<?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.2025.112034
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-142274
   </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 and Multi-Messenger Spin-Offs
   </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>
    480
   </fpage>
   <lpage>
    505
   </lpage>
   <history>
    <date date-type="received">
     <day>
      9,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      24,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      24,
     </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. Also, a solution to the early universe three-body problem at the start of the black holes, and number n selected. 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 of connection to multi-messenger astronomy will be enumerated in the last part of this document.
   </abstract>
   <kwd-group> 
    <kwd>
     Inflation
    </kwd> 
    <kwd>
      Gravitational Waves
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Part 1. Preliminaries, Recounting the Parameters of Black Hole Physics Used in This Essay, as Well as the Importance of a Quantum Number n</title>
   <p>Following <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </xref> using the substitutions outlined so we can re-do the introduction of black hole physics in terms of a quantum number n, to begin this first look at the references to the BEC condensate as given by <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </xref> with respect to scaling.</p>
   <p>i.e. the origins of the black holes have no hair theorem and a preview of what we will be trying to modify.</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142274-"></xref>Our supposition has the no hair idea and starts off with a simple idea. 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>
    <xref ref-type="bibr" rid="scirp.142274-"></xref> 
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mfrac> 
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          t 
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        − 
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      <msup> 
       <mi>
         T 
       </mi> 
       <mn>
         4 
       </mn> 
      </msup> 
     </mrow> 
    </math> (1)</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> 
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          ℏ 
        </mi> 
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           3 
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          8 
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          π 
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          G 
        </mi> 
        <mi>
          M 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (2)</p>
   <p>This leads to, if indeed Equation (1) 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> 
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           ˜ 
         </mo> 
        </mover> 
       </mrow> 
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         ) 
       </mo> 
      </mrow> 
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        ⋅ 
      </mo> 
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       <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> (3)</p>
   <p>As to how we can observe a violation of the black holes which have no hair idea we will need to do parameterization of a mass M, for black holes, in terms of the following inputs</p>
  </sec><sec id="s2">
   <title>2. First of All an Aside as to Muti Messenger Astrophysics, Which Is Relevant to Quantum Number n</title>
   <p>Multi-messenger astrophysics is the observation of multiple signals received from the same <xref ref-type="bibr" rid="scirp.142274-astronomical">
     astronomical
    </xref> event. Many types of cosmological events involve complex interactions between a variety of astrophysical processes, each of which may independently emit signals of a characteristic “messenger” type: <xref ref-type="bibr" rid="scirp.142274-electromagnetic radiation">
     electromagnetic radiation
    </xref> (including <xref ref-type="bibr" rid="scirp.142274-infrared">
     infrared
    </xref>, <xref ref-type="bibr" rid="scirp.142274-visible light">
     visible light
    </xref> and <xref ref-type="bibr" rid="scirp.142274-X-rays">
     X-rays
    </xref>), <xref ref-type="bibr" rid="scirp.142274-gravitational waves">
     gravitational waves
    </xref>, i.e. what we are doing is to set up the template as to how GW and gravitons as generated by primordial black holes may, if characterized by a quantum number n, lead to Electromagnetic spectrum. I.e. our mechanism will start with a new intro as to torsion, Black holes, and quantum number n while ending with possible Photonic traces. In CMBR i.e. we will initially be discussing the process of how GW and gravitons are related to primoridial black holes, of a quantum number n, and end up with speculations as to electromagnetic generation of signals which may be observable observationally.</p>
  </sec><sec id="s3">
   <title>3. Where Torsion May Allow for Understanding a Quantum Number n?</title>
   <p>Following <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref>, we do the introduction of black hole physics in terms of a quantum number n.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msqrt> 
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           Λ 
         </mi> 
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          </mi> 
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              entropy 
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            particles 
          </mtext> 
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        </msub> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (4)</p>
   <p>And then a BEC condensate given by <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </xref> as to</p>
   <p>
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          ⋅ 
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         </mi> 
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            gravitons 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
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         </mi> 
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            B 
          </mi> 
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          </mi> 
         </mrow> 
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          ≈ 
        </mo> 
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         <mrow> 
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           </mi> 
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             P 
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          </msub> 
         </mrow> 
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          <msqrt> 
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             </mi> 
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                gravitons 
              </mtext> 
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          </msqrt> 
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       </mtd> 
      </mtr> 
     </mtable> 
    </math> (5)</p>
   <p>This is promising but needs to utilize <xref ref-type="bibr" rid="scirp.142274-4">
     [4]
    </xref> in which we make use of the following. First a time step</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        τ 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          M 
        </mi> 
        <mi>
          δ 
        </mi> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> (6)</p>
   <p>By use of the HUP <xref ref-type="bibr" rid="scirp.142274-5">
     [5]
    </xref> we use Equation (3) for energy <xref ref-type="bibr" rid="scirp.142274-4">
     [4]
    </xref> for radiation of a particle pair from a black hole,</p>
   <p>
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      <mrow> 
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         | 
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            </mi> 
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            </mi> 
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          </msqrt> 
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         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
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          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (7)</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> 
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      </mi> 
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      <msub> 
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         ℓ 
       </mi> 
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       </mi> 
      </msub> 
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    </math> (8)</p>
   <p>This is of a Plank length, whereas we assume in Equation (7) 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> 
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        α 
      </mi> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
     </mrow> 
    </math> (9)</p>
   <p>If so, we transform Equation (4) to be of the form for a “particle” pair as given in Carlip</p>
   <p>
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        ≈ 
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              ⋅ 
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                 M 
               </mi> 
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                 P 
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               ) 
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              ⋅ 
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               ℓ 
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           ) 
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          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (10)’</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 (10) as the mass of a relic black hole. Now using the following normalization of Planck units, i.e. <xref ref-type="bibr" rid="scirp.142274-6">
     [6]
    </xref>, as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
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       <mi>
         M 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        ℏ 
      </mi> 
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        = 
      </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> (11)</p>
   <p>And, also reference the value of the initial energy, E, as given in reference <xref ref-type="bibr" rid="scirp.142274-5">
     [5]
    </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> (12)</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"> <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> 
      <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> 
        <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> 
        <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> 
     </mrow> 
    </math> (13)</p>
   <p>We then reference Equation (5) 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> (14)</p>
   <p>This is a stunning result. i.e. Equation (5) 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 the following table.</p>
   <p>
    <xref ref-type="table" rid="table1">
     Table 1
    </xref> from reference <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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.142274-"></xref>Table 1. Recycling values of black holes.</title>
    </caption>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="aleft" width="36.64%"><p style="text-align:left">End of Prior Universe time frame</p></td> 
      <td class="aleft" width="30.03%"><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="33.33%"><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="36.64%"><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="30.03%"><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="33.33%"><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="36.64%"><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="30.03%"><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="33.33%"><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.142274-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-4">
     [4]
    </xref> To begin this look at <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> which, which is akin, as we discuss later to <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> <xref ref-type="bibr" rid="scirp.142274-8">
     [8]
    </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> (15)</p>
   <p>In <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref>, the first line is the vacuum energy which is completely cancelled in their formulation of application of Torsion. In our article, we are arguing for the second line. In fact by <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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> (16)</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.142274-7">
     [7]
    </xref>.</p>
   <p>We argue that our application of <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> will be commensurate with Equation (15) which uses the value given in <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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 (15) whereas what is done in Equation (15) by <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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> (17)</p>
   <p>Furthermore, the claim in <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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.142274-2">
     [2]
    </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="s4">
   <title>4. 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.142274-9">
     [9]
    </xref> we have the following, i.e., we have a spin density term of <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </xref>. And this will be what we input black hole physics into as 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> (18)</p>
  </sec><sec id="s5">
   <title>5. Now for the Statement of the Torsion Problem as Given in <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </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.142274-9">
     [9]
    </xref> and is nothing else. Hence, in saying this we wish to delve into what was given in <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </xref> with a subsequent follow up and modification:</p>
   <p>To do this, note that in <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </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> (19)</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.142274-9">
     [9]
    </xref>.</p>
   <p>In <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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.142274-9">
     [9]
    </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> (20)</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> (21)</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> (22)</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> (23)</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> (24)</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> (25)</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> (26)</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> (27)</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> (28)</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> (29)</p>
  </sec><sec id="s6">
   <title>6. How to Modify Equation (28) 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 (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> (30)</p>
   <p>And eventually we have a re-do of Equation (28) 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> (31)</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> (32)</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.142274-9">
     [9]
    </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> (33)</p>
  </sec><sec id="s7">
   <title>7. What <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </xref> Does as to Equation (33) versus What We Would Do and Why</title>
   <p>In the case of <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </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 (33) 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> (34)</p>
   <p>The claim is made in <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </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.142274-9">
     [9]
    </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> (35)</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>−</sup><sup>122</sup> times smaller than the initial vacuum energy.</p>
   <p>The main reason for the difference in Equation (34) and Equation (35) 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="s8">
   <title>8. Filling in the Details of the Equation (34) Collapse of the Cosmological Term, versus the Situation Given in Equation (35) via Numerical Values</title>
   <p>First look at numbers provided by <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </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> (36)</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.142274-9">
     [9]
    </xref> is solely to remove this giant number.</p>
   <p>In order to remove it, the reference <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </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> (37)</p>
   <p>What we are arguing is that instead, one is seeing, instead <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
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            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
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         ) 
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        ⋅ 
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         [ 
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           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        + 
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        <msub> 
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           Λ 
         </mi> 
         <mrow> 
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            P 
          </mi> 
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            l 
          </mi> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           c 
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           2 
         </mn> 
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       </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> (38)</p>
   <p>Our timing as to Equation (36) is to unleash a Planck time interval t about 10<sup>−</sup><sup>43</sup> seconds.</p>
   <p>As to Equation (37) versus Equation (38) 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> (39)</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>
   <p>Future works to be commenced as to derivational tasks</p>
   <p>We will assume for the moment that Equation (36) and Equation (37) share in common Equation (39).</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 (36) by Equation (39) is defined to be an ad hoc creation, as to <xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </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</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>
        ⋅ 
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         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
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           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
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            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> 
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         ) 
       </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.142274-9">
     [9]
    </xref>, i.e. if we have an inflaton field <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-17">
     [17]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
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           | 
         </mo> 
         <mrow> 
          <mtext>
            d 
          </mtext> 
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           <mi>
             p 
           </mi> 
           <mi>
             α 
           </mi> 
          </msub> 
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            d 
          </mtext> 
          <msup> 
           <mi>
             x 
           </mi> 
           <mi>
             α 
           </mi> 
          </msup> 
         </mrow> 
         <mo>
           | 
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        <mo>
          ≈ 
        </mo> 
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         <mi>
           L 
         </mi> 
         <mi>
           l 
         </mi> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mi>
           h 
         </mi> 
         <mi>
           c 
         </mi> 
        </mfrac> 
        <mo>
          ⋅ 
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        <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> 
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            d 
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            </mi> 
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            ] 
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         </mn> 
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        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
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          <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> (40)</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142274-"></xref>Making use of all this leads to <xref ref-type="bibr" rid="scirp.142274-10">
     [10]
    </xref> to making sense of the quantum number n as given by reference to black holes, <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </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.142274-1">
     [1]
    </xref> states that Equation (40) 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 that Equation (38) is due to relic black holes with the suppression of the initially gigantic cosmological vacuum energy.</p>
   <p>The details of what follow 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.142274-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142274-14">
     [14]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
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           ) 
         </mo> 
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        <mo>
          = 
        </mo> 
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         <mi>
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         </mi> 
         <mrow> 
          <mtext>
            initial 
          </mtext> 
         </mrow> 
        </msub> 
        <msup> 
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           t 
         </mi> 
         <mi>
           ν 
         </mi> 
        </msup> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇒ 
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        <mi>
          ϕ 
        </mi> 
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        <mi>
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                   3 
                 </mn> 
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             </mi> 
             <mrow> 
              <mn>
                16 
              </mn> 
              <mi>
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              </mi> 
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         </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> (41)</p>
   <p>A possible future endeavor can also make sense of <xref ref-type="bibr" rid="scirp.142274-15">
     [15]
    </xref> as well</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.142274-9">
     [9]
    </xref>. Secondly it means utilization of Equation (16) which takes into account the black hole energy equation given by Corda in <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </xref> and it also means that the spin density term as given in Equation (18) 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.142274-1">
     [1]
    </xref> largely due to the insufficiency of black hole theory as eloquently given in <xref ref-type="bibr" rid="scirp.142274-16">
     [16]
    </xref> which we will cite their page 366 admonition as to the insufficiency of current 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 acknowledgement and is due to the sterility of much theoretical thinking, as well as the tremendously important Equation (12) which is due to Corda <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </xref>.</p>
   <p>Furthermore, in order to obtain more details of Equation (12) being utilized for black holes, we state that a quantum state of the early universe will utilize <xref ref-type="bibr" rid="scirp.142274-17">
     [17]
    </xref> and its discussion, page 184, as to how Feynman visualized the quantization of the Gravitational field, i.e. Equations 9.121 and 9.122 of <xref ref-type="bibr" rid="scirp.142274-17">
     [17]
    </xref> for an early wavefunction path integral treatment for quantized gravity and its use for black holes. Corda himself <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </xref> has alluded to a path forward in such treatment of how black holes can be modeled which leads to Equation (40).</p>
   <p>In addition, we outlined the stunning result as given as of Equation (14) 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.142274-7">
     [7]
    </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 have no hair theorem, via the inputs of this document.</p>
   <p>In <xref ref-type="bibr" rid="scirp.142274-18">
     [18]
    </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.142274-19">
     [19]
    </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.142274-20">
     [20]
    </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.142274-20">
     [20]
    </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> (42)</p>
   <p>Due to using <xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </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> (43)</p>
   <p>M here being linked to the mass of a BEC black hole, and also using Equation (3) for the loss of a black hole, over time.</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> (44)</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> (45)</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>If so then, and this is for primordial black holes, we then associate this graviton number, n for a graviton as linked to the following from <xref ref-type="bibr" rid="scirp.142274-20">
     [20]
    </xref>, i.e. their 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> (46)</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.142274-20">
     [20]
    </xref> an ADM mass variance of M so then there is, due to gravitons, a rough change in initial Planck sized black holes</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> (47)</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 (5) with <xref ref-type="bibr" rid="scirp.142274-20">
     [20]
    </xref> having a different scale for R, as given in their Equation (60).</p>
   <p>Needless to say, graviton number n, as specified, due to the processes within the primordial black hole we assert would lead to a violation of the black holes have no hair theorem, of <xref ref-type="bibr" rid="scirp.142274-19">
     [19]
    </xref>.</p>
   <p>We assert that this value of n, so obtained, as to gravitons would be as to the Corda result on Equation (12) 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> (48)</p>
   <p>The left hand side of Equation (48) would be fully commensurate with Equation (12) of Corda’s black hole quantum number.</p>
   <p>The right hand side of Equation (48) 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.142274-7">
     [7]
    </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. In <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </xref> we have a model along the lines I considered, and we ascertain that the Corda suggestion of n quantum number for back holes be compared to the quantum number, n, which may be derived from the energy condition in the <xref ref-type="bibr" rid="scirp.142274-8">
     [8]
    </xref> document. In doing so, we will ascertain if our value of n slightly larger than 2 is indeed feasible, and also optimal. The value of an energy, due to a quantum number, n, will be derived and compared with our value of n assumed in this early universe condition. In addition this will be done to give credence to <xref ref-type="bibr" rid="scirp.142274-8">
     [8]
    </xref> and to difficulty of forming primordial black holes.</p>
  </sec><sec id="s9">
   <title>9. Second Section. Now for Applications of the Generalized HUP and Its Applications to Black Hole Physics</title>
   <p>Heavy Gravity is the situation where a graviton has a small rest mass and is not a zero mass particle, and this existence of “heavy gravity” is important since eventually, as illustrated by Will <xref ref-type="bibr" rid="scirp.142274-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142274-10">
     [10]
    </xref> gravitons having a small mass could possibly be observed via their macroscopic effects upon astrophysical events. The second aspect of the inquiry of our manuscript will be to come up with a variant of the Heisenberg Uncertainty principle (HUP), in <xref ref-type="bibr" rid="scirp.142274-11">
     [11]
    </xref>, with</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        x 
      </mi> 
      <mi>
        Δ 
      </mi> 
      <mi>
        p 
      </mi> 
      <mo>
        ≥ 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
       <mn>
         2 
       </mn> 
      </mfrac> 
      <mo>
        + 
      </mo> 
      <mover accent="true"> 
       <mi>
         γ 
       </mi> 
       <mo>
         ˜ 
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      </mover> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          C 
        </mi> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          V 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (49)</p>
   <p>As opposed to</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
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          δ 
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          t 
        </mi> 
        <mi>
          Δ 
        </mi> 
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          E 
        </mi> 
        <mo>
          ≥ 
        </mo> 
        <mfrac> 
         <mi>
           ℏ 
         </mi> 
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          <mi>
            δ 
          </mi> 
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           <mi>
             g 
           </mi> 
           <mrow> 
            <mi>
              t 
            </mi> 
            <mi>
              t 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
        <mo>
          ≠ 
        </mo> 
        <mfrac> 
         <mi>
           ℏ 
         </mi> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mtext>
          Unless 
        </mtext> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ~ 
        </mo> 
        <mi>
          O 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mn>
           1 
         </mn> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (50)</p>
   <p>Which we claim in the Planckian regime will de evolve, as being effectively as being equivalent to</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        x 
      </mi> 
      <mi>
        Δ 
      </mi> 
      <mi>
        p 
      </mi> 
      <mo>
        ≥ 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
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          δ 
        </mi> 
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            t 
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            t 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (51)</p>
   <p>We will be comparing Equation (49) and Equation (50) as well as writing</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          t 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mi>
         a 
       </mi> 
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         2 
       </mn> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        ϕ 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (52)</p>
   <p>The second term in Equation (27) comes directly from a simplified inflaton expression which is <xref ref-type="bibr" rid="scirp.142274-12">
     [12]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-14">
     [14]
    </xref>.</p>
   <p>I.e. go to Equation (41).</p>
   <p>In doing this, we adhere to the starting point of <xref ref-type="bibr" rid="scirp.142274-14">
     [14]
    </xref> <xref ref-type="bibr" rid="scirp.142274-15">
     [15]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        l 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <mi>
        p 
      </mi> 
      <mo>
        ≥ 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
       <mn>
         2 
       </mn> 
      </mfrac> 
     </mrow> 
    </math> (53)</p>
   <p>We will be using the approximation given by Unruh,</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             Δ 
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             l 
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            ) 
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            i 
          </mi> 
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            j 
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        </msub> 
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          = 
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          <mi>
            δ 
          </mi> 
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             g 
           </mi> 
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              i 
            </mi> 
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              j 
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          </msub> 
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        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mi>
           l 
         </mi> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msub> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             Δ 
           </mi> 
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             p 
           </mi> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
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          <mi>
            i 
          </mi> 
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            j 
          </mi> 
         </mrow> 
        </msub> 
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          = 
        </mo> 
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        </mi> 
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           T 
         </mi> 
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            i 
          </mi> 
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            j 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          δ 
        </mi> 
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          t 
        </mi> 
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        </mo> 
        <mi>
          Δ 
        </mi> 
        <mi>
          A 
        </mi> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (54)</p>
   <p>If we use the following, from the Roberson-Walker metric <xref ref-type="bibr" rid="scirp.142274-14">
     [14]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-17">
     [17]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
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         </mi> 
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          <mi>
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          </mi> 
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            t 
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          = 
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          1 
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             ( 
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             t 
           </mi> 
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             ) 
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            1 
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          </mo> 
          <mi>
            k 
          </mi> 
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          </mo> 
          <msup> 
           <mi>
             r 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           g 
         </mi> 
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          <mi>
            θ 
          </mi> 
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            θ 
          </mi> 
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          = 
        </mo> 
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         </mi> 
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           2 
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           ( 
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          ⋅ 
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         <mi>
           r 
         </mi> 
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           2 
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       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
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         <mi>
           g 
         </mi> 
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          <mi>
            ϕ 
          </mi> 
          <mi>
            ϕ 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          = 
        </mo> 
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          − 
        </mo> 
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         <mi>
           a 
         </mi> 
         <mn>
           2 
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        </msup> 
        <mrow> 
         <mo>
           ( 
         </mo> 
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           t 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           sin 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mi>
          θ 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          d 
        </mi> 
        <msup> 
         <mi>
           ϕ 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (55)</p>
   <p>Following Unruh <xref ref-type="bibr" rid="scirp.142274-14">
     [14]
    </xref> <xref ref-type="bibr" rid="scirp.142274-15">
     [15]
    </xref>, write then, an uncertainty of metric tensor as, with the following inputs</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mn>
         2 
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       <mo>
         ( 
       </mo> 
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         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ~ 
      </mo> 
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        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          110 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        , 
      </mo> 
      <mtext>
          
      </mtext> 
      <mi>
        r 
      </mi> 
      <mo>
        ≡ 
      </mo> 
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         l 
       </mi> 
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         P 
       </mi> 
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      <mo>
        ~ 
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        <mn>
          10 
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          − 
        </mo> 
        <mn>
          35 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        meters 
      </mtext> 
     </mrow> 
    </math> (56)</p>
   <p>Then, if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        Δ 
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        ρ 
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     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
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             4 
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             ) 
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          = 
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          δ 
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          ⋅ 
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        <mi>
          Δ 
        </mi> 
        <mi>
          A 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          r 
        </mi> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mi>
          δ 
        </mi> 
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         </mi> 
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          </mi> 
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            t 
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        </mi> 
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        </mi> 
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          ⋅ 
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         <mi>
           r 
         </mi> 
         <mn>
           2 
         </mn> 
        </mfrac> 
        <mo>
          ≥ 
        </mo> 
        <mfrac> 
         <mi>
           ℏ 
         </mi> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ⇔ 
        </mo> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          Δ 
        </mi> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ≥ 
        </mo> 
        <mfrac> 
         <mi>
           ℏ 
         </mi> 
         <mrow> 
          <msup> 
           <mi>
             V 
           </mi> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mn>
               4 
             </mn> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (57)</p>
   <p>This Equation (56) is such that we can extract, up to a point the HUP principle for uncertainty in time and energy, with one very large caveat added, namely if we use the fluid approximation of space-time <xref ref-type="bibr" rid="scirp.142274-17">
     [17]
    </xref> for the stress energy tensor as given in Equation (58) below.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          i 
        </mi> 
        <mi>
          i 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        d 
      </mi> 
      <mi>
        i 
      </mi> 
      <mi>
        a 
      </mi> 
      <mi>
        g 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          ρ 
        </mi> 
        <mo>
          , 
        </mo> 
        <mo>
          − 
        </mo> 
        <mi>
          p 
        </mi> 
        <mo>
          , 
        </mo> 
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          − 
        </mo> 
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          p 
        </mi> 
        <mo>
          , 
        </mo> 
        <mo>
          − 
        </mo> 
        <mi>
          p 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>(58)</p>
   <p>Then</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          t 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <mi>
        ρ 
      </mi> 
      <mo>
        ~ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          Δ 
        </mi> 
        <mi>
          E 
        </mi> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           V 
         </mi> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mn>
             3 
           </mn> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (59)</p>
   <p>Then,</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142274-"></xref> 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mi>
          δ 
        </mi> 
        <mi>
          t 
        </mi> 
        <mi>
          Δ 
        </mi> 
        <mi>
          E 
        </mi> 
        <mo>
          ≥ 
        </mo> 
        <mfrac> 
         <mi>
           ℏ 
         </mi> 
         <mrow> 
          <mi>
            δ 
          </mi> 
          <msub> 
           <mi>
             g 
           </mi> 
           <mrow> 
            <mi>
              t 
            </mi> 
            <mi>
              t 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
        <mo>
          ≠ 
        </mo> 
        <mfrac> 
         <mi>
           ℏ 
         </mi> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mtext>
          Unless 
        </mtext> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ~ 
        </mo> 
        <mi>
          O 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mn>
           1 
         </mn> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (60)</p>
   <p>How likely is 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        δ 
      </mi> 
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         g 
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          t 
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          t 
        </mi> 
       </mrow> 
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        ~ 
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        O 
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         ( 
       </mo> 
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         1 
       </mn> 
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         ) 
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      </mrow> 
     </mrow> 
    </math>? Not going to happen. Why? The homogeneity of the early universe will keep</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          t 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ≠ 
      </mo> 
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       <mi>
         g 
       </mi> 
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        <mi>
          t 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (61)</p>
   <p>In fact, we have that from Giovannini <xref ref-type="bibr" rid="scirp.142274-16">
     [16]
    </xref>, that if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ϕ 
     </mi> 
    </math> is a scalar function, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
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         t 
       </mi> 
       <mo>
         ) 
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      </mrow> 
      <mo>
        ~ 
      </mo> 
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       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          110 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, then if</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          t 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        ϕ 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (62)</p>
   <p>Then, there is no way that Equation (60) is going to come close to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <mi>
        t 
      </mi> 
      <mi>
        Δ 
      </mi> 
      <mi>
        E 
      </mi> 
      <mo>
        ≥ 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
       <mn>
         2 
       </mn> 
      </mfrac> 
     </mrow> 
    </math>. i.e. it depends assuming time is for all purposes fixed at about Planck time to isolate 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>Equation (41) is crucial here, and it depends upon the scalar term in Equation (41) have a time dependence only, which means it is for near Planck time, almost a constant term. I.e. for the sake of argument, in the near Planckian regime, we can figure that Equation (62) will have as far as evaluation of the argument the following configuration, i.e. <xref ref-type="bibr" rid="scirp.142274-15">
     [15]
    </xref> <xref ref-type="bibr" rid="scirp.142274-16">
     [16]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        a 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <msub> 
       <mi>
         a 
       </mi> 
       <mrow> 
        <mtext>
          initial 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             t 
           </mi> 
           <mo>
             / 
           </mo> 
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            <msub> 
             <mi>
               t 
             </mi> 
             <mi>
               P 
             </mi> 
            </msub> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mi>
         v 
       </mi> 
      </msup> 
     </mrow> 
    </math> (63)</p>
   <p>Given this we will be looking at, if we do the set up</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <mi>
        x 
      </mi> 
      <mi>
        Δ 
      </mi> 
      <mi>
        p 
      </mi> 
      <mo>
        ≥ 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
       <mrow> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          = 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               a 
             </mi> 
             <mrow> 
              <mtext>
                initial 
              </mtext> 
             </mrow> 
            </msub> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
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                 <mi>
                   t 
                 </mi> 
                 <mo>
                   / 
                 </mo> 
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                  <msub> 
                   <mi>
                     t 
                   </mi> 
                   <mi>
                     P 
                   </mi> 
                  </msub> 
                 </mrow> 
                </mrow> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mi>
               v 
             </mi> 
            </msup> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mi>
            ln 
          </mi> 
          <msup> 
           <mrow> 
            <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> 
           <mrow> 
            <msqrt> 
             <mrow> 
              <mfrac> 
               <mi>
                 ν 
               </mi> 
               <mrow> 
                <mn>
                  16 
                </mn> 
                <mi>
                  π 
                </mi> 
                <mi>
                  G 
                </mi> 
               </mrow> 
              </mfrac> 
             </mrow> 
            </msqrt> 
           </mrow> 
          </msup> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (64)</p>
   <p>Comparing this Equation (43) with Equation (27), we obtain then if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        = 
      </mo> 
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        c 
      </mi> 
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        = 
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       <mi>
         t 
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        = 
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        = 
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        G 
      </mi> 
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        = 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> the bound for 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <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> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mi>
          exp 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mn>
              16 
            </mn> 
            <msqrt> 
             <mi>
               π 
             </mi> 
            </msqrt> 
           </mrow> 
           <mrow> 
            <msqrt> 
             <mi>
               ν 
             </mi> 
            </msqrt> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <msubsup> 
             <mi>
               a 
             </mi> 
             <mrow> 
              <mi>
                min 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msubsup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mrow> 
                 <mi>
                   t 
                 </mi> 
                 <mo>
                   / 
                 </mo> 
                 <mrow> 
                  <msub> 
                   <mi>
                     t 
                   </mi> 
                   <mi>
                     p 
                   </mi> 
                  </msub> 
                 </mrow> 
                </mrow> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mn>
              2 
            </mn> 
            <mover accent="true"> 
             <mi>
               γ 
             </mi> 
             <mo>
               ˜ 
             </mo> 
            </mover> 
            <mfrac> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                C 
              </mi> 
             </mrow> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                V 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (65)</p>
   <p>So then we are now doing an Evaluation of Equation (65) if we are near Planck time. Two limits.</p>
   <p>1<sup>st</sup>, what if we have expansion of the scale factor initially at greater than the speed of light?</p>
   <p>Set 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ν 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          88 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> and then we can obtain if we are just starting off inflation say 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         a 
       </mi> 
       <mrow> 
        <mi>
          min 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          44 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>. Then</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msup> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            176 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mi>
          exp 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            16 
          </mn> 
          <msqrt> 
           <mi>
             π 
           </mi> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mn>
              2 
            </mn> 
            <mover accent="true"> 
             <mi>
               γ 
             </mi> 
             <mo>
               ˜ 
             </mo> 
            </mover> 
            <mfrac> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                C 
              </mi> 
             </mrow> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                V 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ' 
      </mo> 
     </mrow> 
    </math> (66)</p>
   <p>If we wish to have a Planck energy magnitude of the 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> term, we will then be observing</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           V 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ≅ 
        </mo> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <msup> 
           <mrow> 
            <mn>
              10 
            </mn> 
           </mrow> 
           <mrow> 
            <mn>
              176 
            </mn> 
           </mrow> 
          </msup> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              16 
            </mn> 
            <msqrt> 
             <mi>
               π 
             </mi> 
            </msqrt> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mn>
              1 
            </mn> 
            <mrow> 
             <mn>
               1 
             </mn> 
             <mo>
               + 
             </mo> 
             <mn>
               2 
             </mn> 
             <mover accent="true"> 
              <mi>
                γ 
              </mi> 
              <mo>
                ˜ 
              </mo> 
             </mover> 
             <mfrac> 
              <mrow> 
               <mo>
                 ∂ 
               </mo> 
               <mi>
                 C 
               </mi> 
              </mrow> 
              <mrow> 
               <mo>
                 ∂ 
               </mo> 
               <mi>
                 V 
               </mi> 
              </mrow> 
             </mfrac> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ' 
        </mo> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <munder> 
         <mo>
           → 
         </mo> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mover accent="true"> 
           <mi>
             γ 
           </mi> 
           <mo>
             ˜ 
           </mo> 
          </mover> 
          <mfrac> 
           <mrow> 
            <mo>
              ∂ 
            </mo> 
            <mi>
              C 
            </mi> 
           </mrow> 
           <mrow> 
            <mo>
              ∂ 
            </mo> 
            <mi>
              V 
            </mi> 
           </mrow> 
          </mfrac> 
          <mo>
            ≈ 
          </mo> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <msup> 
             <mrow> 
              <mn>
                10 
              </mn> 
             </mrow> 
             <mrow> 
              <mn>
                88 
              </mn> 
             </mrow> 
            </msup> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
         </mrow> 
        </munder> 
        <mi>
          o 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mn>
           1 
         </mn> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (67)</p>
   <p>i.e. the system complexity will become effectively almost infinite, and this will be explained in the conclusion by use of</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        2 
      </mn> 
      <mover accent="true"> 
       <mi>
         γ 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          C 
        </mi> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          V 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msup> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            88 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⇒ 
      </mo> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <mi>
        o 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mn>
         1 
       </mn> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (68)</p>
   <p>On the other hand, if there is a very small value for 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        2 
      </mn> 
      <mover accent="true"> 
       <mi>
         γ 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          C 
        </mi> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          V 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> we can see the following behavior for Equation(66), namely</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        2 
      </mn> 
      <mover accent="true"> 
       <mi>
         γ 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          C 
        </mi> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          V 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <mi>
        o 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mn>
         1 
       </mn> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⇒ 
      </mo> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msup> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            176 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (69)</p>
   <p>i.e. low complexity in the measurement process will then imply an enormous initial inflaton potential energy.</p>
   <p>2ndly, Now what if we have instead 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        v 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            4 
          </mn> 
          <mi>
            π 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mi>
          exp 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mn>
              16 
            </mn> 
            <msqrt> 
             <mi>
               π 
             </mi> 
            </msqrt> 
           </mrow> 
           <mrow> 
            <msubsup> 
             <mi>
               a 
             </mi> 
             <mrow> 
              <mi>
                min 
              </mi> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msubsup> 
            <mo>
              ⋅ 
            </mo> 
            <msup> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mrow> 
                 <mi>
                   t 
                 </mi> 
                 <mo>
                   / 
                 </mo> 
                 <mrow> 
                  <msub> 
                   <mi>
                     t 
                   </mi> 
                   <mi>
                     p 
                   </mi> 
                  </msub> 
                 </mrow> 
                </mrow> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mn>
              2 
            </mn> 
            <mover accent="true"> 
             <mi>
               γ 
             </mi> 
             <mo>
               ˜ 
             </mo> 
            </mover> 
            <mfrac> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                C 
              </mi> 
             </mrow> 
             <mrow> 
              <mo>
                ∂ 
              </mo> 
              <mi>
                V 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (70)</p>
   <p>The threshold if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        2 
      </mn> 
      <mover accent="true"> 
       <mi>
         γ 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mfrac> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          C 
        </mi> 
       </mrow> 
       <mrow> 
        <mo>
          ∂ 
        </mo> 
        <mi>
          V 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msup> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            88 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> i.e. a huge value for initial complexity would be effectively made insignificant in cutting down the initial inflaton leading to</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            16 
          </mn> 
          <msqrt> 
           <mi>
             π 
           </mi> 
          </msqrt> 
         </mrow> 
         <mrow> 
          <msqrt> 
           <mi>
             ν 
           </mi> 
          </msqrt> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msubsup> 
           <mi>
             a 
           </mi> 
           <mrow> 
            <mi>
              min 
            </mi> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msubsup> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mrow> 
               <mi>
                 t 
               </mi> 
               <mo>
                 / 
               </mo> 
               <mrow> 
                <msub> 
                 <mi>
                   t 
                 </mi> 
                 <mi>
                   p 
                 </mi> 
                </msub> 
               </mrow> 
              </mrow> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <munder> 
       <mo>
         → 
       </mo> 
       <mrow> 
        <msubsup> 
         <mi>
           a 
         </mi> 
         <mrow> 
          <mi>
            min 
          </mi> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msubsup> 
        <mo>
          ≈ 
        </mo> 
        <msup> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            88 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
      </munder> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msup> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            88 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (71)</p>
   <p>i.e. we come to the seemingly counterintuitive expression that the initial inflaton potential would still be infinite if we used Equation (70) in Equation (66).</p>
  </sec><sec id="s10">
   <title>10. Future Developments for Applications of a Primordial HUP? Linking This to a Theory of Complex Initial and Final Structures. Black Holes Brought up</title>
   <p>From <xref ref-type="table" rid="table1">
     Table 1
    </xref> and information from <xref ref-type="bibr" rid="scirp.142274-18">
     [18]
    </xref> assuming Penrose recycling of the Universe as stated in that document. The limits in section four may give structural complexity data relevant to the following development. As given, see <xref ref-type="table" rid="table1">
     Table 1
    </xref>. This increase in complexity can be with work tied into the following for black hole physics <xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </xref> from Equation (1). References from <xref ref-type="bibr" rid="scirp.142274-18">
     [18]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-21">
     [21]
    </xref> are to be generally reviewed as to inspiration as to what we say next. We will try to quantify all this in future research work to explain this in terms of the physics of phase transitions, in the universe and cyclic conformal cosmology. Finally the physics of initial transformations as given in <xref ref-type="table" rid="table1">
     Table 1
    </xref> should have some linkage eventually to <xref ref-type="bibr" rid="scirp.142274-22">
     [22]
    </xref> as to the idea of Gravity breath, as given by Dr. Corda.</p>
  </sec><sec id="s11">
   <title>11. First Major Implication of This Use of the HUP Is to Investigate, i.e. Role of Complexity in Bridge from Black Hole Numbers as Given in <xref ref-type="table" rid="table1">
     Table 1
    </xref></title>
   <p>There are three regimes of black hole numbers given in <xref ref-type="table" rid="table1">
     Table 1
    </xref>. From Pre Planckian, to Planckian and then to post Planckian physics regimes. This is all assuming CCC cosmology. To start to make sense of this, we need to examine how one could achieve the complexity as indicated by <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref> in the Planckian era. To do this at a start, we will pay attention to a datum in reference <xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </xref>, namely a Horizon, like a Schwarzschild black hole construction with <xref ref-type="bibr" rid="scirp.142274-23">
     [23]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         L 
       </mi> 
       <mi>
         A 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mn>
           3 
         </mn> 
         <mi>
           Λ 
         </mi> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> (72)</p>
   <p>In what <xref ref-type="bibr" rid="scirp.142274-23">
     [23]
    </xref> deems as a corpuscular gravity one would have a “kinetic energy term” per graviton</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mo>
         ∈ 
       </mo> 
       <mi>
         G 
       </mi> 
      </msub> 
      <mtext>
          
      </mtext> 
      <mo>
        ≅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mover accent="true"> 
          <mi>
            N 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (73)</p>
   <p>And the mass of a black hole, scaling as <xref ref-type="bibr" rid="scirp.142274-23">
     [23]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mtext>
          black hole 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ≅ 
      </mo> 
      <msqrt> 
       <mover accent="true"> 
        <mi>
          N 
        </mi> 
        <mo>
          ˜ 
        </mo> 
       </mover> 
      </msqrt> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <msub> 
       <mo>
         ∈ 
       </mo> 
       <mi>
         G 
       </mi> 
      </msub> 
     </mrow> 
    </math> (74)</p>
   <p>This in <xref ref-type="bibr" rid="scirp.142274-3">
     [3]
    </xref> has the exact same functional forms as is given in Equation (27) so then we have 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mover accent="true"> 
       <mi>
         N 
       </mi> 
       <mo>
         ˜ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <mi>
        N 
      </mi> 
     </mrow> 
    </math> and furthermore <xref ref-type="bibr" rid="scirp.142274-23">
     [23]
    </xref> also has</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <msub> 
       <mo>
         ∈ 
       </mo> 
       <mi>
         G 
       </mi> 
      </msub> 
      <mtext>
          
      </mtext> 
      <mo>
        ≅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mover accent="true"> 
          <mi>
            N 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        ≅ 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           L 
         </mi> 
         <mi>
           A 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mi>
           N 
         </mi> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (75)</p>
   <p>If so for Black holes, we have the following</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msqrt> 
       <mi>
         Λ 
       </mi> 
      </msqrt> 
      <mo>
        ≅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msqrt> 
         <mn>
           3 
         </mn> 
        </msqrt> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mi>
          ℏ 
        </mi> 
        <msqrt> 
         <mi>
           N 
         </mi> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (76)</p>
   <p>Now as to what is given in <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> as to Torsion, we have that as given in <xref ref-type="bibr" rid="scirp.142274-18">
     [18]
    </xref> that we can do some relevant dimensional scaling.</p>
   <p>First look at numbers provided by <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> as to inputs, i.e. these are very revealing, i.e. we go back to the argument as to the beginning of the document, namely 
    <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></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.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref> is solely to remove this giant number.</p>
   <p>Our timing is to unleash a Planck time interval t about 10<sup>−</sup><sup>43</sup> seconds. Also the creation of the torsion term is due to a presumed “graviton” particle density of 
    <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>.</p>
   <p>This particle density is directly relevant to the basic assumption of how to have relevant Gravitons initially created as to obtain the huge increase in complexity alluded to, in order to obtain the number of micro black holes in the Planckian era <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142274-2">
     [2]
    </xref>.</p>
   <p>I.e. assume that there are, then say initially up to 10<sup>98</sup> gravitons, initially, and then from there, go to <xref ref-type="table" rid="table1">
     Table 1
    </xref> to assume what number of micro sized black holes are available, i.e. <xref ref-type="table" rid="table1">
     Table 1
    </xref> has say a figure of 10<sup>45</sup> to at most 10<sup>50</sup> micro sized black holes, presumably for 10<sup>98</sup> gravitons being released, and this is meaning we have say 10<sup>50</sup> black holes of say of Planck mass, to work with.</p>
  </sec><sec id="s12">
   <title>12. Part 3, the Question of If There Is a Linkage to All This and Structure Formation in the Early Universe and the 3 Body Problem, and the Possible NLED Inputs, into Early Universe Conditions</title>
   <p>
    <xref ref-type="bibr" rid="scirp.142274-"></xref>We recall using that the stronger an early universe magnetic field is, the greater the likelihood of production of about 20 new domains of size 1/H, with H early universe Hubble’s constant, per Planck time interval in evolution. Which leads to statements as to the value of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       α 
     </mi> 
    </math> in a gravitational potential proportional to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mi>
          α 
        </mi> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>.</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142274-"></xref>Part 1: We first of all recall that the scale f actor is affected by the NLED paradigm which in fact also is linked to the idea of “self reproduction” as given in <xref ref-type="bibr" rid="scirp.142274-24">
     [24]
    </xref>, which is a different way as to outline how this affects the evolution of density in the early universe leading to equation for setting the value of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       α 
     </mi> 
    </math> in a gravitational potential proportional to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mi>
          α 
        </mi> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>. This 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       α 
     </mi> 
    </math> has real and complex values, unlike the Newtonian real value, i.e. the problem of the 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       α 
     </mi> 
    </math> in a gravitational potential proportional to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         r 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mi>
          α 
        </mi> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mover accent="true"> 
        <mi>
          φ 
        </mi> 
        <mo>
          ¨ 
        </mo> 
       </mover> 
       <mi>
         k 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mn>
        3 
      </mn> 
      <mi>
        H 
      </mi> 
      <msub> 
       <mover accent="true"> 
        <mi>
          φ 
        </mi> 
        <mo>
          ˙ 
        </mo> 
       </mover> 
       <mi>
         k 
       </mi> 
      </msub> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           k 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <msub> 
       <mi>
         φ 
       </mi> 
       <mi>
         k 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
      <mo>
        , 
      </mo> 
      <mover> 
       <mrow></mrow> 
       <mrow></mrow> 
      </mover> 
      <msub> 
       <mi>
         φ 
       </mi> 
       <mi>
         k 
       </mi> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          H 
        </mi> 
        <mi>
          τ 
        </mi> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            k 
          </mi> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
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         <mrow> 
          <mrow> 
           <mo>
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           </mo> 
           <mrow> 
            <mi>
              i 
            </mi> 
            <mi>
              k 
            </mi> 
            <mi>
              τ 
            </mi> 
           </mrow> 
           <mo>
             ) 
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         </mrow> 
         <mrow> 
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            − 
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            1 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
       <mo>
         ) 
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      </mrow> 
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        ⋅ 
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      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mi>
          i 
        </mi> 
        <mi>
          k 
        </mi> 
        <mi>
          τ 
        </mi> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        , 
      </mo> 
      <mover> 
       <mrow></mrow> 
       <mrow></mrow> 
      </mover> 
      <mo>
        &amp; 
      </mo> 
      <mi>
        τ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <msup> 
       <mi>
         H 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        exp 
      </mi> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mi>
          H 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          t 
        </mi> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (77)</p>
   <p>Here, k is the value of wave number, and H is assumed, in the early universe to be a constant. The net result is that 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        k 
      </mi> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mi>
         λ 
       </mi> 
      </mrow> 
     </mrow> 
    </math>, with 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       λ 
     </mi> 
    </math> proportional to the “width” of a would be pre universe “bubble” as seen in <xref ref-type="bibr" rid="scirp.142274-24">
     [24]
    </xref> place of a singularity, and also that one would have, for a constant H, during this time as seen by</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        H 
      </mi> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mi>
          ρ 
        </mi> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mi>
           κ 
         </mi> 
         <mrow> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        , 
      </mo> 
      <mtext>
          
      </mtext> 
      <mi>
        ρ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        ' 
      </mo> 
      <mtext>
        energy density 
      </mtext> 
      <mo>
        ' 
      </mo> 
      <mo>
        , 
      </mo> 
      <mtext>
          
      </mtext> 
      <mi>
        κ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        ' 
      </mo> 
      <mtext>
        curvature 
      </mtext> 
      <mo>
        ' 
      </mo> 
     </mrow> 
    </math> (78)</p>
   <p>Further use of <xref ref-type="bibr" rid="scirp.142274-1">
     [1]
    </xref> will lead to the situation that</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        H 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mi>
          V 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           φ 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mover accent="true"> 
            <mi>
              φ 
            </mi> 
            <mo>
              ˙ 
            </mo> 
           </mover> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        ⇔ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mover accent="true"> 
          <mi>
            φ 
          </mi> 
          <mo>
            ˙ 
          </mo> 
         </mover> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           3 
         </mn> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mfrac> 
         <mi>
           κ 
         </mi> 
         <mrow> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <mi>
          V 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           φ 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        − 
      </mo> 
      <mi>
        ρ 
      </mi> 
     </mrow> 
    </math> (79)</p>
   <p>Chaotic inflation uses that 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        V 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         φ 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           k 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mi>
         φ 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> and the time derivative is 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mtext>
         d 
       </mtext> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mtext>
          d 
        </mtext> 
        <mi>
          τ 
        </mi> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math>, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        φ 
      </mi> 
      <mo>
        ≡ 
      </mo> 
      <msub> 
       <mi>
         φ 
       </mi> 
       <mi>
         k 
       </mi> 
      </msub> 
     </mrow> 
    </math>, and if so,</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mfrac> 
         <mrow> 
          <msubsup> 
           <mover accent="true"> 
            <mi>
              φ 
            </mi> 
            <mo>
              ˙ 
            </mo> 
           </mover> 
           <mi>
             k 
           </mi> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mrow> 
            <mn>
              8 
            </mn> 
            <mi>
              π 
            </mi> 
            <mi>
              G 
            </mi> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mfrac> 
           <mi>
             κ 
           </mi> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
          <mfrac> 
           <mrow> 
            <msup> 
             <mi>
               k 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             φ 
           </mi> 
           <mi>
             k 
           </mi> 
          </msub> 
          <msup> 
           <mrow /> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            − 
          </mo> 
          <mfrac> 
           <mrow> 
            <mn>
              16 
            </mn> 
           </mrow> 
           <mn>
             3 
           </mn> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             c 
           </mi> 
           <mn>
             1 
           </mn> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mi>
             B 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          &amp; 
        </mo> 
        <mtext>
            
        </mtext> 
        <mi>
          Δ 
        </mi> 
        <mi>
          E 
        </mi> 
        <mo>
          ≈ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
           <mrow> 
            <mn>
              8 
            </mn> 
            <mi>
              π 
            </mi> 
            <mi>
              G 
            </mi> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mfrac> 
           <mi>
             κ 
           </mi> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
          <mfrac> 
           <mrow> 
            <msup> 
             <mi>
               k 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msubsup> 
           <mi>
             φ 
           </mi> 
           <mi>
             k 
           </mi> 
           <mn>
             2 
           </mn> 
          </msubsup> 
          <mo>
            − 
          </mo> 
          <mfrac> 
           <mrow> 
            <mn>
              16 
            </mn> 
           </mrow> 
           <mn>
             3 
           </mn> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             c 
           </mi> 
           <mn>
             1 
           </mn> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mi>
             B 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (80)</p>
   <p>The last line of Equation (80) states that, if we apply it to the Pre Planckian to Planckian regime, that there will be a change in the energy, we then will call this shift in energy, as equivalent to a change in KINETIC energy,</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
         <mo>
           〈 
         </mo> 
         <mrow> 
          <mi>
            ψ 
          </mi> 
          <mo>
            | 
          </mo> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mtext>
              Kinetic Energy 
            </mtext> 
            <mo>
              ≈ 
            </mo> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mfrac> 
               <mn>
                 3 
               </mn> 
               <mrow> 
                <mn>
                  8 
                </mn> 
                <mi>
                  π 
                </mi> 
                <mi>
                  G 
                </mi> 
               </mrow> 
              </mfrac> 
              <mo>
                ⋅ 
              </mo> 
              <mfrac> 
               <mi>
                 κ 
               </mi> 
               <mrow> 
                <msup> 
                 <mi>
                   a 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msup> 
               </mrow> 
              </mfrac> 
              <mo>
                + 
              </mo> 
              <mfrac> 
               <mrow> 
                <msup> 
                 <mi>
                   k 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msup> 
               </mrow> 
               <mrow> 
                <msup> 
                 <mi>
                   a 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msup> 
               </mrow> 
              </mfrac> 
              <mo>
                ⋅ 
              </mo> 
              <msubsup> 
               <mi>
                 φ 
               </mi> 
               <mi>
                 k 
               </mi> 
               <mn>
                 2 
               </mn> 
              </msubsup> 
              <mo>
                − 
              </mo> 
              <mfrac> 
               <mrow> 
                <mn>
                  16 
                </mn> 
               </mrow> 
               <mn>
                 3 
               </mn> 
              </mfrac> 
              <mo>
                ⋅ 
              </mo> 
              <msub> 
               <mi>
                 c 
               </mi> 
               <mn>
                 1 
               </mn> 
              </msub> 
              <mo>
                ⋅ 
              </mo> 
              <msup> 
               <mi>
                 B 
               </mi> 
               <mn>
                 4 
               </mn> 
              </msup> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mo>
            | 
          </mo> 
          <mi>
            ψ 
          </mi> 
         </mrow> 
         <mo>
           〉 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          ≈ 
        </mo> 
        <mrow> 
         <mo>
           〈 
         </mo> 
         <mrow> 
          <mi>
            ψ 
          </mi> 
          <mo>
            | 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mi>
              r 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mo>
              ∇ 
            </mo> 
            <mrow> 
             <mo>
               [ 
             </mo> 
             <mrow> 
              <mi>
                V 
              </mi> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mtext>
                  Potential energy 
                </mtext> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
              <mo>
                ≈ 
              </mo> 
              <mrow> 
               <mrow> 
                <msub> 
                 <mi>
                   c 
                 </mi> 
                 <mn>
                   2 
                 </mn> 
                </msub> 
               </mrow> 
               <mo>
                 / 
               </mo> 
               <mrow> 
                <msup> 
                 <mi>
                   r 
                 </mi> 
                 <mi>
                   α 
                 </mi> 
                </msup> 
               </mrow> 
              </mrow> 
             </mrow> 
             <mo>
               ] 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            | 
          </mo> 
          <mi>
            ψ 
          </mi> 
         </mrow> 
         <mo>
           〉 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (81)</p>
   <p>In the Pre Planckian to Planckian space time, we will approximate, in the instant before time is initialized, formally, the mean value theorem with the results that we obtain</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             3 
           </mn> 
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            <mn>
              8 
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            <mi>
              π 
            </mi> 
            <mi>
              G 
            </mi> 
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          </mfrac> 
          <mo>
            ⋅ 
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          <mfrac> 
           <mi>
             κ 
           </mi> 
           <mrow> 
            <msup> 
             <mi>
               a 
             </mi> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
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           <mrow> 
            <msup> 
             <mi>
               k 
             </mi> 
             <mn>
               2 
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             <mi>
               a 
             </mi> 
             <mn>
               2 
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           </mrow> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msubsup> 
           <mi>
             φ 
           </mi> 
           <mi>
             k 
           </mi> 
           <mn>
             2 
           </mn> 
          </msubsup> 
          <mo>
            − 
          </mo> 
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           <mrow> 
            <mn>
              16 
            </mn> 
           </mrow> 
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             3 
           </mn> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             c 
           </mi> 
           <mn>
             1 
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           <mi>
             B 
           </mi> 
           <mn>
             4 
           </mn> 
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           ) 
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           </mi> 
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          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mtext>
                Planck length 
              </mtext> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mi>
             α 
           </mi> 
          </msup> 
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        </mrow> 
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      </mtr> 
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          ⇔ 
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                 ) 
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           </mrow> 
          </mrow> 
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           ] 
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            16 
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            ⋅ 
          </mo> 
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           <mi>
             κ 
           </mi> 
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             <mi>
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             </mi> 
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             </mn> 
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           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
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           <mrow> 
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             <mi>
               k 
             </mi> 
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             </mn> 
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           </mrow> 
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             </mi> 
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          </mfrac> 
          <mo>
            ⋅ 
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           <mi>
             φ 
           </mi> 
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             k 
           </mi> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (82)</p>
   <p>Here, the magnetic field would be determined in part by the value of B, and the scale factor 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       a 
     </mi> 
    </math>, is given, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         φ 
       </mi> 
       <mi>
         k 
       </mi> 
      </msub> 
     </mrow> 
    </math> is given by Equation(82) This shows in part that 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       α 
     </mi> 
    </math> is no longer strictly real valued but is strongly influenced by the input from 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         φ 
       </mi> 
       <mi>
         k 
       </mi> 
      </msub> 
     </mrow> 
    </math>, i.e. which has real and imaginary components. What we should endeavour through judicious application of Equation (82) is to remove dependence upon the smallness of the third mass, and to examine if this can still, with a non-trivial third mass recover still much of the stability analysis. Later, at an appropriate time this question in terms of a serious application of the value of Equation (82) will be pursued, Secondly, as of <xref ref-type="bibr" rid="scirp.142274-25">
     [25]
    </xref> the section gives on page 154, entitled “6.4 Orbital changes in encounters with planets”, which is a restricted 3 body problem, frequently is used as to the interaction of say comets (small mass) with a planet, circulating the Sun, where we have 2 “massive” masses, and the third body, in this case a comet, which gives usually parameters of how a hyperbolic orbit for a comet, should be reviewed again. This is meant to be in tandem with results as far as self reproduction of structure given in <xref ref-type="bibr" rid="scirp.142274-26">
     [26]
    </xref> which is how we started <xref ref-type="bibr" rid="scirp.142274-24">
     [24]
    </xref>.</p>
   <p>WHAT we will state is that in the early universe is that the scale factor used in Equation(82) will be closely aligned to the regime of when we apply Equation (5) in the earlier universe, which we will consider in future works.</p>
  </sec><sec id="s13">
   <title>13. 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.142274-7">
     [7]
    </xref> is what we will start off with <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </xref> and its given metric as far as a black hole to white hole solution.</p>
   <p>Namely</p>
   <p>
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         2 
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     </mrow> 
    </math> (83)</p>
   <p>We can perform a major simplification by setting, then</p>
   <p>
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      <mi>
        A 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          a 
        </mi> 
       </mrow> 
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         ) 
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        = 
      </mo> 
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        B 
      </mi> 
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         ( 
       </mo> 
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        <mi>
          r 
        </mi> 
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          , 
        </mo> 
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          a 
        </mi> 
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         ) 
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        = 
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        f 
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         ( 
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          r 
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          a 
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       <mo>
         ) 
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     </mrow> 
    </math> (84)</p>
   <p>In doing so, <xref ref-type="bibr" rid="scirp.142274-7">
     [7]
    </xref> gives us the following stress energy tensor values as give</p>
   <p>
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          ⋅ 
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             </mo> 
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             ) 
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           </mn> 
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            ⋅ 
          </mo> 
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             ( 
           </mo> 
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              f 
            </mi> 
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            </mo> 
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    </math> (85)</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.142274-7">
     [7]
    </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>
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   <p>We then make the following connection to energy density in a black hole to white hole system, i.e.</p>
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   <p>This will lead to, if we use Planck units where we normalize h bar to being 1, of</p>
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    </math> (88)</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 (88) 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="s14">
   <title>14. What Sections We Call Part 1, Part 2 and Part 3 and Part 4 Are Saying and Future Prospects of Research</title>
   <p>Part 3 is to the three body problem, and our scale factors assumed as part of the equations of state, of early GW formulation may indeed be modified.</p>
   <p>Part 4 as given in XI. gives us the distinct way to investigate if there is a black hole to white hole pairing from a present to a prior universe, in terms of quantum number n associated with a black hole to white hole linked by a worm hole.</p>
   <p>What we would have to do, find an optimal way to find functions f and g as to Part 3, and to see if that can be linked directly to the Part 1 derivation, and its quantum number as well as <xref ref-type="table" rid="table1">
     Table 1
    </xref>. In doing so we should be aware that the wormhole linkage would be repeated say 50 million times, with the energy density showing up in our analysis of how and why Torsion would be viable in the first place.</p>
   <p>Finding optimal f and g functions will require serious matching condition work. Is it doable? Yes, but we should keep in mind something else, namely that we are also assuming the necessity of a pre Planckian negative energy density,</p>
   <p>Considering that the Corda treatment of black hole energy also involves negative energy values, in <xref ref-type="bibr" rid="scirp.142274-22">
     [22]
    </xref> this is no surprise, but it means we need attendant data set analysis in order to make sense of the entire idea of a gluing parameter 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
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    </math> have to be specified.</p>
   <p>Finally the idea of transvesable wormholes has to be re-investigated to see if in this configuration it makes sense at all in this situation i.e. a 4 dimensional recent treatment of this idea is in <xref ref-type="bibr" rid="scirp.142274-27">
     [27]
    </xref>.</p>
   <p>If the bridge between a prior to a present universe, involves transversable wormholes, via linkage of a black hole to white hole, the author, namely me asserts that if the transversable wormhole is 
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    </math> approaching Planck frequency, of about 10<sup>45</sup> or so Hertz, which has MAJOR inplications as far as High frequency GW. That in itself would be indicating, even if we have MASSIVE red shifting, that we are considering here 10<sup>5</sup> to say 10<sup>10</sup> Hz GW in the present era.</p>
  </sec><sec id="s15">
   <title>15. A Final Pre Messenger Regime for Particle Production Consideration, the Re Acceleration of the Universe</title>
   <p>When we quantize the gravitational field as an effective field theory, we find that it too comes in set “quanta,” called gravitons. In short, we argue that to come up with a graviton based model of DE with reacceleration of the universe, and to have it commensurate with the modification of the 1/r potential, we are really coming up with a program of finding out if gravity can be quantized. In addition, what we have done is complimenting turbulence in the electroweak era. Which in turn is relatable to the question of whether micro black holes, could contribute to cosmology. This means keeping in mind, i.e. the diagram given by Abbott et al. <xref ref-type="bibr" rid="scirp.142274-28">
     [28]
    </xref> (2009) which shows the relation between GW frequency and GW energy density for different cosmological models What we are doing is to try to reconcile 
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    </math> with the idea of graviton production from the early states of the universe. At first glance, this looks hopeless. i.e. the models are incommensurate with each other and we do have a huge problem. A way of having reconciliation may be to consider what is brought up on pages 114 to 115 of Li, Wang, and Wang, <xref ref-type="bibr" rid="scirp.142274-29">
     [29]
    </xref> as we have, then an examination of the equation of state for DE, that is commensurate with re acceleration of the universe as reading,</p>
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   <p>Again, this looks like a very hard problem, but, what we need to accomplish is having the following identification made, which may allow for us to make a concrete bridge between formalisms which otherwise look like they have no linkage to each other, i.e. do the following, namely is there a way to link 
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   <p>Then, we should try to reconcile the following, a way to link 
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     [27]
    </xref>.</p>
   <p>Finally keep in mind this one, i.e. in the early universe a linkage as to Equation (82), and variations as to early space time. And the re acceleration of the Universe problem. i.e. starting with this for the regime of space time</p>
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   <p>i.e. the claim to be investigated is the following. If we solve this correctly as far as black holes, in relic conditions can we tie this heavy graviton effects of space time into to the following?</p>
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       </mover> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mover accent="true"> 
            <mi>
              κ 
            </mi> 
            <mo>
              ˜ 
            </mo> 
           </mover> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mi>
              ρ 
            </mi> 
            <mo>
              + 
            </mo> 
            <mfrac> 
             <mrow> 
              <msup> 
               <mi>
                 ρ 
               </mi> 
               <mn>
                 2 
               </mn> 
              </msup> 
             </mrow> 
             <mrow> 
              <mn>
                2 
              </mn> 
              <mi>
                λ 
              </mi> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mrow> 
          <mi>
            Λ 
          </mi> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mi>
           m 
         </mi> 
         <mrow> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mi>
          K 
        </mi> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (93)</p>
   <p>Maartens <xref ref-type="bibr" rid="scirp.142274-30">
     [30]
    </xref> also gives a 2<sup>nd</sup> Friedman equation:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mover accent="true"> 
        <mi>
          H 
        </mi> 
        <mo>
          ˙ 
        </mo> 
       </mover> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <msup> 
             <mover accent="true"> 
              <mi>
                κ 
              </mi> 
              <mo>
                ˜ 
              </mo> 
             </mover> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </mfrac> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mi>
              p 
            </mi> 
            <mo>
              + 
            </mo> 
            <mi>
              ρ 
            </mi> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mo>
            ⋅ 
          </mo> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mfrac> 
             <mrow> 
              <msup> 
               <mi>
                 ρ 
               </mi> 
               <mn>
                 2 
               </mn> 
              </msup> 
             </mrow> 
             <mi>
               λ 
             </mi> 
            </mfrac> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mrow> 
          <mi>
            Λ 
          </mi> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mn>
          2 
        </mn> 
        <mfrac> 
         <mi>
           m 
         </mi> 
         <mrow> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mi>
           K 
         </mi> 
         <mrow> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (94)</p>
   <p>Also, an observer is in the low redshift regime for cosmology, for which 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ρ 
      </mi> 
      <mo>
        ≅ 
      </mo> 
      <mo>
        − 
      </mo> 
      <mi>
        P 
      </mi> 
     </mrow> 
    </math>, for red-shift values z from zero to 1.0 - 1.5. One obtains exact equality, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ρ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mi>
        P 
      </mi> 
     </mrow> 
    </math>, for z between zero to 5. The net effect will be to obtain, based on Equation (93), assuming 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Λ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
      <mo>
        = 
      </mo> 
      <mi>
        K 
      </mi> 
     </mrow> 
    </math> and using 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        a 
      </mi> 
      <mo>
        ≡ 
      </mo> 
      <mrow> 
       <mrow> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             a 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mrow> 
     </mrow> 
    </math> to get a deceleration parameter q as given in Equation (95).</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        q 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mover accent="true"> 
         <mi>
           a 
         </mi> 
         <mo>
           ¨ 
         </mo> 
        </mover> 
        <mi>
          a 
        </mi> 
       </mrow> 
       <mrow> 
        <msup> 
         <mover accent="true"> 
          <mi>
            a 
          </mi> 
          <mo>
            ˙ 
          </mo> 
         </mover> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mn>
         2 
       </mn> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <msup> 
         <mover accent="true"> 
          <mi>
            κ 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             ρ 
           </mi> 
           <mo>
             / 
           </mo> 
           <mi>
             m 
           </mi> 
          </mrow> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           4 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mrow> 
           <mi>
             ρ 
           </mi> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mi>
              λ 
            </mi> 
           </mrow> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mn>
         2 
       </mn> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          δ 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (95)</p>
   <p>
    <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref> is predicated upon a small 4 dimensional rest mass (stated in Equation (93) for a graviton behaving the same as dark energy… We will state in our discussions section as to what is needed to give experimental confirmation as to what is a current for a “massive” graviton which is appropriate for explaining in part, <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref>.</p>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>Figure 1. Re-acceleration of the universe based on Beckwith <xref ref-type="bibr" rid="scirp.142274-31">
       [31]
      </xref>; (note that q(z) &lt; 0 if z &lt; 0.423.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181271-rId350.jpeg?20250427045230" />
   </fig>
   <p>This idea, with some revisions is similar to, for heavy gravity, at the start of Equation (5) to the following i.e.</p>
   <p>Beckwith <xref ref-type="bibr" rid="scirp.142274-31">
     [31]
    </xref> used a higher-dimensional model of the brane world combined with KK graviton towers per Maartens <xref ref-type="bibr" rid="scirp.142274-30">
     [30]
    </xref>. The energy density 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ρ 
     </mi> 
    </math> of the brane world in the Friedman equation is used in a form similar to Alves et al. <xref ref-type="bibr" rid="scirp.142274-32">
     [32]
    </xref> by Beckwith <xref ref-type="bibr" rid="scirp.142274-31">
     [31]
    </xref> for a non-zero graviton:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ρ 
      </mi> 
      <mo>
        ≡ 
      </mo> 
      <msub> 
       <mi>
         ρ 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </msup> 
      <mo>
        − 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             m 
           </mi> 
           <mi>
             g 
           </mi> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                c 
              </mi> 
              <mo>
                = 
              </mo> 
              <mn>
                1 
              </mn> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             6 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                ℏ 
              </mi> 
              <mo>
                = 
              </mo> 
              <mn>
                1 
              </mn> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            14 
          </mn> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                1 
              </mn> 
              <mo>
                + 
              </mo> 
              <mi>
                z 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             3 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mn>
           2 
         </mn> 
         <mrow> 
          <mn>
            5 
          </mn> 
          <mo>
            ⋅ 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                1 
              </mn> 
              <mo>
                + 
              </mo> 
              <mi>
                z 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (96)</p>
   <p>Keep in mind the following, i.e.</p>
   <p>Consider if there is then also a small graviton mass, i.e., as stated by Beckwith <xref ref-type="bibr" rid="scirp.142274-31">
     [31]
    </xref>:</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         n 
       </mi> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          Gravition 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             n 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             L 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               m 
             </mi> 
             <mrow> 
              <mtext>
                gravition rest mass 
              </mtext> 
             </mrow> 
            </msub> 
            <mo>
              = 
            </mo> 
            <msup> 
             <mrow> 
              <mn>
                10 
              </mn> 
             </mrow> 
             <mrow> 
              <mo>
                − 
              </mo> 
              <mn>
                65 
              </mn> 
             </mrow> 
            </msup> 
            <mtext>
                
            </mtext> 
            <mtext>
              grams 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         n 
       </mi> 
       <mi>
         L 
       </mi> 
      </mfrac> 
      <mo>
        + 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          65 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        grams 
      </mtext> 
     </mrow> 
    </math> (97)</p>
   <p>Note that Rubakov (2002) <xref ref-type="bibr" rid="scirp.142274-33">
     [33]
    </xref> works with KK gravitons, without the tiny mass term for a 4-dimensional rest mass included in Equation (97). To obtain the KK graviton/DM candidate representation along RS dS brane world, Rubakov obtains his values for graviton mass and graviton physical states in space-time after using the following normalization: 
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mstyle displaystyle="true"> 
       <mrow> 
        <mo>
          ∫ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <mtext>
             d 
           </mtext> 
           <mi>
             z 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             a 
           </mi> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mi>
              z 
            </mi> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
         </mfrac> 
        </mrow> 
       </mrow> 
      </mstyle> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           h 
         </mi> 
         <mi>
           m 
         </mi> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           h 
         </mi> 
         <mover accent="true"> 
          <mi>
            m 
          </mi> 
          <mo>
            ˜ 
          </mo> 
         </mover> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           z 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        ≡ 
      </mo> 
      <mi>
        δ 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          m 
        </mi> 
        <mo>
          − 
        </mo> 
        <mover accent="true"> 
         <mi>
           m 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>. Rubakov <xref ref-type="bibr" rid="scirp.142274-33">
     [33]
    </xref> (2002) uses 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         J 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mi>
         J 
       </mi> 
       <mn>
         2 
       </mn> 
      </msub> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mi>
         N 
       </mi> 
       <mn>
         1 
       </mn> 
      </msub> 
      <mo>
        , 
      </mo> 
      <msub> 
       <mi>
         N 
       </mi> 
       <mn>
         2 
       </mn> 
      </msub> 
     </mrow> 
    </math> which are different forms of Bessel functions. His representation of a graviton state is given by</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mrow> 
      <mo>
        − 
      </mo> 
      <mn>
        2 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             m 
           </mi> 
           <mrow> 
            <mtext>
              Plank 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <mover accent="true"> 
       <mi>
         H 
       </mi> 
       <mo>
         ˙ 
       </mo> 
      </mover> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mover accent="true"> 
        <mi>
          ϕ 
        </mi> 
        <mo>
          ˙ 
        </mo> 
       </mover> 
       <mn>
         2 
       </mn> 
      </msup> 
     </mrow> 
    </math> (98)</p>
   <p>Equation (98), which is almost completely acceptable for our problem, since the rest mass of a graviton in four dimensions is so small. If so, then the wave function for a graviton with a tiny 4 dimensional space time rest mass can be written as <xref ref-type="bibr" rid="scirp.142274-33">
     [33]
    </xref>.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mi>
         m 
       </mi> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         z 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mrow> 
         <mi>
           m 
         </mi> 
         <mo>
           / 
         </mo> 
         <mi>
           k 
         </mi> 
        </mrow> 
       </mrow> 
      </msqrt> 
      <mo>
        ⋅ 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           J 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             m 
           </mi> 
           <mo>
             / 
           </mo> 
           <mi>
             k 
           </mi> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           N 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mrow> 
             <mi>
               m 
             </mi> 
             <mo>
               / 
             </mo> 
             <mi>
               k 
             </mi> 
            </mrow> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mo>
            ⋅ 
          </mo> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mi>
              k 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           N 
         </mi> 
         <mn>
           1 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mi>
             m 
           </mi> 
           <mo>
             / 
           </mo> 
           <mi>
             k 
           </mi> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           J 
         </mi> 
         <mn>
           2 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mrow> 
           <mo>
             [ 
           </mo> 
           <mrow> 
            <mrow> 
             <mi>
               m 
             </mi> 
             <mo>
               / 
             </mo> 
             <mi>
               k 
             </mi> 
            </mrow> 
           </mrow> 
           <mo>
             ] 
           </mo> 
          </mrow> 
          <mo>
            ⋅ 
          </mo> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mi>
              k 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               [ 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 J 
               </mi> 
               <mn>
                 1 
               </mn> 
              </msub> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mrow> 
                 <mi>
                   m 
                 </mi> 
                 <mo>
                   / 
                 </mo> 
                 <mi>
                   k 
                 </mi> 
                </mrow> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mo>
               ] 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            + 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               [ 
             </mo> 
             <mrow> 
              <msub> 
               <mi>
                 N 
               </mi> 
               <mn>
                 1 
               </mn> 
              </msub> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mrow> 
                 <mi>
                   m 
                 </mi> 
                 <mo>
                   / 
                 </mo> 
                 <mi>
                   k 
                 </mi> 
                </mrow> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mo>
               ] 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (99)</p>
   <p>Equation (99) is for KK gravitons having a TeV magnitude mass 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         Z 
       </mi> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mi>
        k 
      </mi> 
     </mrow> 
    </math> (i.e., for mass values at 0.5 TeV to above 1 TeV) on a negative tension RS brane. It would be useful to relate this KK graviton, which is moving with a speed proportional to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         H 
       </mi> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> with regards to the negative tension brane with 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ≡ 
      </mo> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mi>
         m 
       </mi> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          z 
        </mi> 
        <mo>
          → 
        </mo> 
        <mn>
          0 
        </mn> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        n 
      </mi> 
      <mi>
        s 
      </mi> 
      <mi>
        t 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mi>
           m 
         </mi> 
         <mi>
           k 
         </mi> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> as an initial starting value for the KK graviton mass. If Equation (98) is for a “massive” graviton with a small 4-dimensional gravition rest mass and if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        h 
      </mi> 
      <mo>
        ≡ 
      </mo> 
      <msub> 
       <mi>
         h 
       </mi> 
       <mi>
         m 
       </mi> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          z 
        </mi> 
        <mo>
          → 
        </mo> 
        <mn>
          0 
        </mn> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        o 
      </mi> 
      <mi>
        n 
      </mi> 
      <mi>
        s 
      </mi> 
      <mi>
        t 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mi>
           m 
         </mi> 
         <mi>
           k 
         </mi> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> represents an initial state, then one may relate the mass of the KK graviton moving at high speed with the initial rest mass of the graviton. This rest mass of a graviton is 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mrow> 
        <mtext>
          gravition 
        </mtext> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          4-Dim GR 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          48 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        eV 
      </mtext> 
     </mrow> 
    </math>, opposed to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         X 
       </mi> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mtext>
          KK Gravition 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <mn>
        0.5 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mn>
         9 
       </mn> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        eV 
      </mtext> 
     </mrow> 
    </math>. Whatever the range of the graviton mass, it may be a way to make sense of what was presented by Dubovsky et al. <xref ref-type="bibr" rid="scirp.142274-34">
     [34]
    </xref>, who argue for a graviton mass, using CMBR measurements, of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mtext>
          KK Gravition 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          20 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        eV 
      </mtext> 
     </mrow> 
    </math>.</p>
  </sec><sec id="s16">
   <title>16. 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>The key to doing this is to take into consideration Equation (82) which has a B (magnetic) field right in its description of scale and interaction issues. i.e. this is the point where we can take up the following <xref ref-type="bibr" rid="scirp.142274-13">
     [13]
    </xref>-<xref ref-type="bibr" rid="scirp.142274-15">
     [15]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <mrow> 
         <mo>
           〈 
         </mo> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                δ 
              </mi> 
              <msub> 
               <mi>
                 g 
               </mi> 
               <mrow> 
                <mi>
                  u 
                </mi> 
                <mi>
                  v 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mover accent="true"> 
                <mi>
                  T 
                </mi> 
                <mo>
                  ^ 
                </mo> 
               </mover> 
               <mrow> 
                <mi>
                  u 
                </mi> 
                <mi>
                  v 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           〉 
         </mo> 
        </mrow> 
        <mo>
          ≥ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             ℏ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msubsup> 
           <mi>
             V 
           </mi> 
           <mrow> 
            <mtext>
              Volume 
            </mtext> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <munder> 
         <mo>
           → 
         </mo> 
         <mrow> 
          <mi>
            u 
          </mi> 
          <mi>
            v 
          </mi> 
          <mo>
            → 
          </mo> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </munder> 
        <mrow> 
         <mo>
           〈 
         </mo> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                δ 
              </mi> 
              <msub> 
               <mi>
                 g 
               </mi> 
               <mrow> 
                <mi>
                  t 
                </mi> 
                <mi>
                  t 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <msub> 
               <mover accent="true"> 
                <mi>
                  T 
                </mi> 
                <mo>
                  ^ 
                </mo> 
               </mover> 
               <mrow> 
                <mi>
                  t 
                </mi> 
                <mi>
                  t 
                </mi> 
               </mrow> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           〉 
         </mo> 
        </mrow> 
        <mo>
          ≥ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             ℏ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msubsup> 
           <mi>
             V 
           </mi> 
           <mrow> 
            <mtext>
              Volume 
            </mtext> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msubsup> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo>
          &amp; 
        </mo> 
        <mo> 
        </mo> 
        <mtext>
            
        </mtext> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            r 
          </mi> 
          <mi>
            r 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ~ 
        </mo> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            θ 
          </mi> 
          <mi>
            θ 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ~ 
        </mo> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            ϕ 
          </mi> 
          <mi>
            ϕ 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ~ 
        </mo> 
        <msup> 
         <mn>
           0 
         </mn> 
         <mo>
           + 
         </mo> 
        </msup> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (100)</p>
   <p>We assume that 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          t 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is a small perturbation and look at 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        δ 
      </mi> 
      <mi>
        t 
      </mi> 
      <mi>
        Δ 
      </mi> 
      <mi>
        E 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         ℏ 
       </mi> 
       <mrow> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> with</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mrow> 
        <mtext>
          time 
        </mtext> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mtext>
          initial 
        </mtext> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mi>
         ℏ 
       </mi> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            δ 
          </mi> 
          <msub> 
           <mi>
             g 
           </mi> 
           <mrow> 
            <mi>
              t 
            </mi> 
            <mi>
              t 
            </mi> 
           </mrow> 
          </msub> 
          <msub> 
           <mi>
             E 
           </mi> 
           <mrow> 
            <mtext>
              initial 
            </mtext> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          ℏ 
        </mi> 
       </mrow> 
       <mrow> 
        <mi>
          δ 
        </mi> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mi>
            t 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           g 
         </mi> 
         <mrow> 
          <mo>
            ∗ 
          </mo> 
          <mi>
            s 
          </mi> 
         </mrow> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            initial 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
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          ⋅ 
        </mo> 
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         <mi>
           T 
         </mi> 
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            initial 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (101)</p>
   <p>This would put a requirement upon a very large initial temperature 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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         T 
       </mi> 
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          initial 
        </mtext> 
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    </math> and so then, if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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       </mi> 
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          volume 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
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           <mi>
             π 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            45 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
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      </mrow> 
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        ⋅ 
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         </mo> 
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           </mi> 
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              initial 
            </mtext> 
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           ) 
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         3 
       </mn> 
      </msup> 
     </mrow> 
    </math> <xref ref-type="bibr" rid="scirp.142274-35">
     [35]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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          particle count 
        </mtext> 
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         ) 
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        ≈ 
      </mo> 
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            volume 
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            45 
          </mn> 
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            </mi> 
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                initial 
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           ) 
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         3 
       </mn> 
      </msup> 
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    </math> (102)</p>
   <p>And if we can write as given in</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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          volume 
        </mtext> 
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        ~ 
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           ( 
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           4 
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           ) 
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        = 
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       </mi> 
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          surface area 
        </mtext> 
       </mrow> 
      </msub> 
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        ⋅ 
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      <mrow> 
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         ( 
       </mo> 
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        </mi> 
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        </mo> 
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         </mi> 
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            Planck 
          </mtext> 
         </mrow> 
        </msub> 
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         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (103)</p>
   <p>Then as to the follow-up to NLED and signals from primordial processes <xref ref-type="bibr" rid="scirp.142274-36">
     [36]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
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          = 
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              4 
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              </mi> 
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              ) 
            </mo> 
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            ] 
          </mo> 
         </mrow> 
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             1 
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             / 
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         </mrow> 
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       </mtd> 
      </mtr> 
     </mtable> 
    </math> (104)</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.142274-36">
     [36]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        B 
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        &gt; 
      </mo> 
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          </mn> 
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          </mi> 
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    </math> (105)</p>
   <p>We submit the following for future investigation, namely the n particle count as presented in Equation (103) is related directly to inputs into Equation (5) and that the quantum number as discussed is linkable to the discussion given in Equation (45) and Equation (46).</p>
   <p>Furthermore, the frequency, as given in Equation (105) would be tied into Equation (14) via the n of that equation as well as specified by <xref ref-type="bibr" rid="scirp.142274-37">
     [37]
    </xref> on page 111, where we have</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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      </mi> 
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       </mi> 
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          r 
        </mi> 
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          r 
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      </msub> 
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        c 
      </mi> 
      <mi>
        k 
      </mi> 
     </mrow> 
    </math> (106)</p>
   <p>Here 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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         g 
       </mi> 
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        </mi> 
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          r 
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       </mrow> 
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    </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 multimessenger astronomy namely the discussion as given in Mohanty, <xref ref-type="bibr" rid="scirp.142274-38">
     [38]
    </xref> namely a temperature, with scale factor as given in page 261</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        T 
      </mi> 
      <mo>
        ~ 
      </mo> 
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       <mn>
         1 
       </mn> 
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           g 
         </mi> 
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           ∗ 
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          a 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (107)</p>
   <p>With temperature T, as proportional to quantum number n as specified, whereas k as in Equation (106) 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.142274-39">
     [39]
    </xref> which can make a connection analytically to mulimessenger Astrophysics explicit <xref ref-type="bibr" rid="scirp.142274-40">
     [40]
    </xref>.</p>
  </sec>
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