then Newton’s Law for gravitational potential is essentially derived from Maxwell’s equations. When time dependence is assumed, in Cartesian coordinates a standard wave equation with traveling gravitational waves that accompany the electromagnetic wave is obtained.</p>
   <p>The final task of exploring quantum mechanics and gravity utilizes the idea of Alan Guth <xref ref-type="bibr" rid="scirp.142321-10">
     [10]
    </xref> that the gravitational field has negative mass and that a gravity wave accompanies the electromagnetic wave. Since a “photon” has an energy of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mi>
        f 
      </mi> 
     </mrow> 
    </math> it should have a mass of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mi>
          h 
        </mi> 
        <mi>
          f 
        </mi> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> the paradox of a massive object going the speed of light is resolved if the accompanying “graviton” has a mass of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mi>
          h 
        </mi> 
        <mi>
          f 
        </mi> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> this also resolves the paradox of the Crookes Radiometer which is discussed below. Negative mass gravitons are presented before the Pauli (algebra) quaternion treatment of the Maxwell’s equations with Newton’s gravitational potential is presented so that the possibly unfamiliar math (see footnote 3), doesn’t distract from the main point of this presentation, that positive mass photons are escorted by negative mass gravitons! Then a model for “dark matter” is also presented.</p>
  </sec><sec id="s2">
   <title>
    <xref ref-type="bibr" rid="scirp.142321-"></xref>2. Negative Mass Gravitons and Photons Becoming “Photo-Gravitons”</title>
   <sec id="s2_1">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>2.1. Photo Graviton and Free Graviton</title>
    <p>In the quaternion electromagnetism formulation, the electromagnetic field quaternion denoted 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mi>
          F 
        </mi> 
        <mo>
          ↔ 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mi>
         G 
       </mi> 
       <mo>
         − 
       </mo> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         + 
       </mo> 
       <mi>
         i 
       </mi> 
       <mover accent="true"> 
        <mi>
          B 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
      </mrow> 
     </math> has a scalar part 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math>, which is usually set equal to 0 due to L. Lorenz (see footnote 2). In Equation (12) below a differential equation for 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> is derived. Although 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> is a trivial solution more physically suggestive solutions exist. It will be suggested below that at least in the Classical Newtonian domain the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> could be proportional to the gravitational field. The time dependent “wave equation” for 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> Equation (12) below suggests in addition to the static solution there is a wave that travels along with electromagnetic wave (which is related to the quanta of light known as the “photon”). It is proposed that the companion 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> wave have a related quanta which should be called the “graviton”. It is proposed that the graviton-photon couple be named the Photo-graviton. Note that the graviton in this model has a spin 1 so that the photo-graviton should have a spin 2. The graviton is proposed to have negative mass extrapolating on the idea in reference <xref ref-type="bibr" rid="scirp.142321-10">
      [10]
     </xref> and that this mass exactly cancels the companion photon mass.</p>
    <p>Whenever mass is created, even a small amount, an appropriate amount of gravity must be created also (with the common assumption that mass and gravity are related). According to an idea by Alan Guth <xref ref-type="bibr" rid="scirp.142321-10">
      [10]
     </xref> a gravitational field should have negative mass, extending this gravitons should have negative mass. When a “graviton” interacts with a positive mass, the positive mass, in order to conserve momentum, the positive mass must react by going in the direction of the graviton source. Since 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         E 
       </mi> 
       <mo>
         = 
       </mo> 
       <mi>
         m 
       </mi> 
       <msup> 
        <mi>
          c 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
      </mrow> 
     </math>, Einstein’s idea that energy and mass are the same thing, when something as simple as a hydrogen atom absorbs an electromagnetic wave of an appropriate frequency, the hydrogen atom’s mass increases by + 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mtext>
         Δ 
       </mtext> 
       <mi>
         m 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mi>
           h 
         </mi> 
         <mi>
           f 
         </mi> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            c 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>. The hydrogen atom must then increase (actually decrease) the energy of its gravitational field by 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mtext>
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       </mtext> 
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         m 
       </mi> 
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            c 
          </mi> 
          <mn>
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        </mrow> 
       </mfrac> 
      </mrow> 
     </math>. At first, this seems to be at odds with classical electromagnetism, however, it is not as will be shown below. If a negative mass graviton rides along with a positive mass photon it explains how a massive photon with 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        <mi>
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            c 
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          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> can go at the speed of light, while other objects of finite mass are restricted by relativity from ever attaining this supposed universal speed limit. Negative mass gravitons in a vacuum are not in conflict with the curved-distorted Euclidean space of general relativity, in fact, they are why the space is distorted.</p>
    <p>
     <xref ref-type="fig" rid="fig1">
      Figure 1
     </xref> shows photo graviton absorption, and the completed Maxwell’s equation to the left, see subsection 6 below. It should be noted that the graviton wave has the “beat frequency” of the interference pattern of the two involved DeBroglie waves or Ψ functions. <xref ref-type="fig" rid="fig2">
      Figure 2
     </xref> shows photo graviton spontaneous emission stimulated by graviton.</p>
   </sec>
   <sec id="s2_2">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>2.2. Gravitational Field’s Involvement in Absorption, Spontaneous Emission, with Comment on Stimulated Emission</title>
    <p>See <xref ref-type="fig" rid="fig1">
      Figure 1
     </xref>, the photo graviton excites the lower state electron, to a higher more energetic state. The extra energy causes an increase in mass of the atom (from Einstein’s 
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       </mi> 
       <msup> 
        <mi>
          c 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
      </mrow> 
     </math>) that mass being; 
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          </mi> 
          <mn>
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        </mrow> 
       </mfrac> 
      </mrow> 
     </math>. With a corresponding decrease in the gravitational field mass of 
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         Δ 
       </mtext> 
       <msub> 
        <mi>
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      </mrow> 
     </math>. as shown by the emitted graviton.</p>
    <fig id="fig1" position="float">
     <label>Figure 1</label>
     <caption>
      <title>Figure 1. The above is a model that depicts an electromagnetic wave associated with a photon having energy E = hf coupled to a graviton wave and posited graviton with Energy E = −hf together they have a zero mass, solving the paradox of how an energetic and therefore massive photon can travel at the speed of light. If both photon and graviton have spin 1 then the “Photo-graviton” has spin 2 as some theories require. When the photo-graviton is absorbed by an atom as depicted by the DeBroglie-Bohr model atom to the right, the photon and graviton split, with the energy and mass of the atom increasing and gravitational field associated with the mass increasing strength, while the mass of the gravitational field decreases.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId88.jpeg?20250428034724" />
    </fig>
    <fig id="fig2" position="float">
     <label>Figure 2</label>
     <caption>
      <title>Figure 2. This depicts the reverse effect of photo-graviton absorption depicted in <xref ref-type="fig" rid="fig1">
        Figure 1
       </xref>. An excited Atom (or in general any quantum state) emits a photo-graviton after interacting with a free graviton. See section on spontaneous emission below.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId89.jpeg?20250428034724" />
    </fig>
    <p>The claim of <xref ref-type="fig" rid="fig2">
      Figure 2
     </xref> is that spontaneous emission is triggered by free gravitons, the quanta of the field 
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         G 
       </mi> 
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        </mn> 
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        <mi>
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        </mi> 
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          → 
        </mo> 
       </mover> 
      </mrow> 
     </math>. This claim is actually reinforced by standard physics graduate school text books such as reference <xref ref-type="bibr" rid="scirp.142321-11">
      [11]
     </xref> which give a simplified and not completely rigorous treatments of spontaneous emission.</p>
    <p>Texts give an interaction Hamiltonian for the simplest spontaneous emission of 
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     </math> where 
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     </math> is the current of electron in upper state this is a gives transition matrix element 
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        </mo> 
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      </mrow> 
     </math> going from the excited state 
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     </math> to the lower state 
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     </math> note that 
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     </math> is the vector potential. In quantum mechanics 
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     </math> substituting this into 
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     </math> note that the interaction Hamiltonian for spontaneous emission contains ( 
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     </math>), which is the vector potential part of what is claimed to be proportional to the gravitational potential 
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     </math> therefore bolstering the claim that gravitational fluctuations or gravitons cause spontaneous emission!</p>
    <p>Devices such as lasers depend on the stimulated emission of light. It should involve a dragging ambient graviton into the process of light amplification however, this topic deserves a better treatment than can be presented here.</p>
   </sec>
  </sec><sec id="s3">
   <title>
    <xref ref-type="bibr" rid="scirp.142321-"></xref>3. Methods</title>
   <p>Pauli representation quaternions are used here because they are more familiar to Physicists<sup>3</sup> while Hamilton quaternions, since the 1980’s, are used by computer scientists. “Pauli Algebra” has been used by a number of researchers see <xref ref-type="bibr" rid="scirp.142321-3">
     [3]
    </xref> for references, however the vector analysis notation rather than the matrix notation will be used for the most part, however, they are equivalent so that Pauli quaternion is a better and more accurate name.</p>
   <sec id="s3_1">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>3.1. Pauli Quaternion Multiplication Rule</title>
    <p>For two “real” Pauli quaternions 
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    <p>
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          </mi> 
          <mi>
            B 
          </mi> 
         </msub> 
         <msub> 
          <mover accent="true"> 
           <mi>
             r 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mi>
            A 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mover accent="true"> 
             <mi>
               r 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              A 
            </mi> 
           </msub> 
           <mo>
             × 
           </mo> 
           <msub> 
            <mover accent="true"> 
             <mi>
               r 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              B 
            </mi> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(1)</p>
    <p>Note that the dot product has a positive sign instead of the negative sign of real quaternions and the cross product becomes imaginary and has the opposite parity of the Hamilton representation (i.e. right-hand rule vs left hand rule).</p>
    <p>A “Complex” Pauli quaternion takes the form;</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
       <mtr> 
        <mtd> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            C 
          </mi> 
         </msub> 
         <mo>
           = 
         </mo> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mi>
              w 
            </mi> 
            <mi>
              R 
            </mi> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mi>
              x 
            </mi> 
            <mi>
              R 
            </mi> 
           </msub> 
           <msub> 
            <mover accent="true"> 
             <mi>
               σ 
             </mi> 
             <mo>
               ^ 
             </mo> 
            </mover> 
            <mn>
              1 
            </mn> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mi>
              y 
            </mi> 
            <mi>
              R 
            </mi> 
           </msub> 
           <msub> 
            <mover accent="true"> 
             <mi>
               σ 
             </mi> 
             <mo>
               ^ 
             </mo> 
            </mover> 
            <mn>
              2 
            </mn> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mi>
              z 
            </mi> 
            <mi>
              R 
            </mi> 
           </msub> 
           <msub> 
            <mover accent="true"> 
             <mi>
               σ 
             </mi> 
             <mo>
               ^ 
             </mo> 
            </mover> 
            <mn>
              3 
            </mn> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mi>
              w 
            </mi> 
            <mi>
              I 
            </mi> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mi>
              x 
            </mi> 
            <mi>
              I 
            </mi> 
           </msub> 
           <msub> 
            <mover accent="true"> 
             <mi>
               σ 
             </mi> 
             <mo>
               ^ 
             </mo> 
            </mover> 
            <mn>
              1 
            </mn> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mi>
              y 
            </mi> 
            <mi>
              I 
            </mi> 
           </msub> 
           <msub> 
            <mover accent="true"> 
             <mi>
               σ 
             </mi> 
             <mo>
               ^ 
             </mo> 
            </mover> 
            <mn>
              2 
            </mn> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mi>
              z 
            </mi> 
            <mi>
              I 
            </mi> 
           </msub> 
           <msub> 
            <mover accent="true"> 
             <mi>
               σ 
             </mi> 
             <mo>
               ^ 
             </mo> 
            </mover> 
            <mn>
              3 
            </mn> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mtd> 
       </mtr> 
       <mtr> 
        <mtd> 
         <mo>
           = 
         </mo> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mi>
              w 
            </mi> 
            <mi>
              R 
            </mi> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mover accent="true"> 
             <mi>
               r 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              R 
            </mi> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mi>
              w 
            </mi> 
            <mi>
              I 
            </mi> 
           </msub> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mover accent="true"> 
             <mi>
               r 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              I 
            </mi> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mtd> 
       </mtr> 
      </mtable> 
     </math>(2)</p>
    <p>the Pauli quaternion has a quasi real (on the left denoted with subscript R) and quasi imaginary part (on the right denoted with subscript I).</p>
    <p>This quaternion in terms of the Pauli matrices, is actually more convenient for the way that human physics has evolved; being usable for Maxwell’s equations, relativity and relativistic quantum mechanics. Although they could be presented in Hamilton Biquaternion form. For now rather than rewrite Physics text books of the last hundred years it is convenient to go along with the Pauli quaternion version of Physics or even the more awkward Pauli Algebra version where matrices are used instead of scalars and vectors.</p>
    <p>The full Pauli quaternion product is given by;</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mover accent="true"> 
         <mi>
           P 
         </mi> 
         <mo>
           ↔ 
         </mo> 
        </mover> 
        <mi>
          A 
        </mi> 
       </msub> 
       <msub> 
        <msup> 
         <mover accent="true"> 
          <mi>
            P 
          </mi> 
          <mo>
            ↔ 
          </mo> 
         </mover> 
         <mo>
           ′ 
         </mo> 
        </msup> 
        <mi>
          B 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            R 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            I 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <msup> 
           <mover accent="true"> 
            <mi>
              P 
            </mi> 
            <mo>
              ↔ 
            </mo> 
           </mover> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mi>
            R 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <msub> 
          <msup> 
           <mover accent="true"> 
            <mi>
              P 
            </mi> 
            <mo>
              ↔ 
            </mo> 
           </mover> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mi>
            I 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            R 
          </mi> 
         </msub> 
         <msub> 
          <msup> 
           <mover accent="true"> 
            <mi>
              P 
            </mi> 
            <mo>
              ↔ 
            </mo> 
           </mover> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mi>
            R 
          </mi> 
         </msub> 
         <mo>
           − 
         </mo> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            I 
          </mi> 
         </msub> 
         <msub> 
          <msup> 
           <mover accent="true"> 
            <mi>
              P 
            </mi> 
            <mo>
              ↔ 
            </mo> 
           </mover> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mi>
            I 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         + 
       </mo> 
       <mi>
         i 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            R 
          </mi> 
         </msub> 
         <msub> 
          <msup> 
           <mover accent="true"> 
            <mi>
              P 
            </mi> 
            <mo>
              ↔ 
            </mo> 
           </mover> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mi>
            I 
          </mi> 
         </msub> 
         <mo>
           + 
         </mo> 
         <msub> 
          <mover accent="true"> 
           <mi>
             P 
           </mi> 
           <mo>
             ↔ 
           </mo> 
          </mover> 
          <mi>
            I 
          </mi> 
         </msub> 
         <msub> 
          <msup> 
           <mover accent="true"> 
            <mi>
              P 
            </mi> 
            <mo>
              ↔ 
            </mo> 
           </mover> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mi>
            R 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(3)</p>
    <p>Pauli quaternions can be used for Maxwell’s Equations, Relativity and Relativistic quantum mechanics.</p>
   </sec>
   <sec id="s3_2">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>3.2. Pauli Quaternion Differential Operator</title>
    <p>The del operator in Pauli quaternion form is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         ≡ 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          1 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           x 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          2 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           y 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          3 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           z 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>(4)</p>
    <p>the quaternion differential operator.</p>
    <p>(Silberstein’s Operator <xref ref-type="bibr" rid="scirp.142321-7">
      [7]
     </xref> <xref ref-type="bibr" rid="scirp.142321-8">
      [8]
     </xref>) Pauli quaternion version is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mi>
          D 
        </mi> 
        <mo>
          ↔ 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mi>
           c 
         </mi> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          1 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           x 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          2 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           y 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          3 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           z 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(5)</p>
    <p>Its parity conjugate is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mover accent="true"> 
         <mi>
           D 
         </mi> 
         <mo>
           ↔ 
         </mo> 
        </mover> 
        <mtext>
          p 
        </mtext> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mi>
           c 
         </mi> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           t 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          1 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           x 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          2 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           y 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mover accent="true"> 
         <mi>
           σ 
         </mi> 
         <mo>
           ^ 
         </mo> 
        </mover> 
        <mn>
          3 
        </mn> 
       </msub> 
       <mfrac> 
        <mo>
          ∂ 
        </mo> 
        <mrow> 
         <mo>
           ∂ 
         </mo> 
         <mi>
           z 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math></p>
    <p>operation on the “real” part of a Pauli quaternion</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mi>
          D 
        </mi> 
        <mo>
          ↔ 
        </mo> 
       </mover> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           ⋅ 
         </mo> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           × 
         </mo> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(6)</p>
    <p>note</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msubsup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
          <mn>
            2 
          </mn> 
         </msubsup> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mo>
            ∇ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(7)</p>
    <p>This is the d’Alembert operator also known as the d’Alembertian it is a scalar operator used in a number of Partial differential Equations.</p>
   </sec>
   <sec id="s3_3">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>3.3. Pauli Algebra</title>
    <p>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>Pauli algebra is basically Pauli quaternions with 2 × 2 matrices rather than unit vectors. The standard Pauli matrix representations (although there are an infinite collection of the matrix representations) are:</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         I 
       </mi> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mtable columnalign="left"> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              1 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
          </mtr> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mn>
              1 
            </mn> 
           </mtd> 
          </mtr> 
         </mtable> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          σ 
        </mi> 
        <mn>
          1 
        </mn> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mtable columnalign="left"> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mn>
              1 
            </mn> 
           </mtd> 
          </mtr> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              1 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
          </mtr> 
         </mtable> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          σ 
        </mi> 
        <mn>
          2 
        </mn> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mtable columnalign="left"> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mrow> 
             <mo>
               − 
             </mo> 
             <mi>
               i 
             </mi> 
            </mrow> 
           </mtd> 
          </mtr> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mi>
              i 
            </mi> 
           </mtd> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
          </mtr> 
         </mtable> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          σ 
        </mi> 
        <mn>
          3 
        </mn> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mtable columnalign="left"> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              1 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
          </mtr> 
          <mtr columnalign="left"> 
           <mtd columnalign="left"> 
            <mn>
              0 
            </mn> 
           </mtd> 
           <mtd columnalign="left"> 
            <mrow> 
             <mo>
               − 
             </mo> 
             <mn>
               1 
             </mn> 
            </mrow> 
           </mtd> 
          </mtr> 
         </mtable> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(8)</p>
   </sec>
  </sec><sec id="s4">
   <title>
    <xref ref-type="bibr" rid="scirp.142321-"></xref>4. Pauli Quaternion Versions of Standard Physics Equations</title>
   <sec id="s4_1">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>4.1. Maxwell’s Equation(s)</title>
    <p>Maxwell’s four Equations can be written as one Pauli Quaternion Equation as follows:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mi>
            E 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mover accent="true"> 
          <mi>
            B 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           ρ 
         </mi> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mover accent="true"> 
           <mi>
             J 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mi>
            c 
          </mi> 
         </mfrac> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(9)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           ⋅ 
         </mo> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         , 
       </mo> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <msub> 
          <mi>
            A 
          </mi> 
          <mn>
            0 
          </mn> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         , 
       </mo> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mi>
         i 
       </mi> 
       <mover accent="true"> 
        <mi>
          B 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           i 
         </mi> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           × 
         </mo> 
         <mover accent="true"> 
          <mi>
            A 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math></p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> = Lorenz condition field, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
       <mi>
         E 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </math> = Electric field, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
       <mi>
         B 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </math> = Magnetic Induction field.</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          A 
        </mi> 
        <mn>
          0 
        </mn> 
       </msub> 
      </mrow> 
     </math> = Scalar Potential, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
       <mi>
         A 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </math> = Vector Potential.</p>
    <p>Conversely all four Maxwell’s equations can be extracted from Eq. (9).</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         ⋅ 
       </mo> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mi>
         ρ 
       </mi> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mo>
          ∂ 
        </mo> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mi>
         G 
       </mi> 
      </mrow> 
     </math> is the real scalar part Coulomb’s Law (modified) (9A)</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         ⋅ 
       </mo> 
       <mover accent="true"> 
        <mi>
          B 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> is the imaginary scalar part No Magnetic monopoles (9B)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         × 
       </mo> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mo>
          ∂ 
        </mo> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mover accent="true"> 
        <mi>
          B 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         − 
       </mo> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> is the real vector part Faraday’s Law (modified) (9C)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         × 
       </mo> 
       <mover accent="true"> 
        <mi>
          B 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         − 
       </mo> 
       <msub> 
        <mo>
          ∂ 
        </mo> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mfrac> 
        <mover accent="true"> 
         <mi>
           J 
         </mi> 
         <mo>
           → 
         </mo> 
        </mover> 
        <mi>
          c 
        </mi> 
       </mfrac> 
      </mrow> 
     </math> is the imaginary vector part Ampere’s Law (9D)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
       <mi>
         E 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </math> is the electric field and 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
       <mi>
         B 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </math> is the magnetic flux density or magnetic induction 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        ρ 
      </mi> 
     </math> is the charge density and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
       <mi>
         j 
       </mi> 
       <mo>
         → 
       </mo> 
      </mover> 
     </math> is the current density.</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> is the Lorenz condition field, typically it is set equal to zero however if 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mo>
          ∂ 
        </mo> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mi>
         G 
       </mi> 
       <mo>
         ≪ 
       </mo> 
       <mn>
         1 
       </mn> 
      </mrow> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mi>
         G 
       </mi> 
       <mo>
         ≪ 
       </mo> 
       <mn>
         1 
       </mn> 
      </mrow> 
     </math> then the standard Maxwell’s equations are obtained. The physical interpretation for 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math> which is more satisfying than the “gauge ambiguity” is that G is proportional to the Newtonian gravitational potential this will be demonstrated in the following:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mi>
            E 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mover accent="true"> 
          <mi>
            B 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           ρ 
         </mi> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mover accent="true"> 
           <mi>
             J 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mi>
            c 
          </mi> 
         </mfrac> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(10)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msubsup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
          <mn>
            2 
          </mn> 
         </msubsup> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mo>
            ∇ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           − 
         </mo> 
         <mover accent="true"> 
          <mi>
            E 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           + 
         </mo> 
         <mi>
           i 
         </mi> 
         <mover accent="true"> 
          <mi>
            B 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mo>
              ∂ 
            </mo> 
            <mn>
              0 
            </mn> 
           </msub> 
           <mi>
             ρ 
           </mi> 
           <mo>
             + 
           </mo> 
           <mover accent="true"> 
            <mo>
              ∇ 
            </mo> 
            <mo>
              → 
            </mo> 
           </mover> 
           <mo>
             ⋅ 
           </mo> 
           <mfrac> 
            <mover accent="true"> 
             <mi>
               J 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              c 
            </mi> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           + 
         </mo> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mo>
             ∇ 
           </mo> 
           <mi>
             ρ 
           </mi> 
           <mo>
             + 
           </mo> 
           <msub> 
            <mo>
              ∂ 
            </mo> 
            <mn>
              0 
            </mn> 
           </msub> 
           <mfrac> 
            <mover accent="true"> 
             <mi>
               J 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              c 
            </mi> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           + 
         </mo> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             i 
           </mi> 
           <mover accent="true"> 
            <mo>
              ∇ 
            </mo> 
            <mo>
              → 
            </mo> 
           </mover> 
           <mo>
             × 
           </mo> 
           <mfrac> 
            <mover accent="true"> 
             <mi>
               J 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              c 
            </mi> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
      </mrow> 
     </math>(11)</p>
    <p>from the continuity equation, the scalar part of the “Electromagnetic quaternion” wave equation is:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msubsup> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
          <mn>
            2 
          </mn> 
         </msubsup> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mo>
            ∇ 
          </mo> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         4 
       </mn> 
       <mi>
         π 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mo>
            ∂ 
          </mo> 
          <mn>
            0 
          </mn> 
         </msub> 
         <mi>
           ρ 
         </mi> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mo>
            ∇ 
          </mo> 
          <mo>
            → 
          </mo> 
         </mover> 
         <mo>
           ⋅ 
         </mo> 
         <mfrac> 
          <mover accent="true"> 
           <mi>
             J 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mi>
            c 
          </mi> 
         </mfrac> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>(12)</p>
    <p>The following is to demonstrate the plausibility of claiming that the scalar part of the electromagnetic field quaternion could be associated with the gravitational potential.</p>
    <p>There are a number of Solutions to Equation (12) the simplest is 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> which the Lorenz condition “gauge” assuming the continuity equation 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mo>
          ∂ 
        </mo> 
        <mn>
          0 
        </mn> 
       </msub> 
       <mi>
         ρ 
       </mi> 
       <mo>
         + 
       </mo> 
       <mover accent="true"> 
        <mo>
          ∇ 
        </mo> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mover accent="true"> 
         <mi>
           J 
         </mi> 
         <mo>
           → 
         </mo> 
        </mover> 
        <mi>
          c 
        </mi> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> is true, while time dependence and angular dependence are not present, Equation (12) becomes Laplace’s equation, 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mo>
          ∇ 
        </mo> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>, so that the simplest non-zero solution (ignoring added integration constants) for the static case in spherical coordinates for the Laplace equation is:</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mi>
          K 
        </mi> 
        <mi>
          r 
        </mi> 
       </mfrac> 
      </mrow> 
     </math>(13)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        K 
      </mi> 
     </math> is an unspecified integration constant. Choosing 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         K 
       </mi> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mi>
         κ 
       </mi> 
       <msub> 
        <msup> 
         <mi>
           G 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
        <mrow> 
         <mi>
           N 
         </mi> 
         <mi>
           e 
         </mi> 
         <mi>
           w 
         </mi> 
         <mi>
           t 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           n 
         </mi> 
        </mrow> 
       </msub> 
       <mi>
         M 
       </mi> 
       <mi>
         m 
       </mi> 
      </mrow> 
     </math> 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         κ 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            q 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mi>
           d 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> so that 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        κ 
      </mi> 
     </math> is an inverse dipole moment from dimensional analysis which yields a form of Newton’s Gravity potential equation.</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msup> 
          <mi>
            q 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mi>
           d 
         </mi> 
        </mrow> 
       </mfrac> 
       <mfrac> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <msub> 
          <msup> 
           <mi>
             G 
           </mi> 
           <mo>
             ′ 
           </mo> 
          </msup> 
          <mrow> 
           <mi>
             N 
           </mi> 
           <mi>
             e 
           </mi> 
           <mi>
             w 
           </mi> 
           <mi>
             t 
           </mi> 
           <mi>
             o 
           </mi> 
           <mi>
             n 
           </mi> 
          </mrow> 
         </msub> 
         <mi>
           M 
         </mi> 
         <mi>
           m 
         </mi> 
        </mrow> 
        <mi>
          r 
        </mi> 
       </mfrac> 
      </mrow> 
     </math>(14)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <msup> 
         <mi>
           G 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
        <mrow> 
         <mi>
           N 
         </mi> 
         <mi>
           e 
         </mi> 
         <mi>
           w 
         </mi> 
         <mi>
           t 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           n 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> is Newton’s gravitational constant. In the typical model with the charge 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        q 
      </mi> 
     </math> on a mass 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        m 
      </mi> 
     </math>, since the model is so simple, a charge 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mi>
         q 
       </mi> 
      </mrow> 
     </math> should appear on 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        M 
      </mi> 
     </math> and 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mi>
          q 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         d 
       </mi> 
       <mo>
         → 
       </mo> 
       <mo>
         − 
       </mo> 
       <mi>
         q 
       </mi> 
       <mi>
         r 
       </mi> 
      </mrow> 
     </math>.</p>
    <p>A Gravitational Traveling wave solution for Equation (12) in rectangular coordinates is</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          G 
        </mi> 
        <mn>
          0 
        </mn> 
       </msub> 
       <msup> 
        <mtext>
          e 
        </mtext> 
        <mrow> 
         <mi>
           i 
         </mi> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mover accent="true"> 
            <mi>
              k 
            </mi> 
            <mo>
              → 
            </mo> 
           </mover> 
           <mo>
             ⋅ 
           </mo> 
           <mover accent="true"> 
            <mi>
              r 
            </mi> 
            <mo>
              → 
            </mo> 
           </mover> 
           <mo>
             − 
           </mo> 
           <mi>
             w 
           </mi> 
           <mi>
             t 
           </mi> 
           <mo>
             + 
           </mo> 
           <mi>
             ϕ 
           </mi> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
       </msup> 
      </mrow> 
     </math>(15)</p>
    <p>Maxwell’s Equations in terms of Potentials are:</p>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable> 
       <mtr> 
        <mtd> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msubsup> 
            <mo>
              ∂ 
            </mo> 
            <mn>
              0 
            </mn> 
            <mn>
              2 
            </mn> 
           </msubsup> 
           <mo>
             − 
           </mo> 
           <msup> 
            <mo>
              ∇ 
            </mo> 
            <mn>
              2 
            </mn> 
           </msup> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mi>
              A 
            </mi> 
            <mn>
              0 
            </mn> 
           </msub> 
           <mo>
             + 
           </mo> 
           <mover accent="true"> 
            <mi>
              A 
            </mi> 
            <mo>
              → 
            </mo> 
           </mover> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           = 
         </mo> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mo>
              ∂ 
            </mo> 
            <mn>
              0 
            </mn> 
           </msub> 
           <mo>
             − 
           </mo> 
           <mover accent="true"> 
            <mo>
              ∇ 
            </mo> 
            <mo>
              → 
            </mo> 
           </mover> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <msub> 
              <mo>
                ∂ 
              </mo> 
              <mn>
                0 
              </mn> 
             </msub> 
             <msub> 
              <mi>
                A 
              </mi> 
              <mn>
                0 
              </mn> 
             </msub> 
             <mo>
               + 
             </mo> 
             <mover accent="true"> 
              <mo>
                ∇ 
              </mo> 
              <mo>
                → 
              </mo> 
             </mover> 
             <mo>
               ⋅ 
             </mo> 
             <mover accent="true"> 
              <mi>
                A 
              </mi> 
              <mo>
                → 
              </mo> 
             </mover> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
           <mo>
             + 
           </mo> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <msub> 
              <mo>
                ∂ 
              </mo> 
              <mn>
                0 
              </mn> 
             </msub> 
             <mover accent="true"> 
              <mi>
                A 
              </mi> 
              <mo>
                → 
              </mo> 
             </mover> 
             <mo>
               + 
             </mo> 
             <mover accent="true"> 
              <mo>
                ∇ 
              </mo> 
              <mo>
                → 
              </mo> 
             </mover> 
             <mtext>
               Φ 
             </mtext> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
           <mo>
             + 
           </mo> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mi>
               i 
             </mi> 
             <mover accent="true"> 
              <mo>
                ∇ 
              </mo> 
              <mo>
                → 
              </mo> 
             </mover> 
             <mo>
               × 
             </mo> 
             <mover accent="true"> 
              <mi>
                A 
              </mi> 
              <mo>
                → 
              </mo> 
             </mover> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mtd> 
       </mtr> 
       <mtr> 
        <mtd> 
         <mo>
           = 
         </mo> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msub> 
            <mo>
              ∂ 
            </mo> 
            <mn>
              0 
            </mn> 
           </msub> 
           <mo>
             − 
           </mo> 
           <mover accent="true"> 
            <mo>
              ∇ 
            </mo> 
            <mo>
              → 
            </mo> 
           </mover> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mo>
             − 
           </mo> 
           <mover accent="true"> 
            <mi>
              E 
            </mi> 
            <mo>
              → 
            </mo> 
           </mover> 
           <mo>
             + 
           </mo> 
           <mi>
             i 
           </mi> 
           <mover accent="true"> 
            <mi>
              B 
            </mi> 
            <mo>
              → 
            </mo> 
           </mover> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           = 
         </mo> 
         <mn>
           4 
         </mn> 
         <mi>
           π 
         </mi> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             ρ 
           </mi> 
           <mo>
             + 
           </mo> 
           <mfrac> 
            <mover accent="true"> 
             <mi>
               J 
             </mi> 
             <mo>
               → 
             </mo> 
            </mover> 
            <mi>
              c 
            </mi> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mtd> 
       </mtr> 
      </mtable> 
     </math>(16)</p>
   </sec>
   <sec id="s4_2">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>4.2. Relativity</title>
    <p>Relativity is an obvious application for quaternions. In addition to discovering the equivalent of Equation (9) without the 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
        G 
      </mi> 
     </math>, the Lorentz Transformation in quaternion form was discovered by both Ludwik Silberstein <xref ref-type="bibr" rid="scirp.142321-7">
      [7]
     </xref> <xref ref-type="bibr" rid="scirp.142321-8">
      [8]
     </xref> <xref ref-type="bibr" rid="scirp.142321-13">
      [13]
     </xref> and Arthur Conway <xref ref-type="bibr" rid="scirp.142321-6">
      [6]
     </xref> <xref ref-type="bibr" rid="scirp.142321-14">
      [14]
     </xref> independently, a minor dispute followed. See <xref ref-type="fig" rid="fig3">
      Figure 3
     </xref>.</p>
    <fig id="fig3" position="float">
     <label>Figure 3</label>
     <caption>
      <title>Figure 3. Silberstein and Conway applied complex quaternions (biquaternions) to Einstein’s 1905 special relativity independently. The choice of Grassmann’s tensor analysis by Minkowski and his friend Hilbert to generalize relativity followed by Einstein, caused the more natural biquaternions to be ignored. Silberstein went on to learn general relativity in both “Tensor” and quaternion form, claiming errors, in the standard general relativity which he pointed out to Einstein, and others, but was dismissed by the mainstream. Interestingly in May of 2021, Silberstein’s heirs (he died in 1948) sold a response letter from Einstein for 1.2 million U.S. dollars.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId219.jpeg?20250428034729" />
    </fig>
   </sec>
   <sec id="s4_3">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>4.3. Lorentz Transformation, Pauli Quaternion Form, Equivalent Reformulation of Silberstein’s Version</title>
    <p>
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           c 
         </mi> 
         <msup> 
          <mi>
            t 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mo>
           + 
         </mo> 
         <msup> 
          <mover accent="true"> 
           <mi>
             r 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mo>
            ′ 
          </mo> 
         </msup> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mi>
         γ 
       </mi> 
       <msqrt> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mover accent="true"> 
           <mi>
             v 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mi>
            c 
          </mi> 
         </mfrac> 
        </mrow> 
       </msqrt> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           c 
         </mi> 
         <mi>
           t 
         </mi> 
         <mo>
           + 
         </mo> 
         <mover accent="true"> 
          <mi>
            r 
          </mi> 
          <mo>
            → 
          </mo> 
         </mover> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <msqrt> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mover accent="true"> 
           <mi>
             v 
           </mi> 
           <mo>
             → 
           </mo> 
          </mover> 
          <mi>
            c 
          </mi> 
         </mfrac> 
        </mrow> 
       </msqrt> 
      </mrow> 
     </math>(17)</p>
    <p>where 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         γ 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             − 
           </mo> 
           <mfrac> 
            <mrow> 
             <msup> 
              <mi>
                v 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
            </mrow> 
            <mrow> 
             <msup> 
              <mi>
                c 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
            </mrow> 
           </mfrac> 
          </mrow> 
         </msqrt> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math>.</p>
   </sec>
  </sec><sec id="s5">
   <title>
    <xref ref-type="bibr" rid="scirp.142321-"></xref>5. Gravitons, Negative Mass</title>
   <sec id="s5_1">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>5.1. Negative Mass</title>
    <p>Recent experiments <xref ref-type="bibr" rid="scirp.142321-15">
      [15]
     </xref> have shown that antimatter i.e. anti-Hydrogen reacted to gravity the same as “normal” matter i.e. Hydrogen. That is, contrary to some speculation, antimatter doesn’t fall up! Alan Guth had previously suggested <xref ref-type="bibr" rid="scirp.142321-10">
      [10]
     </xref> that the gravitational field has negative mass. Agreeing with Guth, this presentation suggests that the gravitational potential field which is claimed to be proportional to the Lorenz condition field, has negative mass! This report also goes a step further, to say that gravitons exist, have negative mass, and curve space, which is not observed in the classical Newtonian region.</p>
   </sec>
   <sec id="s5_2">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>5.2. Photo-Gravitons</title>
    <p>Since the full Maxwell’s equations yield a wave equation for 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         G 
       </mi> 
       <mo>
         − 
       </mo> 
       <mover accent="true"> 
        <mi>
          E 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
       <mo>
         + 
       </mo> 
       <mover accent="true"> 
        <mi>
          B 
        </mi> 
        <mo>
          → 
        </mo> 
       </mover> 
      </mrow> 
     </math> the electromagnetic-gravitational fields, assigning a composite quanta, a “photo-graviton” to it seems appropriate. The photo graviton should have a net mass of zero and a spin of 2.</p>
   </sec>
   <sec id="s5_3">
    <title>
     <xref ref-type="bibr" rid="scirp.142321-"></xref>5.3. Explanation for Crookes Radiometer’s Counter-Intuitive Motion. Experimental Confirmation of Photo-Gravitons</title>
    <p>The zero mass photo-graviton explains the unresolved observations in the so-called Crookes radiometer. The standard explanation was disputed by Maxwell and later Einstein<sup>4</sup> The model presented in <xref ref-type="fig" rid="fig4">
      Figure 4
     </xref> and <xref ref-type="fig" rid="fig5">
      Figure 5
     </xref>. suggests that the reflected part of the Crookes Radiometer does not respond to the zero mass photo-graviton while the absorbing side, absorbs only the positive-mass electromagnetic part of the photo-graviton while the negative mass part of the photo-graviton becomes part of the gravitational field; causing the radiometer to spin in the observed direction. There have been some experiments that have changed the geometry of the Crookes radiometer, but the side that absorbs the most light still is pushed more, an experiment with an extreme vacuum should settle the question of the “radiometer” only working in a “partial vacuum”. So called reflective solar sails in miniature made to fit into a Crookes radiometer might clarify the issue, since they supposedly work by reflection, pitted against the absorbing “dark” side of the radiometer should get the same results that the radiometer gives now.</p>
    <fig id="fig4" position="float">
     <label>Figure 4</label>
     <caption>
      <title>Figure 4. Crookes Radiometer, this was initially thought to measure radiation pressure. The mirrored side would hypothetically reflect back light in an elastic collision type of interaction achieving double the impulse (momentum change) of the dark absorbing side which would be like an inelastic collision. Problem is the apparatus spins in the opposite direction. This has been mysterious since the 1870’s with great physicists like Maxwell and later Einstein unable to come up with a plausible answer They both rejected the standard explanation that air in the partial vacuum near the absorbing plane pushed the dark side. The photo-graviton model of <xref ref-type="fig" rid="fig1">
        Figure 1
       </xref> and <xref ref-type="fig" rid="fig2">
        Figure 2
       </xref>, suggests a simple resolution of the paradox.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId227.jpeg?20250428034731" />
    </fig>
    <fig id="fig5" position="float">
     <label>Figure 5</label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.142321-"></xref>Figure 5. The above depicts a simplified version of the Crookes radiometer. The circular white drawing represents the mirrored side of the Crookes radiometer vanes, while the darken circle represents the absorbing side of the vane. If “photons” have energy of hf then according to Einstein they have mass 

       <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
         <mfrac> 
   
          <mrow> 
    
           <mi>
            
     h
    
           </mi>
    
           <mi>
            
     f
    
           </mi>
   
          </mrow> 
   
          <mrow> 
    
           <msup> 
     
            <mi>
              c 
            </mi> 
     
            <mn>
              2 
            </mn> 
    
           </msup> 
   
          </mrow> 
  
         </mfrac> 
 
        </mrow>

       </math> momentum 

       <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
         <mfrac> 
   
          <mrow> 
    
           <mi>
            
     h
    
           </mi>
    
           <mi>
            
     f
    
           </mi>
   
          </mrow> 
   
          <mi>
           
    c
   
          </mi> 
  
         </mfrac> 
 
        </mrow>

       </math>. The standard physics explanation says that the mirrored side should be pushed twice as hard as the dark absorbing side but the vanes spin in the wrong direction! If a negative mass-momentum graviton rides along with the “photon” as the completed Maxwell’s equation suggests. Then the paradox is resolved.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId228.jpeg?20250428034732" />
    </fig>
   </sec>
  </sec><sec id="s6">
   <title>
    <xref ref-type="bibr" rid="scirp.142321-"></xref>6. Graviton Gas-Gravity Breaking Away from Matter</title>
   <p>It was discovered in the 1970’s that gravity waves exist <xref ref-type="bibr" rid="scirp.142321-16">
     [16]
    </xref> this has been confirmed by a number of other experiments. These gravity waves, break off from the masses that they are associated with and become free. If gravity waves are associated with the quanta known as gravitons then the gravitons are free from the masses that they were associated with. In quantum statistical mechanics there exist photon gas. It is conjectured that there should also be “graviton gas”, the gradient of the gas should be a force even if there is no mass present. This suggests a new model for gravity depicted in <xref ref-type="fig" rid="fig6">
     Figure 6
    </xref>.</p>
   <fig id="fig6" position="float">
    <label>Figure 6</label>
    <caption>
     <title>Figure 6. The above depicts 3 different conceptual models for the gravitational field 1) The lines of force model give the classical force and direction of the gravitational force. 2) The non Euclidean geometry model of Riemann used by Hilbert to complete the work of his deceased friend Minkowski, Einstein claimed he thought of it first and Hilbert yielded credit. 3) The graviton gas model, a quantum model that completes Maxwell’s quaternion equation while being a quantum gravity model with the gravitons being negative energy “bubbles” in what we would consider to be a vacuum, which would seem to curve space.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId233.jpeg?20250428034732" />
   </fig>
  </sec><sec id="s7">
   <title>
    <xref ref-type="bibr" rid="scirp.142321-"></xref>7. Model for “Dark Matter”</title>
   <p>Observations of frequency shifted light from the outer stars from our neighboring spiral galaxy, Andromeda, <xref ref-type="bibr" rid="scirp.142321-17">
     [17]
    </xref> reveal that the stars are moving way too fast to be explained by Newton’s and Einstein’s laws of gravity. Furthermore, similar observations from both Andromeda and the other neighboring spiral galaxy, Triangulum indicate that all three local group spiral galaxies are accelerating towards each other far too strongly for a standard gravity explanation <xref ref-type="bibr" rid="scirp.142321-18">
     [18]
    </xref>. Even more, the local group seems to be pulled toward the Virgo super cluster, again not explained with standard gravity. A standard hypothesis has been something called “dark matter”. A different hypothesis is presented here. To explain this, it is proposed that extra gravitons are created by the absorption of the electromagnetic part of photo gravitons by galactic interstellar dust in the inner parts of galaxies and the intergalactic dust between galaxies. It is proposed that the same thing that causes the Crookes radiometer motion also causes the dark matter “gravity” by flooding the outer reaches with free gravitons (<xref ref-type="fig" rid="fig7">
     Figure 7
    </xref>).</p>
   <fig id="fig7" position="float">
    <label>Figure 7</label>
    <caption>
     <title>Figure 7. The above is an image of a portion of the Milky Way galaxy. It was taken over the horizon and rotated 90 degrees. It shows the stars in the outer milky way galaxy and the vast dust formations in the inner galaxy. It also shows our neighbor galaxy; Andromeda. Vera Rubin and Kent Ford observed that outer stars in Andromeda were moving way too fast for either Newton’s or Einstein’s laws of gravity. If the graviton gas model is correct then the inner galactic dust should absorb electromagnetic radiation and flood the outer galaxy with free gravitons. (The inner galaxy dust acts like the absorbing sides in the Crookes Radiometer. This may explain dark matter.)</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181268-rId234.jpeg?20250428034733" />
   </fig>
  </sec><sec id="s8">
   <title>NOTES</title>
   <p><sup>1</sup>Quaternions are used by computer science for the navigation of aircraft, drones, and robots, also for 3D animation and gaming.</p>
   <p><sup>2</sup>Due to L. Lorenz, not to be confused with the more famous H.A. Lorentz as is done in all the editions of Jackson’s “Classical Electrodynamics” book <xref ref-type="bibr" rid="scirp.142321-9">
     [9]
    </xref>.</p>
   <p><sup>3</sup>In June of 1990, in my quest to learn more about quaternions, I went over to MIT and was told to ask Viki Weisskopf, I went to his office, the door was open I introduced myself, it turns out he didn’t know much about quaternions or that complex quaternions (biquaternions) were the same as Pauli matrices if each matrix was the same as a unit vector. In a way this was discouraging, because Viki knew Pauli and had even co-authored a paper <xref ref-type="bibr" rid="scirp.142321-12">
     [12]
    </xref> with him.</p>
   <p><sup>4</sup>See Wikipedia article on “Crookes Radiometer”.</p>
  </sec>
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