<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article">
 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">
    jhepgc
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of High Energy Physics, Gravitation and Cosmology
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2380-4327
   </issn>
   <issn publication-format="print">
    2380-4335
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jhepgc.2025.112036
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-142316
   </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>
    Relic Black Holes, in Terms of a Quantum Number n&amp;Torsion Leading to Relic GW and How a Tokamak May Permit after Effects of Relic GW Frequencies Being Duplicated
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Andrew Walcott
      </surname>
      <given-names>
       Beckwith
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aPhysics Department, Chongqing University, Chongqing, China
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     18
    </day> 
    <month>
     03
    </month>
    <year>
     2025
    </year>
   </pub-date> 
   <volume>
    11
   </volume> 
   <issue>
    02
   </issue>
   <fpage>
    518
   </fpage>
   <lpage>
    543
   </lpage>
   <history>
    <date date-type="received">
     <day>
      7,
     </day>
     <month>
      March
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      25,
     </day>
     <month>
      March
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      25,
     </day>
     <month>
      April
     </month>
     <year>
      2025
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © Copyright 2014 by authors and Scientific Research Publishing Inc. 
    </copyright-statement>
    <copyright-year>
     2014
    </copyright-year>
    <license>
     <license-p>
      This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/
     </license-p>
    </license>
   </permissions>
   <abstract>
    Our idea for black holes is using Torsion to form a cosmological constant. Planck sized black holes allow for a spin density term canceling Torsion. And we conclude with a generalized uncertainty principle which is then linked to a black hole versus white hole, linked by a worm-hole problem, The spin-offs as the connection to multi-messenger astronomy will be enumerated in the last part of this document. And we can compare the resultant GW generation as could be measured by Lisa from these. In doing so, we review its simulated connections to a Tokamak simulation.
   </abstract>
   <kwd-group> 
    <kwd>
     Relic Black Holes
    </kwd> 
    <kwd>
      Torsion in Cosmology
    </kwd> 
    <kwd>
      Cosmological Constant and Torsion
    </kwd> 
    <kwd>
      Black Hole and White Hole Linkage
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Statement of Purpose of This Document</title>
   <p>The author has in prior work given the idea that a decay of millions of Planck sized BHs within the very early universe as in <xref ref-type="bibr" rid="scirp.142316-1">
     [1]
    </xref> could generate GW and gravitons, due to a breakup of black holes as predicted in <xref ref-type="bibr" rid="scirp.142316-1">
     [1]
    </xref> but with the present GW spectrum of today very conservatively following <xref ref-type="bibr" rid="scirp.142316-2">
     [2]
    </xref>. The breakup of black holes may commence due to what is stated in <xref ref-type="bibr" rid="scirp.142316-1">
     [1]
    </xref> and actually be complemented by what is addressed in <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref> which would be if Gravitons acting as similar to a Bose-Einstein condensate contribute to a resulting DE <xref ref-type="bibr" rid="scirp.142316-1">
     [1]
    </xref>. Either the strict breakup of black holes as in <xref ref-type="bibr" rid="scirp.142316-4">
     [4]
    </xref> or some conflation with <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref> would lead to, likely GW (and Graviton frequencies) initially of the order of 10<sup>10</sup> Hz to maybe 10<sup>19</sup> Hz. In doing so, we can consider the duration of an observed signal, its relative noisiness and stochastic noise contributions of a sort which are covered in <xref ref-type="bibr" rid="scirp.142316-5">
     [5]
    </xref>. In addition, the generation of GW in a Tokamak if commensurate with eLISA data after a step down of 10<sup>−25</sup> to 10<sup>−26</sup> due to 60 or more e-folds <xref ref-type="bibr" rid="scirp.142316-6">
     [6]
    </xref> may allow for a review of adequate polarization states for GW which may or may not need higher dimensions to be in fidelity to the data sets obtained <xref ref-type="bibr" rid="scirp.142316-7">
     [7]
    </xref>. Having said that, what are the justifications for using Tokamaks?</p>
   <p>First of all, there is the question of what sort of polarization would be produced in initial processes. Secondly, if we were able to ascertain 10<sup>10</sup> Hertz gravitational waves, via our laboratory arrangements and if we were later able to confirm, say the existence of 10<sup>−16</sup> Hz GW frequencies via LISA in the present era, this would be stunning proof of the Big Bang hypothesis, and so we summarize what this inquiry may answer. So what is our inquiry good for?</p>
   <p>1) Determination of the fidelity of the e-fold value of 60 in the Big Bang;</p>
   <p>2) Issues of initial GW polarization which may be configured at the start of the Big Bang;</p>
   <p>3) Determination of the relative stability of the production of the GW signal (i.e. if we had a Tokamak running and the resulting GW amplitude and the characteristics of the signal are stable, over a “long time interval” does this imply stability of the eLISA signal? Over time and space?)</p>
   <p>4) Likelihood of noise and Stochastic fluctuations in a produced GW signal.</p>
   <p>If A, B, C and D were determined as to the Tokamak, and GW, we may be able to infer what to look for and to model when examined directly, what a LISA GW signal set of characteristics may be inferring as to early universe conditions. Having said that, let us go to the Tokamak information</p>
  </sec><sec id="s2">
   <title>2. Comparison with Grishchuk and Sachin Results. For Obtaining GW Generation Count</title>
   <p>Russian physicists Grishchuk and Sachin <xref ref-type="bibr" rid="scirp.142316-8">
     [8]
    </xref> obtained the amplitude of a Gravitational wave (GW) in a plasma as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        A 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mi>
          m 
        </mi> 
        <mi>
          p 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          i 
        </mi> 
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          t 
        </mi> 
        <mi>
          u 
        </mi> 
        <mi>
          d 
        </mi> 
        <mi>
          e 
        </mi> 
        <mtext>
            
        </mtext> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         E 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
     </mrow> 
    </math>. This is compared with <xref ref-type="bibr" rid="scirp.142316-9">
     [9]
    </xref>, and we diagram the situation as follows <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref> <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref>.</p>
   <p>Note that a simple model of how to provide a current in the Toroid is provided by a transformer core. This diagram is an example of how to induce the current I, used in the simple Ohms law derivation referred to in the first part of the text. Here, E is the electric field whereas 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is the gravitational wavelength for GW generated by the Tokamak in our model. In the original Griskchuk model, we would have very small strain values, which will be commented upon but which require the following relationship between GW wavelength and resultant frequency. Note, if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mn>
         6 
       </mn> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        Hz 
      </mtext> 
      <mo>
        ⇒ 
      </mo> 
      <msub> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mn>
        300 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        meters 
      </mtext> 
     </mrow> 
    </math>, so we will be assuming a baseline of the order of setting 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mn>
         9 
       </mn> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        Hz 
      </mtext> 
      <mo>
        ⇒ 
      </mo> 
      <msub> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mn>
        0.3 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        meters 
      </mtext> 
     </mrow> 
    </math>, as a baseline measurement for GW detection above the Tokamak. Furthermore,</p>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>Figure 1. Flux directions of gravitational waves relative to tokamak configuration.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181289-rId24.jpeg?20250428033525" />
   </fig>
   <p>We outline the direction of Gravitational wave “flux”. If the arrow in the middle of the Tokamak ring perpendicular to the direction of the current represents the z axis, we represent where to put the GW detection device as 5 meters above the Tokamak ring along the z axis. This diagram was initially from Wesson <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref>.</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mi>
        A 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          GW 
        </mtext> 
        <mtext>
            
        </mtext> 
        <mtext>
          amplitude 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ~ 
      </mo> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mrow> 
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          G 
        </mi> 
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          ⋅ 
        </mo> 
        <msub> 
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           W 
         </mi> 
         <mi>
           E 
         </mi> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           V 
         </mi> 
         <mrow> 
          <mtext>
            volume 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
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          ⋅ 
        </mo> 
        <mover accent="true"> 
         <mi>
           a 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (1)</p>
   <p>Where</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           W 
         </mi> 
         <mi>
           E 
         </mi> 
        </msub> 
        <mo>
          = 
        </mo> 
        <mtext>
          Average energy density 
        </mtext> 
        <mo>
          , 
        </mo> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           V 
         </mi> 
         <mrow> 
          <mtext>
            volume 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          = 
        </mo> 
        <mtext>
          Volume Toroid 
        </mtext> 
        <mo>
          , 
        </mo> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mover accent="true"> 
         <mi>
           a 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
        <mo>
          = 
        </mo> 
        <mtext>
          inner radii 
        </mtext> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            Toroid 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (1a)</p>
   <p>Equation (2) above is due to the 1<sup>st</sup> term of a two-part composition of the strain, with the 2<sup>nd</sup> term of the strain value significantly larger than the first term and due to the ignition of the Plasma in the Tokamak. The first term of strain is largely due to what was calculated by Grishkuk <xref ref-type="bibr" rid="scirp.142316-8">
     [8]
    </xref> et al. The second term is due to Plasma fusion burning. This plasma fusion burning contribution is due to non equilibrium contributions to Plasma ignition, which will be elaborated on in this document. Note that the first term in the strain derivation is due to the electric field within a Toroid, not Plasma fusion burning, and we will first of all discuss how to obtain the requisite strain, for the electric field contribution to the current, inside a Tokamak, making use of Ohms law. See <xref ref-type="bibr" rid="scirp.142316-9">
     [9]
    </xref> for additional details.</p>
  </sec><sec id="s3">
   <title>3. Derivation of Strain Generated by an Electric Field, and Small Strain Values</title>
   <p>We will examine the would-be electric field, contributing to a small strain value similar in part to Ohms law. A generalized Ohm’s law ties in well with <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        J 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        σ 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        E 
      </mi> 
     </mrow> 
    </math>(2)</p>
   <p>In order to obtain a suitable electric field, to be detected via 3DSR technology <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>, we will use a generalized Ohm’s law as given by Wesson <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref> (page 146), where E and B are electric and magnetic fields, and v is velocity.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        E 
      </mi> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mi>
         σ 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        J 
      </mi> 
      <mo>
        − 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        × 
      </mo> 
      <mi>
        B 
      </mi> 
     </mrow> 
    </math>(3)</p>
   <p>Note that the term in Equation (4) given as 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        v 
      </mi> 
      <mo>
        × 
      </mo> 
      <mi>
        B 
      </mi> 
     </mrow> 
    </math> deserves special commentary. If 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       v 
     </mi> 
    </math> is perpendicular to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       B 
     </mi> 
    </math> as occurs in a simple equilibrium case, then of course, Equation (4) would be, simply put, Ohms law, and spatial equilibrium averaging would then lead to</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        E 
      </mi> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mi>
         σ 
       </mi> 
       <mrow> 
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          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        J 
      </mi> 
      <mo>
        − 
      </mo> 
      <mi>
        v 
      </mi> 
      <mo>
        × 
      </mo> 
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        B 
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      <munder> 
       <mo>
         → 
       </mo> 
       <mrow> 
        <mi>
          v 
        </mi> 
        <mtext>
            
        </mtext> 
        <mtext>
          perpendicular 
        </mtext> 
        <mtext>
            
        </mtext> 
        <mtext>
          to 
        </mtext> 
        <mtext>
            
        </mtext> 
        <mi>
          B 
        </mi> 
       </mrow> 
      </munder> 
      <mi>
        E 
      </mi> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mi>
         σ 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        J 
      </mi> 
     </mrow> 
    </math> (4)</p>
   <p>What saves the contribution of Plasma burning as a contributing factor to the Tokamak generation of GW, with far larger strain values commencing is that one does not have the velocity of ions in Plasma perpendicular to B fields at the beginning of Tokamak generation. It is, fortunately for us, a non equilibrium initial process, with thermal irregularities leading to both terms in Equation (5) contributing to the electric field values. We will be looking for an application for radial free electric fields being applied e.g., Wesson <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref> (page 120)</p>
   <p>
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        n 
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       <mi>
         j 
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       <none /> 
      </mmultiscripts> 
      <msub> 
       <mrow></mrow> 
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         j 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           E 
         </mi> 
         <mi>
           r 
         </mi> 
        </msub> 
        <mo>
          + 
        </mo> 
        <msub> 
         <mi>
           v 
         </mi> 
         <mrow> 
          <mo>
            ⊥ 
          </mo> 
          <mi>
            j 
          </mi> 
         </mrow> 
        </msub> 
        <mi>
          B 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
         <mi>
           P 
         </mi> 
         <mi>
           j 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>(5)</p>
   <p>Here, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mi>
         j 
       </mi> 
      </msub> 
     </mrow> 
    </math> = ion density, jth species, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         e 
       </mi> 
       <mi>
         j 
       </mi> 
      </msub> 
     </mrow> 
    </math> = ion charge, jth species, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         r 
       </mi> 
      </msub> 
     </mrow> 
    </math> = radial electric field, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         v 
       </mi> 
       <mrow> 
        <mo>
          ⊥ 
        </mo> 
        <mi>
          j 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> = perpendicular velocity, of jth species, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       B 
     </mi> 
    </math> = magnetic field, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         P 
       </mi> 
       <mi>
         j 
       </mi> 
      </msub> 
     </mrow> 
    </math> = pressure, jth species. The results of Equation (3) and Equation (4) are</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         E 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              C 
            </mi> 
            <mi>
              o 
            </mi> 
            <mi>
              n 
            </mi> 
            <mi>
              s 
            </mi> 
            <mi>
              t 
            </mi> 
           </mrow> 
           <mi>
             R 
           </mi> 
          </mfrac> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <msub> 
             <mi>
               J 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
           </mrow> 
           <mrow> 
            <mi>
              n 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mi>
              e 
            </mi> 
           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
          <msub> 
           <mi>
             v 
           </mi> 
           <mi>
             R 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mtext>
         1 
       </mtext> 
       <mrow> 
        <mtext>
          st 
        </mtext> 
       </mrow> 
      </msup> 
      <mo>
        + 
      </mo> 
      <msup> 
       <mtext>
         2 
       </mtext> 
       <mrow> 
        <mtext>
          nd 
        </mtext> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (6)</p>
   <p>Here, the 1<sup>st</sup> term is due to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        ∇ 
      </mo> 
      <mo>
        × 
      </mo> 
      <mi>
        E 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>, and the 2<sup>nd</sup> term is due to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mi>
         n 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
         <mi>
           P 
         </mi> 
         <mi>
           j 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
         <mi>
           x 
         </mi> 
         <mi>
           n 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mi>
           j 
         </mi> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           e 
         </mi> 
         <mi>
           j 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            v 
          </mi> 
          <mo>
            × 
          </mo> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mi>
         n 
       </mi> 
      </msub> 
     </mrow> 
    </math> with the 1<sup>st</sup> term generating 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          38 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        - 
      </mtext> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          30 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> in terms of GW amplitude strain 5 meters above the Tokamak, whereas the 2<sup>nd</sup> term has an 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          26 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> in terms of GW amplitude above the Tokamak. The article has contributions from amplitude from the 1<sup>st</sup> and 2<sup>nd</sup> terms separately. The second part will be tabulated separately from the first contribution assuming a minimum temperature of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        T 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        T 
      </mi> 
      <mi>
        e 
      </mi> 
      <mi>
        m 
      </mi> 
      <mi>
        p 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <mn>
        10 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        KeV 
      </mtext> 
     </mrow> 
    </math> as from Wesson <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref>. We should also consider the issues in <xref ref-type="bibr" rid="scirp.142316-9">
     [9]
    </xref>, <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref>, and <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>.</p>
  </sec><sec id="s4">
   <title>4. GW h Strain Values When the First Term of Equation (4) Is Used</title>
   <p>We now look at what we can expect with the simple Ohm’s law calculation for strain values. As it is, the effort leads to non-usable GW amplitude values of up to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          38 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        - 
      </mtext> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          30 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> for GW wave amplitudes 5 meters above a Tokamak, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          36 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        - 
      </mtext> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          28 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> in the center of a Tokamak. I.e. this would be using Ohm’s law and these are sample values of the Tokamak generated GW amplitude, using the first term of Equation (4) and obtaining the following value <xref ref-type="bibr" rid="scirp.142316-8">
     [8]
    </xref> with</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mtext>
          First term 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         E 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mi>
             J 
           </mi> 
           <mi>
             σ 
           </mi> 
          </mfrac> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
     </mrow> 
    </math> (7)</p>
   <p>We summarize the results of such in our first table as given for when 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mn>
         9 
       </mn> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        Hz 
      </mtext> 
      <mo>
        ⇒ 
      </mo> 
      <msub> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mn>
        0.3 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        meters 
      </mtext> 
     </mrow> 
    </math> and with conductivity 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        σ 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          tokamak plasma 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ~ 
      </mo> 
      <mn>
        10 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mrow> 
        <msup> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mi>
          sec 
        </mi> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> and with the following provisions as to initial values. What we observe are a range of Tokamak values which are, even in the case of ITER (not yet built) beyond the reach of any technological detection devices which are conceivable in the coming decade. This table and its results, assuming fixed conductivity values 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        σ 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          tokamak plasma 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ~ 
      </mo> 
      <mn>
        10 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mrow> 
        <msup> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mi>
          sec 
        </mi> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> as well as 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mn>
        0.3 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        meters 
      </mtext> 
     </mrow> 
    </math> is why the author, results as to the 2<sup>nd</sup> term of Equation (4) which leads to even when considering the results for the Chinese Tokamak in Hefei to have <xref ref-type="bibr" rid="scirp.142316-13">
     [13]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mtext>
          Second term 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         E 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <msub> 
             <mi>
               J 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
           </mrow> 
           <mrow> 
            <mi>
              n 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mi>
              e 
            </mi> 
           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
          <msub> 
           <mi>
             v 
           </mi> 
           <mi>
             R 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          W 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
     </mrow> 
    </math> (8)</p>
   <p>or values 10,000 larger than the results in ITER due to Equation (6).</p>
   <p>Note that we are setting 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         λ 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mn>
        0.3 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        meters 
      </mtext> 
     </mrow> 
    </math>, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        σ 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          tokamak plasma 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ~ 
      </mo> 
      <mn>
        10 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mrow> 
        <msup> 
         <mi>
           m 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mi>
          sec 
        </mi> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math>, using Equation (6) above for Amplitude of GW. What makes it mandatory to go the 2<sup>nd</sup> term of Equation (4) is that even in the case of ITER, 5 meters above the Tokamak ring, the GW amplitude is 1/10,000 the size of any reasonable GW detection device, and including the new 3DSR technology (Li et al., 2009) <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>. Hence, we need to come up with a better estimate, which is what the value of the 2nd term of Equation (5) is in its formulation.</p>
  </sec><sec id="s5">
   <title>5. Enhancing GW Strain Amplitude via Utilizing a Burning Plasma Drift Current: Equation (4)</title>
   <p>The way forward is to go to Wesson, <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref> <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref> (2011, page 120) and to look at the normal to surface induced electric field contribution</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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         E 
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        = 
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        <mtext>
          d 
        </mtext> 
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           P 
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          d 
        </mtext> 
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         </mi> 
         <mi>
           n 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           n 
         </mi> 
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           j 
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        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           e 
         </mi> 
         <mi>
           j 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            v 
          </mi> 
          <mo>
            × 
          </mo> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mi>
         n 
       </mi> 
      </msub> 
     </mrow> 
    </math>(9)</p>
   <p>If one has for 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         v 
       </mi> 
       <mi>
         R 
       </mi> 
      </msub> 
     </mrow> 
    </math>as the radial velocity of ions in the Tokamak from Tokamak center to its radial distance, R, from center, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         θ 
       </mi> 
      </msub> 
     </mrow> 
    </math> as the direction of a magnetic field in the “face” of a Toroid containing the Plasma, in the angular 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       θ 
     </mi> 
    </math>direction from a minimal toroid radius of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        R 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        a 
      </mi> 
     </mrow> 
    </math>, with 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        θ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>, to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        R 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        a 
      </mi> 
      <mo>
        + 
      </mo> 
      <mi>
        r 
      </mi> 
     </mrow> 
    </math> with 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        θ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        π 
      </mi> 
     </mrow> 
    </math>, one has 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         v 
       </mi> 
       <mi>
         R 
       </mi> 
      </msub> 
     </mrow> 
    </math> for radial drift velocity of ions in the Tokamak, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         θ 
       </mi> 
      </msub> 
     </mrow> 
    </math> having a net approximate value of: with 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         θ 
       </mi> 
      </msub> 
     </mrow> 
    </math> not perpendicular to the ion velocity, so then <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            v 
          </mi> 
          <mo>
            × 
          </mo> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mi>
         n 
       </mi> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msub> 
       <mi>
         v 
       </mi> 
       <mi>
         R 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         θ 
       </mi> 
      </msub> 
     </mrow> 
    </math>(10)</p>
   <p>Also, From Wesson <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref> (page 167) the spatial change in pressure denoted</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
         <mi>
           P 
         </mi> 
         <mi>
           j 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
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           x 
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           n 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         B 
       </mi> 
       <mi>
         θ 
       </mi> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         j 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
     </mrow> 
    </math>(11)</p>
   <p>Here the drift current, using 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ξ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mi>
         a 
       </mi> 
       <mo>
         / 
       </mo> 
       <mi>
         R 
       </mi> 
      </mrow> 
     </mrow> 
    </math>, and drift current 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         j 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
     </mrow> 
    </math> for Plasma charges, i.e.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         j 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           ξ 
         </mi> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           B 
         </mi> 
         <mi>
           θ 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          T 
        </mi> 
        <mi>
          e 
        </mi> 
        <mi>
          m 
        </mi> 
        <mi>
          p 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mrow> 
          <mtext>
            drift 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>(12)</p>
   <p>
    <xref ref-type="fig" rid="fig2">
     Figure 2
    </xref> introduces the role of the drift current, in terms of Tokamaks <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref></p>
   <fig id="fig2" position="float">
    <label>Figure 2</label>
    <caption>
     <title>Figure 2. Bootstrap currents and pressure distribution in tokamak radial direction.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181289-rId118.jpeg?20250428033526" />
   </fig>
   <p>Typical bootstrap currents with a shift due to r/a where r is the radial direction of the Tokamak, and a is the inner radius of the Toroid. This figure is reproduced from Wesson <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref>. Then one has</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
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       </mi> 
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       </mn> 
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      <mo>
        ⋅ 
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      <msup> 
       <mrow> 
        <mrow> 
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           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               j 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               n 
             </mi> 
             <mi>
               j 
             </mi> 
            </msub> 
            <mo>
              ⋅ 
            </mo> 
            <msub> 
             <mi>
               e 
             </mi> 
             <mi>
               j 
             </mi> 
            </msub> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           B 
         </mi> 
         <mi>
           θ 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msubsup> 
         <mi>
           e 
         </mi> 
         <mi>
           j 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           ξ 
         </mi> 
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          <mrow> 
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             1 
           </mn> 
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           </mo> 
           <mn>
             4 
           </mn> 
          </mrow> 
         </mrow> 
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       </mrow> 
       <mrow> 
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         </mi> 
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        </msubsup> 
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        ⋅ 
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           [ 
         </mo> 
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           <mn>
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           </mn> 
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            <msub> 
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             </mi> 
             <mrow> 
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                drift 
              </mtext> 
             </mrow> 
            </msub> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mfrac> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <msub> 
             <mi>
               n 
             </mi> 
             <mrow> 
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                drift 
              </mtext> 
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           <mrow> 
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            </mtext> 
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              r 
            </mi> 
           </mrow> 
          </mfrac> 
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           ] 
         </mo> 
        </mrow> 
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         2 
       </mn> 
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        ~ 
      </mo> 
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         </mi> 
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        ⋅ 
      </mo> 
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       <mrow> 
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           [ 
         </mo> 
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          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
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               n 
             </mi> 
             <mrow> 
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                drift 
              </mtext> 
             </mrow> 
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          </mo> 
          <mfrac> 
           <mrow> 
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            </mtext> 
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             </mi> 
             <mrow> 
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              </mtext> 
             </mrow> 
            </msub> 
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           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              r 
            </mi> 
           </mrow> 
          </mfrac> 
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         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (13)</p>
   <p>Now, the behavior of the numerical density of ions, can be given as follows, namely growing in the radial direction, then <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mi>
         n 
       </mi> 
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        <mtext>
          drift 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mrow> 
        <mrow> 
         <mrow> 
          <msub> 
           <mi>
             n 
           </mi> 
           <mrow> 
            <mtext>
              drift 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           | 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mtext>
          initial 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           α 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          r 
        </mi> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (14)</p>
   <p>This exponential behavior then will lead to the 2<sup>nd</sup> term in Equation (4) having in the center of the Tokamak, for an ignition temperature of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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      </mo> 
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      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        KeV 
      </mtext> 
     </mrow> 
    </math> a value of</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mrow> 
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          2nd 
        </mtext> 
        <mtext>
            
        </mtext> 
        <mtext>
          term 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mi>
         G 
       </mi> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msubsup> 
       <mi>
         B 
       </mi> 
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       </mi> 
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       </mn> 
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        ⋅ 
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         </mo> 
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              ⋅ 
            </mo> 
            <msub> 
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               e 
             </mi> 
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             </mi> 
            </msub> 
           </mrow> 
          </mrow> 
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         <mo>
           ) 
         </mo> 
        </mrow> 
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       <mi>
         λ 
       </mi> 
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        </mi> 
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        </mi> 
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        ⋅ 
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      <mo>
        ⋅ 
      </mo> 
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       <mi>
         λ 
       </mi> 
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        </mi> 
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       </mn> 
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      </mo> 
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          10 
        </mn> 
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       <mrow> 
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        </mo> 
        <mn>
          25 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (15)</p>
  </sec><sec id="s6">
   <title>6. Restating the Energy Density and Power Using the Formalism of Equation (1) Directly</title>
   <p>
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          </mtext> 
         </mrow> 
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    </math> (16)</p>
   <p>The temperature for Plasma fusion burning, is then between 30 to 100 KeV, as given by Wesson <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref>. The corresponding power as given by Wesson is then for the Tokamak <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref></p>
   <p>
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    </math>(17)</p>
   <p>The tie-in with Equation (16) by Equation (18) can be seen by first of all setting the E field as related to the B field, via E (electrostatic) ~10<sup>12</sup> V·m<sup>−1</sup> as equivalent to a magnetic field B ~10<sup>4</sup> T (Torr) as given by <xref ref-type="bibr" rid="scirp.142316-9">
     [9]
    </xref>. In a one-second interval, if we use the input power as an experimentally supplied quantity, then the effective E field is</p>
   <p>
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          Τokamak temperature 
        </mtext> 
       </mrow> 
      </msub> 
     </mrow> 
    </math>(18)</p>
   <p>What is found is, that if Equation (17) and Equation (18) hold. Then by Wesson <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref>, pp. 242-243, if 
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    </math>, 
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    </math>. Then the temperature of a Tokamak, to good approximation would be between 30 to 100 KeV, and then one has <xref ref-type="bibr" rid="scirp.142316-10">
     [10]
    </xref></p>
   <p>
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            Tokamak temperature 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>(19)</p>
   <p>Then the power for the Tokamak is</p>
   <p>
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             </mi> 
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              <mtext>
                Τokamak temperature 
              </mtext> 
             </mrow> 
            </msub> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             9 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
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           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
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            0.87 
          </mn> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             5 
           </mn> 
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           <mn>
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           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (20)</p>
   <p>Then, per second, the author derived the following rate of production per second of a 10<sup>−34</sup> eV graviton, as, if 
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   <p>
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          </mtext> 
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                </mtext> 
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              </msub> 
             </mrow> 
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               ) 
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          <mo>
            ⋅ 
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            </mtext> 
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            ⋅ 
          </mo> 
          <msup> 
           <mi>
             c 
           </mi> 
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           <mrow> 
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              0.87 
            </mn> 
           </mrow> 
           <mrow> 
            <mrow> 
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               5 
             </mn> 
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             </mo> 
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               4 
             </mn> 
            </mrow> 
           </mrow> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
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        </mo> 
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           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mrow> 
          <msubsup> 
           <mi>
             λ 
           </mi> 
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            <mtext>
              Graviton 
            </mtext> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
        </mrow> 
        <mtext>
          scaling 
        </mtext> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (21)</p>
   <p>This graviton density business is what we will try to recover in our relic GW arguments from Torsion and we will try to make a linkage to Equation (21) with Gravitons produced via relic conditions.</p>
   <p>To do this review Graviton production via torsion.</p>
  </sec><sec id="s7">
   <title>7. Where Torsion May Allow for Understanding a Quantum Number n?</title>
   <p>Following <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref>-<xref ref-type="bibr" rid="scirp.142316-13">
     [13]
    </xref> we do the introduction of black hole physics in terms of a quantum number n.</p>
   <p>
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              entropy 
            </mtext> 
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            particles 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (22)</p>
   <p>And then a BEC condensate given by <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-13">
     [13]
    </xref> as to</p>
   <p>
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            gravitons 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           T 
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          <mi>
            B 
          </mi> 
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            H 
          </mi> 
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        </msub> 
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          ≈ 
        </mo> 
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         <mrow> 
          <msub> 
           <mi>
             T 
           </mi> 
           <mi>
             P 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
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             </mi> 
             <mrow> 
              <mtext>
                gravitons 
              </mtext> 
             </mrow> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (23)</p>
   <p>This is promising but needs to utilize <xref ref-type="bibr" rid="scirp.142316-14">
     [14]
    </xref> in which we make use of the following. First a time step</p>
   <p>
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        <mi>
          r 
        </mi> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> (24)</p>
   <p>By use of the HUP, we use Equation (25) for energy <xref ref-type="bibr" rid="scirp.142316-14">
     [14]
    </xref> for radiation of a particle pair from a black hole,</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         | 
       </mo> 
       <mi>
         E 
       </mi> 
       <mo>
         | 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <mi>
              G 
            </mi> 
            <mi>
              M 
            </mi> 
            <mi>
              δ 
            </mi> 
            <mi>
              r 
            </mi> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (25)</p>
   <p>Here we assert that the spatial variation goes as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <mi>
        r 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msub> 
       <mi>
         ℓ 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
     </mrow> 
    </math> (26)</p>
   <p>This is of a Plank length, whereas we assume in Equation (25) that the mass is a Planck sized black hole</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        M 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mi>
        α 
      </mi> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
     </mrow> 
    </math> (27)</p>
   <p>If so, we transform Equation (22) to be of the form for a “particle” pair as given in Carlip <xref ref-type="bibr" rid="scirp.142316-14">
     [14]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         | 
       </mo> 
       <mi>
         E 
       </mi> 
       <mo>
         | 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <mi>
              G 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                α 
              </mi> 
              <msub> 
               <mi>
                 M 
               </mi> 
               <mi>
                 P 
               </mi> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
            <mo>
              ⋅ 
            </mo> 
            <msub> 
             <mi>
               ℓ 
             </mi> 
             <mi>
               P 
             </mi> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (28)</p>
   <p>We argue that for small black holes, that we are talking about intense radiation from a Planck sized black hole, so we approximate Equation (28) as the mass of a relic black hole. Now using the following normalization of Planck units, as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         B 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         ℓ 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (29)</p>
   <p>And, also, the initial energy, E <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          B 
        </mi> 
        <mi>
          h 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mrow> 
          <mtext>
            quantum 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </mfrac> 
     </mrow> 
    </math> (30)</p>
   <p>We then can use for a Black hole the scaling,</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
         <mo>
           | 
         </mo> 
         <mi>
           E 
         </mi> 
         <mo>
           | 
         </mo> 
        </mrow> 
        <mo>
          ≈ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msqrt> 
            <mrow> 
             <mi>
               G 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mi>
                 α 
               </mi> 
               <msub> 
                <mi>
                  M 
                </mi> 
                <mi>
                  P 
                </mi> 
               </msub> 
              </mrow> 
              <mo>
                ) 
              </mo> 
             </mrow> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                ℓ 
              </mi> 
              <mi>
                P 
              </mi> 
             </msub> 
            </mrow> 
           </msqrt> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
        </msup> 
        <mi>
          ℏ 
        </mi> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <munder> 
         <mo>
           → 
         </mo> 
         <mrow> 
          <mi>
            G 
          </mi> 
          <mo>
            = 
          </mo> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             P 
           </mi> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mi>
            ℏ 
          </mi> 
          <mo>
            = 
          </mo> 
          <msub> 
           <mi>
             k 
           </mi> 
           <mi>
             B 
           </mi> 
          </msub> 
          <mo>
            = 
          </mo> 
          <msub> 
           <mi>
             ℓ 
           </mi> 
           <mi>
             P 
           </mi> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mi>
            c 
          </mi> 
          <mo>
            = 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
        </munder> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              / 
            </mo> 
            <mrow> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 B 
               </mi> 
               <mi>
                 H 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </mrow> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             n 
           </mi> 
           <mrow> 
            <mtext>
              quantum 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (31)</p>
   <p>We then reference Equation (23) to observe the following,</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mrow> 
          <mi>
            B 
          </mi> 
          <mi>
            H 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             N 
           </mi> 
           <mrow> 
            <mtext>
              gravitons 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
        </msqrt> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mi>
           P 
         </mi> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              / 
            </mo> 
            <mrow> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 B 
               </mi> 
               <mi>
                 H 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </mrow> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             n 
           </mi> 
           <mrow> 
            <mtext>
              quantum 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 N 
               </mi> 
               <mrow> 
                <mtext>
                  gravitons 
                </mtext> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mrow> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               / 
             </mo> 
             <mn>
               4 
             </mn> 
            </mrow> 
           </mrow> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mrow> 
          <mtext>
            quantum 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mn>
           2 
         </mn> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 N 
               </mi> 
               <mrow> 
                <mtext>
                  gravitons 
                </mtext> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mrow> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               / 
             </mo> 
             <mn>
               4 
             </mn> 
            </mrow> 
           </mrow> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (32)</p>
   <p>This is a stunning result. i.e. Equation (23) is BEC theory, but due to micro sized black holes that we assume that the number of the quantum number, n associated goes way UP. Is this implying that corresponding increases in quantum number, per black hole, n, are commensurate with increasing temperature? We start off with <xref ref-type="table" rid="table1">
     Table 1
    </xref>.</p>
   <p>
    <xref ref-type="table" rid="table1">
     Table 1
    </xref> from <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> assumes Penrose recycling of the Universe as stated in that document.</p>
   <table-wrap id="table1">
    <label>
     <xref ref-type="table" rid="table1">
      Table 1
     </xref></label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.142316-"></xref>Table 1. Distribution of black holes, prior universe to present universe.</title>
    </caption>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="aleft" width="33.34%"><p style="text-align:left">End of Prior Universe time frame</p></td> 
      <td class="aleft" width="29.16%"><p style="text-align:left">Mass (black hole):</p><p style="text-align:left">super massive end of time BH</p><p style="text-align:left">1.98910<sup>+41</sup> to about 10<sup>44</sup> grams</p></td> 
      <td class="aleft" width="37.49%"><p style="text-align:left">Number (black holes)</p><p style="text-align:left">10<sup>6</sup> to 10<sup>9</sup> of them usually from center of galaxies</p></td> 
     </tr> 
     <tr> 
      <td class="aleft" width="33.34%"><p style="text-align:left">Planck era Black hole formation</p><p style="text-align:left">Assuming start of merging of micro black hole pairs</p></td> 
      <td class="aleft" width="29.16%"><p style="text-align:left">Mass (black hole)</p><p style="text-align:left">10<sup>−5</sup> to 10<sup>−4</sup> grams (an order of magnitude of the Planck mass value)</p></td> 
      <td class="aleft" width="37.49%"><p style="text-align:left">Number (black holes)</p><p style="text-align:left">10<sup>40</sup> to about 10<sup>45</sup>, assuming that there was not too much destruction of matter-energy from the Pre Planck conditions to Planck conditions</p></td> 
     </tr> 
     <tr> 
      <td class="aleft" width="33.34%"><p style="text-align:left">Post Planck era black holes with the possibility of using Equation (1) and Equation (2) to have say 10<sup>10</sup> gravitons/second released per black hole</p></td> 
      <td class="aleft" width="29.16%"><p style="text-align:left">Mass (black hole)</p><p style="text-align:left">10 grams to say 10<sup>6</sup> grams per black hole</p></td> 
      <td class="aleft" width="37.49%"><p style="text-align:left">Number (black holes)</p><p style="text-align:left">Due to repeated Black hole pair forming a single black hole multiple time.</p><p style="text-align:left">10<sup>20</sup> to at most 10<sup>25</sup></p></td> 
     </tr> 
    </table>
   </table-wrap>
   <p>The reason for using this table is because of the modification of Dark Energy and the cosmological constant <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>. To begin this look at <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> which is akin, as we discuss later to <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           ρ 
         </mi> 
         <mi>
           Λ 
         </mi> 
        </msub> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          = 
        </mo> 
        <mstyle displaystyle="true"> 
         <mrow> 
          <munderover> 
           <mo>
             ∫ 
           </mo> 
           <mn>
             0 
           </mn> 
           <mrow> 
            <mrow> 
             <mrow> 
              <msub> 
               <mi>
                 E 
               </mi> 
               <mrow> 
                <mtext>
                  Plank 
                </mtext> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mi>
               c 
             </mi> 
            </mrow> 
           </mrow> 
          </munderover> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mn>
               4 
             </mn> 
             <mi>
               π 
             </mi> 
             <msup> 
              <mi>
                p 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
             <mtext>
               d 
             </mtext> 
             <mi>
               p 
             </mi> 
            </mrow> 
            <mrow> 
             <msup> 
              <mrow> 
               <mrow> 
                <mo>
                  ( 
                </mo> 
                <mrow> 
                 <mn>
                   2 
                 </mn> 
                 <mi>
                   π 
                 </mi> 
                 <mi>
                   ℏ 
                 </mi> 
                </mrow> 
                <mo>
                  ) 
                </mo> 
               </mrow> 
              </mrow> 
              <mn>
                3 
              </mn> 
             </msup> 
            </mrow> 
           </mfrac> 
          </mrow> 
         </mrow> 
        </mstyle> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msqrt> 
           <mrow> 
            <msup> 
             <mi>
               p 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <msup> 
             <mi>
               c 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              + 
            </mo> 
            <msup> 
             <mi>
               m 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <msup> 
             <mi>
               c 
             </mi> 
             <mn>
               4 
             </mn> 
            </msup> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                3 
              </mn> 
              <mo>
                × 
              </mo> 
              <msup> 
               <mrow> 
                <mn>
                  10 
                </mn> 
               </mrow> 
               <mrow> 
                <mn>
                  19 
                </mn> 
               </mrow> 
              </msup> 
              <mtext>
                  
              </mtext> 
              <mtext>
                GeV 
              </mtext> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                2 
              </mn> 
              <mi>
                π 
              </mi> 
              <mi>
                ℏ 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             3 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <munder> 
         <mo>
           → 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               E 
             </mi> 
             <mrow> 
              <mtext>
                Plank 
              </mtext> 
             </mrow> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mi>
             c 
           </mi> 
          </mrow> 
          <mo>
            → 
          </mo> 
          <msup> 
           <mrow> 
            <mn>
              10 
            </mn> 
           </mrow> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              30 
            </mn> 
           </mrow> 
          </msup> 
         </mrow> 
        </munder> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                2.5 
              </mn> 
              <mo>
                × 
              </mo> 
              <msup> 
               <mrow> 
                <mn>
                  10 
                </mn> 
               </mrow> 
               <mrow> 
                <mo>
                  − 
                </mo> 
                <mn>
                  11 
                </mn> 
               </mrow> 
              </msup> 
              <mtext>
                  
              </mtext> 
              <mtext>
                GeV 
              </mtext> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                2 
              </mn> 
              <mi>
                π 
              </mi> 
              <mi>
                ℏ 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             3 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (33)</p>
   <p>In <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>, the first line is the vacuum energy which is completely cancelled in their formulation of the application of Torsion. In our article, we are arguing for the second line. In fact by <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mi>
          Δ 
        </mi> 
        <mi>
          E 
        </mi> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          18 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        GeV 
      </mtext> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mrow> 
          <mtext>
            quantum 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          12 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        GeV 
      </mtext> 
     </mrow> 
    </math> (34)</p>
   <p>The term n (quantum) comes from a Corda expression as to energy level of relic black holes <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref>.</p>
   <p>We argue that our application of <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> will be commensurate with Equation (35) which uses the value given in <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> as to the following. i.e. relic black holes will contribute to the generation of a cut-off of the energy of the integral given in Equation (35) whereas what is done in Equation (35) by <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> is restricted to a different venue which is reproduced below, namely cancellation of the following by Torsion</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ρ 
       </mi> 
       <mi>
         Λ 
       </mi> 
      </msub> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <munderover> 
         <mo>
           ∫ 
         </mo> 
         <mn>
           0 
         </mn> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               E 
             </mi> 
             <mrow> 
              <mtext>
                Plank 
              </mtext> 
             </mrow> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mi>
             c 
           </mi> 
          </mrow> 
         </mrow> 
        </munderover> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <mn>
             4 
           </mn> 
           <mi>
             π 
           </mi> 
           <msup> 
            <mi>
              p 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
           <mtext>
             d 
           </mtext> 
           <mi>
             p 
           </mi> 
          </mrow> 
          <mrow> 
           <msup> 
            <mrow> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mn>
                 2 
               </mn> 
               <mi>
                 π 
               </mi> 
               <mi>
                 ℏ 
               </mi> 
              </mrow> 
              <mo>
                ) 
              </mo> 
             </mrow> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mrow> 
          <msup> 
           <mi>
             p 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            + 
          </mo> 
          <msup> 
           <mi>
             m 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              3 
            </mn> 
            <mo>
              × 
            </mo> 
            <msup> 
             <mrow> 
              <mn>
                10 
              </mn> 
             </mrow> 
             <mrow> 
              <mn>
                19 
              </mn> 
             </mrow> 
            </msup> 
            <mtext>
                
            </mtext> 
            <mtext>
              GeV 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mi>
              π 
            </mi> 
            <mi>
              ℏ 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (35)</p>
   <p>Furthermore, the claim in <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> is that there is no cosmological constant, i.e. that Torsion always cancelling Equation (17) which we view is incommensurate with <xref ref-type="table" rid="table1">
     Table 1
    </xref> as of <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>. We claim that the influence of Torsion will aid in the decomposition of what is given in <xref ref-type="table" rid="table1">
     Table 1
    </xref> and will furthermore lead to the influx of primordial black holes which we claim is responsible for the behavior of Equation (17) above.</p>
  </sec><sec id="s8">
   <title>8. Stating What Black Hole Physics Will Be Useful for in Our Modeling of Dark Energy. I.e. Inputs into the Torsion Spin Density Term</title>
   <p>In <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> we have the following, i.e., we have a spin density term of <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>. And this will be what we input black hole physics into to form a spin density term from primordial black holes.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         σ 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          71 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (36)</p>
  </sec><sec id="s9">
   <title>9. Now for the Statement of the Torsion Problem as Given in <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref></title>
   <p>The author is very much aware as to quack science as to purported torsion physics presentations and wishes to state that the torsion problem is not linked to anything other than disruption as to the initial configuration of the expansion of the universe and cosmology, more in the spirit of <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> and is nothing else. Hence, in saying this we wish to delve into what was given in <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> with a subsequent follow-up and modification:</p>
   <p>To do this, note that in <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> the vacuum energy density is stated to be</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ρ 
       </mi> 
       <mrow> 
        <mi>
          v 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mi>
          Λ 
        </mi> 
        <mmultiscripts> 
         <mi>
           c 
         </mi> 
         <mprescripts /> 
         <mrow> 
          <mi>
            e 
          </mi> 
          <mi>
            f 
          </mi> 
          <mi>
            f 
          </mi> 
         </mrow> 
         <none /> 
        </mmultiscripts> 
        <msup> 
         <mrow></mrow> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mn>
          8 
        </mn> 
        <mi>
          π 
        </mi> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> (37)</p>
   <p>Whereas the application is given in terms of an antisymmetric field strength 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         S 
       </mi> 
       <mrow> 
        <mi>
          α 
        </mi> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref>.</p>
   <p>In <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> due to the Einstein Cartan action, in terms of an SL (2, C) gauge theory, we write from <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        L 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mrow> 
       <mi>
         R 
       </mi> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            16 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mrow> 
        <msub> 
         <mi>
           S 
         </mi> 
         <mrow> 
          <mi>
            α 
          </mi> 
          <mi>
            β 
          </mi> 
          <mi>
            γ 
          </mi> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           S 
         </mi> 
         <mrow> 
          <mi>
            α 
          </mi> 
          <mi>
            β 
          </mi> 
          <mi>
            γ 
          </mi> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> (38)</p>
   <p>R here is with regards to Ricci scalar and Tensor notation and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         S 
       </mi> 
       <mrow> 
        <mi>
          α 
        </mi> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is related to a conserved current closing in on the SL (2, C) algebra as given by</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         J 
       </mi> 
       <mi>
         μ 
       </mi> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mi>
         J 
       </mi> 
       <mi>
         μ 
       </mi> 
      </msup> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mn>
         1 
       </mn> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            16 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mrow> 
      <msup> 
       <mi>
         ε 
       </mi> 
       <mrow> 
        <mi>
          μ 
        </mi> 
        <mi>
          α 
        </mi> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msup> 
      <msub> 
       <mi>
         S 
       </mi> 
       <mrow> 
        <mi>
          α 
        </mi> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (39)</p>
   <p>This is where we define</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         S 
       </mi> 
       <mrow> 
        <mi>
          α 
        </mi> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         c 
       </mi> 
       <mi>
         α 
       </mi> 
      </msub> 
      <mo>
        × 
      </mo> 
      <msub> 
       <mi>
         f 
       </mi> 
       <mrow> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (40)</p>
   <p>where 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         c 
       </mi> 
       <mi>
         α 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the structure constant for the group SL (2, C), and</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         f 
       </mi> 
       <mrow> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mover accent="true"> 
       <mi>
         g 
       </mi> 
       <mo>
         ¯ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (41)</p>
   <p>Where</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mi>
         g 
       </mi> 
       <mo>
         ¯ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
        <mo>
          , 
        </mo> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
        <mo>
          , 
        </mo> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mn>
           3 
         </mn> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (43)</p>
   <p>Is for tangent vectors to the gauge generators of SL (2, C), and also for Gauge fields 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         A 
       </mi> 
       <mi>
         γ 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mi>
          β 
        </mi> 
        <mi>
          γ 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mo>
         ∂ 
       </mo> 
       <mi>
         β 
       </mi> 
      </msub> 
      <msub> 
       <mi>
         A 
       </mi> 
       <mi>
         γ 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mo>
         ∂ 
       </mo> 
       <mi>
         γ 
       </mi> 
      </msub> 
      <msub> 
       <mi>
         A 
       </mi> 
       <mi>
         β 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           A 
         </mi> 
         <mi>
           β 
         </mi> 
        </msub> 
        <mo>
          , 
        </mo> 
        <msub> 
         <mi>
           A 
         </mi> 
         <mi>
           γ 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (44)</p>
   <p>And that there is furthermore the restriction that</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mo>
         ∂ 
       </mo> 
       <mi>
         ρ 
       </mi> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msup> 
         <mi>
           ε 
         </mi> 
         <mrow> 
          <mi>
            ρ 
          </mi> 
          <mi>
            α 
          </mi> 
          <mi>
            β 
          </mi> 
          <mi>
            γ 
          </mi> 
         </mrow> 
        </msup> 
        <msub> 
         <mi>
           S 
         </mi> 
         <mrow> 
          <mi>
            α 
          </mi> 
          <mi>
            β 
          </mi> 
          <mi>
            γ 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math> (45)</p>
   <p>Finally in the case of massless particles with torsion present, we have a space time metric</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         s 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         τ 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        + 
      </mo> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         τ 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <msup> 
       <mtext>
         d 
       </mtext> 
       <mn>
         2 
       </mn> 
      </msup> 
      <msub> 
       <mi>
         Ω 
       </mi> 
       <mn>
         3 
       </mn> 
      </msub> 
     </mrow> 
    </math> (46)</p>
   <p>where 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mtext>
         d 
       </mtext> 
       <mn>
         2 
       </mn> 
      </msup> 
      <msub> 
       <mi>
         Ω 
       </mi> 
       <mn>
         3 
       </mn> 
      </msub> 
     </mrow> 
    </math> is the metric of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         S 
       </mi> 
       <mn>
         3 
       </mn> 
      </msup> 
     </mrow> 
    </math>.</p>
   <p>Then the Einstein field equations reduce to in this torsion application, (no mass to particles) as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              a 
            </mi> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              τ 
            </mi> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msubsup> 
             <mi>
               r 
             </mi> 
             <mrow> 
              <mi>
                min 
              </mi> 
             </mrow> 
             <mn>
               4 
             </mn> 
            </msubsup> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               4 
             </mn> 
            </msup> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (47)</p>
   <p>With, if S is the so called spin scalar and identified as the basic 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ℏ 
     </mi> 
    </math> unit of spin</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mi>
          min 
        </mi> 
       </mrow> 
       <mn>
         4 
       </mn> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mn>
          3 
        </mn> 
        <msup> 
         <mi>
           G 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <msup> 
         <mi>
           S 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mn>
          8 
        </mn> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> (48)</p>
  </sec><sec id="s10">
   <title>10. How to Modify Equation (47) in the Presence of Matter via Yang Mills Fields 

    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
      <msubsup> 
   
       <mstyle mathvariant="bold" mathsize="normal">
    
        <mi>
         
     F
    
        </mi>
   
       </mstyle> 
   
       <mrow> 
    
        <mi>
         
     μ
    
        </mi>
    
        <mstyle mathvariant="bold" mathsize="normal">
     
         <mi>
           v 
         </mi>
    
        </mstyle>
   
       </mrow> 
   
       <mi>
        
    β
   
       </mi> 
  
      </msubsup> 
 
     </mrow>

    </math></title>
   <p>First of all, this involves a change of Equation (39) (20) to read</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        L 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mrow> 
       <mi>
         R 
       </mi> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            16 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mrow> 
        <msub> 
         <mi>
           S 
         </mi> 
         <mrow> 
          <mi>
            α 
          </mi> 
          <mi>
            β 
          </mi> 
          <mi>
            γ 
          </mi> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           S 
         </mi> 
         <mrow> 
          <mi>
            α 
          </mi> 
          <mi>
            β 
          </mi> 
          <mi>
            γ 
          </mi> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mrow> 
          <mn>
            4 
          </mn> 
          <msup> 
           <mi>
             g 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mrow> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <msubsup> 
       <mi>
         F 
       </mi> 
       <mrow> 
        <mi>
          μ 
        </mi> 
        <mi>
          v 
        </mi> 
       </mrow> 
       <mi>
         β 
       </mi> 
      </msubsup> 
      <msubsup> 
       <mi>
         F 
       </mi> 
       <mi>
         β 
       </mi> 
       <mrow> 
        <mi>
          μ 
        </mi> 
        <mi>
          ν 
        </mi> 
       </mrow> 
      </msubsup> 
     </mrow> 
    </math> (49)</p>
   <p>And eventually we have a re-do of Equation (47) to read as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              a 
            </mi> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              τ 
            </mi> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               β 
             </mi> 
             <mn>
               1 
             </mn> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               β 
             </mi> 
             <mn>
               2 
             </mn> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               4 
             </mn> 
            </msup> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (50)</p>
   <p>If 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        g 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        ℏ 
      </mi> 
      <mi>
        c 
      </mi> 
     </mrow> 
    </math>we have 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         β 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mi>
          min 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mi>
         β 
       </mi> 
       <mn>
         2 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mi>
          min 
        </mi> 
       </mrow> 
       <mn>
         4 
       </mn> 
      </msubsup> 
     </mrow> 
    </math>, and the minimum radius is identified with a Planck Radius so then</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              a 
            </mi> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              d 
            </mtext> 
            <mi>
              τ 
            </mi> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 β 
               </mi> 
               <mn>
                 1 
               </mn> 
              </msub> 
              <mo>
                = 
              </mo> 
              <msubsup> 
               <mi>
                 ℓ 
               </mi> 
               <mi>
                 P 
               </mi> 
               <mn>
                 2 
               </mn> 
              </msubsup> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 β 
               </mi> 
               <mn>
                 2 
               </mn> 
              </msub> 
              <mo>
                = 
              </mo> 
              <msubsup> 
               <mi>
                 ℓ 
               </mi> 
               <mi>
                 P 
               </mi> 
               <mn>
                 4 
               </mn> 
              </msubsup> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               4 
             </mn> 
            </msup> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (51)</p>
   <p>Eventually in the case of an unpolarized spinning fluid in the immediate aftermath of the big bang, we would see a Roberson Walker universe given as, if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       σ 
     </mi> 
    </math> is a torsion spin term added due to <xref ref-type="bibr" rid="scirp.142316-16">
     [16]
    </xref> as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mover accent="true"> 
            <mover accent="true"> 
             <mi>
               R 
             </mi> 
             <mo>
               ˜ 
             </mo> 
            </mover> 
            <mo>
              ˙ 
            </mo> 
           </mover> 
           <mover accent="true"> 
            <mi>
              R 
            </mi> 
            <mo>
              ˜ 
            </mo> 
           </mover> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mi>
          ρ 
        </mi> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          Λ 
        </mi> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           k 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mover accent="true"> 
          <mi>
            R 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (52)</p>
  </sec><sec id="s11">
   <title>11. What <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> Does as to Equation (52) versus What We Would Do and Why</title>
   <p>In the case of <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref>, we would see 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       σ 
     </mi> 
    </math> be identified as due to torsion so that Equation (52) reduces to</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mover accent="true"> 
            <mover accent="true"> 
             <mi>
               R 
             </mi> 
             <mo>
               ˜ 
             </mo> 
            </mover> 
            <mo>
              ˙ 
            </mo> 
           </mover> 
           <mover accent="true"> 
            <mi>
              R 
            </mi> 
            <mo>
              ˜ 
            </mo> 
           </mover> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mi>
         ρ 
       </mi> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           k 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mover accent="true"> 
          <mi>
            R 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (53)</p>
   <p>The claim is made in <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> that this is due to spinning particles which remain invariant so the cosmological vacuum energy, or cosmological constant is always cancelled.</p>
   <p>Our approach instead will yield <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mover accent="true"> 
            <mover accent="true"> 
             <mi>
               R 
             </mi> 
             <mo>
               ˜ 
             </mo> 
            </mover> 
            <mo>
              ˙ 
            </mo> 
           </mover> 
           <mover accent="true"> 
            <mi>
              R 
            </mi> 
            <mo>
              ˜ 
            </mo> 
           </mover> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mi>
         ρ 
       </mi> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           Λ 
         </mi> 
         <mrow> 
          <mtext>
            0bserved 
          </mtext> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           k 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mover accent="true"> 
          <mi>
            R 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (54)</p>
   <p>I.e. the observed cosmological constant 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Λ 
       </mi> 
       <mrow> 
        <mtext>
          0bserved 
        </mtext> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is 10<sup>−122</sup> times smaller than the initial vacuum energy.</p>
   <p>The main reason for the difference in Equation (53) and Equation (54) is in the following observation.</p>
   <p>Mainly that the reason for the existence of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         σ 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> is due to the dynamics of spinning black holes in the precursor to the big bang, to the Planckian regime, of space time, whereas in the aftermath of the big bang, we would have a vanishing of the torsion spin term. i.e. <xref ref-type="table" rid="table1">
     Table 1
    </xref> dynamics in the aftermath of the Planckian regime of space time would largely eliminate the 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         σ 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> term.</p>
  </sec><sec id="s12">
   <title>12. Filling in the Details of the Equation (53) Collapse of the Cosmological Term, versus the Situation Given in Equation (54) via Numerical Values</title>
   <p>First look at numbers provided by <xref ref-type="bibr" rid="scirp.142316-16">
     [16]
    </xref> as to inputs, i.e. these are very revealing</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Λ 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <msup> 
       <mi>
         c 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          87 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (56)</p>
   <p>This is the number for the vacuum energy and this enormous value is 10<sup>122</sup> times larger than the observed cosmological constant. Torsion physics, as given by <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref> is solely to remove this giant number.</p>
   <p>In order to remove it, the reference <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> proceeds to make the following identification, namely</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          Λ 
        </mi> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math> (57)</p>
   <p>What we are arguing is that instead, one is seeing, instead <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           Λ 
         </mi> 
         <mrow> 
          <mi>
            P 
          </mi> 
          <mi>
            l 
          </mi> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          122 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        × 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             Λ 
           </mi> 
           <mrow> 
            <mi>
              P 
            </mi> 
            <mi>
              l 
            </mi> 
           </mrow> 
          </msub> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (58)</p>
   <p>Our timing as to Equation (56) is to unleash a Planck time interval t about 10<sup>−43</sup> seconds.</p>
   <p>As to Equation (57) versus Equation (58), the creation of the torsion term is due to a presumed particle density of</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          98 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mtext>
          cm 
        </mtext> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (59)</p>
   <p>Finally, we have a spin density term of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         σ 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          71 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> which is due to innumerable black holes initially.</p>
  </sec><sec id="s13">
   <title>13. Future Works to Be Commenced as to Derivational Tasks</title>
   <p>We will assume for the moment that Equation (56) and Equation (57) share in common Equation (59).</p>
   <p>It appears to be trivial, a mere round off, but I can assure you the difference is anything but trivial. And this is where <xref ref-type="table" rid="table1">
     Table 1
    </xref> really plays a role in terms of why there is a torsion term to begin with, i.e. will make the following determination, i.e.</p>
   <p>The term of “spin density” in Equation (56) by Equation (59) is defined to be an ad hoc creation, as to <xref ref-type="bibr" rid="scirp.142316-13">
     [13]
    </xref>. No description as to its origins is really offered.</p>
   <p>1<sup>st</sup></p>
   <p>We state that in the future a task will be to derive in a coherent fashion the following, i.e. the term of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> arising as a result of the dynamics of <xref ref-type="table" rid="table1">
     Table 1
    </xref>, as given in the manuscript.</p>
   <p>2<sup>nd</sup>,</p>
   <p>We state that the term 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> is due to initial micro black holes, as to the creation of a Cosmological term.</p>
   <p>In the case of Pre Planckian space-time the idea is to do the following <xref ref-type="bibr" rid="scirp.142316-16">
     [16]
    </xref>, i.e. if we have an inflaton field <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
         <mo>
           | 
         </mo> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msub> 
           <mi>
             p 
           </mi> 
           <mi>
             α 
           </mi> 
          </msub> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             x 
           </mi> 
           <mi>
             α 
           </mi> 
          </msup> 
         </mrow> 
         <mo>
           | 
         </mo> 
        </mrow> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mi>
           L 
         </mi> 
         <mi>
           l 
         </mi> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mi>
           h 
         </mi> 
         <mi>
           c 
         </mi> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mtext>
               d 
             </mtext> 
             <mi>
               l 
             </mi> 
            </mrow> 
            <mi>
              l 
            </mi> 
           </mfrac> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <munder> 
         <mo>
           → 
         </mo> 
         <mrow> 
          <mi>
            α 
          </mi> 
          <mo>
            = 
          </mo> 
          <mn>
            0 
          </mn> 
         </mrow> 
        </munder> 
        <mrow> 
         <mo>
           | 
         </mo> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
          <msub> 
           <mi>
             p 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mtext>
            d 
          </mtext> 
          <msup> 
           <mi>
             x 
           </mi> 
           <mn>
             0 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           | 
         </mo> 
        </mrow> 
        <mo>
          ≃ 
        </mo> 
        <mrow> 
         <mo>
           | 
         </mo> 
         <mrow> 
          <mi>
            Δ 
          </mi> 
          <mi>
            E 
          </mi> 
          <mi>
            Δ 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
         <mo>
           | 
         </mo> 
        </mrow> 
        <mo>
          ≈ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             h 
           </mi> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msubsup> 
             <mi>
               a 
             </mi> 
             <mrow> 
              <mi>
                i 
              </mi> 
              <mi>
                n 
              </mi> 
              <mi>
                i 
              </mi> 
              <mi>
                t 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msubsup> 
            <mi>
              ϕ 
            </mi> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mi>
               t 
             </mi> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <mfrac> 
         <mi>
           L 
         </mi> 
         <mi>
           l 
         </mi> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mi>
           h 
         </mi> 
         <mi>
           c 
         </mi> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mtext>
               d 
             </mtext> 
             <mi>
               l 
             </mi> 
            </mrow> 
            <mi>
              l 
            </mi> 
           </mfrac> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ≈ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             h 
           </mi> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msubsup> 
             <mi>
               a 
             </mi> 
             <mrow> 
              <mi>
                i 
              </mi> 
              <mi>
                n 
              </mi> 
              <mi>
                i 
              </mi> 
              <mi>
                t 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msubsup> 
            <mi>
              ϕ 
            </mi> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 t 
               </mi> 
               <mrow> 
                <mi>
                  i 
                </mi> 
                <mi>
                  n 
                </mi> 
                <mi>
                  i 
                </mi> 
                <mi>
                  t 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (60)</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142316-"></xref>Making use of all this leads to making sense of the quantum number n as given by reference to black holes, <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref> 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          B 
        </mi> 
        <mi>
          h 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mrow> 
          <mtext>
            quantum 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </mfrac> 
     </mrow> 
    </math>.</p>
   <p>3<sup>rd</sup></p>
   <p>The conclusion of <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> states that Equation (60) would remain invariant for the life of the evolution of the universe. We make no such assumption. We assume that, as will be followed up later Equation (58) (38) is due to relic black holes with the suppression of the initially gigantic cosmological vacuum energy.</p>
   <p>The details of what follows after this initial period of inflation remain a task to be completed in full generality but we are still assuming as a given the following inputs <xref ref-type="bibr" rid="scirp.142316-13">
     [13]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           t 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <msub> 
         <mi>
           a 
         </mi> 
         <mrow> 
          <mtext>
            initial 
          </mtext> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           t 
         </mi> 
         <mi>
           ν 
         </mi> 
        </msup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <mi>
          ϕ 
        </mi> 
        <mo>
          = 
        </mo> 
        <mi>
          ln 
        </mi> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <msqrt> 
            <mrow> 
             <mfrac> 
              <mrow> 
               <mn>
                 8 
               </mn> 
               <mi>
                 π 
               </mi> 
               <mi>
                 G 
               </mi> 
               <msub> 
                <mi>
                  V 
                </mi> 
                <mn>
                  0 
                </mn> 
               </msub> 
              </mrow> 
              <mrow> 
               <mi>
                 ν 
               </mi> 
               <mo>
                 ⋅ 
               </mo> 
               <mrow> 
                <mo>
                  ( 
                </mo> 
                <mrow> 
                 <mn>
                   3 
                 </mn> 
                 <mi>
                   ν 
                 </mi> 
                 <mo>
                   − 
                 </mo> 
                 <mn>
                   1 
                 </mn> 
                </mrow> 
                <mo>
                  ) 
                </mo> 
               </mrow> 
              </mrow> 
             </mfrac> 
            </mrow> 
           </msqrt> 
           <mo>
             ⋅ 
           </mo> 
           <mi>
             t 
           </mi> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <mfrac> 
             <mi>
               ν 
             </mi> 
             <mrow> 
              <mn>
                16 
              </mn> 
              <mi>
                π 
              </mi> 
              <mi>
                G 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
          </msqrt> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <mover accent="true"> 
         <mi>
           ϕ 
         </mi> 
         <mo>
           ˙ 
         </mo> 
        </mover> 
        <mo>
          = 
        </mo> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mi>
             ν 
           </mi> 
           <mrow> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
            <mi>
              G 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msqrt> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           t 
         </mi> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             H 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mover accent="true"> 
          <mi>
            ϕ 
          </mi> 
          <mo>
            ˙ 
          </mo> 
         </mover> 
        </mfrac> 
        <mo>
          ≈ 
        </mo> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
            <mi>
              G 
            </mi> 
           </mrow> 
           <mi>
             ν 
           </mi> 
          </mfrac> 
         </mrow> 
        </msqrt> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          t 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           T 
         </mi> 
         <mn>
           4 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mrow> 
            <mn>
              1.66 
            </mn> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             g 
           </mi> 
           <mo>
             ∗ 
           </mo> 
          </msub> 
         </mrow> 
         <mrow> 
          <msubsup> 
           <mi>
             m 
           </mi> 
           <mi>
             P 
           </mi> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
        </mfrac> 
        <mo>
          ≈ 
        </mo> 
        <msup> 
         <mn>
           10 
         </mn> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            5 
          </mn> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (61)</p>
   <p>1<sup>st</sup> CONCLUSION, how meeting conditions for applying Torsion to obtain the cosmological constant and DE modifies black hole physics in the early universe.</p>
   <p>First of all, it puts a premium upon our <xref ref-type="table" rid="table1">
     Table 1
    </xref> as given and is shown in <xref ref-type="bibr" rid="scirp.142316-12">
     [12]
    </xref>. Secondly it means utilization of Equation (36) which takes into account the black hole energy equation given by Corda in <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref> and it also means that the spin density term as given in Equation (38) is freely utilized.</p>
   <p>We refer to black hole creation as given by torsion this way as a correction to <xref ref-type="bibr" rid="scirp.142316-11">
     [11]
    </xref> largely due to the insufficiency of black hole theory.</p>
   <p>Quote</p>
   <p>Black holes of masses sufficiency smaller than a solar mass cannot be formed by gravitational collapse of a star; such miniholes can only form in the early stages of the universe, from fluctuations in the very dense primordial matter.</p>
   <p>End of quote</p>
   <p>Our torsion argument is directly due to this acknowledgment and is due to the sterility of much theoretical thinking, as well as the tremendously important Equation (32) which is due to Corda <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref>.</p>
   <p>Corda himself <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref> has alluded to a path forward in such treatment of how black holes can be modeled which leads to Equation (60).</p>
   <p>In addition, we outlined the stunning result as given as of Equation (34) as far as a more than an inverse relationship between graviton number, per generated black hole (presumably primordial) and a quantum number n, attached to a black hole as due to <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref>. What we see is that if we have small black holes, with BEC characteristics with small number of gravitons, per primordial black hole, that the quantum number n climbs dramatically. We need to obtain the complete dynamics of this relationship as it pertains to how very small black holes have high quantum number n, which we presume is commensurate with initially high temperatures.</p>
   <p>The details of this development as well as its tie into the dynamics of <xref ref-type="table" rid="table1">
     Table 1
    </xref> as given and Torsion have to be fine tuned.</p>
   <p>More work needs to be done so we can turn early universe gravitational generation and black hole physics into an empirical science.</p>
   <p>2<sup>nd</sup> CONCLUSION, looking directly at a modification of the Black holes has no hair theorem, via the inputs of this document.</p>
   <p>In <xref ref-type="bibr" rid="scirp.142316-17">
     [17]
    </xref> we have the essential black holes have no hair theorem which can be seen roughly as</p>
   <p>Quote</p>
   <p>The idea is that beyond mass, charge and spin, black holes don't have distinguishing features, no hairstyle, cut or color to tell them apart.</p>
   <p>End of quote</p>
   <p>How do we get about this? Note that in <xref ref-type="bibr" rid="scirp.142316-18">
     [18]
    </xref> there is a pseudo extension which we can chalk up to Hawking; but in order to apply a more direct treatment we go to what is given in <xref ref-type="bibr" rid="scirp.142316-30">
     [30]
    </xref>.</p>
   <p>i.e. we go to formula 65 of that reference. This will give a variation of the radius of a black hole, over the radius, according to a quantum number n AGAIN. Before we get there we will do some initial work up to that quantum number, n as used in formula 65 of reference <xref ref-type="bibr" rid="scirp.142316-19">
     [19]
    </xref>.</p>
   <p>i.e. using our Equation (14) for N and also the Planck scale normalization as given by</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         B 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mo>
        = 
      </mo> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         ℓ 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>, and if we take 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
      <mi>
        a 
      </mi> 
      <mo>
        ˜ 
      </mo> 
     </mover> 
    </math> approximately scaled to 1 as well we have that if</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         | 
       </mo> 
       <mi>
         N 
       </mi> 
       <mo>
         | 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <mrow> 
       <mo>
         | 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           N 
         </mi> 
         <mrow> 
          <mtext>
            gravitons 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         | 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mn>
              5 
            </mn> 
            <mi>
              t 
            </mi> 
           </mrow> 
           <mrow> 
            <msup> 
             <mrow> 
              <mn>
                64 
              </mn> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <msup> 
             <mi>
               π 
             </mi> 
             <mn>
               4 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           5 
         </mn> 
        </mrow> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (62)</p>
   <p>Due to using <xref ref-type="bibr" rid="scirp.142316-13">
     [13]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        M 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msqrt> 
       <mi>
         N 
       </mi> 
      </msqrt> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math> (63)</p>
   <p>M here being linked to the mass of a BEC black hole, and also using the following for the loss of a black hole, over time i.e. <xref ref-type="bibr" rid="scirp.142316-14">
     [14]
    </xref>.</p>
   <p>That we begin with the model as to how a black hole mass, M, could lose a loss of its essence. Here, M is a mass, T is temperature, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
      <mi>
        a 
      </mi> 
      <mo>
        ˜ 
      </mo> 
     </mover> 
    </math> is a proportionality term, i.e. what we reference in the primordial era</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mfrac> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          M 
        </mi> 
       </mrow> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mover accent="true"> 
       <mi>
         a 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         T 
       </mi> 
       <mn>
         4 
       </mn> 
      </msup> 
     </mrow> 
    </math> (64)</p>
   <p>In terms of having T as temperature related to black hole mass we use</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        T 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          ℏ 
        </mi> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mn>
          8 
        </mn> 
        <mi>
          π 
        </mi> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           B 
         </mi> 
        </msub> 
        <mi>
          G 
        </mi> 
        <mi>
          M 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (65)</p>
   <p>This leads to, if indeed Equation (64) is observed</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msup> 
       <mi>
         M 
       </mi> 
       <mn>
         5 
       </mn> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          loss 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            5 
          </mn> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mn>
              64 
            </mn> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mover accent="true"> 
         <mi>
           a 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             ℏ 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mrow> 
            <mn>
              12 
            </mn> 
           </mrow> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             π 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
          <msubsup> 
           <mi>
             k 
           </mi> 
           <mi>
             B 
           </mi> 
           <mn>
             4 
           </mn> 
          </msubsup> 
          <msup> 
           <mi>
             G 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> (66)</p>
   <p>Also use</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           | 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             N 
           </mi> 
           <mrow> 
            <mtext>
              gravitons 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           | 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
      </msup> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             p 
           </mi> 
          </msub> 
          <mo>
            ≡ 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
      </msup> 
      <mo>
        ≈ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            5 
          </mn> 
          <mi>
            t 
          </mi> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mn>
              64 
            </mn> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <msup> 
           <mi>
             π 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (67)</p>
   <p>Then use the last equation of Equation (14) to obtain, a quantum number associated with a graviton just outside a BEC primordial black hole</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mtext>
          graviton quantum number 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ≡ 
      </mo> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mtext>
          graviton 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mrow> 
            <mn>
              64 
            </mn> 
           </mrow> 
           <mrow> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               / 
             </mo> 
             <mrow> 
              <mn>
                10 
              </mn> 
             </mrow> 
            </mrow> 
           </mrow> 
          </msup> 
          <msup> 
           <mi>
             π 
           </mi> 
           <mrow> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               / 
             </mo> 
             <mn>
               5 
             </mn> 
            </mrow> 
           </mrow> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mn>
             5 
           </mn> 
           <mrow> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               / 
             </mo> 
             <mrow> 
              <mn>
                20 
              </mn> 
             </mrow> 
            </mrow> 
           </mrow> 
          </msup> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mi>
             t 
           </mi> 
           <mrow> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               / 
             </mo> 
             <mrow> 
              <mn>
                20 
              </mn> 
             </mrow> 
            </mrow> 
           </mrow> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2.16245415907 
        </mn> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           t 
         </mi> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mn>
              20 
            </mn> 
           </mrow> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (68)</p>
   <p>Assuming Planck scale time, or close to it, and renormalization to have Planck time as set to 1.</p>
   <p>This means then that the quantum number, n associated with a graviton with respect to a Planck sized black hole would be close to 2, initially.</p>
   <p>We assert that this value of n, so obtained, as to gravitons would be as to the Corda result on Equation (12) (32) the following</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
      <mtr> 
       <mtd> 
        <mi>
          n 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            black holes 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <mi>
          N 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            graviton number per black hole 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mtext>
            
        </mtext> 
        <mtext>
            
        </mtext> 
        <mo>
          × 
        </mo> 
        <mi>
          n 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            quantum number per graviton 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (69)</p>
   <p>The left hand side of Equation (69) would be fully commensurate with Equation (12) of Corda’s black hole quantum number <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref>.</p>
   <p>The right hand side of Equation (69) would be commensurate with n being for a quantum number per graviton associated per black hole.</p>
   <p>If there are a lot of gravitons, associated with a primordial black hole, this would commence with a very high initial quantum number, n (black holes) associated Cordas great result, as of <xref ref-type="bibr" rid="scirp.142316-15">
     [15]
    </xref>.</p>
   <p>Note that in future works, I told the onlookers that the original idea of my talk was to consider a black hole joined to a White Hole and to consider the generation of quantum number n, in the throat of a connecting worm hole between the black hole and white hole. This also is akin to <xref ref-type="bibr" rid="scirp.142316-20">
     [20]
    </xref>.</p>
  </sec><sec id="s14">
   <title>14. Part 4. Looking at a Worm Hole Connecting a Black Hole and a White Hole, and the Possibility of a Quantum Number n Emerging</title>
   <p>In doing this we should note that we are assuming as a future work that there would be black holes, in our initial configuration, plus a white hole in the immediate pre inflationary regime. Likely in a recycled universe. Reference <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref> is what we will start off with <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref> and its given metric as far as a black hole to white hole solution.</p>
   <p>Namely</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         S 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
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        − 
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        A 
      </mi> 
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         ( 
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          r 
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          , 
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          a 
        </mi> 
       </mrow> 
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         ) 
       </mo> 
      </mrow> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        + 
      </mo> 
      <mi>
        B 
      </mi> 
      <msup> 
       <mrow> 
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           ( 
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            r 
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            , 
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            a 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         r 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        + 
      </mo> 
      <msup> 
       <mi>
         g 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         Ω 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (70)</p>
   <p>We can perform a major simplification by setting, then</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        A 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        B 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        f 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (71)</p>
   <p>In doing so, <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref> gives us the following stress energy tensor values as give</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           t 
         </mi> 
         <mi>
           t 
         </mi> 
        </msubsup> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mi>
             g 
           </mi> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               f 
             </mi> 
             <mo>
               ′ 
             </mo> 
            </msup> 
            <msup> 
             <mi>
               g 
             </mi> 
             <mo>
               ′ 
             </mo> 
            </msup> 
            <mo>
              + 
            </mo> 
            <mn>
              2 
            </mn> 
            <mi>
              f 
            </mi> 
            <msup> 
             <mi>
               g 
             </mi> 
             <mo>
               ″ 
             </mo> 
            </msup> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            − 
          </mo> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <msup> 
             <mi>
               g 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <mi>
              f 
            </mi> 
            <msup> 
             <msup> 
              <mi>
                g 
              </mi> 
              <mo>
                ′ 
              </mo> 
             </msup> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           r 
         </mi> 
         <mi>
           r 
         </mi> 
        </msubsup> 
        <mo>
          = 
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           1 
         </mn> 
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          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
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        </mfrac> 
        <mo>
          ⋅ 
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           ( 
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             1 
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             g 
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            ⋅ 
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             ( 
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               f 
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           </mrow> 
           <mo>
             ) 
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            − 
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           <mn>
             1 
           </mn> 
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            <msup> 
             <mi>
               g 
             </mi> 
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               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
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                g 
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                ′ 
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               2 
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             ) 
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          </mrow> 
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           ) 
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        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           θ 
         </mi> 
         <mi>
           θ 
         </mi> 
        </msubsup> 
        <mo>
          = 
        </mo> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           ϕ 
         </mi> 
         <mi>
           ϕ 
         </mi> 
        </msubsup> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
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          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
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           ( 
         </mo> 
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           <mn>
             1 
           </mn> 
           <mi>
             g 
           </mi> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <msup> 
             <mi>
               f 
             </mi> 
             <mo>
               ′ 
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            </msup> 
            <msup> 
             <mi>
               g 
             </mi> 
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               ′ 
             </mo> 
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            <mo>
              + 
            </mo> 
            <mi>
              f 
            </mi> 
            <msup> 
             <mi>
               g 
             </mi> 
             <mo>
               ″ 
             </mo> 
            </msup> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            + 
          </mo> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mn>
             2 
           </mn> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <msup> 
            <mi>
              f 
            </mi> 
            <mo>
              ″ 
            </mo> 
           </msup> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (72)</p>
   <p>In doing this, we will choose the primed coordinate as representing a derivative with respect to r.</p>
   <p>Also in the case of black hole to white hole joining, we will be looking at a gluing surface as to the worm hole joining a black hole to white hole given as with regards to a gluing surface connecting a black hole to a white hole which we give as 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ξ 
     </mi> 
    </math>. And 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mover accent="true"> 
      <mover accent="true"> 
       <mi>
         n 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mo>
        ˜ 
      </mo> 
     </mover> 
    </math> is a quantum gravity index. Note that in <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref> the authors often set it at 3, if so then for a black hole, to white hole to worm hole configuration they give</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mi>
        g 
      </mi> 
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          r 
        </mi> 
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         { 
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                     r 
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                 ) 
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             <mover accent="true"> 
              <mover accent="true"> 
               <mi>
                 n 
               </mi> 
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             </mover> 
            </msup> 
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              , 
            </mo> 
           </mrow> 
          </mtd> 
          <mtd columnalign="left"> 
           <mrow> 
            <mtext>
              when 
            </mtext> 
            <mtext>
                
            </mtext> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                r 
              </mi> 
              <mo>
                ≤ 
              </mo> 
              <mi>
                ξ 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
          </mtd> 
         </mtr> 
         <mtr columnalign="left"> 
          <mtd columnalign="left"> 
           <mrow> 
            <msup> 
             <mi>
               r 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              , 
            </mo> 
           </mrow> 
          </mtd> 
          <mtd columnalign="left"> 
           <mrow> 
            <mtext>
              when 
            </mtext> 
            <mtext>
                
            </mtext> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                r 
              </mi> 
              <mo>
                &gt; 
              </mo> 
              <mi>
                ρ 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
          </mtd> 
         </mtr> 
        </mtable> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> (73)</p>
   <p>We then make the following connection to energy density in a black hole to white hole system, i.e.</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           ρ 
         </mi> 
         <mrow> 
          <mtext>
            black hole white hole wormhole 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          ≡ 
        </mo> 
        <mo>
          − 
        </mo> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           r 
         </mi> 
         <mi>
           r 
         </mi> 
        </msubsup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ≈ 
        </mo> 
        <mi>
          ℏ 
        </mi> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mtext>
            black hole white hole wormhole 
          </mtext> 
         </mrow> 
        </msub> 
        <msub> 
         <mover accent="true"> 
          <mi>
            n 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
         <mrow> 
          <mtext>
            black hole white hole wormhole 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (74)</p>
   <p>This will lead to, if we use Planck units where we normalize h bar to being 1, of</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mover accent="true"> 
          <mi>
            n 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
         <mrow> 
          <mtext>
            black hole white hole wormhole 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mi>
             g 
           </mi> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
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           <mo>
             ( 
           </mo> 
           <mrow> 
            <msup> 
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               f 
             </mi> 
             <mo>
               ′ 
             </mo> 
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               g 
             </mi> 
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               ′ 
             </mo> 
            </msup> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            − 
          </mo> 
          <mfrac> 
           <mn>
             1 
           </mn> 
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            <msup> 
             <mi>
               g 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
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              − 
            </mo> 
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              f 
            </mi> 
            <msup> 
             <msup> 
              <mi>
                g 
              </mi> 
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                ′ 
              </mo> 
             </msup> 
             <mn>
               2 
             </mn> 
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           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msub> 
           <mi>
             ω 
           </mi> 
           <mrow> 
            <mtext>
              black hole white hole wormhole 
            </mtext> 
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    </math> (75)</p>
   <p>If we are restricting ourselves to quantum geometry at the start of expansion of the universe, it means that say we can set these values to be compared to the inputs of quantum number n used to specify a quantum number n, and furthermore if</p>
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   <p>We get further restrictions as to the quantum number in Equation (75) when we compare it to where we had a value of n given in the first section of our document.</p>
   <p>Furthermore, it means that we can use this to model say, with additional work in a future project how a white hole (specified as in the prior universe.</p>
  </sec><sec id="s15">
   <title>15. And Now for a Grand Slam, i.e. the Connection We Have Been Waiting for, i.e. Quantum n, Primordial Black Holes. And Light Spectrum Issues</title>
   <p>Key to doing this is to take into consideration. i.e. this is the point where we can take up the following <xref ref-type="bibr" rid="scirp.142316-16">
     [16]
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     [22]
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     [24]
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   <p>Then as to the follow up to NLED and signals from primordial processes <xref ref-type="bibr" rid="scirp.142316-26">
     [26]
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                 + 
               </mo> 
               <mn>
                 32 
               </mn> 
               <mover accent="true"> 
                <mi>
                  λ 
                </mi> 
                <mo>
                  ⌢ 
                </mo> 
               </mover> 
               <mrow> 
                <mo>
                  ( 
                </mo> 
                <mrow> 
                 <mtext>
                   defined 
                 </mtext> 
                </mrow> 
                <mo>
                  ) 
                </mo> 
               </mrow> 
               <mo>
                 ⋅ 
               </mo> 
               <msub> 
                <mi>
                  μ 
                </mi> 
                <mn>
                  0 
                </mn> 
               </msub> 
               <mi>
                 ω 
               </mi> 
               <mo>
                 ⋅ 
               </mo> 
               <msubsup> 
                <mi>
                  B 
                </mi> 
                <mn>
                  0 
                </mn> 
                <mn>
                  2 
                </mn> 
               </msubsup> 
              </mrow> 
             </msqrt> 
             <mo>
               − 
             </mo> 
             <msub> 
              <mi>
                α 
              </mi> 
              <mn>
                0 
              </mn> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             4 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (81)</p>
   <p>Where the following is possibly linkable to minimum frequencies linked to E and M fields, and possibly relic Gravitons <xref ref-type="bibr" rid="scirp.142316-26">
     [26]
    </xref> <xref ref-type="bibr" rid="scirp.142316-27">
     [27]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        B 
      </mi> 
      <mo>
        &gt; 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mrow> 
          <mn>
            10 
          </mn> 
          <msub> 
           <mi>
             μ 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <mi>
            ω 
          </mi> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (82)</p>
   <p>Furthermore, the frequency, as given in Equation (82) (105) would be tied into Equation (34) via the n of that equation as well as specified by <xref ref-type="bibr" rid="scirp.142316-28">
     [28]
    </xref> on its page 111, where we have</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ω 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </msub> 
      <mi>
        c 
      </mi> 
      <mi>
        k 
      </mi> 
     </mrow> 
    </math> (83)</p>
   <p>Here 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is nearly zero, as given in Equation (100), and the entire frequency in terms of k, as a wave number as given as this construction would have this consideration, namely.</p>
   <p>A black hole in a traditional sense has no frequency as we normally think of it, or a wave number because it is not a wave phenomenon, but the gravitational waves emitted by a black hole when it interacts with other massive objects can be described by a wave number, which is related to the wavelength of the gravitational wave it creates.</p>
   <p>These details would be important as to obtain ideas as to data sets which would satisfy multi messenger astronomy namely the discussion as given in Mohanty, <xref ref-type="bibr" rid="scirp.142316-29">
     [29]
    </xref> namely a temperature, with scale factor as given in his page 261</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        T 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mi>
           g 
         </mi> 
         <mo>
           ∗ 
         </mo> 
        </msup> 
        <mi>
          a 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (84)</p>
   <p>With temperature T, as proportional to quantum number n as specified, whereas k as in Equation (83) may be tied into the details of Equation (99) of our manuscript.</p>
   <p>Once our ideas of a candidate magnetic field are clarified, i.e. we can then examine some of the ideas of <xref ref-type="bibr" rid="scirp.142316-29">
     [29]
    </xref> which can make a connection analytically to muli messenger Astrophysics explicit <xref ref-type="bibr" rid="scirp.142316-30">
     [30]
    </xref> i.e. for the record consider what is brought up in <xref ref-type="bibr" rid="scirp.142316-17">
     [17]
    </xref> which we also assert can be linked to Tokamaks, i.e. Compare this with tokamak conclusions.</p>
  </sec><sec id="s16">
   <title>16. GW Generation Due to the Thermal Output of Plasma Burning, and Linkage to the Initial GW Strain and Frequency Problem versus Values of Strain and Frequency of GW Today, from the Initial Pre Big Bang</title>
   <p>Further elaboration of this matter in the experimental detection of experimental data sets for massive gravity lies in the viability of the expression derived, namely Equation (19) 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          27 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> for a GW detected 5 meters above a Tokamak represents the decrease in strain, by a factor of about 100, from details which are further elaborated upon in <xref ref-type="bibr" rid="scirp.142316-18">
     [18]
    </xref>, whereas in the center of the Tokamak, we would have, say, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mtext>
          2nd term 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          26 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        - 
      </mtext> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          27 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>. I.e. a difference of 2 orders of magnitude. We state that our rough estimate is that we would see about the same strain values, in the initial starting point of the universe we would have, say 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          25 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> decreasing to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          26 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        - 
      </mtext> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          27 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> today. I.e. a comparatively small change in strain amplitude. Contrast this with the e-folding issues, of <xref ref-type="bibr" rid="scirp.142316-18">
     [18]
    </xref> whereas we would have a difference of 10<sup>26</sup> in frequency magnitude, with 10<sup>10</sup> Hz initially, for GW at start of big bang, decreasing to 10<sup>-16</sup> Hz, due to inflation. If we confirm that last statement observationally, we have confirmed the <xref ref-type="bibr" rid="scirp.142316-19">
     [19]
    </xref> e-folding prediction and taken a huge step forward in observational cosmology. Eventually we could investigate, also, early universe polarization of GW.</p>
  </sec><sec id="s17">
   <title>17. What Can We Say about the Stability of a Plasma Generated Signal Creating GW?</title>
   <p>Among other things to consider, if we do Tokamak generation of GW simulations right as to GW generation we will be able to enhance the likelihood <xref ref-type="bibr" rid="scirp.142316-19">
     [19]
    </xref> <xref ref-type="bibr" rid="scirp.142316-31">
     [31]
    </xref>-<xref ref-type="bibr" rid="scirp.142316-33">
     [33]
    </xref> of having a stable signal (if that is what the Tokamak predicts), or an unstable signal (if that is what the Tokamak predicts) of the LISA data sets. Not necessarily in a fool proof way, but it would be a baseline to review and to refer back to. Another item to consider. Not just as to the type of GW polarizations, and stability of the signal, but also a way to infer through trial and error the duration of the phenomenon creating very early universe GW generation. This is in outlook similar to the opportunities. The author also refers readers to Monitz, as well as <xref ref-type="bibr" rid="scirp.142316-34">
     [34]
    </xref> for the old wavefunction of the universe problem. This all involves using the following frequency relationship</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mtext>
              initial era 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ≡ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             a 
           </mi> 
           <mrow> 
            <mtext>
              today 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             a 
           </mi> 
           <mrow> 
            <mtext>
              initial era 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
        <mo>
          ≈ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msub> 
              <mi>
                ω 
              </mi> 
              <mrow> 
               <mtext>
                 Earth orbit 
               </mtext> 
              </mrow> 
             </msub> 
            </mrow> 
            <mrow> 
             <msub> 
              <mi>
                ω 
              </mi> 
              <mrow> 
               <mtext>
                 initial era 
               </mtext> 
              </mrow> 
             </msub> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mtext>
              initial era 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mtext>
            Earth orbit 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <msup> 
         <mn>
           10 
         </mn> 
         <mrow> 
          <mn>
            25 
          </mn> 
         </mrow> 
        </msup> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mtext>
            Earth orbit 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mtext>
            initial era 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (85)</p>
   <p>And a goal eventually of determining if the following are applicable to GW astronomy, i.e. <xref ref-type="bibr" rid="scirp.142316-35">
     [35]
    </xref> where on page 239 for a quantum cosmology similar to a “dust universe” we are given by Kieffer that</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mrow> 
        <mrow> 
         <mo>
           〈 
         </mo> 
         <mi>
           E 
         </mi> 
         <mo>
           〉 
         </mo> 
        </mrow> 
       </mrow> 
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        <mi>
          κ 
        </mi> 
        <mo>
          = 
        </mo> 
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          n 
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          , 
        </mo> 
        <mi>
          λ 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mrow> 
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           ( 
         </mo> 
         <mrow> 
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            κ 
          </mi> 
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            = 
          </mo> 
          <mi>
            n 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
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          + 
        </mo> 
        <mrow> 
         <mn>
           1 
         </mn> 
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           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
       <mi>
         λ 
       </mi> 
      </mfrac> 
      <munder> 
       <mo>
         → 
       </mo> 
       <mrow> 
        <mi>
          λ 
        </mi> 
        <mo>
          ≈ 
        </mo> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mrow> 
          <mi>
            ℏ 
          </mi> 
          <mi>
            ω 
          </mi> 
         </mrow> 
        </mrow> 
       </mrow> 
      </munder> 
      <mi>
        ℏ 
      </mi> 
      <mi>
        ω 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            κ 
          </mi> 
          <mo>
            = 
          </mo> 
          <mi>
            n 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          + 
        </mo> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (86)</p>
   <p>i.e. to make the bridge with a tokamak we should review the geometry and issues in <xref ref-type="bibr" rid="scirp.142316-36">
     [36]
    </xref>-<xref ref-type="bibr" rid="scirp.142316-41">
     [41]
    </xref> as well as Equation (21).</p>
  </sec><sec id="s18">
   <title>18. Could the Tokamak Actually Get Data Sets as to Confirm This, at Least in Outline? I.e. a Challenge to the Black Holes Have No Hair Problem?</title>
   <p>Assuming Planck scale time, or close to it, and renormalization to have Planck time as set to 1</p>
   <p>This means from <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref>, i.e. their so-called Equation (65), so we have for the radius of a BEC black hole as deformed by this quantum number n, a small change</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mi>
          Δ 
        </mi> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           n 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           n 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ≡ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <msup> 
           <mi>
             n 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            + 
          </mo> 
          <mn>
            2 
          </mn> 
         </mrow> 
        </msqrt> 
       </mrow> 
       <mrow> 
        <mn>
          3 
        </mn> 
        <mi>
          n 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (87)</p>
   <p>If we use the value of n = 2.16245415907 for a graviton “quantum number” at about normalized Planck time, scaled to about 1, and we have according to <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         n 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <msup> 
             <mi>
               n 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              + 
            </mo> 
            <mn>
              2 
            </mn> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <mi>
            n 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         n 
       </mi> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <msub> 
       <mrow> 
        <mrow> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <msqrt> 
               <mrow> 
                <msup> 
                 <mi>
                   n 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msup> 
                <mo>
                  + 
                </mo> 
                <mn>
                  2 
                </mn> 
               </mrow> 
              </msqrt> 
             </mrow> 
             <mrow> 
              <mn>
                3 
              </mn> 
              <mi>
                n 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           | 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          n 
        </mi> 
        <mo>
          ≡ 
        </mo> 
        <mn>
          2.16245415907 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        × 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         n 
       </mi> 
      </msub> 
     </mrow> 
    </math> (88)</p>
   <p>where 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        n 
      </mi> 
      <mo>
        ≥ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mi>
          ε 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             M 
           </mi> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               M 
             </mi> 
             <mi>
               p 
             </mi> 
            </msub> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> and we can compare our value of R, as given in Equation (23) with <xref ref-type="bibr" rid="scirp.142316-21">
     [21]
    </xref> having a different scale for R, as given in their Equation (60).</p>
  </sec><sec id="s19">
   <title>19. Final Long Term Goal, If Done Correctly Making Full Use of Our Tokamak to Early Universe Comparison to Give Data Sets to Understand Quantization and Early Universe Wave Functions</title>
   <p>In order to do this we need to reference all of the material as given in references <xref ref-type="bibr" rid="scirp.142316-35">
     [35]
    </xref> <xref ref-type="bibr" rid="scirp.142316-42">
     [42]
    </xref>-<xref ref-type="bibr" rid="scirp.142316-57">
     [57]
    </xref>.</p>
   <p>Using <xref ref-type="bibr" rid="scirp.142316-42">
     [42]
    </xref> a statement as to quantization for a would be GR term comes straight from</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142316-"></xref> 
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    </math> (89)</p>
   <p>The approximation we are making is to pick one index, so as to have</p>
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    </math>(90)</p>
   <p>This corresponds to say being primarily concerned as to GW generation, which is what we will be examining in our ideas, via using</p>
   <p>
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    </math> (91)</p>
   <p>We will use the following, namely, if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       Λ 
     </mi> 
    </math> is a constant, do the following for the Ricci scalar <xref ref-type="bibr" rid="scirp.142316-47">
     [47]
    </xref> <xref ref-type="bibr" rid="scirp.142316-48">
     [48]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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    </math> (92)</p>
   <p>If so then we can write the following, namely: Equation (91) becomes, if we have an invariant Cosmological constant, so we write 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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         → 
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          all time 
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    </math> everywhere, then</p>
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    </math> (93)</p>
   <p>Then, we have that Equation (89) is re written to be</p>
   <p>
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        </munder> 
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                 16 
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                  3 
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                  0 
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               </msub> 
              </mrow> 
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                ) 
              </mo> 
             </mrow> 
            </mrow> 
            <mo>
              ] 
            </mo> 
           </mrow> 
           <msub> 
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              Ψ 
            </mi> 
            <mrow> 
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               Earlier 
             </mtext> 
            </mrow> 
           </msub> 
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              ( 
            </mo> 
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                t 
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              ) 
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             d 
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              t 
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     </mtable> 
    </math> (94)</p>
  </sec><sec id="s20">
   <title>20. Examining the Behavior of the Earlier Wavefunction in Equation (94)</title>
   <p>
    <xref ref-type="bibr" rid="scirp.142316-43">
     [43]
    </xref> states a Hartle-Hawking wavefunction which we will adapt for the earlier wavefunction as stated in Equation (94) so as to read as follows</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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          Earlier 
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        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ∝ 
      </mo> 
      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mi>
            π 
          </mi> 
         </mrow> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             H 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <mi>
              sinh 
            </mi> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                H 
              </mi> 
              <mi>
                t 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             3 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (95)</p>
   <p>Here, making use of Sarkar <xref ref-type="bibr" rid="scirp.142316-3">
     [3]
    </xref>, we set, if say 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mo>
         ∗ 
       </mo> 
      </msub> 
     </mrow> 
    </math> is the degree of freedom allowed <xref ref-type="bibr" rid="scirp.142316-9">
     [9]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        H 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mn>
          1.66 
        </mn> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             g 
           </mi> 
           <mo>
             ∗ 
           </mo> 
          </msub> 
         </mrow> 
        </msqrt> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            e 
          </mi> 
          <mi>
            m 
          </mi> 
          <mi>
            p 
          </mi> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mrow> 
          <mtext>
            Planck 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> (96)</p>
   <p>We assume initially a relatively uniformly given temperature, that H is constant.</p>
   <p>So then we will be attempting to write out an expansion as to what Equation (94) gives us while we use Equation (95) and Equation (96), with H approximately constant.</p>
  </sec><sec id="s21">
   <title>21. Methods Used in Calculating Equation (94), with Interpretation of the Results</title>
   <p>We will be considering how to express Equation (94). And in doing this we will be looking at having a constant value for Equation (96). If so, then</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Ψ 
       </mi> 
       <mrow> 
        <mtext>
          Later 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <mo>
          ∫ 
        </mo> 
        <mrow> 
         <mi>
           exp 
         </mi> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mfrac> 
            <mi>
              i 
            </mi> 
            <mi>
              ℏ 
            </mi> 
           </mfrac> 
           <mo>
             ⋅ 
           </mo> 
           <mfrac> 
            <mrow> 
             <msup> 
              <mi>
                c 
              </mi> 
              <mn>
                4 
              </mn> 
             </msup> 
             <mo>
               ⋅ 
             </mo> 
             <mi>
               π 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <msup> 
              <mi>
                t 
              </mi> 
              <mn>
                0 
              </mn> 
             </msup> 
            </mrow> 
            <mrow> 
             <mn>
               16 
             </mn> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </mfrac> 
           <mo>
             ⋅ 
           </mo> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mi>
               r 
             </mi> 
             <mo>
               − 
             </mo> 
             <msup> 
              <mi>
                r 
              </mi> 
              <mn>
                3 
              </mn> 
             </msup> 
             <msub> 
              <mi>
                Λ 
              </mi> 
              <mn>
                0 
              </mn> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mi>
            π 
          </mi> 
         </mrow> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             H 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <mi>
              sinh 
            </mi> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                H 
              </mi> 
              <mi>
                t 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             3 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mtext>
        d 
      </mtext> 
      <msup> 
       <mi>
         t 
       </mi> 
       <mn>
         0 
       </mn> 
      </msup> 
     </mrow> 
    </math> (97)</p>
   <p>Then using numerical integration, <xref ref-type="bibr" rid="scirp.142316-50">
     [50]
    </xref>-<xref ref-type="bibr" rid="scirp.142316-52">
     [52]
    </xref> on page 751 of this <xref ref-type="bibr" rid="scirp.142316-52">
     [52]
    </xref> citation</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           Ψ 
         </mi> 
         <mrow> 
          <mtext>
            Later 
          </mtext> 
         </mrow> 
        </msub> 
        <munder> 
         <mo>
           → 
         </mo> 
         <mrow> 
          <msub> 
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             t 
           </mi> 
           <mi>
             M 
           </mi> 
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            → 
          </mo> 
          <msup> 
           <mi>
             ε 
           </mi> 
           <mo>
             + 
           </mo> 
          </msup> 
         </mrow> 
        </munder> 
        <mstyle displaystyle="true"> 
         <mrow> 
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           <mo>
             ∫ 
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           <mn>
             0 
           </mn> 
           <mrow> 
            <msub> 
             <mi>
               t 
             </mi> 
             <mi>
               M 
             </mi> 
            </msub> 
           </mrow> 
          </munderover> 
          <mrow> 
           <msup> 
            <mtext>
              e 
            </mtext> 
            <mrow> 
             <mi>
               i 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mover accent="true"> 
                <mi>
                  α 
                </mi> 
                <mo>
                  ˜ 
                </mo> 
               </mover> 
               <mn>
                 1 
               </mn> 
              </mrow> 
              <mo>
                ) 
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               ⋅ 
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             <mi>
               t 
             </mi> 
             <mo>
               − 
             </mo> 
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                ( 
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                ) 
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                   sinh 
                 </mi> 
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                  <mo>
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                  </mo> 
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                   <mi>
                     H 
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                    ) 
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        </mstyle> 
        <mtext>
          d 
        </mtext> 
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          t 
        </mi> 
       </mtd> 
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          ≈ 
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             t 
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             M 
           </mi> 
          </msub> 
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         </mn> 
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               ) 
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             </mi> 
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                </mi> 
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                     t 
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        </mo> 
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            <msub> 
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             </mi> 
             <mn>
               0 
             </mn> 
            </msub> 
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             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
        <mo>
          , 
        </mo> 
        <mtext>
            
        </mtext> 
        <mtext>
            
        </mtext> 
        <mover accent="true"> 
         <mi>
           α 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
        <mn>
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        </mn> 
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          = 
        </mo> 
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         </mi> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            G 
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           </mi> 
           <mn>
             2 
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          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (98)</p>
   <p>Notice the terms for the H factor, and from here we will be making our prediction.</p>
   <p>If the energy, E, has the following breakdown</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mi>
          H 
        </mi> 
        <mo>
          = 
        </mo> 
        <mrow> 
         <mrow> 
          <mn>
            1.66 
          </mn> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
               g 
             </mi> 
             <mo>
               ∗ 
             </mo> 
            </msub> 
           </mrow> 
          </msqrt> 
          <msubsup> 
           <mi>
             T 
           </mi> 
           <mrow> 
            <mi>
              t 
            </mi> 
            <mi>
              e 
            </mi> 
            <mi>
              m 
            </mi> 
            <mi>
              p 
            </mi> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
         <mo>
           / 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mrow> 
            <mtext>
              Planck 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <mi>
          E 
        </mi> 
        <mo>
          ≈ 
        </mo> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           B 
         </mi> 
        </msub> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            T 
          </mi> 
          <mi>
            e 
          </mi> 
          <mi>
            m 
          </mi> 
          <mi>
            p 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <mi>
          ℏ 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mtext>
            signal 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
        </mo> 
        <msub> 
         <mi>
           ω 
         </mi> 
         <mrow> 
          <mtext>
            signal 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             k 
           </mi> 
           <mi>
             B 
           </mi> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
               M 
             </mi> 
             <mrow> 
              <mtext>
                Planck 
              </mtext> 
             </mrow> 
            </msub> 
            <mi>
              H 
            </mi> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mrow> 
          <mi>
            ℏ 
          </mi> 
          <mo>
            ⋅ 
          </mo> 
          <msqrt> 
           <mrow> 
            <mn>
              1.66 
            </mn> 
            <msqrt> 
             <mrow> 
              <msub> 
               <mi>
                 g 
               </mi> 
               <mo>
                 ∗ 
               </mo> 
              </msub> 
             </mrow> 
            </msqrt> 
           </mrow> 
          </msqrt> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (99)</p>
   <p>constant in this sort of problem, i.e. the way to do it would be to analyze a Kieffer “dust solution” as a signal from the Wormhole. i.e. look at <xref ref-type="bibr" rid="scirp.142316-35">
     [35]
    </xref>. I.e. in this case we will write having</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         ω 
       </mi> 
       <mrow> 
        <mtext>
          signal 
        </mtext> 
       </mrow> 
      </msub> 
      <mi>
        Δ 
      </mi> 
      <mi>
        t 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (100)</p>
   <p>If so then we can assume that the time would be small enough so that</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        t 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          ℏ 
        </mi> 
        <msqrt> 
         <mrow> 
          <mn>
            1.66 
          </mn> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
               g 
             </mi> 
             <mo>
               ∗ 
             </mo> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
        </msqrt> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           B 
         </mi> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mrow> 
            <mtext>
              Planck 
            </mtext> 
           </mrow> 
          </msub> 
          <mi>
            H 
          </mi> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (101)</p>
   <p>If Equation (101) is of a value somewhat close to t, in terms of general initial time, we can write</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mi>
         ψ 
       </mi> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           n 
         </mi> 
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           ˜ 
         </mo> 
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        <mo>
          , 
        </mo> 
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          λ 
        </mi> 
       </mrow> 
      </msub> 
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    </math> (102)</p>
   <p>Here the time t would be proportional to Planck time, and r would be proportional to Planck length, whereas we set</p>
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    </math> (103)</p>
   <p>Then a preliminary emergent space-time wave function would take the form of</p>
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    </math> (104)</p>
   <p>Just at the surface of the bubble of space-time, with 
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   <p>What we wish to do in our procedure is to come up with data sets which may be able to take the real version of the above wave function, also, make accessible the <xref ref-type="bibr" rid="scirp.142316-57">
     [57]
    </xref> reference data sets, if wormholes exist from a prior to the present universe, which contributes to the Big Bang.</p>
  </sec>
 </body><back>
  <ref-list>
   <title>References</title>
   <ref id="scirp.142316-ref1">
    <label>1</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Beckwith, A. (2021) A Solution of the Cosmological Constant and DE Using Breakup of Primordial Black Holes, via a Criteria Brought Up by Dr. Freeze which Initiates DE as Linked to Inflation. Preprints. 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref2">
    <label>2</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Gladyshev, V. and Fomin, I. (2019) The Early Universe as a Source of Gravitational Waves. &gt;https://www.intechopen.com/books/progress-in-relativity/the-early-universe-as-a-source-of-gravitational-waves 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref3">
    <label>3</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Fukuyama, T. and Morikawa, M. (2007) Relativistic Bose-Einstein Condensation Model for Dark Matter and Dark Energy. In: Aschenbach, B., Burwitz, V., Hasinger, G. and Leibundgut, B., Eds., ESO Astrophysics Symposia, Springer, 95-97. &gt;https://doi.org/10.1007/978-3-540-74713-0_21
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref4">
    <label>4</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Freese, K., Brown, M.G. and Kinney, W.H. (2011) The Phantom Bounce: A New Proposal for an Oscillating Cosmology. In: Mersini-Houghton, L. and Vaas, R., Eds., The Arrows of Time, Springer, 149-156. &gt;https://doi.org/10.1007/978-3-642-23259-6_7
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref5">
    <label>5</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Maggiore, M. (2008) Gravitational Waves, Volume 1, Theory and Experiment. Ox-ford University Press.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref6">
    <label>6</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Rahvar, S. (2017) Cosmic Initial Conditions for a Habitable Universe. Monthly Notices of the Royal Astronomical Society, 470, 3095-3102. &gt;https://doi.org/10.1093/mnras/stx1448
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref7">
    <label>7</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Li, F., Wen, H., Fang, Z., Li, D. and Zhang, T. (2020) Electromagnetic Response to High-Frequency Gravitational Waves Having Additional Polarization States: Distinguishing and Probing Tensor-Mode, Vector-Mode and Scalar-Mode Gravitons. The European Physical Journal C, 80, Article No. 879. &gt;https://doi.org/10.1140/epjc/s10052-020-08429-2
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref8">
    <label>8</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Grishchuk, L.P. and Sazchin, M.V. (1975) Excitation and Detection of Standing Gravitational Waves. Journal of Experimental and Theoretical Physics, 68, 1569-1582.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref9">
    <label>9</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Li, F., Tang, M., Luo, J. and Li, Y. (2000) Electrodynamical Response of a High-Energy Photon Flux to a Gravitational Wave. Physical Review D, 62, Article 044018. &gt;https://doi.org/10.1103/physrevd.62.044018
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref10">
    <label>10</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Wesson, J. (2011) Tokamaks. 4th Edition, Oxford Science Publications.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref11">
    <label>11</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     de Sabbata, V. and Sivaram, C. (1991) Torsion, Quantum Effects and the Problem of Cosmological Constant. In: Zichichi, A., de Sabbata, V. and Sánchez, N., Eds., Gravitation and Modern Cosmology, Springer, 19-36. &gt;https://doi.org/10.1007/978-1-4899-0620-5_4
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref12">
    <label>12</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Beckwith, A.W. (2024) How Torsion as Presented by De Sabbata and Sivaram in Erice 1990 Argument as Modified May Permit Cosmological Constant, and Baseline as to Dark Energy. Journal of High Energy Physics, Gravitation and Cosmology, 10, 138-148. &gt;https://doi.org/10.4236/jhepgc.2024.101012
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref13">
    <label>13</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Padmanabhan, T. (2006) An Invitation to Astrophysics. World Scientific, 384. &gt;https://doi.org/10.1142/6010
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref14">
    <label>14</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Chavanis, P. (2014) Self-Gravitating Bose-Einstein Condensates. In: Calmet, X., Ed., Fundamental Theories of Physics, Springer International Publishing, 151-194. &gt;https://doi.org/10.1007/978-3-319-10852-0_6
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref15">
    <label>15</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Carlip, S. (n.d.) Black Hole Thermodynamics and Statistical Mechanics. In: Papantonopoulos, E., Ed., Lecture Notes in Physics, Springer, 89-123. &gt;https://doi.org/10.1007/978-3-540-88460-6_3
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref16">
    <label>16</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Downes, T.G. and Milburn, G.J. (2020) Optimal Quantum Estimation for Gravitation. arXiv:1108.5220 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref17">
    <label>17</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Kuroyanagi, S., Ringeval, C. and Takahashi, T. (2013) Early Universe Tomography with CMB and Gravitational Waves. Physical Review D, 87, Article 083502. &gt;https://doi.org/10.1103/physrevd.87.083502 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref18">
    <label>18</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Beckwith, A.W. (2017) Part 2: Review of Tokamak Physics as a Way to Construct a Device Optimal for Graviton Detection and Generation within a Confined Small Spatial Volume, as Opposed to Dyson’s “Infinite Astrophysical Volume” Calculations. Journal of High Energy Physics, Gravitation and Cosmology, 3, 138-155. &gt;https://doi.org/10.4236/jhepgc.2017.31015 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref19">
    <label>19</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Chongchitnan, S. (2016) Inflation Model Building with an Accurate Measure of E-Folding. arXiv:1605.04871v2&gt;https://arxiv.org/pdf/1605.04871.pdf
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref20">
    <label>20</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Corda and Christian (2023) Black Hole Spectra from Vaz’s Quantum Gravitational Collapse. Fortschritte der Physik-Progress of Physics, 11 p. arXiv:2305.02184&gt;https://arxiv.org/abs/2305.02184 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref21">
    <label>21</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Casadio, R. and Micu, O. (2024) Quantum Matter Core of Black Holes (and Quantum Hair). In: Malafarina, D. and Joshi, P.S., Eds., Springer Series in Astrophysics and Cosmology, Springer, 53-84. &gt;https://doi.org/10.1007/978-981-97-1172-7_2 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref22">
    <label>22</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Feng, Z., Ling, Y., Wu, X. and Jiang, Q. (2024) New Black-to-White Hole Solutions with Improved Geometry and Energy Conditions. Science China Physics, Mechanics&amp;Astronomy, 67, Article No. 270412. &gt;https://doi.org/10.1007/s11433-023-2373-0 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref23">
    <label>23</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Unruh, W.G. (1986) Why Study Quantum Theory? Canadian Journal of Physics, 64, 128-130. &gt;https://doi.org/10.1139/p86-019 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref24">
    <label>24</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Unruh, W.G. (1986) Erratum: Why Study Quantum Theory? Canadian Journal of Physics, 64, 1453-1453. &gt;https://doi.org/10.1139/p86-257 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref25">
    <label>25</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Casadio, R. and Giusti, A. (2021) Classicalizing Gravity. In: Saridakis, E.N., et al., Eds., Modified Gravity and Cosmology, Springer International Publishing, 405-418. &gt;https://doi.org/10.1007/978-3-030-83715-0_27 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref26">
    <label>26</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Beckwith, A.W. (2018) Structure Formation and Non Linear Electrodynamics with Attendant Changes in Gravitational Potential and Its Relationship to the 3 Body Problem. Journal of High Energy Physics, Gravitation and Cosmology, 4, 779-786. &gt;https://doi.org/10.4236/jhepgc.2018.44043 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref27">
    <label>27</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Camara, C.S., de Garcia Maia, M.R., Carvalho, J.C. and Lima, J.A.S. (2004) Nonsingular FRW Cosmology and Nonlinear Electrodynamics. Physical Review D, 69, Article 123504. &gt;https://doi.org/10.1103/physrevd.69.123504 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref28">
    <label>28</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Dieter, L. and Vleeshouwers, S. (2019) Black Hole Information and Thermodynamics. In: Springer Briefs in Physics, Springer Verlag.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref29">
    <label>29</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Mohanty, S. (2020) Astroparticle Physics and Cosmology, Perspectives in the Multimessenger Era. Springer Nature. &gt;https://doi.org/10.1007/978-3-030-56201-4
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref30">
    <label>30</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Bartos, I. and Kowalski, M. (2017) Multimessenger Astronomy. IOP Publishing. &gt;https://doi.org/10.1088/978-0-7503-1369-8
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref31">
    <label>31</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Cornish, N. and Robson, T. (2017) Galactic Binary Science with the New LISA Design. Journal of Physics: Conference Series, 840, Article 012024. &gt;https://doi.org/10.1088/1742-6596/840/1/012024
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref32">
    <label>32</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     The Elisa Consortium (2013) The Gravitational Universe. arXiv:1305.5720
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref33">
    <label>33</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Astier, P., Guy, J., Regnault, N., Pain, R., Aubourg, E., Balam, D., et al. (2006) The Supernova Legacy Survey: Measurement of Ω
     <sub>Μ</sub>, Ω
     <sub>Λ</sub> and W from the First Year Data Set. Astronomy&amp;Astrophysics, 447, 31-48. &gt;https://doi.org/10.1051/0004-6361:20054185
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref34">
    <label>34</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Monitz, P.V. (2010) Quantum Cosmology-The Supersymmetric Perspective-Vol. 1, Fundamentals. In: Citro, R., Hänggi, P., Hartmann, B., et al., Eds., Lecture Notes in Physics, Springer Nature.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref35">
    <label>35</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Kieffer, K. (2012) Quantum Gravity. 3rd Edition, Oxford University Press.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref36">
    <label>36</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Maldacena, J., Milekhin, A. and Popov, F. (2020) Traversable Wormholes in Four Dimensions. arXiv:1807.04726. &gt;https://arxiv.org/abs/1807.04726 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref37">
    <label>37</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     The LIGO Scientific Collaboration&amp;The Virgo Collaboration (2009) An Upper Limit on the Stochastic Gravitational-Wave Background of Cosmological Origin. Nature, 460, 990-994. &gt;https://doi.org/10.1038/nature08278
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref38">
    <label>38</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Li, M., Li, X., Wang, S. and Wang, Y. (2015) Dark Energy. In: Peking University World Scientific Advance Physics Series, Vol. 1, World Scientific.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref39">
    <label>39</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Maartens, R. (2004) Brane-World Gravity. Living Reviews in Relativity, 7, Article No. 7. &gt;https://doi.org/10.12942/lrr-2004-7
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref40">
    <label>40</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Dubovsky, S., et al. (2009) Signatures of a Graviton Mass in the Cosmic Microwave Background. arXiv:0907.1658. &gt;http://arxiv.org/abs/0907.1658
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref41">
    <label>41</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Kolb, E. and Turner, M. (1990) The Early Universe. Addison-Wesley Publishing Company.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref42">
    <label>42</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Weber, J. (2004) General Relativity and Gravitational Waves. Dover Publications, Incorporated.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref43">
    <label>43</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Lu, H.Q., Fang, W., Huang, Z.G. and Ji, P.Y. (2008) The Consistent Result of Cosmological Constant from Quantum Cosmology and Inflation with Born-Infeld Scalar Field. The European Physical Journal C, 55, 329-335. &gt;https://doi.org/10.1140/epjc/s10052-008-0564-z
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref44">
    <label>44</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Sarkar and Utpal (2008) Particle and Astroparticle Physics. Taylor&amp;Francis Group.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref45">
    <label>45</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Popov, A.A. and Sushkov, S.V. (2001) Vacuum Polarization of a Scalar Field in Wormhole Spacetimes. Physical Review D, 63, Article 044017. &gt;https://doi.org/10.1103/physrevd.63.044017
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref46">
    <label>46</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     DeBenedictis, A. and Das, A. (2001) On a General Class of Wormhole Geometries. Classical and Quantum Gravity, 18, 1187-1204. &gt;https://doi.org/10.1088/0264-9381/18/7/304
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref47">
    <label>47</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Einstein, A. and Rosen, N. (1935) The Particle Problem in the General Theory of Relativity. Physical Review, 48, 73-77. &gt;https://doi.org/10.1103/physrev.48.73
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref48">
    <label>48</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Visser, M. (2002) The Quantum Physics of Chronology Protection. arXiv:gr-qc/0204022&gt;https://arxiv.org/abs/gr-qc/0204022 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref49">
    <label>49</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Lightman, A., Press, W., Price, R. and Teukolsky, S. (1975) Problem Book in Relativity and Gravitation. Princeton University Press. 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref50">
    <label>50</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Kolb, E. and Turner, M. (1990) The Early Universe. Addison-Wesley Publishing Company.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref51">
    <label>51</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     McCracken, D.D. and Dorn, W.S. (1977) Numerical Methods and Fortran Programming with Application in Engineering and Science. Publishing House Mir, 584 p.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref52">
    <label>52</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Philip, J.D. and Rabinowitz, P. (2007) Methods of Numerical Integration. 2nd Edition, Dover Publishers. 
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref53">
    <label>53</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Zwillinger, D. (2003) CRC Standard Mathematical Tables and Formulae. 31st Edition, Chapman and Hall/CRC.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref54">
    <label>54</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Barrow and John, D. (2002) The Constants of Nature, from Alpha to Omega—The Numbers that Encode the Deepest Secrets of the Universe. Pantheon Books.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref55">
    <label>55</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Planck and Max (1899) Über irreversible strahlungsvorgänge. Sitzungsberichte der königlich preußischen akademie der wissenschaften zu berlin (in German). 5, 440-480. Pp. 478-480 Contain the First Appearance of the Planck Base Units Other than the Planck Charge, and of Planck’s Constant, which Planck denoted by B. A and F in This Paper Correspond to K and G in Modern Usage.
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref56">
    <label>56</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Aldaya, V., Barceló, C. and Jaramillo, J.L. (2011) Spanish Relativity Meeting (ERE 2010): Gravity as a Crossroad in Physics. Journal of Physics: Conference Series, 314, Article 011001. &gt;https://doi.org/10.1088/1742-6596/314/1/011001
    </mixed-citation>
   </ref>
   <ref id="scirp.142316-ref57">
    <label>57</label>
    <mixed-citation publication-type="other" xlink:type="simple">
     Gecim, G. and Sucu, Y. (2020) Quantum Gravity Correction to Hawking Radiation of the 2 + 1-Dimensional Wormhole. Advances in High Energy Physics, 2020, Article 7516789. &gt;https://doi.org/10.1155/2020/7516789
    </mixed-citation>
   </ref>
  </ref-list>
 </back>
</article>