<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article">
 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">
    jhepgc
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of High Energy Physics, Gravitation and Cosmology
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2380-4327
   </issn>
   <issn publication-format="print">
    2380-4335
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jhepgc.2024.104101
   </article-id>
   <article-id pub-id-type="publisher-id">
    jhepgc-136741
   </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>
    Solving the Conundrum of Dark Matter and Dark Energy in Galaxy Clusters
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Manuel
      </surname>
      <given-names>
       Abarca
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aIndependent Researcher, Granada, Spain
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     28
    </day> 
    <month>
     08
    </month>
    <year>
     2024
    </year>
   </pub-date> 
   <volume>
    10
   </volume> 
   <issue>
    04
   </issue>
   <fpage>
    1785
   </fpage>
   <lpage>
    1805
   </lpage>
   <history>
    <date date-type="received">
     <day>
      21,
     </day>
     <month>
      May
     </month>
     <year>
      2024
     </year>
    </date>
    <date date-type="published">
     <day>
      20,
     </day>
     <month>
      May
     </month>
     <year>
      2024
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      20,
     </day>
     <month>
      October
     </month>
     <year>
      2024
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © Copyright 2014 by authors and Scientific Research Publishing Inc. 
    </copyright-statement>
    <copyright-year>
     2014
    </copyright-year>
    <license>
     <license-p>
      This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/
     </license-p>
    </license>
   </permissions>
   <abstract>
    This paper develops the Dark Matter by Quantum Gravitation theory, DMbQG theory hereafter, in clusters of galaxies in the cosmologic model ΛCDM of the Universe. Originally this theory was developed by the author for galaxies, especially using MW and M31 rotation curves. An important result got by the DMbQG theory is that the total mass associated to a galactic halo depend on the square root of radius, being its dominion unbounded. Apparently, this result would be absurd because of divergence of the total mass. As the DE is negligible at galactic scale, it is needed to extend the theory to clusters in order to study the capacity of DE to counterbalance to DM. Thanks this property, the DMbQG theory finds unexpected theoretical results. In this work, it is defined, the total mass as baryonic matter plus DM and the gravitating mass as the addition of the total mass plus the negative mass associated to dark energy. In clusters it is defined the zero gravity radius (R
    <sub>ZG</sub> hereafter) as the radius needed by the dark energy to counterbalance the total mass. It has been found that the ratio R
    <sub>ZG</sub>/R
    <sub>VIRIAL</sub> ≈ 7.3 and its Total mass associated at R
    <sub>ZG</sub> is ≈2.7 M
    <sub>VIRIAL</sub>. In addition, it has been calculated that the sphere with the extended halo radius R
    <sub>E</sub> = 1.85 R
    <sub>ZG</sub> has a ratio DM density versus DE density equal to 3/7 and its total mass associated at R
    <sub>E</sub> is ≈3.6 M
    <sub>VIRIAL</sub>. This works postulates that the factor 3.6 may equilibrate perfectly the strong imbalance between the Local mater density parameter (0.08) versus the current Global matter density one (0.3). Currently, this fact is a big conundrum in cosmology, see chapter 7. Also it has been found that the zero velocity radius, R
    <sub>ZV</sub> hereafter, i.e. the cluster border because of the Hubble flow, is ≈0.6 R
    <sub>ZG</sub> and its gravitating mass is ≈ 1.5 M
    <sub>VIR</sub>. By derivation of gravitating mass function, it is calculated that at 0.49 R
    <sub>ZG</sub>, this function reaches its maximum whose value is ≈1.57 M
    <sub>VIR</sub>. Throughout the paper, some of these results have been validated with recent data published for the Virgo cluster. As Virgo is the nearest big cluster, it is the perfect benchmark to validate any new theory about DM and DE. These new theoretical findings offer to scientific community a wide number of tests to validate or reject the theory. The validation of DMbQG theory would mean to know the nature of DM that at the present, it is an important challenge for the astrophysics science.
   </abstract>
   <kwd-group> 
    <kwd>
     Dark Matter
    </kwd> 
    <kwd>
      Dark Energy
    </kwd> 
    <kwd>
      Galaxy Clusters
    </kwd> 
    <kwd>
      Quantum Gravitation
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <p>The bases of this paper are developed in <xref ref-type="bibr" rid="scirp.136741-1">
     [1]
    </xref> Abarca, M. 2023, so it is highly recommended to read it to understand the meaning of this paper. The dark matter by quantum gravitation theory, DMbQG theory hereafter, is an original theory developed since 2013 through more than 20 papers, although in <xref ref-type="bibr" rid="scirp.136741-1">
     [1]
    </xref> Abarca, M. 2023 is published the best version as physical as mathematically. The theory has been stated studying the galactic rotation curves, specially the ones associated to MW and M31, see <xref ref-type="bibr" rid="scirp.136741-2">
     [2]
    </xref> Sofue, Y. 2015 and <xref ref-type="bibr" rid="scirp.136741-3">
     [3]
    </xref> Sofue, Y. 2020. Therefore, it is not possible to understand this paper if readers have not at least a general knowledge about the DMbQG theory.</p>
   <p>The hypothesis of DMbQG theory is that the DM is generated by the own gravitational field. In order to study purely the DM phenomenon, it is needed to consider a radius dominion where it is supposed that baryonic matter is negligible. For example, for MW galaxy the radius must be bigger than 30 kpc and bigger than 40 kpc for M31 galaxy. For galactic clusters, the radius must be bigger than its virial radius.</p>
   <p>This hypothesis has two main consequences: the first one is that the law of dark matter generation, in the halo region, has to be the same for all the galaxies and clusters; the second one is that the DM haloes are unlimited so the total dark matter goes up without limit.</p>
   <p>The DMbQG theory has been developed assuming the hypothesis that DM is a quantum gravitational effect. See <xref ref-type="bibr" rid="scirp.136741-4">
     [4]
    </xref> Corda, C. 2012. However, it is possible to remain into the Newtonian framework to develop the theory. In my opinion, there are two factors to manage the DM phenomenon with a quite simple theory.</p>
   <p>The first one, that it is developed into the halo region, where baryonic matter is negligible. The second one, that the mechanics movements of celestial bodies are very slow regarding velocity of light, which is supposed to be the speed of gravitational bosons. It is known that community of physics is researching a quantum gravitation theory since many years ago, but does not exist yet; however, my works in this area support strongly that DM is a quantum gravitation phenomenon.</p>
   <p>Use a more simple theory instead the general theory is a typical procedure in physics.</p>
   <p>For example, the Kirchhoff’s laws are the consequence of Maxwell theory for direct current and remain valid for alternating current, introducing complex impe-dances, on condition that signals must have low frequency.</p>
   <p>In <xref ref-type="bibr" rid="scirp.136741-1">
     [1]
    </xref> Abarca, M. 2023, in the framework of DMbQG, is demonstrated mathematically that the total mass (baryonic plus DM) enclosed by a sphere with a specific radius is given by the Direct mass into the galactic halo and that the total mass goes up proportionally to the root square of radius, formula (4.1).</p>
   <p>It is well known that DE may be modelled as a constant density of negative mass in the whole space, see <xref ref-type="bibr" rid="scirp.136741-5">
     [5]
    </xref> Chernin, A.D. et al. 2013, therefore the total amount of DE grows up with the cubic power of the sphere radius, so it is clear that DE is able to counterbalance the total mass of the clusters, which grows up more slowly. Precisely, the main goal of this paper is to study the relation between both phenomenons in clusters. Namely in cluster haloes.</p>
   <p>This paper explores the mutual counterbalance between DM and DE in the framework of DMbQG theory and the result got have been fructiferous, with a dozen of new formulas never published before.</p>
   <p>The following paragraphs will be introduced the paper structure:</p>
   <p>The newness of the important results got in this paper are due to the possibility to approximate the virial radius to R<sub>200</sub> and the virial mass to M<sub>200</sub>, the chapter 3 is dedicated to validate this approximation using recent data published for some important clusters such as Virgo or some others.</p>
   <p>The chapter 4 is dedicated to extend the direct mass formula to clusters. The direct mass formula (4.1) has only one parameter “a<sup>2</sup>” whose units are m<sup>5/2</sup>/s<sup>2</sup>. Using the approximation R<sub>200</sub> as virial radius and M<sub>200</sub> as virial mass into the direct mass formula it is got the formula 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            G 
          </mi> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mrow> 
            <mi>
              V 
            </mi> 
            <mi>
              I 
            </mi> 
            <mi>
              R 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          5 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          6 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            10 
          </mn> 
          <mo>
            ⋅ 
          </mo> 
          <mi>
            H 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> which is on the basis for some important results got in the following chapters.</p>
   <p>The chapter 5 contains three main concepts:</p>
   <p>Firstly, it is defined the zero gravity radius, R<sub>ZG</sub>, as the sphere radius where the total mass is counterbalanced by the DE. It is found that the ratio R<sub>ZG</sub>/R<sub>VIRIAL</sub> ≈ 7.3 is universal.</p>
   <p>Secondly, it is defined the gravitating mass as the addition of total mass plus the dark energy and the gravitating mass function using a dimensionless parameter f = Radius/R<sub>ZG</sub>. It is found that for any cluster at ≈0.5 R<sub>ZG</sub> is reached the maximum of gravitating mass and its value is M<sub>G</sub> (&lt;R<sub>M</sub>) ≈ 1.57 M<sub>VIR</sub>.</p>
   <p>Finally, it is defined the concept of extended halo (R<sub>E</sub>) as the spherical region where the ratio 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <mi>
          D 
        </mi> 
        <mi>
          e 
        </mi> 
        <mi>
          n 
        </mi> 
        <mi>
          s 
        </mi> 
        <mi>
          i 
        </mi> 
        <mi>
          t 
        </mi> 
        <msubsup> 
         <mi>
           y 
         </mi> 
         <mrow> 
          <mi>
            T 
          </mi> 
          <mi>
            M 
          </mi> 
         </mrow> 
         <mrow> 
          <mi>
            S 
          </mi> 
          <mi>
            P 
          </mi> 
          <mi>
            H 
          </mi> 
          <mi>
            E 
          </mi> 
          <mi>
            R 
          </mi> 
          <mi>
            E 
          </mi> 
         </mrow> 
        </msubsup> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mo>
            &lt; 
          </mo> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             E 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           ρ 
         </mi> 
         <mrow> 
          <mi>
            D 
          </mi> 
          <mi>
            E 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mn>
         3 
       </mn> 
       <mo>
         / 
       </mo> 
       <mn>
         7 
       </mn> 
      </mrow> 
     </mrow> 
    </math> i.e. the local ratio of such densities is equal to the current global ratio one, and it is found that R<sub>E</sub> ≈1.85 R<sub>ZG</sub>.</p>
   <p>In the sixth chapter it is defined the zero velocity radius, R<sub>ZV</sub>, as the sphere radius where the escape velocity is zero because of the Hubble flow. It is demonstrated that the ratio R<sub>ZV</sub>/R<sub>ZG</sub> ≈ 0.602 is universal.</p>
   <p>In the seventh chapter, it is validated the gravitating mass formula into the Virgo cluster for a couple of radius. Namely at 7.3 Mpc and at 3.4 Mpc. The calculus made with the formula of gravitating mass is compared successfully with recent results published in 2020. Also it is validated the theoretical result of R<sub>ZV</sub>/R<sub>ZG</sub> ≈ 0.602 with result of measures published.</p>
   <p>Two of the most important results got in this work are the formula 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          T 
        </mi> 
        <mi>
          O 
        </mi> 
        <mi>
          T 
        </mi> 
        <mi>
          A 
        </mi> 
        <mi>
          L 
        </mi> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mo>
          &lt; 
        </mo> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mrow> 
          <mi>
            Z 
          </mi> 
          <mi>
            G 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mtext>
          
      </mtext> 
      <mi>
        U 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          V 
        </mi> 
        <mi>
          I 
        </mi> 
        <mi>
          R 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> being U≈ 2.7 and the formula 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mtext>
          TOTAL 
        </mtext> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mo>
          &lt; 
        </mo> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           E 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        3.67 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          V 
        </mi> 
        <mi>
          I 
        </mi> 
        <mi>
          R 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> associated to zero gravity radius and the extended radius respectively.</p>
   <p>Thanks these formulas this work suggest the possibility to solve the current discrepancy between the local parameter of matter density, 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         Ω 
       </mi> 
       <mi>
         m 
       </mi> 
       <mrow> 
        <mtext>
          local 
        </mtext> 
       </mrow> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mn>
        0.08 
      </mn> 
     </mrow> 
    </math>, see <xref ref-type="bibr" rid="scirp.136741-6">
     [6]
    </xref> Karachentsev et al. 2014, and the current global one 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         Ω 
       </mi> 
       <mi>
         m 
       </mi> 
       <mrow> 
        <mtext>
          global 
        </mtext> 
       </mrow> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mn>
        0.3 
      </mn> 
     </mrow> 
    </math>. This discrepancy is an open problem for the current cosmology.</p>
   <p>Finally the chapter 8 is devoted to the concluding remarks.</p>
   <p>The reader can consult the paper <xref ref-type="bibr" rid="scirp.136741-7">
     [7]
    </xref> Abarca, M, 2024, which is an extension of this paper, 24 pages, where the theory is validated through the Local Group and the Coma cluster data published as well.</p>
  </sec><sec id="s2">
   <title>
    <xref ref-type="bibr" rid="scirp.136741-"></xref>2. Virial Mass and Virial Radius in Cluster of Galaxies</title>
   <p>In cluster, it is a good estimation about virial radius and virial mass to consider R<sub>vir</sub> = R<sub>200</sub> and M<sub>vir</sub> = M<sub>200</sub>. Where R<sub>200</sub> is the radius of a sphere whose mean density is 200 times bigger than the critic density of Universe</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ρ 
       </mi> 
       <mi>
         C 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          3 
        </mn> 
        <msup> 
         <mi>
           H 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mn>
          8 
        </mn> 
        <mi>
          π 
        </mi> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (2.1)</p>
   <p>and M<sub>200</sub> is the total mass enclosed by the radius R<sub>200</sub>.</p>
   <p>Considering the spherical volume formula, it is right to get the following relation between both concepts</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         R 
       </mi> 
       <mrow> 
        <mi>
          V 
        </mi> 
        <mi>
          I 
        </mi> 
        <mi>
          R 
        </mi> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </msubsup> 
      <mo>
        ≈ 
      </mo> 
      <msubsup> 
       <mi>
         R 
       </mi> 
       <mrow> 
        <mn>
          200 
        </mn> 
       </mrow> 
       <mn>
         3 
       </mn> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mo>
          ⋅ 
        </mo> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mrow> 
          <mn>
            200 
          </mn> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          100 
        </mn> 
        <mo>
          ⋅ 
        </mo> 
        <msup> 
         <mi>
           H 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (2.2)</p>
   <p>or</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          V 
        </mi> 
        <mi>
          I 
        </mi> 
        <mi>
          R 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mn>
          200 
        </mn> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          100 
        </mn> 
        <msup> 
         <mi>
           H 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <msubsup> 
         <mi>
           R 
         </mi> 
         <mrow> 
          <mn>
            200 
          </mn> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </msubsup> 
       </mrow> 
       <mi>
         G 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> (2.3)</p>
   <sec id="s2_1">
    <title>Checking the Virial Mass Aproximation on a Sample of Clusters and Group of Galaxies</title>
    <p>See <xref ref-type="table" rid="table1">
      Table 1
     </xref>. The data of second and third column have been taken from <xref ref-type="bibr" rid="scirp.136741-8">
      [8]
     </xref> R. Ragusa et al. 2022 and using the formula 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo> 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mn>
           200 
         </mn> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           100 
         </mn> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mn>
             200 
           </mn> 
          </mrow> 
          <mn>
            3 
          </mn> 
         </msubsup> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
      </mrow> 
     </math> it is calculated its mass associated for each radius. In the last column shows the relative difference for masses, which is always under 10%.</p>
    <table-wrap id="table1">
     <label>
      <xref ref-type="table" rid="table1">
       Table 1
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 1. Data <xref ref-type="bibr" rid="scirp.136741-8">
        [8]
       </xref> R. Ragusa et al. 2022.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="34.78%"><p style="text-align:center">Group of galaxies G.</p><p style="text-align:center">or Clusters C.</p></td> 
       <td class="custom-bottom-td aleft" width="11.61%"><p style="text-align:left">Virial Radius</p></td> 
       <td class="custom-bottom-td aleft" width="17.96%"><p style="text-align:left">Virial Mass</p></td> 
       <td class="custom-bottom-td acenter" width="17.55%"><p style="text-align:center">Mass</p><p style="text-align:center">calculated</p></td> 
       <td class="custom-bottom-td acenter" width="18.11%"><p style="text-align:center">Relative diff for M</p></td> 
      </tr> 
      <tr> 
       <td class="custom-bottom-td custom-top-td acenter" width="34.78%"><p style="text-align:center">Name</p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="11.61%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="17.96%"><p style="text-align:center">×10<sup>13</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="17.55%"><p style="text-align:center">×10<sup>13</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="18.11%"><p style="text-align:center">%</p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="34.78%"><p style="text-align:center">Antlia C.</p></td> 
       <td class="custom-top-td acenter" width="11.61%"><p style="text-align:center">1.28</p></td> 
       <td class="custom-top-td acenter" width="17.96%"><p style="text-align:center">26.3</p></td> 
       <td class="custom-top-td acenter" width="17.55%"><p style="text-align:center">2.39E+01</p></td> 
       <td class="custom-top-td acenter" width="18.11%"><p style="text-align:center">−9.21E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC596/584 G.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">0.5</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">1.55</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">1.42E+00</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−8.18E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC 3268 G.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">0.9</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">8.99</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">8.30E+00</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−7.67E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC 4365Virgo SubG.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">0.32</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">0.4</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">3.73E-01</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−6.73E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC 4636 Virgo SubG.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">0.63</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">3.02</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">2.85E+00</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−5.73E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC 4697Virgo Sub G.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">1.29</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">26.9</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">2.44E+01</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−9.14E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC 5846 G.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">1.1</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">16.6</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">1.52E+01</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−8.71E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="34.78%"><p style="text-align:center">NGC 6868 G.</p></td> 
       <td class="acenter" width="11.61%"><p style="text-align:center">0.6</p></td> 
       <td class="acenter" width="17.96%"><p style="text-align:center">2.69</p></td> 
       <td class="acenter" width="17.55%"><p style="text-align:center">2.46E+00</p></td> 
       <td class="acenter" width="18.11%"><p style="text-align:center">−8.57E+00</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>As the Virgo cluster is the nearest between the big clusters it is crucial to check the approximation for virial mass and radius with its data.</p>
    <p>See in <xref ref-type="table" rid="table2">
      Table 2
     </xref> the data of Virgo cluster, according <xref ref-type="bibr" rid="scirp.136741-9">
      [9]
     </xref> Olga Kashibadze, I. Kara-chentsev. 2020.</p>
    <p>Using formula (2.3) with R<sub>200</sub> =1.7 Mpc it is got M<sub>200</sub> = 5.59 × 10<sup>14</sup> 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          Θ 
        </mi> 
       </msub> 
      </mrow> 
     </math> which matches with the mass published if it is considered the range of errors.</p>
    <table-wrap id="table2">
     <label>
      <xref ref-type="table" rid="table2">
       Table 2
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 2. Virgo cluster.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="16.09%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="20.97%"><p style="text-align:center">Virial Radius</p></td> 
       <td class="custom-bottom-td acenter" width="20.99%"><p style="text-align:center">Virial mass</p></td> 
       <td class="custom-bottom-td acenter" width="20.97%"><p style="text-align:center">Calculated M<sub>200</sub></p></td> 
       <td class="custom-bottom-td acenter" width="20.99%"><p style="text-align:center">Relative diff.</p><p style="text-align:center">of mass</p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="16.09%"><p style="text-align:center">Cluster</p></td> 
       <td class="custom-top-td acenter" width="20.97%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="20.99%"><p style="text-align:center">×10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-top-td acenter" width="20.97%"><p style="text-align:center">×10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-top-td acenter" width="20.99%"><p style="text-align:center">%</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="16.09%"><p style="text-align:center">Virgo</p></td> 
       <td class="acenter" width="20.97%"><p style="text-align:center">1.7</p></td> 
       <td class="acenter" width="20.99%"><p style="text-align:center">6.3 ± 0.9</p></td> 
       <td class="acenter" width="20.97%"><p style="text-align:center">5.59</p></td> 
       <td class="acenter" width="20.99%"><p style="text-align:center">11</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>In conclusion: R<sub>200</sub> and M<sub>200</sub> are a very good estimation for the virial radius and the virial mass for a group of galaxies and a cluster of galaxies, when they are in dynamical equilibrium.</p>
   </sec>
  </sec><sec id="s3">
   <title>
    <xref ref-type="bibr" rid="scirp.136741-"></xref>3. Virial Theorem as a Method to Get the Direct Mass Formula in Galaxy Clusters</title>
   <p>In chapter 9, of paper <xref ref-type="bibr" rid="scirp.136741-1">
     [1]
    </xref> Abarca, M. 2023 was demonstrated that the direct formula</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          T 
        </mi> 
        <mi>
          O 
        </mi> 
        <mi>
          T 
        </mi> 
        <mi>
          A 
        </mi> 
        <mi>
          L 
        </mi> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mo>
          &lt; 
        </mo> 
        <mi>
          r 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mi>
           r 
         </mi> 
        </msqrt> 
       </mrow> 
       <mi>
         G 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> (3.1)</p>
   <p>is the most suitable formula to calculate the total mass (baryonic and DM) depending on radius in the galactic halo.</p>
   <sec id="s3_1">
    <title>3.1. Parameter a<sup>2</sup> Formula Depending on Virial Radius and Virial Mass</title>
    <p>Due to the fact that the Direct mass formula has one parameter only, is enough to know the mass associated to a specific radius to be able to calculate parameter a<sup>2</sup>. That is the situation when it is known the virial mass and the virial radius for a cluster of galaxies.</p>
    <p>If it is considered that the virial radius is the border of halo cluster where galaxies are in dynamical equilibrium and at the same time is negligible the amount of Baryonic matter outside the sphere with such radius, then according DMbQG theory is possible to do an equation between M<sub>VIRIAL</sub> (&lt;R<sub>VIRIAL</sub>) = M<sub>DIRECT</sub> (&lt;R<sub>VIRIAL</sub>) (3.2.1) i.e.</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               A 
             </mi> 
             <mi>
               L 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
      </mrow> 
     </math> (3.2)</p>
    <p>and clearing up</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               A 
             </mi> 
             <mi>
               L 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (3.3)</p>
    <p>this formula is called parameter a<sup>2</sup> (M<sub>VIR</sub>, R<sub>VIR</sub>) because depend on both measures.</p>
   </sec>
   <sec id="s3_2">
    <title>3.2. Parameter a<sup>2</sup> Formula Depending on Virial Mass Only</title>
    <p>In chapter 2 was got this formula 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mn>
           100 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (2.2) as a good approximation between virial mass and virial radius. So using that formula and by substitution of virial radius in 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               A 
             </mi> 
             <mi>
               L 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (3.3) it is right to get parameter a<sup>2</sup> depending on M<sub>VIR</sub> only</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           6 
         </mn> 
        </mrow> 
       </msup> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mn>
             10 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <mi>
             H 
           </mi> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           3 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math> (3.4)</p>
    <p>This formula will be called parameter a<sup>2</sup> (M<sub>VIR</sub>) as depend on M<sub>VIR</sub> only.</p>
    <p>With the virial data for Virgo cluster, see <xref ref-type="table" rid="table2">
      Table 2
     </xref>, will be calculated its parameter a<sup>2</sup> with the formula (3.3) i.e. a<sup>2</sup> (M<sub>VIR</sub>, R<sub>VIR</sub>) and with the formula (3.4) i.e. a<sup>2</sup> (M<sub>VIR</sub>).</p>
    <p>The last formula is an approximation of the previous formula as it is supposed that R<sub>VIR</sub> ≈ R<sub>200</sub>. In <xref ref-type="table" rid="table3">
      Table 3
     </xref> are calculated both formulas and fortunately its relative difference is negligible.</p>
    <table-wrap id="table3">
     <label>
      <xref ref-type="table" rid="table3">
       Table 3
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 3. Calculated data.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="14.46%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="37.84%"><p style="text-align:center">Parameter a<sup>2</sup> (M<sub>VIR</sub>, R<sub>VIR</sub>)</p></td> 
       <td class="custom-bottom-td acenter" width="29.91%"><p style="text-align:center">Parameter a<sup>2</sup> (M<sub>VIR</sub>)</p></td> 
       <td class="custom-bottom-td acenter" width="25.64%"><p style="text-align:center">Relative diff.</p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="14.46%"><p style="text-align:center">Clusters</p></td> 
       <td class="custom-top-td acenter" width="37.84%"><p style="text-align:center">I.S. units m<sup>5/2</sup>/s<sup>2</sup></p></td> 
       <td class="custom-top-td acenter" width="29.91%"><p style="text-align:center">I.S. units m<sup>5/2</sup>/s<sup>2</sup></p></td> 
       <td class="custom-top-td acenter" width="25.64%"><p style="text-align:center">%</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="14.46%"><p style="text-align:center">Virgo</p></td> 
       <td class="acenter" width="37.84%"><p style="text-align:center">3.6527E23</p></td> 
       <td class="acenter" width="29.91%"><p style="text-align:center">3.581E23</p></td> 
       <td class="acenter" width="25.64%"><p style="text-align:center">2</p></td> 
      </tr> 
     </table>
    </table-wrap>
   </sec>
  </sec><sec id="s4">
   <title>4. Dark Matter Is Counter Balanced by Dark Energy at Zero Gravity Radius</title>
   <p>The basic concepts about DE on the current cosmology can be studied in <xref ref-type="bibr" rid="scirp.136741-5">
     [5]
    </xref> Chernin, A.D.</p>
   <p>As currently there is a tension regarding the experimental value of Hubble constant, in this paper will be used H = 70 Km/s/Mpc and 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Ω 
       </mi> 
       <mrow> 
        <mi>
          D 
        </mi> 
        <mi>
          E 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.7 
      </mn> 
     </mrow> 
    </math> as the fraction of Universal density of DE.</p>
   <sec id="s4_1">
    <title>4.1. Zero Gravity Radius Depending on Parameter a<sup>2</sup> Formula</title>
    <p>According <xref ref-type="bibr" rid="scirp.136741-5">
      [5]
     </xref> Chernin, A. D. in the current cosmologic model 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         Λ 
       </mi> 
       <mi>
         C 
       </mi> 
       <mi>
         D 
       </mi> 
       <mi>
         M 
       </mi> 
      </mrow> 
     </math>, dark energy has an effect equivalent to antigravity i.e. the mass associated to dark energy is negative and the dark energy have a constant density for all the Universe equal to 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          ρ 
        </mi> 
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           D 
         </mi> 
         <mi>
           E 
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        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          Ω 
        </mi> 
        <mrow> 
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           D 
         </mi> 
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           E 
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       </msub> 
       <mo>
         = 
       </mo> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <mn>
         6.444 
       </mn> 
       <mo>
         × 
       </mo> 
       <msup> 
        <mrow> 
         <mn>
           10 
         </mn> 
        </mrow> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mn>
           27 
         </mn> 
        </mrow> 
       </msup> 
       <msup> 
        <mrow> 
         <mtext>
           kg/m 
         </mtext> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msup> 
      </mrow> 
     </math> being 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          Ω 
        </mi> 
        <mrow> 
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           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0.7 
       </mn> 
      </mrow> 
     </math> and</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           3 
         </mn> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         9.205 
       </mn> 
       <mo>
         × 
       </mo> 
       <msup> 
        <mrow> 
         <mn>
           10 
         </mn> 
        </mrow> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mn>
           27 
         </mn> 
        </mrow> 
       </msup> 
       <msup> 
        <mrow> 
         <mtext>
           kg/m 
         </mtext> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msup> 
      </mrow> 
     </math> the critic density of the Universe.</p>
    <p>As DE density is constant, the total DE mass is proportional to Radius with power 3, whereas DM mass grows with radius power 0.5 so it is right to get a radius where DM is counter balanced by DE.</p>
    <p>According to <xref ref-type="bibr" rid="scirp.136741-5">
      [5]
     </xref> Chernin, A. D.</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
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           &lt; 
         </mo> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mtext>
           
       </mtext> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            ρ 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
         </msub> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <msup> 
          <mi>
            R 
          </mi> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </mfrac> 
      </mrow> 
     </math>, (4.1)</p>
    <p>Is the mass associated to DE or equivalently</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mfrac> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <msup> 
          <mi>
            R 
          </mi> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          R 
        </mi> 
        <mn>
          3 
        </mn> 
       </msup> 
      </mrow> 
     </math> (4.2)</p>
    <p>Notice that the author multiplies by two the volume of a sphere by reasons explained in his work.</p>
    <p>
     <xref ref-type="bibr" rid="scirp.136741-5">
      [5]
     </xref> Chernin defines gravitating mass</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
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          ( 
        </mo> 
        <mrow> 
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           &lt; 
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         <mi>
           R 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         + 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math> (4.3)</p>
    <p>where M<sub>TOTAL</sub> is baryonic plus dark matter mass, and defines R<sub>ZG</sub>, Radius at zero Gravity as the radius where 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
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         </mi> 
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           E 
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        </mrow> 
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       <mrow> 
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          ) 
        </mo> 
       </mrow> 
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         + 
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          M 
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         </mi> 
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        </mrow> 
       </msub> 
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          ( 
        </mo> 
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         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
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             Z 
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             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math>. i.e. where the gravitating mass is zero.</p>
    <p>According to the previous equation it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
          <mrow></mrow> 
         </msubsup> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mfrac> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
          <mn>
            3 
          </mn> 
         </msubsup> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </mfrac> 
      </mrow> 
     </math> (4.4)</p>
    <p>Using (3.1) formula 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
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           T 
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           O 
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         </mi> 
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           A 
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           L 
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        </mrow> 
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            R 
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             G 
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          </mrow> 
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        </mrow> 
        <mo>
          ) 
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       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
      </mrow> 
     </math> the Equation (4.4) leads to</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
          <mn>
            3 
          </mn> 
         </msubsup> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </mfrac> 
      </mrow> 
     </math>, (4.5)</p>
    <p>where it is possible to clear up</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mn>
               3 
             </mn> 
             <msup> 
              <mi>
                a 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
            </mrow> 
            <mrow> 
             <mn>
               8 
             </mn> 
             <mi>
               π 
             </mi> 
             <mi>
               G 
             </mi> 
             <msub> 
              <mi>
                ρ 
              </mi> 
              <mrow> 
               <mi>
                 D 
               </mi> 
               <mi>
                 E 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           5 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math> (4.6)</p>
    <p>and as</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           3 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </mfrac> 
       <msub> 
        <mi>
          Ω 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mtext>
           
       </mtext> 
      </mrow> 
     </math> (4.7)</p>
    <p>then by substitution</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            [ 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <msup> 
              <mi>
                a 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
            </mrow> 
            <mrow> 
             <msup> 
              <mi>
                H 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                Ω 
              </mi> 
              <mrow> 
               <mi>
                 D 
               </mi> 
               <mi>
                 E 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ] 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           5 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math> (4.8)</p>
    <p>This formula will be called R<sub>ZG</sub> (parameter a<sup>2</sup>).</p>
    <p>As the radius R<sub>ZG</sub> is the distance to cluster centre where is zero the gravitating mass, it is right to consider R<sub>ZG</sub> as the halo radius and its sphere defined as the halo cluster.</p>
   </sec>
   <sec id="s4_2">
    <title>4.2. Zero Gravity Radius Formula Depending on Virial Mass</title>
    <p>In previous chapter was got the value for 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           6 
         </mn> 
        </mrow> 
       </msup> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mn>
             10 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <mi>
             H 
           </mi> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           3 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math> (3.4), depending on M<sub>VIR</sub>, so by substitution in (4.8) it is right to get</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mrow> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mi>
               G 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 V 
               </mi> 
               <mi>
                 I 
               </mi> 
               <mi>
                 R 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             15 
           </mn> 
          </mrow> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (4.9)</p>
    <p>In <xref ref-type="table" rid="table4">
      Table 4
     </xref> are calculated R<sub>ZG</sub> by two ways: Formulas (4.8) and (4.9). Both calculi are mathematically equivalents. See in <xref ref-type="table" rid="table4">
      Table 4
     </xref> how the both values match perfectly. See in <xref ref-type="table" rid="table2">
      Table 2
     </xref> the values for the Virial mass of Virgo.</p>
    <table-wrap id="table4">
     <label>
      <xref ref-type="table" rid="table4">
       Table 4
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 4. Calculi for Virgo Rzg.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="15.95%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="21.00%"><p style="text-align:center">Parameter a<sup>2</sup> (M<sub>VIR</sub>)</p></td> 
       <td class="custom-bottom-td acenter" width="21.02%"><p style="text-align:center">R<sub>ZG</sub> (parameter a<sup>2</sup>)</p></td> 
       <td class="custom-bottom-td acenter" width="21.02%"><p style="text-align:center">R<sub>ZG</sub> (M<sub>VIR</sub>)</p></td> 
       <td class="custom-bottom-td acenter" width="21.02%"><p style="text-align:center">Relative</p><p style="text-align:center">diff.</p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="15.95%"><p style="text-align:center">Clusters</p></td> 
       <td class="custom-top-td acenter" width="21.00%"><p style="text-align:center">I.S. units m<sup>5/2</sup>/s<sup>2</sup></p></td> 
       <td class="custom-top-td acenter" width="21.02%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="21.02%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="21.02%"><p style="text-align:center">%</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="15.95%"><p style="text-align:center">Virgo</p></td> 
       <td class="acenter" width="21.00%"><p style="text-align:center">3.581E23</p></td> 
       <td class="acenter" width="21.02%"><p style="text-align:center">12.871</p></td> 
       <td class="acenter" width="21.02%"><p style="text-align:center">12.871</p></td> 
       <td class="acenter" width="21.02%"><p style="text-align:center">0</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>With this important cluster of galaxies, it has been illustrated how the total mass,</p>
    <p>calculated by 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           r 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msqrt> 
          <mi>
            r 
          </mi> 
         </msqrt> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
      </mrow> 
     </math>, is counter balanced by dark energy at mega</p>
    <p>parsecs scale, and precisely this Radius at zero gravity determines the region size where the cluster has gravitational influence.</p>
   </sec>
   <sec id="s4_3">
    <title>4.3. Zero Gravity Radius versus Virial Radius</title>
    <p>From (2.2) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msubsup> 
       <mo>
         ≈ 
       </mo> 
       <msubsup> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mn>
           200 
         </mn> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
          <mrow> 
           <mn>
             200 
           </mn> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mn>
           100 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         ≈ 
       </mo> 
       <mfrac> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mn>
           100 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> it is right to get 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mi>
               G 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 V 
               </mi> 
               <mi>
                 I 
               </mi> 
               <mi>
                 R 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mrow> 
             <mn>
               100 
             </mn> 
             <mo>
               ⋅ 
             </mo> 
             <msup> 
              <mi>
                H 
              </mi> 
              <mn>
                2 
              </mn> 
             </msup> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           3 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math>. In previous epigraph was got 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mrow> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mi>
               G 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 V 
               </mi> 
               <mi>
                 I 
               </mi> 
               <mi>
                 R 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             15 
           </mn> 
          </mrow> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (4.9). So it is right to get the ratio</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mn>
               100 
             </mn> 
            </mrow> 
            <mrow> 
             <msub> 
              <mi>
                Ω 
              </mi> 
              <mrow> 
               <mi>
                 D 
               </mi> 
               <mi>
                 E 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           5 
         </mn> 
        </mrow> 
       </msup> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         7.277 
       </mn> 
      </mrow> 
     </math> (4.10)</p>
    <p>which is universal as it does not depend on virial mass associated to a specific cluster.</p>
    <p>Using the data from <xref ref-type="table" rid="table1">
      Table 1
     </xref>, first, second and third columns, the fourth column of <xref ref-type="table" rid="table5">
      Table 5
     </xref> is calculated the zero gravity radius formula (4.9). In the last column is calculated the ratio.</p>
    <p>It is clear that the ratio R<sub>ZG</sub>/R<sub>VIR</sub> got in this sample of celestial bodies match very well with the theoretical ratio formula (4.10)</p>
    <table-wrap id="table5">
     <label>
      <xref ref-type="table" rid="table5">
       Table 5
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 5. Celestial bodies.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="21.24%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="19.69%"><p style="text-align:center">Virial Radius</p></td> 
       <td class="custom-bottom-td acenter" width="19.69%"><p style="text-align:center">Virial Mass</p></td> 
       <td class="custom-bottom-td acenter" width="22.30%"><p style="text-align:center">Zero Gravity R.</p></td> 
       <td class="custom-bottom-td acenter" width="17.08%"><p style="text-align:center">Ratio</p></td> 
      </tr> 
      <tr> 
       <td class="custom-bottom-td custom-top-td acenter" width="21.24%"><p style="text-align:center">Celestial Body</p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="19.69%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="19.69%"><p style="text-align:center">1E13 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="22.30%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-bottom-td custom-top-td acenter" width="17.08%"><p style="text-align:center">R<sub>ZG</sub>/R<sub>VIR</sub></p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="21.24%"><p style="text-align:center">Antlia cluster</p></td> 
       <td class="custom-top-td acenter" width="19.69%"><p style="text-align:center">1.28</p></td> 
       <td class="custom-top-td acenter" width="19.69%"><p style="text-align:center">26.3</p></td> 
       <td class="custom-top-td acenter" width="22.30%"><p style="text-align:center">9.62E+00</p></td> 
       <td class="custom-top-td acenter" width="17.08%"><p style="text-align:center">7.52E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC596/584</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">0.5</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">1.55</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">3.74E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.49E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC 3268</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">0.9</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">8.99</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">6.73E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.47E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC 4365</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">0.32</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">0.4</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">2.38E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.45E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC 4636</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">0.63</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">3.02</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">4.68E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.42E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC 4697</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">1.29</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">26.9</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">9.69E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.51E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC 5846</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">1.1</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">16.6</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">8.25E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.50E+00</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="21.24%"><p style="text-align:center">NGC 6868</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">0.6</p></td> 
       <td class="acenter" width="19.69%"><p style="text-align:center">2.69</p></td> 
       <td class="acenter" width="22.30%"><p style="text-align:center">4.50E+00</p></td> 
       <td class="acenter" width="17.08%"><p style="text-align:center">7.50E+00</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>Similarly in <xref ref-type="table" rid="table6">
      Table 6
     </xref>, it is done the same ratio for the Virgo cluster with an optimal result, for the Virial radius see <xref ref-type="table" rid="table3">
      Table 3
     </xref>, for the Zero gravity radius see <xref ref-type="table" rid="table4">
      Table 4
     </xref>.</p>
    <table-wrap id="table6">
     <label>
      <xref ref-type="table" rid="table6">
       Table 6
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 6. Virgo cluster.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="19.49%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="18.09%"><p style="text-align:center">VirialRadius</p></td> 
       <td class="custom-bottom-td acenter" width="18.09%"><p style="text-align:center">Zero Grav R</p></td> 
       <td class="custom-bottom-td acenter" width="18.09%"><p style="text-align:center">Ratio</p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="19.49%"><p style="text-align:center">Cluster</p></td> 
       <td class="custom-top-td acenter" width="18.09%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="18.09%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="18.09%"><p style="text-align:center">R<sub>ZG</sub>/R<sub>VIR</sub></p></td> 
      </tr> 
      <tr> 
       <td class="custom-bottom-td acenter" width="19.49%"><p style="text-align:center">Virgo </p></td> 
       <td class="custom-bottom-td acenter" width="18.09%"><p style="text-align:center">1.7</p></td> 
       <td class="custom-bottom-td acenter" width="18.09%"><p style="text-align:center">12.871</p></td> 
       <td class="custom-bottom-td acenter" width="18.09%"><p style="text-align:center">7.57</p></td> 
      </tr> 
     </table>
    </table-wrap>
   </sec>
   <sec id="s4_4">
    <title>
     <xref ref-type="bibr" rid="scirp.136741-"></xref>4.4. Total Mass Associated to a Cluster of Galaxies</title>
    <p>In epigraph 4.1 was shown how this equation 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mo stretchy="false">
         ( 
       </mo> 
       <mo>
         &lt; 
       </mo> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo stretchy="false">
         ) 
       </mo> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
          <mn>
            3 
          </mn> 
         </msubsup> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </mfrac> 
      </mrow> 
     </math> see (4.4) is used to define R<sub>ZG</sub>. By simplification it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <msubsup> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mi>
         M 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msubsup> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msubsup> 
      </mrow> 
     </math> (4.11)</p>
    <p>being M = 5.3984·10<sup>−</sup><sup>26</sup> (I.S.)</p>
    <p>So that is the total mass formula, using the equation between total mass and dark energy at zero gravity radius.</p>
    <p>In <xref ref-type="table" rid="table7">
      Table 7
     </xref> is shown calculus of total mass for Virgo.</p>
    <table-wrap id="table7">
     <label>
      <xref ref-type="table" rid="table7">
       Table 7
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 7. Calculus of total mass for Virgo.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="20.87%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="19.24%"><p style="text-align:center">Radius ZG</p></td> 
       <td class="custom-bottom-td acenter" width="36.33%"><p style="text-align:center">M<sub>TOTAL</sub> (&lt;R<sub>ZG</sub>) = M·R<sup>3</sup><sub>ZG</sub></p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="20.87%"><p style="text-align:center">Clusters</p></td> 
       <td class="custom-top-td acenter" width="19.24%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="36.33%"><p style="text-align:center"> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="20.87%"><p style="text-align:center">Virgo </p></td> 
       <td class="acenter" width="19.24%"><p style="text-align:center">12.871</p></td> 
       <td class="acenter" width="36.33%"><p style="text-align:center">1.699945E15</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>Using rightly the direct mass formula see (3.1) at R<sub>ZG</sub> it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
      </mrow> 
     </math> (4.12)</p>
    <p>By substitution of (3.4) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msup> 
        <mi>
          a 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           6 
         </mn> 
        </mrow> 
       </msup> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mn>
             10 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <mi>
             H 
           </mi> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           3 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math> and (4.9) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mrow> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mi>
               G 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 V 
               </mi> 
               <mi>
                 I 
               </mi> 
               <mi>
                 R 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             15 
           </mn> 
          </mrow> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> in (4.12) it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mtext>
           
       </mtext> 
       <mfrac> 
        <mrow> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.13)</p>
    <p>and calling</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         U 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (4.14)</p>
    <p>U ≈ 2.7 then</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.15)</p>
    <p>So may be stated that according Dark matter by gravitation theory, the total mass (baryonic plus DM) enclosed by the sphere with radius R<sub>ZG</sub> is equivalent to 2.7 times the Virial Mass.</p>
    <p>In <xref ref-type="table" rid="table8">
      Table 8
     </xref> are compared the masses for Virgo using the formula (4.15) and the previous one (4.11). It is clear that both are mathematically equivalents.</p>
    <table-wrap id="table8">
     <label>
      <xref ref-type="table" rid="table8">
       Table 8
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 8. Compared data.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="15.86%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="17.79%"><p style="text-align:center">Virial mass</p></td> 
       <td class="custom-bottom-td acenter" width="32.82%"><p style="text-align:center">M<sub>TOTAL</sub> (&lt;R<sub>ZG</sub>) = U·M<sub>V</sub><sub>IR</sub></p></td> 
       <td class="custom-bottom-td acenter" width="31.13%"><p style="text-align:center">M<sub>TOTAL</sub> (&lt;R<sub>ZG</sub>) =M·R<sup>3</sup><sub>ZG</sub></p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="15.86%"><p style="text-align:center">Clusters</p></td> 
       <td class="custom-top-td acenter" width="17.79%"><p style="text-align:center">·10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-top-td acenter" width="32.82%"><p style="text-align:center"> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-top-td acenter" width="31.13%"><p style="text-align:center"> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="15.86%"><p style="text-align:center">Virgo</p></td> 
       <td class="acenter" width="17.79%"><p style="text-align:center">6.3 ± 0.9</p></td> 
       <td class="acenter" width="32.82%"><p style="text-align:center">1.6994E15</p></td> 
       <td class="acenter" width="31.13%"><p style="text-align:center">1.6994E15</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>By the direct formula for total mass, may be calculated the total mass associated to a radius, which is a fraction of R<sub>ZG</sub>, with the following property: if 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mi>
           R 
         </mi> 
         <mo>
           = 
         </mo> 
         <mi>
           f 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math> then</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
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           f 
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           ⋅ 
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            R 
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             Z 
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             G 
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        <mo>
          ) 
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       <mo>
         = 
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        <mrow> 
         <mi>
           f 
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           ⋅ 
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         <msub> 
          <mi>
            R 
          </mi> 
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             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            a 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mi>
          G 
        </mi> 
       </mfrac> 
       <mo> 
       </mo> 
       <mo>
         = 
       </mo> 
       <msqrt> 
        <mi>
          f 
        </mi> 
       </msqrt> 
       <mo>
         ⋅ 
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         U 
       </mi> 
       <mo>
         ⋅ 
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        <mi>
          M 
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           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.16)</p>
    <p>because 
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          M 
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        </mrow> 
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      </mrow> 
     </math>. See (4.15)</p>
    <p>e.g., using the data for Virgo cluster R<sub>ZG</sub> = 12.87 and R<sub>VIR</sub> = R<sub>200</sub> = 1.7687 Mpc, then R<sub>VIR</sub>/R<sub>ZG</sub> = f = 0.137428 and by the formula (4.16)</p>
    <p>
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        </mrow> 
       </msub> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         0.99999 
       </mn> 
       <msub> 
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          M 
        </mi> 
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        </mrow> 
       </msub> 
      </mrow> 
     </math>.</p>
   </sec>
   <sec id="s4_5">
    <title>
     <xref ref-type="bibr" rid="scirp.136741-"></xref>4.5. Total Dark Energy at Zero Gravity Radius</title>
    <p>The formula (4.2) at R<sub>ZG</sub> becomes</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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         = 
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           ⋅ 
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         ⋅ 
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        </mrow> 
        <mn>
          3 
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       </msubsup> 
      </mrow> 
     </math> (4.17)</p>
    <p>that it is just the opposite value to 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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         = 
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       <mfrac> 
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          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
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        </mrow> 
        <mrow> 
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          <mi>
            Ω 
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          <mrow> 
           <mn>
             1 
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             5 
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         ⋅ 
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      </mrow> 
     </math> see (4.13) because the total gravitating mass enclosed into the sphere of zero gravity radius is zero by definition.</p>
    <p>
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          ) 
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       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> (4.18)</p>
    <p>See epigraph 4.1</p>
    <p>Therefore 
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        <mrow> 
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          <mrow> 
           <mn>
             100 
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            5 
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        </mrow> 
        <mrow> 
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          <mi>
            Ω 
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             D 
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             1 
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             / 
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             5 
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         ⋅ 
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        </mrow> 
       </msub> 
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     </math> see (4.15), being U ≈ 2.7, so joining (4.17) and (4.18) it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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          ) 
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         = 
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        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.19)</p>
    <p>The formula (4.19) may be used to calculate the mass associated to DE at a specific radius R, writing such radius as a fraction of R<sub>ZG</sub> i.e. 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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          </mrow> 
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        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math> then (4.2) is written as</p>
    <p>
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          M 
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            3 
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           ⋅ 
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            2 
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           ⋅ 
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        <mi>
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       <mo>
         ⋅ 
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       <msubsup> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
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         </mi> 
        </mrow> 
        <mn>
          3 
        </mn> 
       </msubsup> 
       <mo>
         = 
       </mo> 
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         − 
       </mo> 
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        <mi>
          f 
        </mi> 
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          3 
        </mn> 
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       <mo>
         ⋅ 
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       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.20)</p>
    <p>For example using the Virgo data R<sub>ZG</sub> =12.871 Mpc and R<sub>VIR</sub> = R<sub>200</sub> = 1.7687 Mpc, the ratio R<sub>VIR</sub>/R<sub>ZG</sub> = f = 0.137428 and 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mtext>
           
       </mtext> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           f 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <msup> 
        <mi>
          f 
        </mi> 
        <mn>
          3 
        </mn> 
       </msup> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mn>
         0.007 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> i.e. M<sub>DE</sub> (&lt;R<sub>VIR</sub>) is negligible, whereas 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mtext>
           
       </mtext> 
       <mo>
         − 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>.</p>
   </sec>
   <sec id="s4_6">
    <title>4.6. Gravitating Mass Function</title>
    <p>In the epigraph 4.1 was defined the gravitating mass M<sub>G</sub> = M<sub>DE</sub> + M<sub>TOTAL</sub>, where M<sub>TOTAL</sub> is baryonic plus dark matter mass and M<sub>DE</sub> is the negative mass associated to DE.</p>
    <p>The best way to calculate the gravitating mass is using the formulas got in epigraph 4.4 and 4.5 where are calculated the both types of masses associated to a radius, which is a fraction of R<sub>ZG</sub>, i.e. 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         R 
       </mi> 
       <mo>
         = 
       </mo> 
       <mi>
         f 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>, these formulas are (4.16) and (4.20).</p>
    <p>Joining both ones it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           R 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           f 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <msqrt> 
          <mi>
            f 
          </mi> 
         </msqrt> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mi>
            f 
          </mi> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.21)</p>
    <p>where 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         U 
       </mi> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         2.7 
       </mn> 
      </mrow> 
     </math>. This way the gravitating mass depends on the dimensionless factor f.</p>
    <p>As the gravitating mass is defined into the halo cluster, its dominion begins at R<sub>VIR</sub> so the gravitating mass depending on f begins at R<sub>VIR</sub>/R<sub>ZG</sub>. By (4.10) formula R<sub>ZG</sub>/R<sub>VIR</sub> =7.277 then R<sub>VIR</sub>/R<sub>ZG</sub> = 1/7.277 therefore the dominion of the gravitating mass function depending on 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         f 
       </mi> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mi>
          R 
        </mi> 
        <mo>
          / 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mrow> 
      </mrow> 
     </math> begins at 0.13732.</p>
    <p>In this epigraph this function will be studied up to f = 1 i.e. when the radius reaches the zero gravity radius.</p>
    <p>In <xref ref-type="fig" rid="fig1">
      Figure 1
     </xref> is represented the ratio gravitating mass/virial mass versus the ratio f = R/R<sub>ZG</sub> in its dominion and close to f = 0.5 the function reach the maximum.</p>
    <fig id="fig1" position="float">
     <label>Figure 1</label>
     <caption>
      <title>Figure 1. Gravitating mass function/Virial mass vs f.</title>
     </caption>
     <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/2181121-rId164.jpeg?20241023084557" />
    </fig>
   </sec>
   <sec id="s4_7">
    <title>4.7. Calculus for the Maximum of the Gravitating Mass</title>
    <p>It is clear that such function will have a maximum, that it is found easily by derivation, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          f 
        </mi> 
        <mi>
          M 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <mroot> 
          <mrow> 
           <mn>
             36 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
         </mroot> 
        </mrow> 
       </mfrac> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         0.488 
       </mn> 
      </mrow> 
     </math>, so the radius at maximum is</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mi>
          M 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <mroot> 
          <mrow> 
           <mn>
             36 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
         </mroot> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         0.488 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>. (4.22)</p>
    <p>By substitution of this value f<sub>M</sub> into the mass gravitating formula (5.21) it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
        <mrow> 
         <mi>
           M 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           X 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           M 
         </mi> 
         <mi>
           U 
         </mi> 
         <mi>
           M 
         </mi> 
        </mrow> 
       </msubsup> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mi>
            M 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         1.57 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.23)</p>
    <p>So may be stated the following important result:</p>
    <p>For any cluster of galaxies at a half of R<sub>ZG</sub>, it is reached the maximum of gravitating mass which is 1.57·M<sub>VIR</sub>.</p>
   </sec>
   <sec id="s4_8">
    <title>4.8. Density of the Total Mass into the Halo Cluster Theorem</title>
    <p>Assuming the hypothesis that R<sub>vir</sub> = R<sub>200</sub> and M<sub>vir</sub> = M<sub>200</sub>, i.e. the virial sphere 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         D 
       </mi> 
       <mi>
         e 
       </mi> 
       <mi>
         n 
       </mi> 
       <mi>
         s 
       </mi> 
       <mi>
         i 
       </mi> 
       <mi>
         t 
       </mi> 
       <msub> 
        <mi>
          y 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mo> 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
          <mrow> 
           <mi>
             v 
           </mi> 
           <mi>
             i 
           </mi> 
           <mi>
             r 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           o 
         </mi> 
         <msub> 
          <mi>
            l 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mn>
         200 
       </mn> 
       <mtext>
           
       </mtext> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
      </mrow> 
     </math> being 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           3 
         </mn> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mrow> 
         <mn>
           8 
         </mn> 
         <mi>
           π 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> the critical density of Universe.</p>
    <p>Then into the halo cluster sphere the</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo> 
       </mo> 
       <mi>
         D 
       </mi> 
       <mi>
         e 
       </mi> 
       <mi>
         n 
       </mi> 
       <mi>
         s 
       </mi> 
       <mi>
         i 
       </mi> 
       <mi>
         t 
       </mi> 
       <msub> 
        <mi>
          y 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
         <mo> 
         </mo> 
         <mi>
           M 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           S 
         </mi> 
         <mi>
           S 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         1.4 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
      </mrow> 
     </math> (4.24)</p>
    <p>Being R<sub>ZG</sub> the halo radius.</p>
    <p>Proof:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
       <mtr> 
        <mtd> 
         <mi>
           D 
         </mi> 
         <mi>
           e 
         </mi> 
         <mi>
           n 
         </mi> 
         <mi>
           s 
         </mi> 
         <mi>
           i 
         </mi> 
         <mi>
           t 
         </mi> 
         <msubsup> 
          <mi>
            y 
          </mi> 
          <mrow> 
           <mi>
             T 
           </mi> 
           <mi>
             O 
           </mi> 
           <mi>
             T 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
           <mo> 
           </mo> 
           <mi>
             M 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             S 
           </mi> 
           <mi>
             S 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             C 
           </mi> 
           <mi>
             L 
           </mi> 
           <mi>
             U 
           </mi> 
           <mi>
             S 
           </mi> 
           <mi>
             T 
           </mi> 
           <mi>
             E 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msubsup> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mo>
             &lt; 
           </mo> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
         <mo>
           = 
         </mo> 
         <mfrac> 
          <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mrow> 
             <mi>
               T 
             </mi> 
             <mi>
               O 
             </mi> 
             <mi>
               T 
             </mi> 
             <mi>
               A 
             </mi> 
             <mi>
               L 
             </mi> 
            </mrow> 
           </msub> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mo>
               &lt; 
             </mo> 
             <msub> 
              <mi>
                R 
              </mi> 
              <mrow> 
               <mi>
                 Z 
               </mi> 
               <mi>
                 G 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             o 
           </mi> 
           <msub> 
            <mi>
              l 
            </mi> 
            <mrow> 
             <mi>
               C 
             </mi> 
             <mi>
               L 
             </mi> 
            </mrow> 
           </msub> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mo>
               &lt; 
             </mo> 
             <msub> 
              <mi>
                R 
              </mi> 
              <mrow> 
               <mi>
                 Z 
               </mi> 
               <mi>
                 G 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
         </mfrac> 
         <mo>
           = 
         </mo> 
         <mfrac> 
          <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
            </mrow> 
           </msub> 
           <mo>
             ⋅ 
           </mo> 
           <mi>
             U 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             o 
           </mi> 
           <msub> 
            <mi>
              l 
            </mi> 
            <mrow> 
             <mi>
               v 
             </mi> 
             <mi>
               i 
             </mi> 
             <mi>
               r 
             </mi> 
            </mrow> 
           </msub> 
           <mo>
             ⋅ 
           </mo> 
           <msup> 
            <mrow> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mfrac> 
                <mrow> 
                 <msub> 
                  <mi>
                    R 
                  </mi> 
                  <mrow> 
                   <mi>
                     Z 
                   </mi> 
                   <mi>
                     G 
                   </mi> 
                  </mrow> 
                 </msub> 
                </mrow> 
                <mrow> 
                 <msub> 
                  <mi>
                    R 
                  </mi> 
                  <mrow> 
                   <mi>
                     V 
                   </mi> 
                   <mi>
                     I 
                   </mi> 
                   <mi>
                     R 
                   </mi> 
                  </mrow> 
                 </msub> 
                </mrow> 
               </mfrac> 
              </mrow> 
              <mo>
                ) 
              </mo> 
             </mrow> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
         <mo>
           = 
         </mo> 
         <mfrac> 
          <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mrow> 
             <mi>
               V 
             </mi> 
             <mi>
               I 
             </mi> 
             <mi>
               R 
             </mi> 
            </mrow> 
           </msub> 
           <mo>
             ⋅ 
           </mo> 
           <mi>
             U 
           </mi> 
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           </mi> 
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             o 
           </mi> 
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            <mi>
              l 
            </mi> 
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             </mi> 
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               i 
             </mi> 
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               r 
             </mi> 
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           </msub> 
           <mo>
             ⋅ 
           </mo> 
           <msup> 
            <mi>
              U 
            </mi> 
            <mn>
              6 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
        </mtd> 
       </mtr> 
       <mtr> 
        <mtd> 
         <mo>
           = 
         </mo> 
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          <mrow> 
           <mn>
             200 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              ρ 
            </mi> 
            <mi>
              C 
            </mi> 
           </msub> 
          </mrow> 
          <mrow> 
           <msup> 
            <mi>
              U 
            </mi> 
            <mn>
              5 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
         <mo>
           = 
         </mo> 
         <mfrac> 
          <mrow> 
           <mn>
             200 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              ρ 
            </mi> 
            <mi>
              C 
            </mi> 
           </msub> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              Ω 
            </mi> 
            <mrow> 
             <mi>
               D 
             </mi> 
             <mi>
               E 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
         </mfrac> 
         <mo>
           = 
         </mo> 
         <mn>
           1.4 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            ρ 
          </mi> 
          <mi>
            C 
          </mi> 
         </msub> 
        </mtd> 
       </mtr> 
      </mtable> 
     </math></p>
    <p>In that chained equalities has been used two properties before got: (4.15) and (4.10).</p>
    <p>As into the current 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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         Λ 
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       </mi> 
      </mrow> 
     </math> model the DE density has a constant value, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        <mi>
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       <mo>
         = 
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       <mn>
         0.7 
       </mn> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
      </mrow> 
     </math>in every place, in particular</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         D 
       </mi> 
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         e 
       </mi> 
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         n 
       </mi> 
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         s 
       </mi> 
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         i 
       </mi> 
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         t 
       </mi> 
       <msubsup> 
        <mi>
          y 
        </mi> 
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           D 
         </mi> 
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           A 
         </mi> 
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         </mi> 
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         </mi> 
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           E 
         </mi> 
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           N 
         </mi> 
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           E 
         </mi> 
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           R 
         </mi> 
         <mi>
           G 
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         </mi> 
         <mi>
           L 
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           U 
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           S 
         </mi> 
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           T 
         </mi> 
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           E 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msubsup> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0.7 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          c 
        </mi> 
       </msub> 
      </mrow> 
     </math> (4.25)</p>
    <p>Corolarius</p>
    <p>The ratio density of total mass versus density of DE into the halo cluster is 2.</p>
   </sec>
   <sec id="s4_9">
    <title>4.9. Extended Halo Where the Ratio Total Mass versus Dark Energy Is 3/7</title>
    <p>At the present, it is accepted that 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        <mrow> 
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            M 
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       <mo>
         = 
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        <mn>
          3 
        </mn> 
        <mo>
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        </mo> 
        <mn>
          7 
        </mn> 
       </mrow> 
      </mrow> 
     </math> as a global average in the current Universe, so it is worth to calculate an extension of halo cluster, R<sub>E</sub>, where it is reached such ratio. Now it is calculated the radius of a sphere that verify</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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             P 
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         <mrow> 
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            ( 
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             &lt; 
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              E 
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            ) 
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        </mrow> 
        <mrow> 
         <msub> 
          <mi>
            ρ 
          </mi> 
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           <mi>
             D 
           </mi> 
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             E 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mn>
          3 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          7 
        </mn> 
       </mrow> 
      </mrow> 
     </math> (4.26)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         A 
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      </mrow> 
     </math> and by (4.2) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        <mi>
          M 
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      </mrow> 
     </math></p>
    <p>then by substitution into (4.26) it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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       <mo>
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           ⋅ 
         </mo> 
         <msub> 
          <mi>
            M 
          </mi> 
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             T 
           </mi> 
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             M 
           </mi> 
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         </msub> 
         <mrow> 
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            ( 
          </mo> 
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             &lt; 
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           </mi> 
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            ) 
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            M 
          </mi> 
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           <mi>
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           </mi> 
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           </mi> 
          </mrow> 
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         <mrow> 
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            ( 
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       <mo>
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        </mo> 
        <mn>
          7 
        </mn> 
       </mrow> 
      </mrow> 
     </math> (4.27)</p>
    <p>Using (4.16) and (4.20) it is right to get the second one equality below.</p>
    <p>
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          </mi> 
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          </mi> 
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          </mi> 
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           </mi> 
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          </mi> 
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        <mrow> 
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          </mi> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (4.28)</p>
    <p>By equation (4.27) and (4.28) it is got 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msqrt> 
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            f 
          </mi> 
         </msqrt> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            f 
          </mi> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mn>
          3 
        </mn> 
        <mn>
          7 
        </mn> 
       </mfrac> 
      </mrow> 
     </math> whose solution is</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         f 
       </mi> 
       <mo>
         = 
       </mo> 
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        <mrow> 
         <mrow> 
          <mo>
            ( 
          </mo> 
          <mrow> 
           <mfrac> 
            <mrow> 
             <mn>
               14 
             </mn> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </mfrac> 
          </mrow> 
          <mo>
            ) 
          </mo> 
         </mrow> 
        </mrow> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           5 
         </mn> 
        </mrow> 
       </msup> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         1.85 
       </mn> 
      </mrow> 
     </math> (4.29)</p>
    <p>Therefore the radius of extended halo searched is</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mi>
          E 
        </mi> 
       </msub> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         1.85 
       </mn> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.30)</p>
    <p>and by (4.16)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
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          M 
        </mi> 
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           T 
         </mi> 
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         </mi> 
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         </mi> 
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         </mi> 
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       <mrow> 
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          ( 
        </mo> 
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         </msub> 
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        <mo>
          ) 
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       <mo>
         ≈ 
       </mo> 
       <mn>
         3.67 
       </mn> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
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         </mi> 
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         </mi> 
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      </mrow> 
     </math> (4.31)</p>
    <p>In order to validate such calculus is enough to check that the Density of total mass at R<sub>E</sub> radius is 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo> 
       </mo> 
       <mn>
         0.3 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
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          ρ 
        </mi> 
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          C 
        </mi> 
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     </math></p>
    <p>
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          ) 
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       <mo>
         = 
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           ⋅ 
         </mo> 
         <mi>
           U 
         </mi> 
         <mo>
           ⋅ 
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         <msqrt> 
          <mrow> 
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             1.85 
           </mn> 
          </mrow> 
         </msqrt> 
        </mrow> 
        <mrow> 
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           V 
         </mi> 
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           o 
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            l 
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             v 
           </mi> 
           <mi>
             i 
           </mi> 
           <mi>
             r 
           </mi> 
          </mrow> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mrow> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mfrac> 
              <mrow> 
               <msub> 
                <mi>
                  R 
                </mi> 
                <mrow> 
                 <mi>
                   Z 
                 </mi> 
                 <mi>
                   G 
                 </mi> 
                </mrow> 
               </msub> 
              </mrow> 
              <mrow> 
               <msub> 
                <mi>
                  R 
                </mi> 
                <mrow> 
                 <mi>
                   V 
                 </mi> 
                 <mi>
                   I 
                 </mi> 
                 <mi>
                   R 
                 </mi> 
                </mrow> 
               </msub> 
              </mrow> 
             </mfrac> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mn>
            3 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mrow> 
           <mn>
             1.85 
           </mn> 
          </mrow> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           200 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            ρ 
          </mi> 
          <mi>
            C 
          </mi> 
         </msub> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mn>
           100 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msup> 
          <mrow> 
           <mn>
             1.85 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             5 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           1.4 
         </mn> 
        </mrow> 
        <mrow> 
         <msup> 
          <mrow> 
           <mn>
             1.85 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             5 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </msup> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0.3 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          ρ 
        </mi> 
        <mi>
          C 
        </mi> 
       </msub> 
      </mrow> 
     </math>(4.32)</p>
    <p>as it was expected.</p>
    <p>For example for the Virgo cluster R<sub>E</sub> = 1.85·12.9 Mpc = 23.9 Mpc.</p>
   </sec>
  </sec><sec id="s5">
   <title>
    <xref ref-type="bibr" rid="scirp.136741-"></xref>5. Zero Velocity Radius Because of the Hubble Flow</title>
   <p>It is defined the zero velocity radius as the distance to the cluster centre, where the escape velocity from gravitation field is equal to Hubble flow velocity. i.e.</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mi>
         E 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mi>
          H 
        </mi> 
        <mi>
          F 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (5.1)</p>
   <p>From classical dynamic it is taken the formula</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           V 
         </mi> 
         <mi>
           E 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mi>
        V 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         R 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>. (5.2)</p>
   <p>i.e. the kinetic energy associated to escape velocity compensates the potential energy getting zero as total energy ad infinitum.</p>
   <p>It is not possible to use the classical escape velocity formula</p>
   <p>
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         V 
       </mi> 
       <mi>
         E 
       </mi> 
       <mn>
         2 
       </mn> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          G 
        </mi> 
        <mi>
          M 
        </mi> 
       </mrow> 
       <mi>
         R 
       </mi> 
      </mfrac> 
     </mrow> 
    </math>. (5.3)</p>
   <p>because of two reasons:</p>
   <p>1) The gravitational potential in DMbG they is different to 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        V 
      </mi> 
      <mo>
        = 
      </mo> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          M 
        </mi> 
       </mrow> 
       <mi>
         R 
       </mi> 
      </mfrac> 
     </mrow> 
    </math>.</p>
   <p>2) The border of the halo cluster is R<sub>ZG</sub> where the gravitating mass is zero.</p>
   <sec id="s5_1">
    <title>5.1. Gravitational Potential into the Halo Cluster</title>
    <p>The gravitating mass is zero at R<sub>ZG</sub> the line integral for potential goes up to R<sub>ZG</sub>, so the formula is</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         V 
       </mi> 
       <mo>
         = 
       </mo> 
       <munderover> 
        <mstyle mathsize="140%" displaystyle="true"> 
         <mo>
           ∫ 
         </mo> 
        </mstyle> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </munderover> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <mo>
             − 
           </mo> 
           <mi>
             G 
           </mi> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              G 
            </mi> 
           </msub> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mo>
               &lt; 
             </mo> 
             <mi>
               r 
             </mi> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mrow> 
           <msup> 
            <mi>
              r 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mtext>
         d 
       </mtext> 
       <mi>
         r 
       </mi> 
      </mrow> 
     </math> (5.4)</p>
    <p>The gravitating mass 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           r 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           f 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <msqrt> 
          <mi>
            f 
          </mi> 
         </msqrt> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mi>
            f 
          </mi> 
          <mn>
            3 
          </mn> 
         </msup> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (4.21) will be used to do the integral, doing some little changes.</p>
    <p>As 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         f 
       </mi> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          / 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mrow> 
      </mrow> 
     </math> and calling 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         K 
       </mi> 
       <mo>
         = 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>, by substitution in (4.21) it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           r 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mi>
         K 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <msqrt> 
            <mi>
              r 
            </mi> 
           </msqrt> 
          </mrow> 
          <mrow> 
           <msqrt> 
            <mrow> 
             <msub> 
              <mi>
                R 
              </mi> 
              <mrow> 
               <mi>
                 Z 
               </mi> 
               <mi>
                 G 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </msqrt> 
          </mrow> 
         </mfrac> 
         <mo>
           − 
         </mo> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              r 
            </mi> 
            <mn>
              3 
            </mn> 
           </msup> 
          </mrow> 
          <mrow> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
      </mrow> 
     </math> (5.5)</p>
    <p>that by substitution in (5.4) results</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          R 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mi>
         G 
       </mi> 
       <mi>
         K 
       </mi> 
       <munderover> 
        <mstyle mathsize="140%" displaystyle="true"> 
         <mo>
           ∫ 
         </mo> 
        </mstyle> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </munderover> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              r 
            </mi> 
            <mrow> 
             <mo>
               − 
             </mo> 
             <mn>
               3 
             </mn> 
             <mo>
               / 
             </mo> 
             <mn>
               2 
             </mn> 
            </mrow> 
           </msup> 
          </mrow> 
          <mrow> 
           <msqrt> 
            <mrow> 
             <msub> 
              <mi>
                R 
              </mi> 
              <mrow> 
               <mi>
                 Z 
               </mi> 
               <mi>
                 G 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </msqrt> 
          </mrow> 
         </mfrac> 
         <mo>
           − 
         </mo> 
         <mfrac> 
          <mi>
            r 
          </mi> 
          <mrow> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <mtext>
         d 
       </mtext> 
       <mi>
         r 
       </mi> 
      </mrow> 
     </math> (5.6)</p>
    <p>whose result is</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          r 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mi>
           G 
         </mi> 
         <mi>
           K 
         </mi> 
        </mrow> 
        <mrow> 
         <mn>
           2 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mfrac> 
       <mo> 
       </mo> 
       <mo> 
       </mo> 
       <mo>
         − 
       </mo> 
       <mi>
         G 
       </mi> 
       <mi>
         K 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mn>
            2 
          </mn> 
          <mrow> 
           <msqrt> 
            <mi>
              r 
            </mi> 
           </msqrt> 
           <mo>
             ⋅ 
           </mo> 
           <msqrt> 
            <mrow> 
             <msub> 
              <mi>
                R 
              </mi> 
              <mrow> 
               <mi>
                 Z 
               </mi> 
               <mi>
                 G 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </msqrt> 
          </mrow> 
         </mfrac> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              r 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
          </mrow> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo> 
       </mo> 
       <mo> 
       </mo> 
      </mrow> 
     </math> (5.7)</p>
    <p>where its dominion ranges from R<sub>VIR</sub> up to R<sub>ZG</sub>.</p>
    <p>Notice that 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math> and 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          r 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math> is negative inside its dominion.</p>
   </sec>
   <sec id="s5_2">
    <title>5.2. Equation for Zero Velocity Radius</title>
    <p>In this epigraph will be developed the equation 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          V 
        </mi> 
        <mi>
          E 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          r 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          V 
        </mi> 
        <mrow> 
         <mi>
           H 
         </mi> 
         <mi>
           F 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          r 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math> (5.1) to calculate the 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           V 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math></p>
    <p>From (5.2) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          V 
        </mi> 
        <mi>
          E 
        </mi> 
        <mn>
          2 
        </mn> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mo>
         − 
       </mo> 
       <mn>
         2 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          R 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math> So</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo>
         − 
       </mo> 
       <mn>
         2 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         V 
       </mi> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mi>
          R 
        </mi> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msubsup> 
        <mi>
          V 
        </mi> 
        <mrow> 
         <mi>
           H 
         </mi> 
         <mi>
           F 
         </mi> 
        </mrow> 
        <mn>
          2 
        </mn> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mi>
          H 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          R 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
      </mrow> 
     </math> (5.8)</p>
    <p>and by substitution of potential formula (5.7) it is got</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo> 
       </mo> 
       <mo> 
       </mo> 
       <mfrac> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mn>
           5 
         </mn> 
         <mi>
           G 
         </mi> 
         <mi>
           K 
         </mi> 
        </mrow> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mfrac> 
       <mo> 
       </mo> 
       <mo>
         + 
       </mo> 
       <mn>
         2 
       </mn> 
       <mi>
         G 
       </mi> 
       <mi>
         K 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mn>
            2 
          </mn> 
          <mrow> 
           <msqrt> 
            <mi>
              r 
            </mi> 
           </msqrt> 
           <mo>
             ⋅ 
           </mo> 
           <msqrt> 
            <mrow> 
             <msub> 
              <mi>
                R 
              </mi> 
              <mrow> 
               <mi>
                 Z 
               </mi> 
               <mi>
                 G 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
           </msqrt> 
          </mrow> 
         </mfrac> 
         <mo>
           + 
         </mo> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              r 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
          </mrow> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             ⋅ 
           </mo> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msup> 
        <mi>
          H 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
      </mrow> 
     </math> (5.9)</p>
    <p>reorganising that equation it is got:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <mn>
           4 
         </mn> 
         <mi>
           G 
         </mi> 
         <mi>
           K 
         </mi> 
        </mrow> 
        <mrow> 
         <msqrt> 
          <mrow> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            r 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mi>
             K 
           </mi> 
          </mrow> 
          <mrow> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              3 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
         <mo>
           − 
         </mo> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mn>
           5 
         </mn> 
         <mi>
           G 
         </mi> 
         <mi>
           K 
         </mi> 
        </mrow> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mfrac> 
       <mo> 
       </mo> 
      </mrow> 
     </math> (5.10)</p>
    <p>and multiplying that equation by the factor 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mi>
           K 
         </mi> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> it is got a better expression</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <msqrt> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            r 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mn>
            1 
          </mn> 
          <mrow> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              2 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
         <mo>
           − 
         </mo> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              H 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mi>
             K 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mn>
         5 
       </mn> 
      </mrow> 
     </math> (5.11)</p>
    <p>Which is the equation for zero velocity radius.</p>
    <p>That equation is not possible to solve with algebraic methods, but is quite easy to solve numerically for specific data.</p>
   </sec>
   <sec id="s5_3">
    <title>
     <xref ref-type="bibr" rid="scirp.136741-"></xref>5.3. Zero Velocity Radius for Virgo Cluster</title>
    <p>In <xref ref-type="table" rid="table9">
      Table 9
     </xref> there are the Virgo cluster data. Virial radius and mass data come from <xref ref-type="bibr" rid="scirp.136741-9">
      [9]
     </xref> O. Kashi-badze.</p>
    <table-wrap id="table9">
     <label>
      <xref ref-type="table" rid="table9">
       Table 9
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 9. Virgo cluster data.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="16.60%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="23.50%"><p style="text-align:center">Virial Radius</p></td> 
       <td class="custom-bottom-td acenter" width="19.24%"><p style="text-align:center">Virial mass</p></td> 
       <td class="custom-bottom-td acenter" width="19.22%"><p style="text-align:center">R<sub>ZG</sub></p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="16.60%"><p style="text-align:center">Cluster</p></td> 
       <td class="custom-top-td acenter" width="23.50%"><p style="text-align:center">Mpc</p></td> 
       <td class="custom-top-td acenter" width="19.24%"><p style="text-align:center">·10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="custom-top-td acenter" width="19.22%"><p style="text-align:center"></p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="16.60%"><p style="text-align:center">Virgo</p></td> 
       <td class="acenter" width="23.50%"><p style="text-align:center">1.7</p></td> 
       <td class="acenter" width="19.24%"><p style="text-align:center">6.3 ± 0.9</p></td> 
       <td class="acenter" width="19.22%"><p style="text-align:center">12.87 Mpc</p></td> 
      </tr> 
     </table>
    </table-wrap>
    <p>Using such data it is possible to calculate the coefficient for the equation (5.11)</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <msqrt> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            r 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mn>
            1 
          </mn> 
          <mrow> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              2 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
         <mo>
           − 
         </mo> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              H 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mi>
             K 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mn>
         5 
       </mn> 
      </mrow> 
     </math> As U ≈ 2.7 and K = U·M<sub>VIR</sub> then</p>
    <p>GK = 2.259E+35 (I.S. units), 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mn>
            2 
          </mn> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mi>
           K 
         </mi> 
        </mrow> 
       </mfrac> 
       <mo> 
       </mo> 
       <mo>
         = 
       </mo> 
       <mn>
         9.047 
       </mn> 
       <mtext>
         E 
       </mtext> 
       <mo>
         − 
       </mo> 
       <mn>
         48 
       </mn> 
       <msup> 
        <mrow> 
         <mtext>
           m 
         </mtext> 
        </mrow> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math>, 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
          <mn>
            2 
          </mn> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mo> 
       </mo> 
       <mn>
         6.3397 
       </mn> 
       <mtext>
         E 
       </mtext> 
       <mo>
         − 
       </mo> 
       <mn>
         48 
       </mn> 
       <mtext> 
       </mtext> 
       <msup> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mo>
           − 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math> and 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <msqrt> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </msqrt> 
       <mo>
         = 
       </mo> 
       <mn>
         2.5208 
       </mn> 
       <mtext>
         E 
       </mtext> 
       <mo>
         + 
       </mo> 
       <mn>
         12 
       </mn> 
       <msup> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </msup> 
      </mrow> 
     </math></p>
    <p>The equation (5.11) is easy to be solved numerically.</p>
    <p>Using f = Radius/R<sub>ZG</sub> it is got that f = 0.602 is a very good approximation for the solution. Therefore the R<sub>ZV</sub> = f·R<sub>ZG</sub> = 7.75 Mpc.</p>
   </sec>
   <sec id="s5_4">
    <title>5.4. Zero Velocity Radius Theorem</title>
    <p>Considering (5.11) as the equation for the R<sub>ZV </sub>then according DMbQG theory the ratio R<sub>ZV</sub>/R<sub>ZG</sub> is universal and its value is R<sub>ZV</sub>/R<sub>ZG</sub> ≈ 0.602016.</p>
    <p>Proof</p>
    <p>The equation (5.11) is 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <msqrt> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            r 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mn>
            1 
          </mn> 
          <mrow> 
           <msubsup> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
            <mn>
              2 
            </mn> 
           </msubsup> 
          </mrow> 
         </mfrac> 
         <mo>
           − 
         </mo> 
         <mfrac> 
          <mrow> 
           <msup> 
            <mi>
              H 
            </mi> 
            <mn>
              2 
            </mn> 
           </msup> 
           <mo>
             ⋅ 
           </mo> 
           <msub> 
            <mi>
              R 
            </mi> 
            <mrow> 
             <mi>
               Z 
             </mi> 
             <mi>
               G 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mi>
             K 
           </mi> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mn>
         5 
       </mn> 
      </mrow> 
     </math> where 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         K 
       </mi> 
       <mo>
         = 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> being 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         U 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (4.14) and 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mrow> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mi>
               G 
             </mi> 
             <mo>
               ⋅ 
             </mo> 
             <msub> 
              <mi>
                M 
              </mi> 
              <mrow> 
               <mi>
                 V 
               </mi> 
               <mi>
                 I 
               </mi> 
               <mi>
                 R 
               </mi> 
              </mrow> 
             </msub> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <mo>
           ⋅ 
         </mo> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             15 
           </mn> 
          </mrow> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msup> 
          <mi>
            H 
          </mi> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
         </msup> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             2 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
      </mrow> 
     </math> (4.9) then using the values for K, U and R<sub>ZG</sub> , doing some algebraic substitutions and transformations it is not difficult to get the following equation.</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <msqrt> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            r 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msubsup> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
          <mn>
            2 
          </mn> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo> 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <msub> 
            <mi>
              Ω 
            </mi> 
            <mrow> 
             <mi>
               D 
             </mi> 
             <mi>
               E 
             </mi> 
            </mrow> 
           </msub> 
           <mo> 
           </mo> 
           <mo>
             − 
           </mo> 
           <mn>
             1 
           </mn> 
          </mrow> 
          <mrow> 
           <msub> 
            <mi>
              Ω 
            </mi> 
            <mrow> 
             <mi>
               D 
             </mi> 
             <mi>
               E 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          r 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mn>
         5 
       </mn> 
      </mrow> 
     </math> (5.12)</p>
    <p>and defining 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         f 
       </mi> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mi>
          r 
        </mi> 
        <mo>
          / 
        </mo> 
        <mrow> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
       </mrow> 
      </mrow> 
     </math> the equation (5.12) becomes</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            f 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <msub> 
            <mi>
              Ω 
            </mi> 
            <mrow> 
             <mi>
               D 
             </mi> 
             <mi>
               E 
             </mi> 
            </mrow> 
           </msub> 
           <mo> 
           </mo> 
           <mo>
             − 
           </mo> 
           <mn>
             1 
           </mn> 
          </mrow> 
          <mrow> 
           <msub> 
            <mi>
              Ω 
            </mi> 
            <mrow> 
             <mi>
               D 
             </mi> 
             <mi>
               E 
             </mi> 
            </mrow> 
           </msub> 
          </mrow> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          f 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mn>
         5 
       </mn> 
      </mrow> 
     </math> (5.13)</p>
    <p>that considering 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          Ω 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         0.7 
       </mn> 
      </mrow> 
     </math> becomes:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         4 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <mfrac> 
        <mn>
          1 
        </mn> 
        <mrow> 
         <msqrt> 
          <mi>
            f 
          </mi> 
         </msqrt> 
        </mrow> 
       </mfrac> 
       <mo>
         + 
       </mo> 
       <mrow> 
        <mo>
          [ 
        </mo> 
        <mrow> 
         <mfrac> 
          <mrow> 
           <mo>
             − 
           </mo> 
           <mn>
             3 
           </mn> 
          </mrow> 
          <mn>
            7 
          </mn> 
         </mfrac> 
        </mrow> 
        <mo>
          ] 
        </mo> 
       </mrow> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          f 
        </mi> 
        <mn>
          2 
        </mn> 
       </msup> 
       <mo>
         = 
       </mo> 
       <mn>
         5 
       </mn> 
      </mrow> 
     </math> (5.14)</p>
    <p>By elementary algebraic operations it is got this equivalent equation:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mn>
         9 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          f 
        </mi> 
        <mn>
          5 
        </mn> 
       </msup> 
       <mo>
         + 
       </mo> 
       <mtext> 
       </mtext> 
       <mn>
         210 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msup> 
        <mi>
          f 
        </mi> 
        <mn>
          3 
        </mn> 
       </msup> 
       <mo>
         + 
       </mo> 
       <mn>
         1225 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         f 
       </mi> 
       <mo>
         − 
       </mo> 
       <mn>
         784 
       </mn> 
       <mo>
         = 
       </mo> 
       <mn>
         0 
       </mn> 
      </mrow> 
     </math></p>
    <p>Thanks Wolfram alpha software, this is its only real solution</p>
    <p>f ≈ 0.602016 (5.15)</p>
    <p>By this new formulation of the equation for R<sub>ZV</sub> calculus, it has been demonstrated that the ratio f = R<sub>ZV</sub>/R<sub>ZG</sub> is universal and depends on 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          Ω 
        </mi> 
        <mrow> 
         <mi>
           D 
         </mi> 
         <mi>
           E 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> solely.</p>
    <p>Notice how close are the value (5.15) with the one got for Virgo in epigraph 5.3.</p>
   </sec>
   <sec id="s5_5">
    <title>5.5. Gravitating Mass at Zero Velocity Radius</title>
    <p>Using the gravitating mass formula (4.21) being 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           V 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mi>
         f 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mi>
           Z 
         </mi> 
         <mi>
           G 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> and by substitution of 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         f 
       </mi> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         0.602 
       </mn> 
      </mrow> 
     </math> at formula (4.21) where 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         U 
       </mi> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msup> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msup> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         2.6976 
       </mn> 
      </mrow> 
     </math> it is right to get that</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo> 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             V 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         ≈ 
       </mo> 
       <mn>
         1.5 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (5.16)</p>
   </sec>
  </sec><sec id="s6">
   <title>6. Validation of the Theory with Results Published about Virgo Cluster</title>
   <p>In this chapter, some theoretical results got in this paper will be validated with three results published about the Virgo cluster.</p>
   <p>The first test is relative to the R<sub>ZV</sub> and its associated mass. These results were studied in chapter 5.</p>
   <p>The second test is relative to the gravitating mass associated to the twice of virial radius.</p>
   <p>In the third test, the most important, it is postulated that DMbQG theory is able to multiply by the factor 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        U 
      </mi> 
      <mo>
        ⋅ 
      </mo> 
      <msqrt> 
       <mrow> 
        <mn>
          1.85 
        </mn> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <mn>
        2.7 
      </mn> 
      <mo>
        × 
      </mo> 
      <mn>
        1.36 
      </mn> 
      <mo>
        = 
      </mo> 
      <mn>
        3.67 
      </mn> 
     </mrow> 
    </math> the current parameter of local matter density 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         Ω 
       </mi> 
       <mi>
         m 
       </mi> 
       <mrow> 
        <mi>
          l 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          c 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mn>
        0.08 
      </mn> 
     </mrow> 
    </math>. reaching 0.294 which match with the value 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mi>
         Ω 
       </mi> 
       <mi>
         m 
       </mi> 
       <mrow> 
        <mi>
          G 
        </mi> 
        <mi>
          l 
        </mi> 
        <mi>
          o 
        </mi> 
        <mi>
          b 
        </mi> 
        <mi>
          a 
        </mi> 
        <mi>
          l 
        </mi> 
       </mrow> 
      </msubsup> 
      <mo>
        = 
      </mo> 
      <mn>
        0.3 
      </mn> 
     </mrow> 
    </math>. accepted currently by the scientific community.</p>
   <sec id="s6_1">
    <title>6.1. Gravitating Mass Associated to the Zero Velocity Radius at 7.3 Mpc</title>
    <p>In the clipped text below, from <xref ref-type="bibr" rid="scirp.136741-9">
      [9]
     </xref> O. Kashibadze. 2020, the authors gives the interval for [7, 7.3] Mpc for the R<sub>ZV</sub>.</p>
    <p>rding DMbQG theory, the zero velocity radius R<sub>ZV</sub> =7.75 Mpc, see epigraph 5.3, so the relative difference is only 6%.</p>
    <p>This is a very good match between experimental results and theoretical results by DMbQG theory.</p>
    <p>Also at the concluding remarks from <xref ref-type="bibr" rid="scirp.136741-9">
      [9]
     </xref> O. Kashibadze.2020, the authors give for the total mass M<sub>T</sub> (&lt;R<sub>0</sub>) = (7.4 ± 0.9)·10<sup>14</sup> 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          Θ 
        </mi> 
       </msub> 
      </mrow> 
     </math>. As this value is got by dynamical measures in fact this value must be considered as gravitational mass.</p>
    <p>The theoretical value (5.12) calculated in epigraph 5.5 is M<sub>G</sub> (&lt;R<sub>ZV</sub>) ≈1.5·M<sub>VIR</sub> = 9.48E14 
     <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          Θ 
        </mi> 
       </msub> 
      </mrow> 
     </math> which is 14 % bigger regarding the value given by the authors, if it is considered the upper value of the interval. So both results may be considered compatibles.</p>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="custom-bottom-td acenter" width="100.00%"><p style="text-align:center">Clipped text of <xref ref-type="bibr" rid="scirp.136741-9">
         [9]
        </xref> O. Kashibadze. 2020</p></td> 
     </tr> 
     <tr> 
      <td class="custom-top-td aleft" width="100.00%"><p style="text-align:left">7. Concluding remarks</p><p style="text-align:left">The analysis of galaxy motions in the outskirts of the Virgo cluster makes it possible to measure the radius of the zero velocity surface, Ro = 7 - 7.3 Mpc (Karachentsev et al. 2014, Shaya et al. 2017, Kashibadze et al. 2018) corresponding to the total mass of the Virgo cluster M<sub>T</sub> = (7.4 ± 0.9) × 10<sup>14</sup> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             Θ 
           </mi> 
          </msub> 
         </mrow> 
        </math> inside the Ro. The numerical simulated trajectories of nearby galaxies with accurate distance estimates performed by Shaya et al. (2017) confirmed the obtained estimate of the total mass of the cluster. The virial mass of the cluster, being determined independently at the scale Rg = 1.7 Mpc from the internal motions, is nearly the same M<sub>VIR</sub> (6.3 ± 0.9) × 10<sup>14</sup> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             Θ 
           </mi> 
          </msub> 
         </mrow> 
        </math>.</p></td> 
     </tr> 
    </table>
    <p>
     <xref ref-type="table" rid="table10">
      Table 10
     </xref> summarized and compared the observational results and theoretical results.</p>
    <table-wrap id="table10">
     <label>
      <xref ref-type="table" rid="table10">
       Table 10
      </xref></label>
     <caption>
      <title>
       <xref ref-type="bibr" rid="scirp.136741-"></xref>Table 10. Virgo cluster.</title>
     </caption>
     <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
      <tr> 
       <td class="custom-bottom-td acenter" width="20.87%"><p style="text-align:center"></p></td> 
       <td class="custom-bottom-td acenter" width="29.93%"><p style="text-align:center">
         <xref ref-type="bibr" rid="scirp.136741-9">
          [9]
         </xref> O. Kashibadze</p></td> 
       <td class="custom-bottom-td acenter" width="34.19%"><p style="text-align:center">DMbG theory</p></td> 
       <td class="custom-bottom-td acenter" width="23.50%"><p style="text-align:center">Relative</p><p style="text-align:center">difference</p></td> 
      </tr> 
      <tr> 
       <td class="custom-top-td acenter" width="20.87%"><p style="text-align:center">R<sub>ZV</sub></p></td> 
       <td class="custom-top-td acenter" width="29.93%"><p style="text-align:center">[7, 7.3] Mpc</p></td> 
       <td class="custom-top-td acenter" width="34.19%"><p style="text-align:center">7.75 Mpc</p></td> 
       <td class="custom-top-td acenter" width="23.50%"><p style="text-align:center">6%—Very good</p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="20.87%"><p style="text-align:center">M<sub>VIR</sub></p></td> 
       <td class="acenter" width="29.93%"><p style="text-align:center">(6.3 <u>+</u> 0.9)·10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="acenter" width="34.19%"><p style="text-align:center"></p></td> 
       <td class="acenter" width="23.50%"><p style="text-align:center"></p></td> 
      </tr> 
      <tr> 
       <td class="acenter" width="20.87%"><p style="text-align:center">M<sub>G</sub> (&lt;R<sub>ZV</sub>)</p></td> 
       <td class="acenter" width="29.93%"><p style="text-align:center">(7.4 ± 0.9)·10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="acenter" width="34.19%"><p style="text-align:center">1.5·M<sub>VIR</sub> = 9.45·10<sup>14</sup> 
         <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
           <msub> 
            <mi>
              M 
            </mi> 
            <mi>
              Θ 
            </mi> 
           </msub> 
          </mrow> 
         </math></p></td> 
       <td class="acenter" width="23.50%"><p style="text-align:center">14%</p><p style="text-align:center">Compatibles</p></td> 
      </tr> 
     </table>
    </table-wrap>
   </sec>
   <sec id="s6_2">
    <title>6.2. Gravitating Mass Associated Up to the Twice of Virial Radius</title>
    <p>As R<sub>VIR</sub> = 1.7 Mpc its twice value is 3.4 Mpc. As R<sub>ZG</sub> = 12.9 Mpc then f = 3.4/12.9 = 0.2635 and by (4.21) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          G 
        </mi> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mn>
           2 
         </mn> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         1.335 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mtext> 
       </mtext> 
       <mn>
         8.4 
       </mn> 
       <mo>
         × 
       </mo> 
       <msup> 
        <mrow> 
         <mn>
           10 
         </mn> 
        </mrow> 
        <mrow> 
         <mn>
           14 
         </mn> 
        </mrow> 
       </msup> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          Θ 
        </mi> 
       </msub> 
      </mrow> 
     </math>.</p>
    <p>This value match perfectly with the interval of masses given below in the clipped text.</p>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="custom-bottom-td acenter" width="100.09%"><p style="text-align:center">Clipped text from page 9 of <xref ref-type="bibr" rid="scirp.136741-9">
         [9]
        </xref> O. Kashibadze.2020</p></td> 
     </tr> 
     <tr> 
      <td class="custom-top-td aleft" width="100.09%"><p style="text-align:left">The Plank collaboration (2016) performed a detailed study of the Virgo cluster through Sunyaev-Zeldovich effect and found the total mass of warm/hot gas to be (1.4 - 1.6) × 10<sup>14</sup> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             Θ 
           </mi> 
          </msub> 
         </mrow> 
        </math>. Assuming the cosmic value for the baryon fraction, 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             f 
           </mi> 
           <mi>
             b 
           </mi> 
          </msub> 
          <mtext>
              
          </mtext> 
          <mo>
            = 
          </mo> 
          <mtext>
              
          </mtext> 
          <mrow> 
           <mrow> 
            <msub> 
             <mi>
               Ω 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <msub> 
             <mi>
               Ω 
             </mi> 
             <mi>
               m 
             </mi> 
            </msub> 
           </mrow> 
          </mrow> 
          <mtext>
              
          </mtext> 
          <mtext>
              
          </mtext> 
          <mo>
            = 
          </mo> 
          <mn>
            0.1834 
          </mn> 
         </mrow> 
        </math>, they found that the total mass of the cluster would be (7.4 - 8.7) × 10<sup>14</sup> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             Θ 
           </mi> 
          </msub> 
         </mrow> 
        </math> on a scale up to 2 times larger than the virial radius.</p></td> 
     </tr> 
    </table>
    <p>The total mass mentioned in Kashibadze paper it is considered in this paper as gravitating mass because in the whole paper of Kashibadze et al. they use always the concept of total mass as a result of dynamical measures so it is more suitable to interpret his total mass as gravitating mass.</p>
    <p>Anyway, considering the total mass given by the formula (4.16) then</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mn>
           2 
         </mn> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         1.386 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mn>
         8.73 
       </mn> 
       <mo>
         × 
       </mo> 
       <msup> 
        <mrow> 
         <mn>
           10 
         </mn> 
        </mrow> 
        <mrow> 
         <mn>
           14 
         </mn> 
        </mrow> 
       </msup> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mi>
          Θ 
        </mi> 
       </msub> 
      </mrow> 
     </math> that match with the upper value of mass range given by the authors.</p>
   </sec>
   <sec id="s6_3">
    <title>6.3. Solving the Conundrum: The Local Density Matter versus the Global Density Matter</title>
    <p>Below is the clipped text of a paper published for a team of well known astrophysicist.</p>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="custom-bottom-td acenter" width="100.09%"><p style="text-align:center">Clipped text from introduction of paper <xref ref-type="bibr" rid="scirp.136741-6">
         [6]
        </xref> Karachentsev I. D., R. Brent Tully. 2014</p></td> 
     </tr> 
     <tr> 
      <td class="custom-top-td aleft" width="100.09%"><p style="text-align:left">As it has been noted by different authors (Vennik, 1984, Tully, 1987, Crook et al. 2007, Makarov &amp; Karachentsev, 2011, Karachentsev, 2012), the total virial masses of nearby groups and clusters leads to a mean local density of matter 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             Ω 
           </mi> 
           <mi>
             m 
           </mi> 
          </msub> 
          <mo>
            ≈ 
          </mo> 
          <mn>
            0.8 
          </mn> 
         </mrow> 
        </math>, that is 1/3 the mean global density 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             Ω 
           </mi> 
           <mi>
             m 
           </mi> 
          </msub> 
          <mo>
            ≈ 
          </mo> 
          <mn>
            0.24 
          </mn> 
          <mo>
            ± 
          </mo> 
          <mn>
            0.03 
          </mn> 
         </mrow> 
        </math> (Spergel et al., 2007). One possible explanation of the disparity between the local and global density estimates may be that the outskirts of groups and clusters contain significant amount of dark matter beyond their virial radii, beyond what is anticipated from the integrated light of galaxies within the infall domain. If so, to get agreement between local and global values of 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             Ω 
           </mi> 
           <mi>
             m 
           </mi> 
          </msub> 
         </mrow> 
        </math>, the total mass of the Virgo cluster (and other clusters) must be 3 times their virial masses.</p></td> 
     </tr> 
    </table>
    <p>In page 3 of that paper, they state that at the nearby clusters the mean local density of matter is 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           c 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.08 
       </mn> 
      </mrow> 
     </math>, whereas the global mass density in the Universe is 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           b 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.24 
       </mn> 
      </mrow> 
     </math> (data year 2007).</p>
    <p>Currently that data updated for scientific community is 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           b 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.3 
       </mn> 
      </mrow> 
     </math>.</p>
    <p>The authors suggest that a possible solution for this tension would be that the total mass for cluster haloes must be three times the virial mass. That is justly what is found in this paper studying the DM at cluster scale as universal law in the framework of DMbQG theory.</p>
    <p>In chapter 4, the formula (4.13) 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mtext>
           
       </mtext> 
       <mfrac> 
        <mrow> 
         <mroot> 
          <mrow> 
           <mn>
             100 
           </mn> 
          </mrow> 
          <mn>
            5 
          </mn> 
         </mroot> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             5 
           </mn> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
       <mo>
         = 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>,</p>
    <p>shows that the total mass (baryonic and DM) enclosed into the halo cluster is U ≈ 2.7 times the virial mass equal to 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             V 
           </mi> 
           <mi>
             I 
           </mi> 
           <mi>
             R 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo> 
       </mo> 
       <mo>
         ≈ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mn>
           200 
         </mn> 
        </mrow> 
       </msub> 
      </mrow> 
     </math>.</p>
    <p>However in the epigraph 4.9 has been calculated an extension of the halo cluster</p>
    <p>up to radius R<sub>E</sub> = 1.85·R<sub>ZG</sub> to obtain a ratio 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mfrac> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             T 
           </mi> 
           <mi>
             M 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             L 
           </mi> 
           <mi>
             O 
           </mi> 
           <mi>
             C 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msubsup> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             L 
           </mi> 
           <mi>
             O 
           </mi> 
           <mi>
             C 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mfrac> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             T 
           </mi> 
           <mi>
             M 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mi>
             L 
           </mi> 
           <mi>
             O 
           </mi> 
           <mi>
             B 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msubsup> 
        </mrow> 
        <mrow> 
         <msubsup> 
          <mi>
            Ω 
          </mi> 
          <mrow> 
           <mi>
             D 
           </mi> 
           <mi>
             E 
           </mi> 
          </mrow> 
          <mrow> 
           <mi>
             G 
           </mi> 
           <mi>
             L 
           </mi> 
           <mi>
             O 
           </mi> 
           <mi>
             B 
           </mi> 
           <mi>
             A 
           </mi> 
           <mi>
             L 
           </mi> 
          </mrow> 
         </msubsup> 
        </mrow> 
       </mfrac> 
       <mo>
         = 
       </mo> 
       <mrow> 
        <mn>
          3 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          7 
        </mn> 
       </mrow> 
      </mrow> 
     </math>. Now using the formula (4.16) it is right to calculate the total mass enclosed by such sphere 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mi>
            E 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <mi>
           f 
         </mi> 
         <mo>
           ⋅ 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mrow> 
           <mi>
             Z 
           </mi> 
           <mi>
             G 
           </mi> 
          </mrow> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <msqrt> 
        <mi>
          f 
        </mi> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> being f = 1.85 and the factor 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msqrt> 
        <mi>
          f 
        </mi> 
       </msqrt> 
       <mo>
         ⋅ 
       </mo> 
       <mi>
         U 
       </mi> 
       <mo>
         = 
       </mo> 
       <mn>
         3.67 
       </mn> 
      </mrow> 
     </math></p>
    <p>then</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mo> 
       </mo> 
       <mo> 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           T 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           T 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msub> 
       <mrow> 
        <mo>
          ( 
        </mo> 
        <mrow> 
         <mo>
           &lt; 
         </mo> 
         <msub> 
          <mi>
            R 
          </mi> 
          <mi>
            E 
          </mi> 
         </msub> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
       <mo>
         = 
       </mo> 
       <mn>
         3.67 
       </mn> 
       <mo>
         ⋅ 
       </mo> 
       <msub> 
        <mi>
          M 
        </mi> 
        <mrow> 
         <mi>
           V 
         </mi> 
         <mi>
           I 
         </mi> 
         <mi>
           R 
         </mi> 
        </mrow> 
       </msub> 
      </mrow> 
     </math> (6.1)</p>
    <p>Therefore with such factor the parameter 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           c 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.08 
       </mn> 
      </mrow> 
     </math> is increased up to a</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           c 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.08 
       </mn> 
       <mo>
         × 
       </mo> 
       <mn>
         3.67 
       </mn> 
       <mo>
         = 
       </mo> 
       <mn>
         0.2936 
       </mn> 
      </mrow> 
     </math> (6.2)</p>
    <p>because according <xref ref-type="bibr" rid="scirp.136741-6">
      [6]
     </xref> Karachentsev et al. 2014, the coefficient 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           c 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.08 
       </mn> 
      </mrow> 
     </math> is calculated considering the virial masses of clusters into the Local Universe, and as according DMbQG such total mass is increased by the factor 3.67 if it is considered an extended halo with radius R<sub>E</sub> = 1.85·R<sub>ZG</sub> then the coefficient 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           c 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.08 
       </mn> 
       <mo>
         × 
       </mo> 
       <mn>
         3.67 
       </mn> 
       <mo>
         = 
       </mo> 
       <mn>
         0.293 
       </mn> 
      </mrow> 
     </math> match perfectly with 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           g 
         </mi> 
         <mi>
           l 
         </mi> 
         <mi>
           o 
         </mi> 
         <mi>
           b 
         </mi> 
         <mi>
           a 
         </mi> 
         <mi>
           l 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.3 
       </mn> 
      </mrow> 
     </math>.</p>
    <p>This result enables an experimental test to validate these theoretical findings: If at the present Universe, the average distance between clusters is about its R<sub>E</sub> associated to each one, then the DMbQG theory would explain the current 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mi>
           L 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           B 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <mn>
         0.3 
       </mn> 
      </mrow> 
     </math>.</p>
    <p>In other words, considering that almost the total baryonic matter at the current Universe is enclosed inside the virial radius of the clusters, as it is confirmed by multiples measures, the DMbQG is able to justify that 
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           L 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           C 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msubsup> 
       <mo>
         = 
       </mo> 
       <msubsup> 
        <mi>
          Ω 
        </mi> 
        <mi>
          m 
        </mi> 
        <mrow> 
         <mi>
           G 
         </mi> 
         <mi>
           L 
         </mi> 
         <mi>
           O 
         </mi> 
         <mi>
           B 
         </mi> 
         <mi>
           A 
         </mi> 
         <mi>
           L 
         </mi> 
        </mrow> 
       </msubsup> 
      </mrow> 
     </math> on condition that the average distance between clusters is the extended radius R<sub>E</sub>.</p>
   </sec>
  </sec><sec id="s7">
   <title>7. Concluding Remarks</title>
   <p>Thanks direct mass 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          D 
        </mi> 
        <mi>
          I 
        </mi> 
        <mi>
          R 
        </mi> 
        <mi>
          E 
        </mi> 
        <mi>
          C 
        </mi> 
        <mi>
          T 
        </mi> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mo>
          &lt; 
        </mo> 
        <mi>
          r 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          ⋅ 
        </mo> 
        <msqrt> 
         <mi>
           r 
         </mi> 
        </msqrt> 
       </mrow> 
       <mi>
         G 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> (3.1) and using the approximation of virial mass for M<sub>200</sub> and the virial radius for R<sub>200</sub> it is possible to get the formula 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mi>
         a 
       </mi> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            G 
          </mi> 
          <mo>
            ⋅ 
          </mo> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mrow> 
            <mi>
              V 
            </mi> 
            <mi>
              I 
            </mi> 
            <mi>
              R 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          5 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          6 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            10 
          </mn> 
          <mo>
            ⋅ 
          </mo> 
          <mi>
            H 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (3.4).</p>
   <p>In chapter 3, the direct mass has been extended to clusters, and it is possible to state that all the new theoretical results obtained in this paper are based on this formula, co working with the well known properties of DE.</p>
   <p>The main results got in this paper are summarized below.</p>
   <p>A) The universality of ratio R<sub>ZG</sub>/R<sub>VIR</sub> ≈ 7.3 (4.10) and its total mass associated, being M<sub>TOTAL</sub> (&lt;R<sub>ZG</sub>) ≈ 2.7 M<sub>VIR</sub> (4.15).</p>
   <p>B) For any cluster at 0.488 R<sub>ZG</sub> (4.22) is reached the maximum of gravitating mass and M<sub>G</sub> (&lt;R<sub>M</sub>) ≈ 1.57·M<sub>VIR</sub> (4.23).</p>
   <p>C) The universality of the ratio R<sub>ZV</sub>/R<sub>ZG</sub> ≈ 0.602 (5.15) and its gravitating mass M<sub>G</sub> (&lt;R<sub>ZV</sub>) ≈ 1.5 M<sub>VIR</sub> (5.16).</p>
   <p>D) The universality of the ratio R<sub>E</sub>/R<sub>ZG</sub> ≈ 1.85, (4.29) where the ratio total mass density versus DE density is 3/7 and its total mass 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          T 
        </mi> 
        <mi>
          O 
        </mi> 
        <mi>
          T 
        </mi> 
        <mi>
          A 
        </mi> 
        <mi>
          L 
        </mi> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mo>
          &lt; 
        </mo> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           E 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mn>
        3.67 
      </mn> 
      <mo>
        ⋅ 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mrow> 
        <mi>
          V 
        </mi> 
        <mi>
          I 
        </mi> 
        <mi>
          R 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> (4.31).</p>
   <p>Finally in chapter 6, some results published about Virgo cluster are introduced that back fully the previous theoretical findings:</p>
   <p>1) Regarding the property D) may be consulted <xref ref-type="bibr" rid="scirp.136741-6">
     [6]
    </xref> Karachentsev I. D., R. Brent Tully 2014 to understand more in deep the current tension between the low value for Local mass density parameter 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Ω 
       </mi> 
       <mi>
         m 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.08 
      </mn> 
     </mrow> 
    </math> and the current global matter density parameter 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Ω 
       </mi> 
       <mi>
         m 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        0.3 
      </mn> 
     </mrow> 
    </math>.</p>
   <p>2) Calculus of the zero velocity radius and its associated gravitating mass of Virgo are compatibles with the result published by <xref ref-type="bibr" rid="scirp.136741-9">
     [9]
    </xref> Olga Kashibadze et al. 2020, see epigraph 6.1.</p>
   <p>3) Calculus of the mass gravitating at two times the virial radius match fully with the result published by <xref ref-type="bibr" rid="scirp.136741-9">
     [9]
    </xref> Olga Kashibadze et al. 2020, see epigraph 6.2.</p>
   <p>These new theoretical findings offer to scientific community a number of tests to validate the theory. The validation of DMbQG theory would suggest that DM is a quantum gravitation effect, see <xref ref-type="bibr" rid="scirp.136741-4">
     [4]
    </xref> Corda 2012, see <xref ref-type="bibr" rid="scirp.136741-10">
     [10]
    </xref> Corda 2018 and see <xref ref-type="bibr" rid="scirp.136741-11">
     [11]
    </xref> Abarca 2014, giving to scientific community new elements to continue searching a quantum gravitation theory.</p>
  </sec>
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