<?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">
    jamp
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of Applied Mathematics and Physics
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2327-4352
   </issn>
   <issn publication-format="print">
    2327-4379
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jamp.2025.133043
   </article-id>
   <article-id pub-id-type="publisher-id">
    jamp-141457
   </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>
    Special Theory of Relativity and Generalization of Relativistic Momentum
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Thalanayar
      </surname>
      <given-names>
       Santhanam
      </given-names>
     </name> 
     <xref ref-type="aff" rid="aff1"> 
      <sup>1</sup>
     </xref>
    </contrib>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Balu
      </surname>
      <given-names>
       Santhanam
      </given-names>
     </name> 
     <xref ref-type="aff" rid="aff2"> 
      <sup>2</sup>
     </xref>
    </contrib>
   </contrib-group> 
   <aff id="aff1">
    <addr-line>
     aDepartment of Physics, Saint Louis University, Saint Louis, Missouri, USA
    </addr-line> 
   </aff> 
   <aff id="aff2">
    <addr-line>
     aDepartment of ECE, University of New Mexico, Albuquerque, USA
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     13
    </day> 
    <month>
     03
    </month>
    <year>
     2025
    </year>
   </pub-date> 
   <volume>
    13
   </volume> 
   <issue>
    03
   </issue>
   <fpage>
    838
   </fpage>
   <lpage>
    843
   </lpage>
   <history>
    <date date-type="received">
     <day>
      10,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      21,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      21,
     </day>
     <month>
      March
     </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>
    Lorentz invariance admits more general definitions for the relativistic momen- tum. In this paper, we study some consequences that follow one such gene- ralization.
   </abstract>
   <kwd-group> 
    <kwd>
     Special Theory of Relativity
    </kwd> 
    <kwd>
      Relativistic Momentum
    </kwd> 
    <kwd>
      Lorentz Invariance
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <p>The cardinal principle of momentum conservation (linear and additive) was at stake under Lorentz transformations (nonlinear) if momentum is defined as Newton did via:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mi>
         N 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        m 
      </mi> 
      <mi>
        c 
      </mi> 
      <mi>
        β 
      </mi> 
      <mo>
        , 
      </mo> 
      <mtext>
          
      </mtext> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mo>
         / 
       </mo> 
       <mi>
         c 
       </mi> 
      </mrow> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(1)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       m 
     </mi> 
    </math> is the mass, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> is the velocity and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       c 
     </mi> 
    </math> is the speed of light. Einstein was left with two options, either to change Newton’s definition of momentum or to give up the conservation of momentum. He opted for the first to maintain Lorentz invariance, the stroke of genius, Einstein defined the relativistic momentum as <xref ref-type="bibr" rid="scirp.141457-1">
     [1]
    </xref>:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        m 
      </mi> 
      <mi>
        c 
      </mi> 
      <mi>
        γ 
      </mi> 
      <mi>
        β 
      </mi> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(2)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       γ 
     </mi> 
    </math> is the Lorentz factor,</p>
   <p>
    <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> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>(3)</p>
   <p>The rest of special theory of relativity is just a routine follow-up and standard kinetic energy turns out to be:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <mo>
          ∫ 
        </mo> 
        <mrow> 
         <mi>
           β 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <mtext>
           d 
         </mtext> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            p 
          </mi> 
         </mstyle> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          γ 
        </mi> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mi>
        m 
      </mi> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math>(4)</p>
   <p>The velocity independent term (the constant of integration) is 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        m 
      </mi> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> which is the rest energy 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
     </mrow> 
    </math> given by:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        m 
      </mi> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math>(5)</p>
   <p>Einstein defined the total energy as:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        E 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        m 
      </mi> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        + 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        γ 
      </mi> 
      <mi>
        m 
      </mi> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math>(6)</p>
   <p>This mass-energy equivalence is the crux and the most famous landmark of science almost synonymous with the name of Einstein <xref ref-type="bibr" rid="scirp.141457-2">
     [2]
    </xref>. Equations (2) and (6) lead to the fundamental equation:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mi>
             E 
           </mi> 
           <mrow> 
            <msub> 
             <mi>
               E 
             </mi> 
             <mi>
               o 
             </mi> 
            </msub> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        − 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              c 
            </mi> 
            <msub> 
             <mstyle mathvariant="bold" mathsize="normal"> 
              <mi>
                P 
              </mi> 
             </mstyle> 
             <mi>
               E 
             </mi> 
            </msub> 
           </mrow> 
           <mrow> 
            <msub> 
             <mi>
               E 
             </mi> 
             <mi>
               o 
             </mi> 
            </msub> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math>(7)</p>
   <p>Equation (7) is the result of the identity:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         γ 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        − 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            γ 
          </mi> 
          <mi>
            β 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math>(8)</p>
  </sec><sec id="s2">
   <title>2. New Relativistic Momentum</title>
   <p>As has been remarked on by many <xref ref-type="bibr" rid="scirp.141457-3">
     [3]
    </xref> <xref ref-type="bibr" rid="scirp.141457-4">
     [4]
    </xref>, Equation (7) was never used by Einstein in his papers or letters. In an earlier communication <xref ref-type="bibr" rid="scirp.141457-5">
     [5]
    </xref>, we showed that the identity in Equation (8) admits a more general definition of relativistic momentum given by:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mi>
         r 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        m 
      </mi> 
      <mi>
        c 
      </mi> 
      <msup> 
       <mrow> 
        <mi>
          tanh 
        </mi> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         β 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(9)</p>
   <p>which satisfies the Legendre equation:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mtext>
         d 
       </mtext> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          β 
        </mi> 
       </mrow> 
      </mfrac> 
      <mrow> 
       <mo>
         { 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              P 
            </mi> 
           </mstyle> 
           <mi>
             r 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            β 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         } 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(10)</p>
   <p>which has singular points at 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        ± 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>. If the main motive is to preserve the linear (and additive) momentum conservation under Lorentz transformation (non-linear), a natural choice will be to use the inverse hyperbolic definition for the relativistic momentum. In fact, the hyperbolic transformation <xref ref-type="bibr" rid="scirp.141457-6">
     [6]
    </xref> <xref ref-type="bibr" rid="scirp.141457-7">
     [7]
    </xref>:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        γ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        cosh 
      </mi> 
      <mi>
        ϕ 
      </mi> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        γ 
      </mi> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        sinh 
      </mi> 
      <mi>
        ϕ 
      </mi> 
     </mrow> 
    </math></p>
   <p>has been used in special theory for the invariant space-time 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           x 
         </mi> 
        </mstyle> 
        <mo>
          , 
        </mo> 
        <mi>
          c 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> distance:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         d 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          x 
        </mi> 
       </mstyle> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        − 
      </mo> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math></p>
   <p>We have chosen the hyperbolic angle 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ϕ 
     </mi> 
    </math> as:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ϕ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           P 
         </mi> 
         <mi>
           r 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mi>
          m 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math></p>
   <p>It follows that:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mi>
         r 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          m 
        </mi> 
        <mi>
          c 
        </mi> 
        <mtext>
          d 
        </mtext> 
        <mi>
          β 
        </mi> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math>(11)</p>
   <p>The expression for kinetic energy then becomes:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        T 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <mo>
          ∫ 
        </mo> 
        <mrow> 
         <mi>
           β 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <mtext>
           d 
         </mtext> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             P 
           </mi> 
          </mstyle> 
          <mi>
            r 
          </mi> 
         </msub> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <mo>
          ∫ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <mi>
             β 
           </mi> 
           <mo>
             ⋅ 
           </mo> 
           <mtext>
             d 
           </mtext> 
           <mi>
             β 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             − 
           </mo> 
           <msup> 
            <mi>
              β 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mi>
        ln 
      </mi> 
      <mi>
        γ 
      </mi> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(12)</p>
   <p>where we have chosen the constant of integration to be 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        m 
      </mi> 
      <mi>
        c 
      </mi> 
     </mrow> 
    </math>. Notice that the expression for the Lorentz factor becomes:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        γ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           E 
         </mi> 
         <mi>
           o 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mi>
           E 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           E 
         </mi> 
         <mi>
           o 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <msub> 
               <mstyle mathvariant="bold" mathsize="normal"> 
                <mi>
                  P 
                </mi> 
               </mstyle> 
               <mi>
                 E 
               </mi> 
              </msub> 
             </mrow> 
             <mrow> 
              <mi>
                m 
              </mi> 
              <mi>
                c 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <mtext>
        cosh 
      </mtext> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              P 
            </mi> 
           </mstyle> 
           <mi>
             r 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <mi>
            m 
          </mi> 
          <mi>
            c 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math>(13)</p>
   <p>Therefore,</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
      <mtr> 
       <mtd> 
        <mfrac> 
         <mi>
           E 
         </mi> 
         <mrow> 
          <msub> 
           <mi>
             E 
           </mi> 
           <mi>
             o 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msub> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 P 
               </mi> 
              </mstyle> 
              <mi>
                E 
              </mi> 
             </msub> 
            </mrow> 
            <mrow> 
             <mi>
               m 
             </mi> 
             <mi>
               c 
             </mi> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           8 
         </mn> 
        </mfrac> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msub> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 P 
               </mi> 
              </mstyle> 
              <mi>
                E 
              </mi> 
             </msub> 
            </mrow> 
            <mrow> 
             <mi>
               m 
             </mi> 
             <mi>
               c 
             </mi> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mn>
           4 
         </mn> 
        </msup> 
        <mo>
          + 
        </mo> 
        <mo>
          ⋯ 
        </mo> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          = 
        </mo> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msub> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 P 
               </mi> 
              </mstyle> 
              <mi>
                r 
              </mi> 
             </msub> 
            </mrow> 
            <mrow> 
             <mi>
               m 
             </mi> 
             <mi>
               c 
             </mi> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            24 
          </mn> 
         </mrow> 
        </mfrac> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msub> 
              <mstyle mathvariant="bold" mathsize="normal"> 
               <mi>
                 P 
               </mi> 
              </mstyle> 
              <mi>
                r 
              </mi> 
             </msub> 
            </mrow> 
            <mrow> 
             <mi>
               m 
             </mi> 
             <mi>
               c 
             </mi> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mn>
           4 
         </mn> 
        </msup> 
        <mo>
          + 
        </mo> 
        <mo>
          ⋯ 
        </mo> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math>(14)</p>
   <p>The existing body of experimental evidence overwhelmingly supporting Einstein’s formulation of special relativity rests on the mass-energy equivalence in Equation (7) and this still remains unchanged with the proposed generalization in Equation (9). The real test will be the relation between relativistic momentum and velocity depicted in <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref>.</p>
   <p>We remark that there is no change in Einstein’s Equation (6) and thus all results related to the Lorentz factor 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       γ 
     </mi> 
    </math> (since they are based on 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math>). While the velocity dependence on E (the measured ones) remains the same, the critical difference is in the dependence of E on the momentum and the dependence of relativistic momentum on velocity:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        E 
      </mi> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          γ 
        </mi> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         o 
       </mi> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msup> 
         <mtext>
           e 
         </mtext> 
         <mrow> 
          <mfrac> 
           <mi>
             T 
           </mi> 
           <mrow> 
            <msub> 
             <mi>
               E 
             </mi> 
             <mi>
               o 
             </mi> 
            </msub> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msup> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>(15)</p>
   <p>The change from 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mi>
         E 
       </mi> 
      </msub> 
     </mrow> 
    </math> to 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mi>
         r 
       </mi> 
      </msub> 
     </mrow> 
    </math> then leads to the expression for the force:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         F 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            P 
          </mi> 
         </mstyle> 
         <mi>
           r 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          m 
        </mi> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           a 
         </mi> 
        </mstyle> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mi>
         γ 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mi>
        m 
      </mi> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         a 
       </mi> 
      </mstyle> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(16)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        a 
      </mi> 
     </mstyle> 
    </math> is the acceleration. Notice that for small momentum (non-relativistic): 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mi>
         r 
       </mi> 
      </msub> 
     </mrow> 
    </math>. Equation (7) now becomes only approximate Dirac’s equation <xref ref-type="bibr" rid="scirp.141457-8">
     [8]
    </xref> which is based on the quadratic equation in Equation (7) now becomes only approximate in terms of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mi>
         r 
       </mi> 
      </msub> 
     </mrow> 
    </math> but is still quadratic in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
     </mrow> 
    </math>, but 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        m 
      </mi> 
      <mi>
        c 
      </mi> 
      <mi>
        sinh 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             P 
           </mi> 
           <mi>
             r 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <mi>
            m 
          </mi> 
          <mi>
            c 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> The relativistic correction to the kinetic energy which is (negative) is given by <xref ref-type="bibr" rid="scirp.141457-9">
     [9]
    </xref>:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        Δ 
      </mtext> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mn>
         8 
       </mn> 
      </mfrac> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           P 
         </mi> 
         <mi>
           E 
         </mi> 
         <mn>
           4 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           m 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        , 
      </mo> 
     </mrow> 
    </math>(17)</p>
   <p>and according to the usual description, now becomes (positive):</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        Δ 
      </mtext> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         r 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          24 
        </mn> 
       </mrow> 
      </mfrac> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           P 
         </mi> 
         <mi>
           r 
         </mi> 
         <mn>
           4 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           m 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math>(18)</p>
   <p>This change has a profound impact on the atomic spectrum. The relativistic</p>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>Figure 1. (a) comparison of different relativistic momentum expressions versus velocity and (b) comparison of different energy expressions versus momentum.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724060-rId97.jpeg?20250324024222" />
   </fig>
   <p>correction Equation (17) along with the correction due to spin-orbit interaction, in standard treatments, would imply that the fine-structure spectrum rests only on the total spin and not individually on orbital angular momentum or the spin. For instance, this would imply that the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        2 
      </mn> 
      <msub> 
       <mi>
         p 
       </mi> 
       <mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        2 
      </mn> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> states of the hydrogen atom are degenerate (apart from Lamb’s shift) <xref ref-type="bibr" rid="scirp.141457-10">
     [10]
    </xref>. The relativistic correction in Equation (18) along with the correction due to spin-orbit interaction will lift this observed degeneracy of these states. All this means is that in addition to relativistic and spin-orbit corrections there must be some other sources of correction in order to restore this observed degeneracy. We cannot use Dirac’s equation for this purpose since it is based on Equation (7). Dirac matrices are indeed built from Pauli spin matrices.</p>
  </sec><sec id="s3">
   <title>3. Summary</title>
   <p>We have shown that Lorentz invariance admits a more general definition of relativistic momentum that alters the relationship between energy and momentum. Since most of the measurements are based on the measurement of velocity, they still hold with the new definition of relativistic momentum. Since 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          m 
        </mi> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> is still 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       γ 
     </mi> 
    </math>, there is no change in the kinematics. The main change is in the dynamics.</p>
  </sec><sec id="s4">
   <title>Acknowledgements</title>
   <p>We thank the Professors, Hans Ohanian, John Fields, and R. Jaganathan for their strong criticisms of the generalization to relativistic momentum.</p>
  </sec>
 </body><back>
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