<?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.2025.112033
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-142237
   </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 and the Presence of Barbour’s Shape Dynamics to Explain Different Pathways for a Change of Energy State at the Start of Inflation
   </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>
    464
   </fpage>
   <lpage>
    479
   </lpage>
   <history>
    <date date-type="received">
     <day>
      9,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      22,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      22,
     </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. The formation of a cosmological constant is akin to use Torsion in order to obtain the cosmological constant, but in order to do so, we need a starting point as far as emergence of energy from the onset of the Big Bang. This paper is dedicated to that proposition, using Barbour shape formulation to obtain emergent energy values which are less disruptive to pre Planckian to Planckian physics than the usual paradigms. In particular, our emergent energy values are using Padmanabhan scalar field construction, combined with a modified HUP construction, which we then try to tie into black hole physics.
   </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.142237-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-3">
     [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 a reference to the BEC condensate given by <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-3">
     [3]
    </xref> as 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.142237-"></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 
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      <mi>
        a 
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    </math> is a proportionality term, i.e. what we reference in the primordial era</p>
   <p>
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    </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> 
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        = 
      </mo> 
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       </mrow> 
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    </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> 
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         ( 
       </mo> 
       <mrow> 
        <mtext>
          loss 
        </mtext> 
       </mrow> 
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         ) 
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        = 
      </mo> 
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         ( 
       </mo> 
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         <mrow> 
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            − 
          </mo> 
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            5 
          </mn> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mn>
              64 
            </mn> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          ⋅ 
        </mo> 
        <mover accent="true"> 
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           a 
         </mi> 
         <mo>
           ˜ 
         </mo> 
        </mover> 
       </mrow> 
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         ) 
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        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             ℏ 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mrow> 
            <mn>
              12 
            </mn> 
           </mrow> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             π 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
          <msubsup> 
           <mi>
             k 
           </mi> 
           <mi>
             B 
           </mi> 
           <mn>
             4 
           </mn> 
          </msubsup> 
          <msup> 
           <mi>
             G 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> (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. In order to do this, though we need to consider where the energy budget for black holes initially came from in the primordial Universe.</p>
  </sec><sec id="s2">
   <title>2. A Brief Explainer as to How Shape Dynamics, May Induce an Energy Flux for the Creation of Relic Black Holes, with an Initially Incorrect Value of the Cosmological Constant</title>
   <p>In (<xref ref-type="bibr" rid="scirp.142237-4">
     [4]
    </xref>, p. 265), Barbour uses shape dynamics to come up with a delta t expression in a way which we can rewrite as having the following input into formation of initial cosmological constant energy starting with <xref ref-type="bibr" rid="scirp.142237-5">
     [5]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-7">
     [7]
    </xref> which we will use.</p>
   <p>Namely, we will be working with <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> <xref ref-type="bibr" rid="scirp.142237-4">
     [4]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-7">
     [7]
    </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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          = 
        </mo> 
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         </mi> 
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          ℏ 
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          ⇔ 
        </mo> 
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            initial 
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           ) 
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    </math> (4)</p>
   <p>i.e. the fluctuation 
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    </math> dramatically boosts initial entropy. Not what it would be if 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        ≈ 
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        1 
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     </mrow> 
    </math>. The next question to ask would be how could one actually have <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-3">
     [3]
    </xref> <xref ref-type="bibr" rid="scirp.142237-6">
     [6]
    </xref> <xref ref-type="bibr" rid="scirp.142237-7">
     [7]
    </xref></p>
   <p>
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      </mi> 
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         → 
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    </math> (5)</p>
   <p>In short, we require an enormous “inflaton” style 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ϕ 
     </mi> 
    </math> valued scalar function, and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        </mo> 
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        </mn> 
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      </msup> 
     </mrow> 
    </math> How could 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ϕ 
     </mi> 
    </math> be initially quite large? Within Planck time the following for mass holds, as a lower bound <xref ref-type="bibr" rid="scirp.142237-6">
     [6]
    </xref> <xref ref-type="bibr" rid="scirp.142237-7">
     [7]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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          graviton 
        </mtext> 
       </mrow> 
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      <mo>
        ≥ 
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      <mfrac> 
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           2 
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        </msubsup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (6)</p>
   <p>This is in terms of an initial HUP which is defined by <xref ref-type="bibr" rid="scirp.142237-4">
     [4]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-7">
     [7]
    </xref></p>
   <p>
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           〈 
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    </math> (7)</p>
   <p>Also if</p>
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   <p>Then</p>
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    </math> (9)</p>
   <p>This uses the following, i.e. to keep in mind in terms of visualizing the initial HUP</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142237-"></xref> 
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    </math> (10)</p>
   <p>If we use the following, from the Roberson-Walker metric <xref ref-type="bibr" rid="scirp.142237-14">
     [14]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </xref></p>
   <p>
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    </math> (11)</p>
   <p>Following Unruh <xref ref-type="bibr" rid="scirp.142237-14">
     [14]
    </xref> <xref ref-type="bibr" rid="scirp.142237-15">
     [15]
    </xref>, write then, an uncertainty of metric tensor as, with the following inputs</p>
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    </math> (12)</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142237-"></xref>Then, if 
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    </math> (13)</p>
   <p>Here, we have that the lead-up of all of this, if we merely assume a massive energy flux is an enormous vacuum energy term.</p>
   <p>Here, <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-6">
     [6]
    </xref></p>
   <p>
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    </math> (14)</p>
   <p>Then <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-6">
     [6]
    </xref> <xref ref-type="bibr" rid="scirp.142237-7">
     [7]
    </xref></p>
   <p>
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    </math> (15)</p>
   <p>We will proceed to isolate out an energy flux term which will be able to ascertain how to make sense of this enormous change in an inflation environment, and here is what we are trying to avoid, i.e. a simple model will be presented, which we state gives the wrong value for a cosmological constant term I.e. in doing so, we will utilize the following namely</p>
  </sec><sec id="s3">
   <title>3. How Could Anyone Get the Acceleration of the Universe Factored into Our Scale Factor?</title>
   <p>Begin looking at material from page 483-485 of <xref ref-type="bibr" rid="scirp.142237-8">
     [8]
    </xref></p>
   <p>
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        = 
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        0 
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    </math> (16)</p>
   <p>Then, consider two cases of what to do with the ration of 
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    </math> and solve the above as a cubic equation.</p>
   <p>1) What if 
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    </math> vanishingly small contribution. (low acceleration)</p>
   <p>
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    </math> (17)</p>
   <p>Then, using the idea of a “repressed cubic” we will have the following solution for 
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    </math>, namely <xref ref-type="bibr" rid="scirp.142237-9">
     [9]
    </xref></p>
   <p>
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    </math> (18)</p>
   <p>2) Solutions for Equation (17), in reduced Cubic form for Equation (17)</p>
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    </math> (19)</p>
   <p>
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    </math> (20)</p>
   <p>Then using <xref ref-type="bibr" rid="scirp.142237-9">
     [9]
    </xref></p>
   <p>
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    </math> (21)</p>
   <p>
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          roots 
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        <mtext>
            
        </mtext> 
        <mtext>
          unequal 
        </mtext> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (22)</p>
   <p>The situation to watch is when the time, t, is extremely small. Then one has to work with the situation where 
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    </math>, i.e. the situation is then dominated with one real root and two imaginary roots. The value of what happens to 
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    </math> is one which will be commented upon if there is one real root, and two imaginary. What would be a possible constraint upon would be if we had, for non-dimensionalized units</p>
   <p>
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           2 
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     </mtable> 
    </math> (23)</p>
   <p>i.e. for the case that one uses non-dimensionalized units we would have, then</p>
   <p>
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      <mi>
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    </math> (24)</p>
   <p>i.e. this means that if we have small t i.e. almost at the start of inflation, a HUGE vacuum energy. And this is what we want to avoid, i.e. How likely is this to happen, in the Pre Planckian regime? Not likely. In fact, the construction of Equation (24) almost completely voids out how to obtain a vacuum energy which is going to be avoided first by working with the following expression for scalar fields <xref ref-type="bibr" rid="scirp.142237-10">
     [10]
    </xref></p>
   <p>
    <xref ref-type="bibr" rid="scirp.142237-"></xref> 
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          ⋅ 
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         <mi>
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         </mi> 
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           4 
         </mn> 
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          ⋅ 
        </mo> 
        <mfrac> 
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              1.66 
            </mn> 
           </mrow> 
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          </mo> 
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           <mi>
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           </mi> 
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           </mo> 
          </msub> 
         </mrow> 
         <mrow> 
          <msubsup> 
           <mi>
             m 
           </mi> 
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           </mi> 
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             2 
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         </mrow> 
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        </mo> 
        <msup> 
         <mn>
           10 
         </mn> 
         <mrow> 
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            − 
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          <mn>
            5 
          </mn> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (25)</p>
   <p>We will from here obtain a range of energy flux expressions which avoid the mess created by Equation (23).</p>
  </sec><sec id="s4">
   <title>4. How to Come up with an Alternate Initial Energy Expression Which May Avoid the Situation in Equation (23)?</title>
   <p>First of all, rather than use the scalar field as given in Equation (8) and Equation (9) we use a different approach, as given by (19) and we also look at a different application of the shape function argument for incremental time. As pioneered by Barbour <xref ref-type="bibr" rid="scirp.142237-4">
     [4]
    </xref></p>
   <p>
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    </math> (26)</p>
   <p>In our case, our simplication is to rewrite this by using Equation (19)</p>
   <p>
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            → 
          </mo> 
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           </mi> 
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           </mi> 
          </msub> 
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            → 
          </mo> 
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            1 
          </mn> 
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        <msqrt> 
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              8 
            </mn> 
            <mi>
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            </mi> 
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    </math> (27)</p>
   <p>Then in doing so, we will be obtained by the initial uncertainty principle as of Equation (4)</p>
   <p>
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                </mn> 
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                </mi> 
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                  G 
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                 </mi> 
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                 </mn> 
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                </mi> 
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                  ⋅ 
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                   [ 
                 </mo> 
                 <mrow> 
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                    3 
                  </mn> 
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                    α 
                  </mi> 
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                  </mo> 
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                   ] 
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           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (28)</p>
   <p>Here, i.e. if the mass of a graviton is not zero, and if we have an initial potential 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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    </math> as well as time not set equal to zero as well as an initial scale factor not equal to zero, we will be able to obtain values which are not incommensurate as to formation of primordial black holes. And also Equation (27) can be compared against</p>
   <p>We assume 
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   <p>
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            s 
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            initial 
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           ) 
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          ⋅ 
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            initial 
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    </math> (29)</p>
   <p>This would put a requirement upon a very large initial temperature 
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    </math> and so then, if 
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        ⋅ 
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           ) 
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    </math> <xref ref-type="bibr" rid="scirp.142237-11">
     [11]
    </xref></p>
   <p>
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         ) 
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        ≈ 
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           ) 
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    </math> (30)</p>
   <p>Having said that how do we obtain a quantum number, n, as to Black holes, and the phenomenon of Torsion? To come up with a finite value of the cosmological constant?</p>
  </sec><sec id="s5">
   <title>5. Where Torsion May Allow for Understanding a Quantum Number n?</title>
   <p>Following <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [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> 
         <mi>
           Λ 
         </mi> 
        </msqrt> 
        <mo>
          = 
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           </mi> 
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          </mi> 
          <mi>
            c 
          </mi> 
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            </mtext> 
           </mrow> 
          </msub> 
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        </mfrac> 
       </mtd> 
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       <mtd> 
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          = 
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           N 
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            particles 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (31)</p>
   <p>And then a BEC condensate given by <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-3">
     [3]
    </xref> as to</p>
   <p>
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             N 
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            </mtext> 
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        <mo>
          ⋅ 
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          ⋅ 
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        <msub> 
         <mi>
           N 
         </mi> 
         <mrow> 
          <mtext>
            gravitons 
          </mtext> 
         </mrow> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            B 
          </mi> 
          <mi>
            H 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          ≈ 
        </mo> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             T 
           </mi> 
           <mi>
             P 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
               N 
             </mi> 
             <mrow> 
              <mtext>
                gravitons 
              </mtext> 
             </mrow> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
        </mfrac> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (32)</p>
   <p>This is promising but needs to utilize <xref ref-type="bibr" rid="scirp.142237-12">
     [12]
    </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> 
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        </mi> 
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    </math> (33)</p>
   <p>By use of the HUP <xref ref-type="bibr" rid="scirp.142237-13">
     [13]
    </xref> we use Equation (34) for energy <xref ref-type="bibr" rid="scirp.142237-12">
     [12]
    </xref> for radiation of a particle pair from a black hole, via use of <xref ref-type="bibr" rid="scirp.142237-12">
     [12]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         | 
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       <mi>
         E 
       </mi> 
       <mo>
         | 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
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        <mrow> 
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           ( 
         </mo> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <mi>
              G 
            </mi> 
            <mi>
              M 
            </mi> 
            <mi>
              δ 
            </mi> 
            <mi>
              r 
            </mi> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (34)</p>
   <p>Here we assert that the spatial variation goes as</p>
   <p>
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        δ 
      </mi> 
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        ≈ 
      </mo> 
      <msub> 
       <mi>
         ℓ 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
     </mrow> 
    </math> (35)</p>
   <p>This is of a Plank length, whereas we assume in Equation (33) that the mass is a Planck sized black hole</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        M 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mi>
        α 
      </mi> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
     </mrow> 
    </math> (36)</p>
   <p>If so, we transform Equation (34) to be of the form for a “particle” pair as given in Carlip <xref ref-type="bibr" rid="scirp.142237-12">
     [12]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         | 
       </mo> 
       <mi>
         E 
       </mi> 
       <mo>
         | 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <mi>
              G 
            </mi> 
            <mo>
              ⋅ 
            </mo> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mi>
                α 
              </mi> 
              <msub> 
               <mi>
                 M 
               </mi> 
               <mi>
                 P 
               </mi> 
              </msub> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
            <mo>
              ⋅ 
            </mo> 
            <msub> 
             <mi>
               ℓ 
             </mi> 
             <mi>
               P 
             </mi> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mi>
        ℏ 
      </mi> 
     </mrow> 
    </math> (37)</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 (37) as the mass of a relic black hole. Now using the following normalization of Planck units, i.e. <xref ref-type="bibr" rid="scirp.142237-13">
     [13]
    </xref> as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         B 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         ℓ 
       </mi> 
       <mi>
         P 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (38)</p>
   <p>And, also, the initial energy, E <xref ref-type="bibr" rid="scirp.142237-14">
     [14]
    </xref> <xref ref-type="bibr" rid="scirp.142237-15">
     [15]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         E 
       </mi> 
       <mrow> 
        <mi>
          B 
        </mi> 
        <mi>
          h 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           n 
         </mi> 
         <mrow> 
          <mtext>
            quantum 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </mfrac> 
     </mrow> 
    </math> (39)</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> (40)</p>
   <p>We then reference Equation (32) 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> (41)</p>
   <p>This is a stunning result, i.e. Equation (32) 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 <xref ref-type="table" rid="table1">
     Table 1
    </xref>.</p>
   <p>
    <xref ref-type="table" rid="table1">
     Table 1
    </xref> from <xref ref-type="bibr" rid="scirp.142237-2">
     [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.142237-"></xref>Table 1. Penrose recycling of the Universe.</title>
    </caption>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="custom-top-td aleft" width="33.34%"><p style="text-align:left">End of Prior Universe time frame</p></td> 
      <td class="custom-top-td aleft" width="33.33%"><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="custom-top-td 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="33.34%"><p style="text-align:left">Planck era Black hole formation</p><p style="text-align:left">Assuming start of merging of micro black hole pairs</p></td> 
      <td class="aleft" width="33.33%"><p style="text-align:left">Mass (black hole)</p><p style="text-align:left">10<sup>−</sup><sup>5</sup> to 10<sup>−</sup><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="33.34%"><p style="text-align:left">Post Planck era black holes with the possibility of using Equation (1) and Equation (2) to have say 10<sup>10</sup> gravitons/second released per black hole</p></td> 
      <td class="aleft" width="33.33%"><p style="text-align:left">Mass (black hole)</p><p style="text-align:left">10 grams to say 10^6 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.142237-1">
     [1]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-4">
     [4]
    </xref>. To begin this look at <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref>, which is akin, as we discuss later to <xref ref-type="bibr" rid="scirp.142237-16">
     [16]
    </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> (42)</p>
   <p>In <xref ref-type="bibr" rid="scirp.142237-2">
     [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.142237-2">
     [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> (43)</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.142237-7">
     [7]
    </xref>.</p>
   <p>We argue that our application of <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> will be commensurate with Equation (42) which uses the value given in <xref ref-type="bibr" rid="scirp.142237-2">
     [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 (42) by <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> is restricted to a different venue which is reproduced below, namely cancellation of the following by Torsion <xref ref-type="bibr" rid="scirp.142237-16">
     [16]
    </xref></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> (44)</p>
   <p>Furthermore, the claim in <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> is that there is no cosmological constant, i.e. that Torsion always cancelling Equation (44) which we view is incommensurate with <xref ref-type="table" rid="table1">
     Table 1
    </xref> as of <xref ref-type="bibr" rid="scirp.142237-2">
     [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 (44) above.</p>
  </sec><sec id="s6">
   <title>6. 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.142237-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </xref>, we have the following, i.e., we have a spin density term of <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </xref>. And this will be what we input black hole physics into to form a spin density term from primordial black holes.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         σ 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          71 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (45)</p>
  </sec><sec id="s7">
   <title>7. Now for the Statement of the Torsion Problem as Given in <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> <xref ref-type="bibr" rid="scirp.142237-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </xref></title>
   <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.142237-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </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> (46)</p>
  </sec><sec id="s8">
   <title>8. What <xref ref-type="bibr" rid="scirp.142237-9">
     [9]
    </xref> Does as to Equation (46) versus What We Would Do and Why</title>
   <p>In the case of <xref ref-type="bibr" rid="scirp.142237-1">
     [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 (46) 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> (47)</p>
   <p>The claim is made in <xref ref-type="bibr" rid="scirp.142237-2">
     [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.142237-9">
     [9]
    </xref> <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </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> (48)</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 (47) and Equation (48) 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="s9">
   <title>9. Filling in the Details of the Equation (47) Collapse of the Cosmological Term, versus the Situation Given in Equation (48) via Numerical Values</title>
   <p>First look at numbers provided by <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </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> (49)</p>
   <p>This is the number for the vacuum energy and this enormous value is 10^122 times larger than the observed cosmological constant. Torsion physics, as given by <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </xref> is solely to remove this giant number.</p>
   <p>In order to remove it, the reference <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </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> (50)</p>
   <p>What we are arguing is that instead, one is seeing, instead <xref ref-type="bibr" rid="scirp.142237-17">
     [17]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
      <mo>
        + 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           Λ 
         </mi> 
         <mrow> 
          <mi>
            P 
          </mi> 
          <mi>
            l 
          </mi> 
         </mrow> 
        </msub> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </mfrac> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          122 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        × 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             Λ 
           </mi> 
           <mrow> 
            <mi>
              P 
            </mi> 
            <mi>
              l 
            </mi> 
           </mrow> 
          </msub> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (51)</p>
   <p>Our timing as to Equation (50) is to unleash a Planck time interval t about 10^−43 seconds.</p>
   <p>As to Equation (50) versus Equation (51), 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> (52)</p>
   <p>Finally, we have a spin density term of 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         σ 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         n 
       </mi> 
       <mrow> 
        <mi>
          P 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msub> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          71 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> which is due to innumerable black holes initially.</p>
  </sec><sec id="s10">
   <title>10. Future Works to Be Commenced as to Derivational Tasks</title>
   <p>We will assume for the moment that Equation (50) and Equation (51) share in common Equation (52).</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 (50) by Equation (52) is defined to be an ad hoc creation, as to <xref ref-type="bibr" rid="scirp.142237-3">
     [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 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> arising as a result of the dynamics of <xref ref-type="table" rid="table1">
     Table 1
    </xref>, as given in the manuscript.</p>
   <p>2<sup>nd</sup></p>
   <p>We state that the term 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            8 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         [ 
       </mo> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mi>
            π 
          </mi> 
          <mi>
            G 
          </mi> 
          <msup> 
           <mi>
             σ 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <mn>
            3 
          </mn> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             4 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ] 
       </mo> 
      </mrow> 
     </mrow> 
    </math> is due to initial micro black holes, as to the creation of a Cosmological term.</p>
  </sec><sec id="s11">
   <title>11. Conclusion, Looking Directly at a Modification of the Black Holes Which Have No Hair Theorem, via the Inputs of This Document</title>
   <p>In <xref ref-type="bibr" rid="scirp.142237-18">
     [18]
    </xref>, we have the essential black holes that 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.142237-19">
     [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.142237-20">
     [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.142237-20">
     [20]
    </xref>.</p>
   <p>I.e. using our equation 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>
    <xref ref-type="bibr" rid="scirp.142237-"></xref> 
    <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> (53)</p>
   <p>Due to using <xref ref-type="bibr" rid="scirp.142237-3">
     [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> (54)</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>
    <xref ref-type="bibr" rid="scirp.142237-"></xref> 
    <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> (55)</p>
   <p>Then use the last equation of Equation (32) to obtain, a quantum number associated with a graviton just outside a BEC primordial black hole</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142237-"></xref> 
    <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> (56)</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.142237-20">
     [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> (57)</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.142237-20">
     [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> (58)</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142237-"></xref>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 (32) with <xref ref-type="bibr" rid="scirp.142237-20">
     [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.142237-19">
     [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 (39) the following</p>
   <p>
    <xref ref-type="bibr" rid="scirp.142237-"></xref> 
    <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> (59)</p>
   <p>The left hand side of Equation (59) would be fully commensurate with Equation (39) of Corda’s black hole quantum number <xref ref-type="bibr" rid="scirp.142237-16">
     [16]
    </xref>.</p>
   <p>The right hand side of Equation (59) 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.142237-17">
     [17]
    </xref>.</p>
  </sec><sec id="s12">
   <title>12. 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> from Appendix 2, of <xref ref-type="bibr" rid="scirp.142237-18">
     [18]
    </xref> assuming Penrose recycling of the Universe as stated in that document.</p>
   <p>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>, Appendix 2. This increase in complexity can be with work tied into the following for black hole physics <xref ref-type="bibr" rid="scirp.142237-3">
     [3]
    </xref> from Equation (1). References from <xref ref-type="bibr" rid="scirp.142237-18">
     [18]
    </xref>-<xref ref-type="bibr" rid="scirp.142237-21">
     [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.</p>
  </sec><sec id="s13">
   <title>13. 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="table" rid="table1">
     Table 1
    </xref> in the Planckian era. To do this at the start, we will pay attention to a datum in reference <xref ref-type="bibr" rid="scirp.142237-3">
     [3]
    </xref>, namely a Horizon, like a Schwarzschild black hole construction with <xref ref-type="bibr" rid="scirp.142237-22">
     [22]
    </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> (60)</p>
   <p>In what <xref ref-type="bibr" rid="scirp.142237-22">
     [22]
    </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> (61)</p>
   <p>And the mass of a black hole, scaling as <xref ref-type="bibr" rid="scirp.142237-22">
     [22]
    </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> (62)</p>
   <p>This in <xref ref-type="bibr" rid="scirp.142237-3">
     [3]
    </xref> has the exact same functional forms as is given in Equation (41) 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.142237-22">
     [22]
    </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> (63)</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> (64)</p>
   <p>Now as to what is given in <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> as to Torsion, we have that as given in <xref ref-type="bibr" rid="scirp.142237-18">
     [18]
    </xref> that we can do some relevant dimensional scaling.</p>
   <p>First look at numbers provided by <xref ref-type="bibr" rid="scirp.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> as to inputs, i.e. these are very revealing, i.e. we go back to the arguments 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.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [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.142237-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.142237-2">
     [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 said 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 to say 10<sup>50</sup> black holes of say of Planck mass, to work with an initial volume for the production of black holes set as</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mtext>
          volume 
        </mtext> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            initial 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </msub> 
      <mo>
        ~ 
      </mo> 
      <msup> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mn>
           4 
         </mn> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mi>
        δ 
      </mi> 
      <mi>
        t 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <mi>
        Δ 
      </mi> 
      <msub> 
       <mi>
         A 
       </mi> 
       <mrow> 
        <mtext>
          surface area 
        </mtext> 
       </mrow> 
      </msub> 
      <mo>
        ⋅ 
      </mo> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          ≤ 
        </mo> 
        <msub> 
         <mi>
           l 
         </mi> 
         <mrow> 
          <mtext>
            Planck 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (65)</p>
   <p>Then as to the follow up to NLED and signals from primordial processes <xref ref-type="bibr" rid="scirp.142237-21">
     [21]
    </xref></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mtable columnalign="left"> 
      <mtr> 
       <mtd> 
        <msub> 
         <mi>
           α 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          = 
        </mo> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
            <mi>
              G 
            </mi> 
           </mrow> 
           <mrow> 
            <mn>
              3 
            </mn> 
            <msub> 
             <mi>
               μ 
             </mi> 
             <mn>
               0 
             </mn> 
            </msub> 
            <mi>
              c 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msqrt> 
        <msub> 
         <mi>
           B 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mover accent="true"> 
         <mi>
           λ 
         </mi> 
         <mo>
           ⌢ 
         </mo> 
        </mover> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            defined 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <mrow> 
         <mrow> 
          <mi>
            Λ 
          </mi> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mo>
           / 
         </mo> 
         <mn>
           3 
         </mn> 
        </mrow> 
        <mo> 
        </mo> 
        <mo> 
        </mo> 
       </mtd> 
      </mtr> 
      <mtr> 
       <mtd> 
        <mo> 
        </mo> 
        <msub> 
         <mi>
           a 
         </mi> 
         <mrow> 
          <mi>
            min 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          = 
        </mo> 
        <msub> 
         <mi>
           a 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msub> 
              <mi>
                α 
              </mi> 
              <mn>
                0 
              </mn> 
             </msub> 
            </mrow> 
            <mrow> 
             <mn>
               2 
             </mn> 
             <mover accent="true"> 
              <mi>
                λ 
              </mi> 
              <mo>
                ⌢ 
              </mo> 
             </mover> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mtext>
                 defined 
               </mtext> 
              </mrow> 
              <mo>
                ) 
              </mo> 
             </mrow> 
            </mrow> 
           </mfrac> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <msqrt> 
              <mrow> 
               <msubsup> 
                <mi>
                  α 
                </mi> 
                <mn>
                  0 
                </mn> 
                <mn>
                  2 
                </mn> 
               </msubsup> 
               <mo>
                 + 
               </mo> 
               <mn>
                 32 
               </mn> 
               <mover accent="true"> 
                <mi>
                  λ 
                </mi> 
                <mo>
                  ⌢ 
                </mo> 
               </mover> 
               <mrow> 
                <mo>
                  ( 
                </mo> 
                <mrow> 
                 <mtext>
                   defined 
                 </mtext> 
                </mrow> 
                <mo>
                  ) 
                </mo> 
               </mrow> 
               <mo>
                 ⋅ 
               </mo> 
               <msub> 
                <mi>
                  μ 
                </mi> 
                <mn>
                  0 
                </mn> 
               </msub> 
               <mi>
                 ω 
               </mi> 
               <mo>
                 ⋅ 
               </mo> 
               <msubsup> 
                <mi>
                  B 
                </mi> 
                <mn>
                  0 
                </mn> 
                <mn>
                  2 
                </mn> 
               </msubsup> 
              </mrow> 
             </msqrt> 
             <mo>
               − 
             </mo> 
             <msub> 
              <mi>
                α 
              </mi> 
              <mn>
                0 
              </mn> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             4 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mtd> 
      </mtr> 
     </mtable> 
    </math> (66)</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.142237-21">
     [21]
    </xref></p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        B 
      </mi> 
      <mo>
        &gt; 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mrow> 
          <mn>
            10 
          </mn> 
          <msub> 
           <mi>
             μ 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            ⋅ 
          </mo> 
          <mi>
            ω 
          </mi> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (67)</p>
   <p>We submit the following for future investigation, namely the n particle count 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 (67) would be tied into Equation (14) via the n of that equation as well as specified by <xref ref-type="bibr" rid="scirp.142237-22">
     [22]
    </xref> on its page 111, where we have</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ω 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </msub> 
      <mi>
        c 
      </mi> 
      <mi>
        k 
      </mi> 
     </mrow> 
    </math> (68)</p>
   <p>Here 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         g 
       </mi> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mi>
          r 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is nearly zero, 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 to obtain ideas as to data sets which would satisfy multi-messenger astronomy namely the discussion as given in Mohanty, <xref ref-type="bibr" rid="scirp.142237-23">
     [23]
    </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> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msup> 
         <mi>
           g 
         </mi> 
         <mo>
           ∗ 
         </mo> 
        </msup> 
        <mi>
          a 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (69)</p>
   <p>With temperature T, as proportional to quantum number n as specified.</p>
   <p>Here, we also have to consider the issues about primordial black holes as raised in <xref ref-type="bibr" rid="scirp.142237-24">
     [24]
    </xref> which are still unanswered as well as <xref ref-type="bibr" rid="scirp.142237-25">
     [25]
    </xref> as raised by Ruffini et al. as well as <xref ref-type="bibr" rid="scirp.142237-26">
     [26]
    </xref> and <xref ref-type="bibr" rid="scirp.142237-27">
     [27]
    </xref> as well as review the information on fifth forces given in <xref ref-type="bibr" rid="scirp.142237-2">
     [2]
    </xref> and other such constructions.</p>
  </sec>
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