<?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">
    jmp
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of Modern Physics
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2153-1196
   </issn>
   <issn publication-format="print">
    2153-120X
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jmp.2024.1511075
   </article-id>
   <article-id pub-id-type="publisher-id">
    jmp-136677
   </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>
    Predicting High Precision Hubble Constant Determinations Based on a New Theoretical Relationship between CMB Temperature and H
    <sub>0</sub>
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Eugene Terry
      </surname>
      <given-names>
       Tatum
      </given-names>
     </name> 
     <xref ref-type="aff" rid="aff1"> 
      <sup>1</sup>
     </xref>
    </contrib>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Espen Gaarder
      </surname>
      <given-names>
       Haug
      </given-names>
     </name> 
     <xref ref-type="aff" rid="aff2"> 
      <sup>2</sup>
     </xref>
    </contrib>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Stéphane
      </surname>
      <given-names>
       Wojnow
      </given-names>
     </name> 
     <xref ref-type="aff" rid="aff3"> 
      <sup>3</sup>
     </xref>
    </contrib>
   </contrib-group> 
   <aff id="aff1">
    <addr-line>
     aBowling Green, KY, USA
    </addr-line> 
   </aff> 
   <aff id="aff2">
    <addr-line>
     aNorwegian University of Life Sciences, Ås, Norway
    </addr-line> 
   </aff> 
   <aff id="aff3">
    <addr-line>
     aLimoges, France
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     30
    </day> 
    <month>
     09
    </month>
    <year>
     2024
    </year>
   </pub-date> 
   <volume>
    15
   </volume> 
   <issue>
    11
   </issue>
   <fpage>
    1708
   </fpage>
   <lpage>
    1716
   </lpage>
   <history>
    <date date-type="received">
     <day>
      6,
     </day>
     <month>
      September
     </month>
     <year>
      2024
     </year>
    </date>
    <date date-type="published">
     <day>
      15,
     </day>
     <month>
      September
     </month>
     <year>
      2024
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      15,
     </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>
    Based on considerable progress made in understanding the Cosmic Microwave Background (CMB) temperature from a deep theoretical perspective, this paper demonstrates a useful and simple relationship between the CMB temperature and the Hubble constant. This allows us to predict the Hubble constant with much higher precision than before by using the CMB temperature. This is of great importance, since it will lead to much higher precision in various global parameters of the cosmos, such as the Hubble radius and the age of the universe. We have improved uncertainty in the Hubble constant all the way down to 66.8712 ± 0.0019 km/s/Mpc based on data from one of the most recent CMB studies. Previous studies based on other methods have rarely reported an uncertainty much less than approximately ±1 km/s/Mpc for the Hubble constant. Our deeper understanding of the CMB and its relation to 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        H
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
     </mrow> 
    </math> seems to be opening a new era of high-precision cosmology, which may well be the key to solving the Hubble tension, as alluded to herein. Naturally, our results should also be scrutinized by other researchers over time, but we believe that, even at this stage, this deeper understanding of the CMB deserves attention from the research community.
   </abstract>
   <kwd-group> 
    <kwd>
     Hubble Constant
    </kwd> 
    <kwd>
      CMB
    </kwd> 
    <kwd>
      Planck Temperature
    </kwd> 
    <kwd>
      Upsilon Constant
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>
    <xref ref-type="bibr" rid="scirp.136677-"></xref>1. Introduction: Hubble Constant from CMB Temperature</title>
   <p>This paper is motivated by very recent developments in theoretical cosmology, specifically where it concerns new cosmological models. For example, in 2015, Tatum et al. <xref ref-type="bibr" rid="scirp.136677-1">
     [1]
    </xref> offered their own model, including its formula for the cosmic temperature in the following form:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          ℏ 
        </mi> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
        </msub> 
        <mn>
          8 
        </mn> 
        <mi>
          π 
        </mi> 
        <mi>
          G 
        </mi> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             M 
           </mi> 
           <mi>
             c 
           </mi> 
          </msub> 
          <msub> 
           <mi>
             m 
           </mi> 
           <mi>
             p 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (1)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the Hubble temperature, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the Boltzmann constant, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ℏ 
     </mi> 
    </math> is the reduced Planck constant, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       c 
     </mi> 
    </math> is the speed of light, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math> is the gravitational constant, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the Planck mass and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         c 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the critical mass in the Friedmann <xref ref-type="bibr" rid="scirp.136677-2">
     [2]
    </xref> equation 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         c 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          G 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> that also is part of Einstein’s <xref ref-type="bibr" rid="scirp.136677-3">
     [3]
    </xref> general relativity and theΛ-CDM cosmological model, as well as other lesser-known cosmological models. Equation (1) was initially investigated heuristically as many good ideas often start out; however, a more solid foundation must be established over time. A derivation of Equation (1) based on the Stefan-Boltzmann law has just been published <xref ref-type="bibr" rid="scirp.136677-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.136677-5">
     [5]
    </xref> and clearly shows that the formula is valid within thermodynamics and general relativity theory. Whether our way to predict the Hubble constant can be incorporated into the Λ-CDM model should be the subject of future investigation.</p>
   <p>However, it is also important to investigate its predictive capacity for different so-called 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         h 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> cosmological models <xref ref-type="bibr" rid="scirp.136677-6">
     [6]
    </xref>-<xref ref-type="bibr" rid="scirp.136677-11">
     [11]
    </xref> that are consistent with general relativity theory, including growing black hole models. Equation (1) was introduced in Tatum et al.’s growing black hole 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         h 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> cosmological model. Such cosmological models are actively discussed to this day; see, for example <xref ref-type="bibr" rid="scirp.136677-12">
     [12]
    </xref>-<xref ref-type="bibr" rid="scirp.136677-16">
     [16]
    </xref>. We are pointing this out because it is too early to say which cosmological models will ultimately be found consistent with this way to predict the Hubble constant and which ones will not. The most important point in this article is that our proposed mathematical relationship between the Hubble constant and the CMB temperature should lead to much lower uncertainty in Hubble constant determinations based on measurement of the CMB temperature. This approach might also improve the prediction of how the CMB temperature evolved in the past, such as the exact time of the decoupling of the CMB. However, correlation with past cosmic epochs is outside the scope of this paper.</p>
   <p>The formula above can also be expressed as:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          C 
        </mi> 
        <mi>
          M 
        </mi> 
        <mi>
          B 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          8 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <msub> 
           <mi>
             l 
           </mi> 
           <mi>
             p 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <msub> 
             <mi>
               H 
             </mi> 
             <mn>
               0 
             </mn> 
            </msub> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          8 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <msub> 
           <mi>
             l 
           </mi> 
           <mi>
             p 
           </mi> 
          </msub> 
          <msub> 
           <mi>
             H 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
         <mi>
           c 
         </mi> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> (2)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          C 
        </mi> 
        <mi>
          M 
        </mi> 
        <mi>
          B 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is the CMB temperature, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is the Hubble radius, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> is the Hubble constant, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       c 
     </mi> 
    </math> is the speed of light, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the Planck <xref ref-type="bibr" rid="scirp.136677-17">
     [17]
    </xref> temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         l 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the Planck length. Equations (1) and (2) are just two ways to write the same formula, so we can start with either of these and solve for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. Solving for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> gives:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            C 
          </mi> 
          <mi>
            M 
          </mi> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           p 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
      </mfrac> 
      <mfrac> 
       <mrow> 
        <mn>
          64 
        </mn> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <msub> 
         <mi>
           l 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (3)</p>
   <p>And since the Planck length 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         l 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mi>
            G 
          </mi> 
          <mi>
            ℏ 
          </mi> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             3 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mi>
            ℏ 
          </mi> 
          <msup> 
           <mi>
             c 
           </mi> 
           <mn>
             5 
           </mn> 
          </msup> 
         </mrow> 
         <mi>
           G 
         </mi> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>, if we insert that into Equation (3), we get:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            C 
          </mi> 
          <mi>
            M 
          </mi> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mn>
               1 
             </mn> 
             <mrow> 
              <msub> 
               <mi>
                 k 
               </mi> 
               <mi>
                 b 
               </mi> 
              </msub> 
             </mrow> 
            </mfrac> 
            <msqrt> 
             <mrow> 
              <mfrac> 
               <mrow> 
                <mi>
                  ℏ 
                </mi> 
                <msup> 
                 <mi>
                   c 
                 </mi> 
                 <mn>
                   5 
                 </mn> 
                </msup> 
               </mrow> 
               <mi>
                 G 
               </mi> 
              </mfrac> 
             </mrow> 
            </msqrt> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mfrac> 
       <mrow> 
        <mn>
          64 
        </mn> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              G 
            </mi> 
            <mi>
              ℏ 
            </mi> 
           </mrow> 
           <mrow> 
            <msup> 
             <mi>
               c 
             </mi> 
             <mn>
               3 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            C 
          </mi> 
          <mi>
            M 
          </mi> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mn>
               1 
             </mn> 
             <mrow> 
              <msub> 
               <mi>
                 k 
               </mi> 
               <mi>
                 b 
               </mi> 
              </msub> 
             </mrow> 
            </mfrac> 
            <mi>
              c 
            </mi> 
            <mi>
              ℏ 
            </mi> 
            <msqrt> 
             <mrow> 
              <mfrac> 
               <mrow> 
                <msup> 
                 <mi>
                   c 
                 </mi> 
                 <mn>
                   3 
                 </mn> 
                </msup> 
               </mrow> 
               <mrow> 
                <mi>
                  ℏ 
                </mi> 
                <mi>
                  G 
                </mi> 
               </mrow> 
              </mfrac> 
             </mrow> 
            </msqrt> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mfrac> 
       <mrow> 
        <mn>
          32 
        </mn> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              G 
            </mi> 
            <mi>
              ℏ 
            </mi> 
           </mrow> 
           <mrow> 
            <msup> 
             <mi>
               c 
             </mi> 
             <mn>
               3 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mrow> 
          <mi>
            C 
          </mi> 
          <mi>
            M 
          </mi> 
          <mi>
            B 
          </mi> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msubsup> 
        <msubsup> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
        <mn>
          32 
        </mn> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mi>
          ℏ 
        </mi> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <msup> 
             <mi>
               c 
             </mi> 
             <mn>
               3 
             </mn> 
            </msup> 
            <mi>
              ℏ 
            </mi> 
           </mrow> 
           <mi>
             G 
           </mi> 
          </mfrac> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (4)</p>
   <p>In the equation above, we can even separate out the part only containing constants:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
        <mn>
          32 
        </mn> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mi>
          ℏ 
        </mi> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <msup> 
             <mi>
               c 
             </mi> 
             <mn>
               3 
             </mn> 
            </msup> 
            <mi>
              ℏ 
            </mi> 
           </mrow> 
           <mi>
             G 
           </mi> 
          </mfrac> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
        <mn>
          32 
        </mn> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <msup> 
         <mi>
           G 
         </mi> 
         <mrow> 
          <mrow> 
           <mn>
             1 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mrow> 
          <mrow> 
           <mn>
             5 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
        <msup> 
         <mi>
           ℏ 
         </mi> 
         <mrow> 
          <mrow> 
           <mn>
             3 
           </mn> 
           <mo>
             / 
           </mo> 
           <mn>
             2 
           </mn> 
          </mrow> 
         </mrow> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        2.91845601 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          19 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.00003279 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          19 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         K 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (5)</p>
   <p>And we could call this composite constant Upsilon: ϑ (Latin version of Upsilon). The uncertainty in Upsilon only comes from the uncertainty in 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        G 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        6.67430 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          11 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.00015 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          15 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <msup> 
       <mtext>
         m 
       </mtext> 
       <mn>
         3 
       </mn> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mrow> 
        <mtext>
          kg 
        </mtext> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          2 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, as all other constants in the composite constant are defined exactly in NIST CODATA 2018. The relation between the Hubble constant and the CMB temperature is, therefore, just a composite constant multiplied by the CMB temperature squared:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        ℧ 
      </mi> 
      <msubsup> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          C 
        </mi> 
        <mi>
          M 
        </mi> 
        <mi>
          B 
        </mi> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msubsup> 
     </mrow> 
    </math> (6)</p>
   <p>Still, naturally, part of this Upsilon composite constant contains 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>, and we would still naturally need to take into account uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>, as well as the uncertainty in the CMB temperature when finding the uncertainty in the Hubble constant from this method, so the uncertainty will be the same as we will get from Equation (4), as will be explored in the next section.</p>
   <p>To summarize this section, all of the above formulae are effectively produced by different substitutions and rearrangements of Equation (1). The results are the same with respect to calculating the value and precision of the Hubble constant for a given CMB temperature value <xref ref-type="bibr" rid="scirp.136677-18">
     [18]
    </xref>. In the next section, we will demonstrate that this formula is not only of theoretical interest to describe the relationship between the Hubble constant and the CMB temperature, but that it surprisingly leads to much higher precision in Hubble constant predictions after properly accounting for the full uncertainty in all input parameters.</p>
  </sec><sec id="s2">
   <title>
    <xref ref-type="bibr" rid="scirp.136677-"></xref>2. High Precision Hubble Constant</title>
   <p>Since the discoveries by Lemaître <xref ref-type="bibr" rid="scirp.136677-19">
     [19]
    </xref> and Hubble <xref ref-type="bibr" rid="scirp.136677-20">
     [20]
    </xref>, extensive observational studies have been ongoing for many decades in order to increase the precision in the Hubble constant, something that is of great importance for a more precise understanding of the cosmos. See, for example <xref ref-type="bibr" rid="scirp.136677-21">
     [21]
    </xref>-<xref ref-type="bibr" rid="scirp.136677-30">
     [30]
    </xref>. Even the more precise of these studies have not much less than 1 standard deviation uncertainty in their measured or estimated Hubble constant values in units of 1 km/s/Mpc.</p>
   <p>In our formulae, we are using the NIST CODATA (2018) value for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>, which is 6.67430 × 10<sup>−</sup><sup>11</sup> ± 0.00015 × 10<sup>−</sup><sup>11</sup> m<sup>3</sup>·kg<sup>−</sup><sup>1</sup>·s<sup>−</sup><sup>2</sup>. Therefore, we are fully accounting for the uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>. Additionally, we consider the uncertainty in CMB temperature as provided in the respective studies we represent in <xref ref-type="table" rid="table1">
     Table 1
    </xref>. The speed of light 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        c 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        299792458 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         s 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, the reduced Planck constant (also known as the Dirac constant) 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ℏ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         h 
       </mi> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          π 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        1.054571817 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          34 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        J 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <mtext>
        s 
      </mtext> 
     </mrow> 
    </math> and the Boltzmann constant 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        1.380649 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          23 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        J 
      </mtext> 
      <mo>
        ⋅ 
      </mo> 
      <msup> 
       <mtext>
         K 
       </mtext> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> that we need as inputs have no uncertainty, as they are exactly defined according to NIST 2018 CODATA. This approach allows us to incorporate the complete input uncertainty into predicting 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>To convert our value into units km/s/Mpc, we use the resolution B2 adopted at the 2015 General Assembly of the International Astronomical Union (IAU), where the parsec is defined as exactly 648,000/π astronomical units, and for AU, we use 149,597,870,700 m (IAU 2012 Resolution B1). So, the conversion factor we need to multiply the results from our formula is the product of 1000 × 648,000/π × 149,597,870,700 km/Mpc. There is no uncertainty in these conversion numbers, since they are merely conversion factors that are exactly defined.</p>
   <p>For example, from the recent Dhal et al.’s <xref ref-type="bibr" rid="scirp.136677-31">
     [31]
    </xref> CMB study, we obtain a value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        66.8712 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.0019 
      </mn> 
     </mrow> 
    </math> km/s/Mpc. This uncertainty of ±0.0019 km/s/Mpc represents one standard deviation. Compared to other published methods and studies, our Equations (4) and (6) provide for dramatically improved precision. We do not know of a previous study with much less than about 1 standard deviation below 1 km/s/Mpc. This breakthrough lies in a much deeper understanding of the relationship between the CMB temperature and the Hubble constant. <xref ref-type="table" rid="table1">
     Table 1
    </xref> displays Hubble constant values ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>) estimated from a series of different CMB studies, but using our new high-precision method to determine 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> while accounting for the full uncertainty in the input parameters.</p>
   <table-wrap id="table1">
    <label>
     <xref ref-type="table" rid="table1">
      Table 1
     </xref></label>
    <caption>
     <title>
      <xref ref-type="bibr" rid="scirp.136677-"></xref>Table 1. This table shows Hubble constant estimates using our new calculation method from several different CMB studies.</title>
    </caption>
    <table class="MsoTableGrid custom-table" border="0" cellspacing="0" cellpadding="0"> 
     <tr> 
      <td class="custom-bottom-td acenter" width="25.86%"><p style="text-align:center">CMB Study</p></td> 
      <td class="custom-bottom-td acenter" width="32.34%"><p style="text-align:center">Temperature Measurement</p></td> 
      <td class="custom-bottom-td acenter" width="41.80%"><p style="text-align:center">High-Precision Method for 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             H 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
        </math></p></td> 
     </tr> 
     <tr> 
      <td class="custom-top-td aleft" width="25.86%"><p style="text-align:left">Dhal et al. <xref ref-type="bibr" rid="scirp.136677-31">
         [31]
        </xref></p></td> 
      <td class="custom-top-td acenter" width="32.34%"><p style="text-align:center">2.725007 ± 0.000024K</p></td> 
      <td class="custom-top-td acenter" width="41.80%"><p style="text-align:center"> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             H 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mn>
            66.8712 
          </mn> 
          <mo>
            ± 
          </mo> 
          <mn>
            0.0019 
          </mn> 
          <mtext>
              
          </mtext> 
          <mrow> 
           <mrow> 
            <mrow> 
             <mrow> 
              <mtext>
                km 
              </mtext> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mtext>
               s 
             </mtext> 
            </mrow> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              Mpc 
            </mtext> 
           </mrow> 
          </mrow> 
         </mrow> 
        </math></p></td> 
     </tr> 
     <tr> 
      <td class="aleft" width="25.86%"><p style="text-align:left">Noterdaeme et al. <xref ref-type="bibr" rid="scirp.136677-32">
         [32]
        </xref></p></td> 
      <td class="acenter" width="32.34%"><p style="text-align:center">2.725 ± 0.002K</p></td> 
      <td class="acenter" width="41.80%"><p style="text-align:center"> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             H 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mn>
            66.8708 
          </mn> 
          <mo>
            ± 
          </mo> 
          <mn>
            0.0989 
          </mn> 
          <mtext>
              
          </mtext> 
          <mrow> 
           <mrow> 
            <mrow> 
             <mrow> 
              <mtext>
                km 
              </mtext> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mtext>
               s 
             </mtext> 
            </mrow> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              Mpc 
            </mtext> 
           </mrow> 
          </mrow> 
         </mrow> 
        </math></p></td> 
     </tr> 
     <tr> 
      <td class="aleft" width="25.86%"><p style="text-align:left">Fixsen et al. <xref ref-type="bibr" rid="scirp.136677-33">
         [33]
        </xref></p></td> 
      <td class="acenter" width="32.34%"><p style="text-align:center">2.72548 ± 0.00057K</p></td> 
      <td class="acenter" width="41.80%"><p style="text-align:center"> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             H 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mn>
            66.8944 
          </mn> 
          <mo>
            ± 
          </mo> 
          <mn>
            0.0287 
          </mn> 
          <mtext>
              
          </mtext> 
          <mrow> 
           <mrow> 
            <mrow> 
             <mrow> 
              <mtext>
                km 
              </mtext> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mtext>
               s 
             </mtext> 
            </mrow> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              Mpc 
            </mtext> 
           </mrow> 
          </mrow> 
         </mrow> 
        </math></p></td> 
     </tr> 
     <tr> 
      <td class="aleft" width="25.86%"><p style="text-align:left">Fixsen et al. <xref ref-type="bibr" rid="scirp.136677-34">
         [34]
        </xref></p></td> 
      <td class="acenter" width="32.34%"><p style="text-align:center">2.721 ± 0.010K</p></td> 
      <td class="acenter" width="41.80%"><p style="text-align:center"> 
        <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
          <msub> 
           <mi>
             H 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
          <mo>
            = 
          </mo> 
          <mn>
            66.68 
          </mn> 
          <mo>
            ± 
          </mo> 
          <mn>
            0.49 
          </mn> 
          <mtext>
              
          </mtext> 
          <mrow> 
           <mrow> 
            <mrow> 
             <mrow> 
              <mtext>
                km 
              </mtext> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mtext>
               s 
             </mtext> 
            </mrow> 
           </mrow> 
           <mo>
             / 
           </mo> 
           <mrow> 
            <mtext>
              Mpc 
            </mtext> 
           </mrow> 
          </mrow> 
         </mrow> 
        </math></p></td> 
     </tr> 
    </table>
   </table-wrap>
   <p>
    <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref> graphically illustrates the estimates provided in <xref ref-type="table" rid="table1">
     Table 1
    </xref>, along with error bars of 1 Standard Deviation (STD), using our new theoretical understanding of the precise relationship between the Cosmic Microwave Background (CMB) temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. The error bars in the most recent study by Dhal et al. <xref ref-type="bibr" rid="scirp.136677-31">
     [31]
    </xref> are so small that they are barely discernible on the graph, without significantly reducing the visibility of the observation points themselves. This is why we are confident enough to claim that this appears to be leading us into a new realm of high-precision cosmology. The improvement in precision is so dramatic that it is easy to think that it is too good to be true. We were initially skeptical as well, but have carefully retraced our steps, and it is clear that it is the newly established direct theoretical relationships between CMB temperature and the Hubble constant that make this possible. We naturally do not ask any researcher to take this for granted, but hope that more researchers will scrutinize this method carefully as well as determine its relevance with respect to the different cosmological models in the literature.</p>
   <p>
    <xref ref-type="bibr" rid="scirp.136677-"></xref></p>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>Figure 1. Hubble constant estimates from different CMB studies using new method.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/7505427-rId106.jpeg?20241018030846" />
   </fig>
   <p>An outstanding issue in relation to the Hubble constant is the Hubble tension, as discussed in, for example <xref ref-type="bibr" rid="scirp.136677-27">
     [27]
    </xref> <xref ref-type="bibr" rid="scirp.136677-35">
     [35]
    </xref> <xref ref-type="bibr" rid="scirp.136677-36">
     [36]
    </xref>. This tension results from markedly different Hubble constant measurements based on apparently conflicting early universe <xref ref-type="bibr" rid="scirp.136677-28">
     [28]
    </xref> and local universe <xref ref-type="bibr" rid="scirp.136677-26">
     [26]
    </xref> research studies. However, on the basis of the new theoretical relationship between the CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> introduced herein, we have recently published preprints <xref ref-type="bibr" rid="scirp.136677-37">
     [37]
    </xref> <xref ref-type="bibr" rid="scirp.136677-38">
     [38]
    </xref>, presently in the journal submission stage, in which we claim to have solved the Hubble tension in favor of the Planck Collaboration Hubble constant value. We believe that the basis for this longstanding tension hinges upon using the correct distance-vs-redshift formula appropriate for the original Tatum et al.’s growing black hole 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         h 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> cosmological model. We now refer to the model that uses such a distance-vs-redshift formula as the Haug-Tatum cosmological model, which can be explored by our readers in our highly detailed preprints referenced above. In addition, because the Haug-Tatum model naturally implies a cosmic age significantly greater than 13.8 billion years, we also refer readers to preprints that give a cosmic age value of approximately 14.622 billion years <xref ref-type="bibr" rid="scirp.136677-39">
     [39]
    </xref> <xref ref-type="bibr" rid="scirp.136677-40">
     [40]
    </xref>. This significantly longer cosmic time frame may well have important implications with respect to better understanding the surprisingly “early” galaxy structure formation recently observed in the early universe.</p>
  </sec><sec id="s3">
   <title>
    <xref ref-type="bibr" rid="scirp.136677-"></xref>3. High Precision Hubble Cosmology</title>
   <p>Due to a significantly higher precision in the determination of the Hubble constant, we can now predict various cosmological parameters that employ the Hubble constant, such as the Hubble time and the Hubble radius, with much greater accuracy than before. The Hubble radius, denoted as 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </msub> 
     </mrow> 
    </math>, is typically calculated using the formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>. Since there is no uncertainty in the speed of light 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       c 
     </mi> 
    </math>, the uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
     </mrow> 
    </math> is essentially the same as that in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. The Hubble time, defined as 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mi>
         h 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>, similarly benefits from the reduced uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. In addition, because of the linear nature of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         h 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> models, the concept of an accelerating dark energy is not relevant to the derivations of the key equations presented herein.</p>
   <p>In the context of the Λ-CDM model, the critical mass, denoted as 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         c 
       </mi> 
      </msub> 
     </mrow> 
    </math>, is calculated as 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         c 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          G 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>. Here, the uncertainty is slightly higher due to the additional factor of the gravitational constant 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>. Nonetheless, this method still provides significantly higher precision in such a model than any other approaches, thanks to the considerably reduced uncertainty in the Hubble constant value.</p>
  </sec><sec id="s4">
   <title>
    <xref ref-type="bibr" rid="scirp.136677-"></xref>4. Conclusion</title>
   <p>Any of our quantum cosmology formulae displayed in Section 1 can predict 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> with much higher precision than before due to a breakthrough in understanding the CMB temperature in relation to 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. Based on recent high-precision CMB temperature observations in combination with our new and deeper understanding of the relationship between CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, we obtain a 1 standard deviation uncertainty of no greater than ±0.49 km/s/Mpc, when using the 2004 data by Fixen et al. <xref ref-type="bibr" rid="scirp.136677-34">
     [34]
    </xref>, to as low as one standard deviation of ±0.0019 km/s/Mpc from the 2023 data provided by Dhal et al. <xref ref-type="bibr" rid="scirp.136677-31">
     [31]
    </xref>. We claim that our formulaic method to find 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> from precise CMB temperature observations is quite revolutionary and deserves attention from the research community. As a prime example of its potential value, we refer the reader to the above-mentioned Haug and Tatum’s references, which provide a highly detailed analysis and apparent solution of the Hubble tension problem. Over time, the research community can either confirm our findings or point out possible weaknesses in our reasoning. So far, we have not identified any such weaknesses, despite searching for them. It indeed appears that the recent breakthrough in understanding the theoretical relationship between CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> offers significantly improved precision regarding the large-scale global parameters of the universe. However, a theory must undergo scrutiny by multiple researchers over time to demonstrate its robustness. Therefore, the first step must be to make our discoveries accessible. We sincerely hope that this publication will encourage more researchers to look into this fascinating relationship between CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>.</p>
  </sec><sec id="s5">
   <title>Data Availability Statements</title>
   <p>All data used in this article are properly referenced and incorporated into our table and figure, so that anyone can easily check our calculations (“predictions”) in comparison to observations.</p>
  </sec><sec id="s6">
   <title>Acknowledgements</title>
   <p>We sincerely thank Dr. Ratan Kumar Paul for suggesting to present the table information also as a whisker chart.</p>
  </sec>
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