<?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.2024.103060
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-134472
   </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 Gravitational Interaction between Moving Mass Particles Explained by the Theory of Informatons
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Antoine
      </surname>
      <given-names>
       Acke
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aRetired Professor Kaho Sint-Lieven, Now Faculty of Engineering Technology, KU Leuven, Ghent Campus, Gent, Belgium
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     06
    </day> 
    <month>
     06
    </month>
    <year>
     2024
    </year>
   </pub-date> 
   <volume>
    10
   </volume> 
   <issue>
    03
   </issue>
   <fpage>
    986
   </fpage>
   <lpage>
    1002
   </lpage>
   <history>
    <date date-type="received">
     <day>
      21,
     </day>
     <month>
      March
     </month>
     <year>
      2024
     </year>
    </date>
    <date date-type="published">
     <day>
      9,
     </day>
     <month>
      March
     </month>
     <year>
      2024
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      9,
     </day>
     <month>
      July
     </month>
     <year>
      2024
     </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>
    In the article “Newtons Law of Universal Gravitation Explained by the Theory of Informatons” the gravitational interaction between mass particles at rest has been explained by the hypothesis that g-information carried by informatons is the substance of the medium that the interaction in question makes possible. It has been showed that, on the macroscopic level, that medium—the “gravitational field”—manifests itself as the vector field 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal">
        <mi>
         E
        </mi>
       </mstyle> 
       <mi>
        g
       </mi> 
      </msub> 
     </mrow> 
    </math> . In this article we will deduce from the postulate of the emission of informatons, that the informatons emitted by a moving mass particle carry not only information about the position (g-information) but also about the velocity (“β-information”) of their emitter. It follows that the gravitational field of a moving mass particle is a dual entity always having a field- and an induction-component (
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal">
        <mi>
         E
        </mi>
       </mstyle> 
       <mi>
        g
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal">
        <mi>
         B
        </mi>
       </mstyle> 
       <mi>
        g
       </mi> 
      </msub> 
     </mrow> 
    </math> ) simultaneously created by their common sources: time-variable masses and mass flows and that the gravitational interaction is the effect of the fact that an object in a gravitational field always tends to become “blind” for that field by accelerating according to a Lorentz-like law.
   </abstract>
   <kwd-group> 
    <kwd>
     Gravity
    </kwd> 
    <kwd>
      Gravitational Field
    </kwd> 
    <kwd>
      Gravitational Interaction
    </kwd> 
    <kwd>
      Informatons
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <p>The theory of informatons <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.134472-3">
     [3]
    </xref> starts from the hypothesis that a material object at rest manifests its presence in space by continuously emitting “informatons”, granular entities carrying “information” about the position of the emitter. The emission of informatons by a material object anchored in an inertial reference frame (IRF) O, is governed by the “postulate of the emission of informatons”:</p>
   <p>A. The emission of informatons by a particle at rest is governed by the following rules:</p>
   <p>1. The emission is uniform in all directions of space, and the informatons diverge with the speed of light (c = 3 × 10<sup>8</sup> m/s) along radial trajectories relative to the position of the emitter.</p>
   <p>2. 
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          N 
        </mi> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>, the rate at which a particle emits informatons<sup>1</sup>, is time independent and proportional to the rest mass m<sub>0</sub> of the emitter. So there is a constant K so that:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math></p>
   <p>3. The constant K is equal to the ratio of the square of the speed of light (c) to the Planck constant (h):</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        K 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mi>
         h 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        1.36 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          50 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mtext>
          kg 
        </mtext> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math></p>
   <p>B. We call the essential attribute of an informaton its g-index. The g-index of an informaton refers to information about the position of its emitter and equals the elementary quantity of g-information. It is represented by a vectoral quantity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>:</p>
   <p>1. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> points to the position of the emitter.</p>
   <p>2. The elementary quantity of g-information is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mi>
          K 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        6.18 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          60 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mtext>
         m 
       </mtext> 
       <mn>
         3 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math></p>
   <p>where 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         η 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        1.19 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mn>
         9 
       </mn> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        kg 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         m 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, G being the gravitational constant.</p>
   <p>In the article “Newtons law of universal gravitation explained by the theory of informatons” <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref> it is shown that this postulate leads to the conclusion that the gravitational field—the medium that the gravitational interaction between objects makes possible—is a cloud of “g-information”, i.e. information carried by informatons. At the macroscopic level it is, in the case of an object at rest, completely defined by the vector field 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>. E<sub>g</sub>, the magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> at any point P, is the density of the flow of g-information at that point (the rate per unit area at which g-information at P flows through an elementary surface perpendicular to the direction of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>).</p>
   <p>In this article (the follow-up article of <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref>) we will deduce from the postulate of the emission of informatons that the gravitational field of a moving mass particle is a dual entity always having a field- and an induction-component ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>) simultaneously created by their common sources: time-variable masses and mass flows. At an arbitrary point P the magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the density of the flow of g-information at that point and the magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the density of the cloud of β-information at P. β-information is the information that informatons carry regarding the velocity of their source. This implies that the gravitational field of a moving object besides g-information, i.e. this is information about the position of the emitter, contains also information about its velocity.</p>
   <p>We will also show that the gravitational interaction is the effect of the fact that an object in a gravitational field always tends to become “blind” for that field by accelerating according to a Lorentz-like law.</p>
  </sec><sec id="s2">
   <title>2. Rest Mass and Relativistic Mass</title>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>Figure 1. A mass particle m<sub>0</sub> moving with constant velocity relative to an IRF O.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181089-rId47.jpeg?20240712014728" />
   </fig>
   <p>In <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref>, we consider a mass point with rest mass m<sub>0</sub> that moves with constant velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         z 
       </mi> 
      </msub> 
     </mrow> 
    </math> along the Z-axis of an IRF O. At the moment t = 0, it passes through the origin O and at the moment t = t through the point P<sub>1</sub>.</p>
   <p>We extend rule A.1 of the postulate of the emission of information to a mass point that is moving relative to an IRF O:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          N 
        </mi> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>, the rate at which a particle emits informatons, is independent of the </p>
   <p>motion of the emitter and proportional to its rest mass m<sub>0</sub>. So there is a constant K so that:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math></p>
   <p>That implies that, if the time is read on a standard clock anchored in O, dN, the number of informatons that during the time interval dt is emitted by a—whether or not moving—point mass, is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <mi>
        N 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math></p>
   <p>To emit dN informatons relative to O'—the “proper IRF” of the mass particle (i.e. the IRF anchored to the moving particle)—it takes a time interval dt'. The Lorentz transformation relation between dt and dt' is <xref ref-type="bibr" rid="scirp.134472-4">
     [4]
    </xref>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <mi>
        t 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msup> 
         <mi>
           t 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>where 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         v 
       </mi> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> is the dimensionless speed of the particle.</p>
   <p>So:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <mi>
        N 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        t 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msup> 
         <mi>
           t 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mover accent="true"> 
        <mi>
          N 
        </mi> 
        <mo>
          ˙ 
        </mo> 
       </mover> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mrow> 
    </math></p>
   <p>and:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          N 
        </mi> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msup> 
         <mi>
           t 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mover accent="true"> 
        <mi>
          N 
        </mi> 
        <mo>
          ˙ 
        </mo> 
       </mover> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        m 
      </mi> 
     </mrow> 
    </math></p>
   <p>with</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        m 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>the “relativistic mass” of the particle.</p>
   <p>We conclude:</p>
   <p>The rate at which a mass particle moving with constant velocity relative to an IRF O emits informatons is determined by its “rest mass”. Relative to its proper IRF O’ it is determined by its “relativistic mass”. In other words: the rest mass of a particle is representative for the rate at which it emits informatons relative to the IRF of the observer and its relative mass for the emission rate relative to its proper IRF.</p>
  </sec><sec id="s3">
   <title>3. The g-Field of a Mass Particle Moving with Constant Velocity</title>
   <p>In <xref ref-type="fig" rid="fig2(a)">
     Figure 2(a)
    </xref>, we consider a particle with rest mass m<sub>0</sub> that is moving with constant velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         z 
       </mi> 
      </msub> 
     </mrow> 
    </math> along the Z-axis of an IRF O. At the moment t = 0, it passes through the origin O and at the moment t = t through the point P<sub>1</sub>. It is evident that:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        O 
      </mi> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           P 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math></p>
   <p>P is an arbitrary fixed point in O with space coordinates (x, y, z). Its position relative to the moving particle is determined by the time dependent position vector 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         r 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         P 
       </mi> 
      </mstyle> 
     </mrow> 
    </math>.</p>
   <p>We introduce the IRF O' (<xref ref-type="fig" rid="fig2(b)">
     Figure 2(b)
    </xref>), the proper IRF of the particle, whose origin is anchored to the moving particle and we assume that t = t' = 0 when it passes through O.</p>
   <p>Relative to O' (<xref ref-type="fig" rid="fig1(b)">
     Figure 1(b)
    </xref>), the position of P is determined by the time dependent position vector 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <msup> 
        <mi>
          O 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         P 
       </mi> 
      </mstyle> 
     </mrow> 
    </math> and in O' the space coordinates of P are (x', y', z').</p>
   <p>The particle is at rest in O'. So 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>, its g-field relative to O', is completely defined by the vectoral quantity <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             t 
           </mi> 
           <mo>
             ′ 
           </mo> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
      </msub> 
     </mrow> 
    </math></p>
   <fig id="fig2" position="float">
    <label>Figure 2</label>
    <caption>
     <title>Figure 2. The g-field of a mass particle moving with constant velocity relative to an IRF O.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181089-rId76.jpeg?20240712014728" />
   </fig>
   <p>dN is the number of informatons that during the time interval dt' pass through an elementary surface dS' that in O' is perpendicular to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        c 
      </mi> 
     </mstyle> 
    </math>, the velocity of these informatons.</p>
   <p>Thus 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is—relative to O'—the density of the g-information flow at P and the magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the rate per unit area at which—relative to O'—g-information flows through an elementary surface dS' that at P is perpendicular to the velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        c 
      </mi> 
     </mstyle> 
    </math> of the informatons that carry that information.</p>
   <p>The components of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> in O', are:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          E 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <msup> 
         <mi>
           x 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             t 
           </mi> 
           <mo>
             ′ 
           </mo> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         x 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          E 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <msup> 
         <mi>
           y 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             t 
           </mi> 
           <mo>
             ′ 
           </mo> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         y 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          E 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <msup> 
         <mi>
           z 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             t 
           </mi> 
           <mo>
             ′ 
           </mo> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         z 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mrow> 
    </math></p>
   <p>They determine at P the densities of the flows of g-information respectively through a surface element dy'∙dz' perpendicular to the X'-axis, through a surface element dz'∙dx' perpendicular to the Y'-axis and through a surface element dx'∙dy' perpendicular to the Z'-axis.</p>
   <p>Thus, the amount of information that the particle during the time-interval dt' sends through the different surface elements at P are:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          E 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <msup> 
         <mi>
           x 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         y 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         z 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             t 
           </mi> 
           <mo>
             ′ 
           </mo> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           x 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <msup> 
          <mi>
            r 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         y 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         z 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mrow> 
    </math></p>
   <p>
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           y 
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        ⋅ 
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        d 
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            d 
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            r 
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            ′ 
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           3 
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        ⋅ 
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    </math></p>
   <p>
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        ⋅ 
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       </mi> 
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         ′ 
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        = 
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        − 
      </mo> 
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       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
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            N 
          </mi> 
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            d 
          </mtext> 
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           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         x 
       </mi> 
       <mo>
         ′ 
       </mo> 
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        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
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         y 
       </mi> 
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         ′ 
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        ⋅ 
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        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mrow> 
    </math></p>
   <p>Informatons propagate at the speed of light that—in free space—has the same value in all IRFs. That implies that, by applicating the Lorenz transformation equations, the amount of g-information that during the time interval dt flows through the surface element dS that in O is perpendicular to the velocity of the informatons at P can be derived from the quantity that during the corresponding time interval dt' flows through the corresponding surface element dS' in O'.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
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       </mi> 
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        = 
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      </mi> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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       <mi>
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        = 
      </mo> 
      <mi>
        y 
      </mi> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         z 
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        = 
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        </mo> 
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          v 
        </mi> 
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          ⋅ 
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        <mi>
          t 
        </mi> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          z 
        </mi> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <msub> 
           <mi>
             P 
           </mi> 
           <mn>
             1 
           </mn> 
          </msub> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>The elementary time intervals by: 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mo>
         ′ 
       </mo> 
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      <mo>
        = 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        t 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         r 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mi>
        r 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mrow> 
            <mi>
              sin 
            </mi> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mi>
            θ 
          </mi> 
         </mrow> 
        </msqrt> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>So relative to O, the rates at which the moving particle sends g-information in the positive direction through the surface elements dy∙dz, dz∙dx and dx∙dy at P are:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
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            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
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         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        x 
      </mi> 
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        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        y 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        z 
      </mi> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        − 
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      <mfrac> 
       <mrow> 
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         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
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         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
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        <mi>
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        </mi> 
        <mo>
          ⋅ 
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        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
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       <mrow> 
        <mn>
          1 
        </mn> 
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          − 
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         <mi>
           β 
         </mi> 
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           2 
         </mn> 
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       </mrow> 
       <mrow> 
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              1 
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              − 
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               β 
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               2 
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              ⋅ 
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              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
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            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
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        y 
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        ⋅ 
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        d 
      </mtext> 
      <mi>
        x 
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        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        z 
      </mi> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
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         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            N 
          </mi> 
         </mrow> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           s 
         </mi> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          z 
        </mi> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <msub> 
           <mi>
             P 
           </mi> 
           <mn>
             1 
           </mn> 
          </msub> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        x 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        z 
      </mi> 
     </mrow> 
    </math></p>
   <p>By definition, the densities at P of the flows of g-information in the direction of the X-, the Y- and the Z-axis are the components of the g-field caused by the moving particle m<sub>0</sub> at P in O.</p>
   <p>Taking into account that</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          N 
        </mi> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mi>
          K 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>We obtain:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mi>
          x 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        x 
      </mi> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mi>
          y 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        y 
      </mi> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mi>
          z 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          z 
        </mi> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <msub> 
           <mi>
             P 
           </mi> 
           <mn>
             1 
           </mn> 
          </msub> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>From which it follows that the g-field caused by the particle at the fixed point P is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         r 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         r 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>We conclude:</p>
   <p>A particle describing a uniform rectilinear movement relative to an inertial reference frame O, creates in the space linked to that frame a time dependent gravitational field. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>, the g-field at an arbitrary point P, points at any time to the position of the mass at that moment<sup>2</sup> and its magnitude is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (1)</p>
   <p>The magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> at an arbitrary point P in the g-field of m<sub>0</sub> is the rate per unit area at which g-information at that point flows—relative to O—through an elementary surface perpendicular to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>With N the density of the flow of informatons at P (the number of informatons that per unit time and per unit area crosses an elementary surface perpendicular to the direction of their movement), 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> can be expressed as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        N 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>Because the rate at which g-information that escapes from an enclosed space is completely determined by the rate at which g-information is generated inside that space (conservation of g-information):</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <mo>
          ∯ 
        </mo> 
        <mrow> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             E 
           </mi> 
          </mstyle> 
          <mi>
            g 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mtext>
           d 
         </mtext> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            S 
          </mi> 
         </mstyle> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>If the speed of the mass particle is much smaller than the speed of light, the expression (1) reduces to that valid in the case of a mass particle at rest. This non-relativistic result could directly be obtained if one assumes that the displacement of the mass particle during the time interval that the informatons need to move from the emitter to P can be neglected compared to the distance they travel during that period.</p>
  </sec><sec id="s4">
   <title>4. The Emission of Informatons by a Mass Particle Moving with Constant Velocity</title>
   <fig id="fig3" position="float">
    <label>Figure 3</label>
    <caption>
     <title>Figure 3. An informaton emitted by a mass particle moving with constant velocity.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181089-rId143.jpeg?20240712014728" />
   </fig>
   <p>In <xref ref-type="fig" rid="fig3">
     Figure 3
    </xref> we consider a mass particle with rest mass m<sub>0</sub> that is moving with constant velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> along the Z-axis of an inertial reference frame O. Its instantaneous position (at the arbitrary moment t) is P<sub>1</sub>. The position of P, an arbitrary fixed point in space, is defined by the vector 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         r 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          P 
        </mi> 
       </mstyle> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         P 
       </mi> 
      </mstyle> 
     </mrow> 
    </math>. This position vector 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        r 
      </mi> 
     </mstyle> 
    </math>—just like the distance r and the angle θ—is time dependent because the position of P<sub>1</sub> is constantly changing.</p>
   <p>The informatons that—with the speed of light—at the moment t are passing near P, are emitted when m<sub>0</sub> was at P<sub>0</sub>. Bridging the distance 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mi>
        P 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         r 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> took the time interval 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        t 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           r 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math>.</p>
   <p>During their rush from P<sub>0</sub> to P their emitter, the particle, moved from P<sub>0</sub> to P<sub>1</sub>: 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math>.</p>
   <p>1. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        c 
      </mi> 
     </mstyle> 
    </math>, the velocity of the informatons, points in the direction of their movement, thus along the radius P<sub>0</sub>P;</p>
   <p>2. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>, their g-index, points to P<sub>1</sub>, the position of m<sub>0</sub> at the moment t. This is an implication of rule B.1 of the postulate of the emission of informatons, confirmed by the conclusion of §3.</p>
   <p>The lines carrying 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        c 
      </mi> 
     </mstyle> 
    </math> form an angle Δθ. We call this angle—that is characteristic for the speed of the mass particle—the “characteristic angle” or the “characteristic deviation”. The quantity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          Δ 
        </mi> 
        <mi>
          θ 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>, referring to the speed of its emitter, is called the “characteristic g-information” or the “β-information” of an informaton.</p>
   <p>We conclude that an informaton emitted by a moving particle, transports information referring to the velocity of that particle. This information is represented by its “gravitational characteristic vector” or its “β-index” 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
     </mrow> 
    </math> that is defined as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           c 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>In the case of <xref ref-type="fig" rid="fig3">
     Figure 3
    </xref> the β-indices have the orientation of the positive X-axis.</p>
   <p>Applying the sine-rule to the triangle P<sub>0</sub>P<sub>1</sub>P, we obtain:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mi>
          sin 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <mi>
            θ 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          v 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          Δ 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          sin 
        </mi> 
        <mi>
          θ 
        </mi> 
       </mrow> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          Δ 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>From which it follows:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mi>
         v 
       </mi> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        θ 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        β 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        θ 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         s 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         β 
       </mi> 
       <mo>
         ⊥ 
       </mo> 
      </msub> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         β 
       </mi> 
       <mo>
         ⊥ 
       </mo> 
      </msub> 
     </mrow> 
    </math> is the component of the dimensionless velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> perpendicular to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>Taking into account the orientation of the different vectors, the β-index of an informaton emitted by a point mass moving with constant velocity, can also be expressed as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math></p>
  </sec><sec id="s5">
   <title>5. The Gravitational Induction (or the g-Induction) of a Mass Particle Moving with Constant Velocity</title>
   <p>We consider again the situation of <xref ref-type="fig" rid="fig3">
     Figure 3
    </xref>. All informatons in dV—the volume element at P—carry both g-information and β-information. The β-information refers to the velocity of the emitting particle and is represented by the β-indices 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
     </mrow> 
    </math>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           c 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>If n is the density at P of the cloud of informatons (number of informatons per unit volume) at the moment t, the amount of β-information in dV is determined by the magnitude of the vector:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        V 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           c 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        V 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        V 
      </mi> 
     </mrow> 
    </math></p>
   <p>So the density of the β-information (characteristic information per unit volume) at P is determined by:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           c 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>We call this (time dependent) vectoral quantity—that will be represented by 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> (s<sup>−</sup><sup>1</sup>)—the “gravitational induction” or the “g-induction” at P<sup>3</sup>. Its magnitude 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> determines the density of the β-information at P and its orientation determines the orientation of the β-indices 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
     </mrow> 
    </math> of the informatons passing near that point.</p>
   <p>So, the g-induction caused by the moving particle with res mass m<sub>0</sub> (<xref ref-type="fig" rid="fig3">
     Figure 3
    </xref>) at P is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        × 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          n 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>N—the density of the flow of informatons at P (the rate per unit area at which the informatons cross an elementary surface perpendicular to the direction of their movement)—and n—the density of the cloud of informatons at P (number of informatons per unit volume)—are connected by the relation:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        n 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         N 
       </mi> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>With 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        N 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>, we can express the gravitational induction at P as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        × 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          N 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            s 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>Taking the result of §3 into account, we find:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>We define the constant 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ν 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ν 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        9.34 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          27 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mtext>
          kg 
        </mtext> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math></p>
   <p>And finally, we obtain:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ν 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> at P is perpendicular to the plane formed by P and the path of the point mass; its orientation is defined by the rule of the corkscrew; and its magnitude is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ν 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        θ 
      </mi> 
     </mrow> 
    </math></p>
   <p>If the speed of the mass is much smaller than the speed of light, the expression for the gravitational induction reduces itself to:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ν 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>This non-relativistic result could directly be obtained if one assumes that the displacement of the point mass during the time interval that the informatons need to move from the emitter to P can be neglected compared to the distance they travel during that period.</p>
   <p>So if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        v 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mi>
        c 
      </mi> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> at P is perpendicular to the plane formed by P and the path of the mass particle; its orientation is defined by the rule of the corkscrew; and its magnitude is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ν 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        sin 
      </mi> 
      <mi>
        θ 
      </mi> 
     </mrow> 
    </math></p>
  </sec><sec id="s6">
   <title>6. The Gravitational Field of a Mass Particle Moving with Constant Velocity</title>
   <p>A particle with rest mass m<sub>0</sub>, moving with constant velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         z 
       </mi> 
      </msub> 
     </mrow> 
    </math> along the Z-axis of an IRF, creates and maintains an expanding cloud of informatons that are carriers of both g- and β-information. That cloud can be identified with a time dependent continuum. It is called the gravitational field<sup>4</sup> of the particle. It is characterized by two time dependent vectoral quantities: the gravitational field (short: g-field) 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> and the gravitational induction (short: g-induction) 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>
    <xref ref-type="bibr" rid="scirp.134472-"></xref>1. With N the density of the flow of informatons at P (the rate per unit area at which the informatons cross an elementary surface perpendicular to their direction of movement), the g-field at that point is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        N 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         r 
       </mi> 
      </mstyle> 
     </mrow> 
    </math></p>
   <p>The magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the rate per unit area at which g-information is crossing an elementary surface perpendicular to the orientation of the g-indices of the constituent informatons. It’s clear that the direction of the flow of g-information at P is not the same as the direction of the flow of informatons.</p>
   <p>2. With n, the density of the cloud of informatons at P (number of informatons per unit volume), the g-induction at that point is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        n 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          s 
        </mi> 
       </mstyle> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ν 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mi>
                sin 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mi>
              θ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>The magnitude of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the density of the cloud of β-information at P (amount of β-information per unit volume). The orientation of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> is determined by the orientation of the β-indices of the constituent informatons.</p>
   <p>One can verify that:</p>
   <p>1. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        d 
      </mi> 
      <mi>
        i 
      </mi> 
      <mi>
        v 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math></p>
   <p>2. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        d 
      </mi> 
      <mi>
        i 
      </mi> 
      <mi>
        v 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math></p>
   <p>3. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        r 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        t 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>4. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        r 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        t 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>These relations are the laws of Maxwell-Heaviside.</p>
   <p>If 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        v 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mi>
        c 
      </mi> 
     </mrow> 
    </math>, the expressions for the g-field and the g-induction reduce to:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         r 
       </mi> 
      </mstyle> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ν 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msup> 
         <mi>
           r 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           r 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
  </sec><sec id="s7">
   <title>7. The Gravitational Field of a Set of Particles Moving with Constant Velocities</title>
   <p>We consider a set of particles 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        , 
      </mo> 
      <mo>
        ⋯ 
      </mo> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         i 
       </mi> 
      </msub> 
      <mo>
        , 
      </mo> 
      <mo>
        ⋯ 
      </mo> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         n 
       </mi> 
      </msub> 
     </mrow> 
    </math> that move with constant velocities 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        , 
      </mo> 
      <mo>
        ⋯ 
      </mo> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mi>
         i 
       </mi> 
      </msub> 
      <mo>
        , 
      </mo> 
      <mo>
        ⋯ 
      </mo> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mi>
         n 
       </mi> 
      </msub> 
     </mrow> 
    </math> relative to an IRF O. It creates and maintains a gravitational field that in O at each point, is characterised by the vector pair ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>).</p>
   <p>1. Each mass m<sub>i</sub> continuously emits g-information and contributes with an amount 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mi>
          i 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> to the g-field at an arbitrary point P. As in <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref> we conclude that the effective g-field 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> at P is defined as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mstyle displaystyle="true"> 
       <mo>
         ∑ 
       </mo> 
       <mrow> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
         <mrow> 
          <mi>
            g 
          </mi> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mstyle> 
     </mrow> 
    </math></p>
   <p>2. If it is moving, each mass m<sub>i</sub> emits also β-information, contributing to the g-induction at P with an amount 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mi>
          i 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math>. It is evident that the β-information in the volume element dV at P at each moment t is expressed by:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle displaystyle="true"> 
       <mo>
         ∑ 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              B 
            </mi> 
           </mstyle> 
           <mrow> 
            <mi>
              g 
            </mi> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <mtext>
            d 
          </mtext> 
          <mi>
            V 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle displaystyle="true"> 
         <mo>
           ∑ 
         </mo> 
         <mrow> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              B 
            </mi> 
           </mstyle> 
           <mrow> 
            <mi>
              g 
            </mi> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mstyle> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        V 
      </mi> 
     </mrow> 
    </math></p>
   <p>Thus, the effective g-induction 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> at P is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mstyle displaystyle="true"> 
       <mo>
         ∑ 
       </mo> 
       <mrow> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
         <mrow> 
          <mi>
            g 
          </mi> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mstyle> 
     </mrow> 
    </math></p>
   <p>On the basis of the superposition principle we can conclude that the laws of Maxwell-Heaviside mentioned in the previous section remain valid for the effective g-field and g-induction in the case of the gravitational field of a set of particles describing uniform rectilinear motions.</p>
  </sec><sec id="s8">
   <title>8. The Gravitational Field of a Stationary Mass Flow</title>
   <p>The term “stationary mass flow” refers to the movement of a homogeneous and incompressible fluid that, in an invariable way, flows relative to an IRF. The intensity of the flow at an arbitrary point P is characterized by the flow density 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          J 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math>. The magnitude of this vectoral quantity at P equals the rate per unit area at which the mass flows through a surface element that is perpendicular to the flow at P. The orientation of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          J 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math> corresponds to the direction of that flow. So, the rate at which the flow transports—in the positive sense (defined by the orientation of the surface vectors 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         S 
       </mi> 
      </mstyle> 
     </mrow> 
    </math>)—mass through an arbitrary surface ΔS, is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         i 
       </mi> 
       <mi>
         G 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <msub> 
         <mo>
           ∬ 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <mi>
            S 
          </mi> 
         </mrow> 
        </msub> 
        <mrow> 
         <msub> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             J 
           </mi> 
          </mstyle> 
          <mi>
            G 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <mtext>
           d 
         </mtext> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            S 
          </mi> 
         </mstyle> 
        </mrow> 
       </mrow> 
      </mstyle> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         i 
       </mi> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the intensity of the mass flow through ΔS.</p>
   <p>Since a stationary mass flow is the macroscopic manifestation of moving mass elements 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ρ 
       </mi> 
       <mi>
         G 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <mi>
        V 
      </mi> 
     </mrow> 
    </math>, it creates and maintains a gravitational field. And since the velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> of the mass element at a certain point is time independent, the gravitational field of a stationary mass flow will be time independent. It is evident that the rules for a static g-field <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref> also apply for this time independent g-field:</p>
   <p>1. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        d 
      </mi> 
      <mi>
        i 
      </mi> 
      <mi>
        v 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           ρ 
         </mi> 
         <mi>
           G 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>2. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        r 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        t 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math> what implies: 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mi>
        g 
      </mi> 
      <mi>
        r 
      </mi> 
      <mi>
        a 
      </mi> 
      <mi>
        d 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>One can prove <xref ref-type="bibr" rid="scirp.134472-2">
     [2]
    </xref> <xref ref-type="bibr" rid="scirp.134472-3">
     [3]
    </xref> that the rules for the time independent g-induction are:</p>
   <p>1. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        d 
      </mi> 
      <mi>
        i 
      </mi> 
      <mi>
        v 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math> what implies the existence of a vector gravitational potential function 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          A 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> for which 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        r 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        t 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          A 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>2. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        r 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        t 
      </mi> 
      <mtext>
          
      </mtext> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         ν 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          J 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
  </sec><sec id="s9">
   <title>9. The Gravitational Interaction between Moving Objects</title>
   <p>We consider a number of mass particles moving relative to an inertial reference frame O. They create and maintain a gravitational field that at each point of the space linked to O is defined by the vectors 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>. Each mass is “immersed” in a cloud of informatons carrying both g- and β-information. At each point, except at its own position, each particle contributes to the construction of that cloud.</p>
   <p>Let us consider the particle with rest mass m<sub>0</sub> that, at the moment t, goes with velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> through the point P.</p>
   <p>1. If the other particles were not there 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>—the g-field in the immediate vicinity of m<sub>0</sub>—would, according to §3, be symmetric relative to the carrier line of the velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> of m<sub>0</sub>. In reality that symmetry is disturbed by the g-information that the other particles send to P. 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>, the instantaneous value of the g-field at P, defines the extent to which this occurs.</p>
   <p>2. If the other particles were not there 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           B 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>—the g-induction near m<sub>0</sub>—would, according to §5, “rotate” around the carrier line of the vector 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math>. The pseudo-gravitational-field 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           E 
         </mi> 
         <mo>
           ″ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        × 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           B 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> defined by the vector product of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> with the g-induction that characterizes the proper β-field of m<sub>0</sub>, would also be symmetric relative to the carrier line of the velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math>. In reality this symmetry is disturbed by the β-information send to P by the other particles. The vector product ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        × 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>) of the instantaneous values of the velocity of m<sub>0</sub> and the g-induction at P, characterizes the extent to which this occurs.</p>
   <p>So, the characteristic symmetry of the cloud of g-information around a moving particle (the proper gravitational field) is in the immediate vicinity of that particle disturbed by 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> regarding the proper g-field and by ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        × 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>) regarding the proper β-induction.</p>
   <p>If it is free to move, the particle m<sub>0</sub> could restore the characteristic symmetry in its immediate vicinity by accelerating—relative to its proper IRF O'—with an amount 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>. In that manner it would become “blind” for the disturbance of symmetry of the gravitational field in its immediate vicinity. These insights form the basis of the following postulate.</p>
   <p>A particle with rest mass m<sub>0</sub>, moving with velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> in a gravitational field ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>), tends to become blind for the influence of that field on the symmetry of its proper gravitational field. If it is free to move, it will accelerate relative to its proper inertial reference frame with an amount 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mstyle> 
    </math>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
  </sec><sec id="s10">
   <title>10. The Gravitational Force Law</title>
   <p>The action of the gravitational field ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>) on a particle with rest mass m<sub>0</sub> that is moving with velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        v 
      </mi> 
     </mstyle> 
    </math> relative to the IRF O, is called the gravitational force 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          F 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math> on that particle. In extension of <xref ref-type="bibr" rid="scirp.134472-1">
     [1]
    </xref> we define 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          F 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math> as:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          F 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            E 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
        <mo>
          + 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             v 
           </mi> 
          </mstyle> 
          <mo>
            × 
          </mo> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              B 
            </mi> 
           </mstyle> 
           <mi>
             g 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>If it is free to move, the effect of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          F 
        </mi> 
        <mo>
          ¯ 
        </mo> 
       </mover> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math> on a particle with rest mass m<sub>0</sub> is that this will be accelerated relative to the its proper IRF O' with an amount 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
     </mstyle> 
    </math>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           v 
         </mi> 
        </mstyle> 
        <mo>
          × 
        </mo> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            B 
          </mi> 
         </mstyle> 
         <mi>
           g 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>This acceleration can be decomposed in a tangential ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         T 
       </mi> 
      </msub> 
     </mrow> 
    </math>) and a normal component ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         N 
       </mi> 
      </msub> 
     </mrow> 
    </math>):</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         T 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         T 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         T 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mo>
           ′ 
         </mo> 
        </msup> 
       </mstyle> 
       <mi>
         N 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         N 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         N 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>where 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         T 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          e 
        </mi> 
       </mstyle> 
       <mi>
         N 
       </mi> 
      </msub> 
     </mrow> 
    </math> are the unit vectors, respectively along the tangent and along the normal to the path of the point mass in O' (and in O).</p>
   <p>We express 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         T 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         N 
       </mi> 
      </msub> 
     </mrow> 
    </math> in function of the characteristics of the motion relative to the IRF O <xref ref-type="bibr" rid="scirp.134472-4">
     [4]
    </xref>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         T 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          v 
        </mi> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mi>
         N 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           v 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mi>
          R 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>(R is the radius of curvature of the path in O, and that radius in O' is 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        R 
      </mi> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math>.)</p>
   <p>The gravitational force is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
      <mtr> 
       <mtd> 
        <msub> 
         <mstyle mathvariant="bold" mathsize="normal"> 
          <mi>
            F 
          </mi> 
         </mstyle> 
         <mi>
           G 
         </mi> 
        </msub> 
        <mo>
          = 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mo>
            ′ 
          </mo> 
         </msup> 
        </mstyle> 
        <mo>
          = 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <msup> 
            <mi>
              a 
            </mi> 
            <mo>
              ′ 
            </mo> 
           </msup> 
           <mi>
             T 
           </mi> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              e 
            </mi> 
           </mstyle> 
           <mi>
             T 
           </mi> 
          </msub> 
          <mo>
            + 
          </mo> 
          <msub> 
           <msup> 
            <mi>
              a 
            </mi> 
            <mo>
              ′ 
            </mo> 
           </msup> 
           <mi>
             N 
           </mi> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              e 
            </mi> 
           </mstyle> 
           <mi>
             N 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          = 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <msup> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mn>
                  1 
                </mn> 
                <mo>
                  − 
                </mo> 
                <msup> 
                 <mi>
                   β 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msup> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mrow> 
              <mfrac> 
               <mn>
                 3 
               </mn> 
               <mn>
                 2 
               </mn> 
              </mfrac> 
             </mrow> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mfrac> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              v 
            </mi> 
           </mrow> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              t 
            </mi> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              e 
            </mi> 
           </mstyle> 
           <mi>
             T 
           </mi> 
          </msub> 
          <mo>
            + 
          </mo> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <msup> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mn>
                  1 
                </mn> 
                <mo>
                  − 
                </mo> 
                <msup> 
                 <mi>
                   β 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msup> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mrow> 
              <mfrac> 
               <mn>
                 1 
               </mn> 
               <mn>
                 2 
               </mn> 
              </mfrac> 
             </mrow> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mfrac> 
           <mrow> 
            <msup> 
             <mi>
               v 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
           <mi>
             R 
           </mi> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mstyle mathvariant="bold" mathsize="normal"> 
            <mi>
              e 
            </mi> 
           </mstyle> 
           <mi>
             N 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mtext>
           d 
         </mtext> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </mfrac> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <msub> 
             <mi>
               m 
             </mi> 
             <mn>
               0 
             </mn> 
            </msub> 
           </mrow> 
           <mrow> 
            <msqrt> 
             <mrow> 
              <mn>
                1 
              </mn> 
              <mo>
                − 
              </mo> 
              <msup> 
               <mi>
                 β 
               </mi> 
               <mn>
                 2 
               </mn> 
              </msup> 
             </mrow> 
            </msqrt> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mstyle mathvariant="bold" mathsize="normal"> 
           <mi>
             v 
           </mi> 
          </mstyle> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math></p>
   <p>With:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        = 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         p 
       </mi> 
      </mstyle> 
     </mrow> 
    </math></p>
   <p>We finally obtain:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          F 
        </mi> 
       </mstyle> 
       <mi>
         G 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mstyle mathvariant="bold" mathsize="normal"> 
         <mi>
           p 
         </mi> 
        </mstyle> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mstyle mathvariant="bold" mathsize="normal"> 
      <mi>
        p 
      </mi> 
     </mstyle> 
    </math> is the linear momentum of the particle relative to the IRF O. It depends on the relativistic mass m op the particle:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        m 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <msup> 
           <mi>
             β 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>In §2 it has been showed that m is the parameter of the mass particle that determines the rate at which it emits informatons relative to its proper IRF. Thus it is representative for the density of the cloud of informatons generated in that IRF and thus for the ability to persist in its dynamic state. It is a measure for its inertia.</p>
  </sec><sec id="s11">
   <title>11. The Interaction between Two Moving Particles</title>
   <p>Two particles with rest masses m<sub>1</sub> and m<sub>2</sub> (<xref ref-type="fig" rid="fig4">
     Figure 4
    </xref>) are anchored in the IRF O' that is moving relative to the inertial reference frame O with constant velocity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          v 
        </mi> 
       </mstyle> 
       <mo stretchy="true">
         → 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mstyle mathvariant="bold" mathsize="normal"> 
       <mi>
         v 
       </mi> 
      </mstyle> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           e 
         </mi> 
         <mo stretchy="true">
           → 
         </mo> 
        </mover> 
       </mrow> 
       <mi>
         z 
       </mi> 
      </msub> 
     </mrow> 
    </math>. The distance between the masses is R.</p>
   <fig id="fig4" position="float">
    <label>Figure 4</label>
    <caption>
     <title>Figure 4. The gravitational interaction between moving particles.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181089-rId366.jpeg?20240712014729" />
   </fig>
   <p>According to §6, the components of the gravitational field created and maintained by m<sub>1</sub> at the position of m<sub>2</sub> are—in magnitude—determined by:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <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></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <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> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mi>
         v 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> points to the position of m<sub>1</sub> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> points in the direction of the X-axis.</p>
   <p>And according to the force law F<sub>12</sub>, the magnitude of the force exerted by the gravitational field ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mrow> 
        <mi>
          g 
        </mi> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msub> 
     </mrow> 
    </math>) on m<sub>2</sub>—this is the attraction force of m<sub>1</sub> on m<sub>2</sub>—is:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mn>
         2 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           E 
         </mi> 
         <mrow> 
          <mi>
            g 
          </mi> 
          <mn>
            2 
          </mn> 
         </mrow> 
        </msub> 
        <mo>
          − 
        </mo> 
        <mi>
          v 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           B 
         </mi> 
         <mrow> 
          <mi>
            g 
          </mi> 
          <mn>
            2 
          </mn> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math></p>
   <p>After substitution:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <msub> 
       <msup> 
        <mi>
          F 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math></p>
   <p>with:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <msup> 
        <mi>
          F 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>the magnitude of the force that m<sub>1</sub>, according Newtons universal law of gravitation, in the IRF O'—where both particles are at rest—exerts on m<sub>2</sub>.</p>
   <p>In the same way we find:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mn>
          21 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <msub> 
       <msup> 
        <mi>
          F 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math></p>
   <p>We conclude that the moving masses attract each other with a force:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        F 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mn>
          21 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mi>
         F 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mi>
           β 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math></p>
   <p>This result perfectly agrees with that based on S.R.T. Indeed, relative to O' the particles are at rest. According to Newton’s law of universal gravitation, they exert on each other equal but opposite forces:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         F 
       </mi> 
       <mo>
         ′ 
       </mo> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msub> 
       <msup> 
        <mi>
          F 
        </mi> 
        <mo>
          ′ 
        </mo> 
       </msup> 
       <mrow> 
        <mn>
          12 
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       </mrow> 
      </msub> 
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        = 
      </mo> 
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        <mi>
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        </mi> 
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          ′ 
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       <mrow> 
        <mn>
          21 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
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        G 
      </mi> 
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        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
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           1 
         </mn> 
        </msub> 
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          ⋅ 
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        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          4 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           η 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
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       <mrow> 
        <msub> 
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           m 
         </mi> 
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           1 
         </mn> 
        </msub> 
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          ⋅ 
        </mo> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
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         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>Relative to O both masses are moving with constant speed v in the direction of the Z-axis. From the transformation equations between an inertial frame O and another inertial frame O', in which a point mass experiencing a force F' is instantaneously at rest, we can immediately deduce the force F that the point masses exert on each other in O <xref ref-type="bibr" rid="scirp.134472-4">
     [4]
    </xref>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        F 
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        = 
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       <mrow> 
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          12 
        </mn> 
       </mrow> 
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        = 
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       </mi> 
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          21 
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        = 
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        ⋅ 
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       <mrow> 
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          1 
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             ( 
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             ) 
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      </msqrt> 
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         </mi> 
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        </msup> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math></p>
   <p>From the above we can also conclude that the component of the gravitational force due to the g-induction is β-times smaller than that due to the g-field. This implies that, for speeds much smaller than the speed of light, the effects of the β-information are masked.</p>
   <p>It can be shown that the β-information emitted by moving gravitating objects is responsible for deviations (as the advance of Mercury Perihelion) of the real orbits of planets with respect to these predicted by the classical theory of gravitation <xref ref-type="bibr" rid="scirp.134472-5">
     [5]
    </xref>.</p>
  </sec><sec id="s12">
   <title>12. Conclusions</title>
   <p>A mass particle moving relative to an inertial IRF O is the emitter of informatons that are carriers of information regarding the positon (g-information) and regarding the velocity (β-information) of their source. As a result, the gravitational field, of a moving mass particle (and by extension of a set of moving particles, a moving material object and a mass flow) manifests itself at the macroscopic level in O as a dual entity, always having a field- and an induction component ( 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          B 
        </mi> 
       </mstyle> 
       <mi>
         g 
       </mi> 
      </msub> 
     </mrow> 
    </math>) simultaneously created by their common sources.</p>
   <p>The interaction between material objects in that field is made possible by the intermediation of the gravitational field. An object in a gravitational field tends to become blind for that field. It experiences a force described by a Lorentz like law.</p>
   <p>Thus, it is clear that the kinematics of the gravitating objects play a role in the gravitational phenomena. This is taken into account in the framework of the gravitoelectromagnetic description of gravitation <xref ref-type="bibr" rid="scirp.134472-6">
     [6]
    </xref> <xref ref-type="bibr" rid="scirp.134472-7">
     [7]
    </xref> (GEM) where the idea is developed that the gravitational field must be isomorphic with the electromagnetic field in a vacuum.</p>
   <p>Because the role of the kinematics of the gravitating objects is not relevant when the speed of the object is small relative to the speed of light, this phenomenon is not taken into account in the “classical” description of the gravitational phenomena and laws.</p>
  </sec><sec id="s13">
   <title>13. Epilogue</title>
   <p>In the follow-up article “The Maxwell-Heaviside Equations Explained by the Theory of Informatons” we mathematically deduce the Maxwell-Heaviside equations from the kinematics of the informatons. That deduction indicates that there is no causal link between 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mstyle mathvariant="bold" mathsize="normal"> 
        <mi>
          E 
        </mi> 
       </mstyle> 
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         g 
       </mi> 
      </msub> 
     </mrow> 
    </math> and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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          B 
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       </mstyle> 
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         g 
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      </msub> 
     </mrow> 
    </math>.</p>
  </sec><sec id="s14">
   <title>NOTES</title>
   <p><sup>1</sup>We neglect the possible stochastic nature of the emission, that is responsible for noise on the quantities that characterize the gravitational field. So, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
      <mi>
        N 
      </mi> 
      <mo>
        ˙ 
      </mo> 
     </mover> 
    </math><xref ref-type="bibr" rid="scirp.134472-#QUOTE"></xref> is the average emission rate.</p>
   <p><sup>2</sup>The orientation of the g-field implies that the g-indices of the informatons that at a certain moment pass near P, point at that moment to the position of the emitting mass and not to its light delayed position.</p>
   <p><sup>3</sup>also called “gravitomagnetic induction”.</p>
   <p><sup>4</sup>Also called: “gravito-electromagnetic” (GEM field) or “gravito-magnetic” field (GM field).</p>
  </sec>
 </body><back>
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