<?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">
    jamp
   </journal-id>
   <journal-title-group>
    <journal-title>
     Journal of Applied Mathematics and Physics
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2327-4352
   </issn>
   <issn publication-format="print">
    2327-4379
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/jamp.2025.132033
   </article-id>
   <article-id pub-id-type="publisher-id">
    jamp-140972
   </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 Hubble Tension Using the PantheonPlusSH0ES Supernova Database
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Espen Gaarder
      </surname>
      <given-names>
       Haug
      </given-names>
     </name>
    </contrib>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Eugene Terry
      </surname>
      <given-names>
       Tatum
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aTempus Gravitational Laboratory, Ås, Norway
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     10
    </day> 
    <month>
     02
    </month>
    <year>
     2025
    </year>
   </pub-date> 
   <volume>
    13
   </volume> 
   <issue>
    02
   </issue>
   <fpage>
    593
   </fpage>
   <lpage>
    622
   </lpage>
   <history>
    <date date-type="received">
     <day>
      15,
     </day>
     <month>
      January
     </month>
     <year>
      2025
     </year>
    </date>
    <date date-type="published">
     <day>
      25,
     </day>
     <month>
      January
     </month>
     <year>
      2025
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      25,
     </day>
     <month>
      February
     </month>
     <year>
      2025
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © Copyright 2014 by authors and Scientific Research Publishing Inc. 
    </copyright-statement>
    <copyright-year>
     2014
    </copyright-year>
    <license>
     <license-p>
      This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/
     </license-p>
    </license>
   </permissions>
   <abstract>
    Making use of a CMB temperature formula derivable from the Stefan-Boltzmann law, we have discovered a duality between the Particle Data Group (PDG) CMB temperature of 2.7255 K and its implied Hubble constant 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        H
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
     </mrow> 
    </math> value of approximately 66.9 km/s/Mpc, which can be used to predict the 2287 observed supernova redshifts in the PantheonPlusSH0ES database. Both values of this duality fall within constraints set for these cosmological parameters by the Particle Data Group. Notably, because our solution requires a rigorous mathematical derivation of a cosmological distance-vs-redshift formula pertaining to a variant of the 
    <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> cosmology model, our supernova redshift-matching solution fits only within the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        H
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
     </mrow> 
    </math> constraints of the 2018 Planck Collaboration and the PDG. It is our conclusion that, by matching the entire PantheonPlusSH0ES dataset of 2287 observations with the Planck Collaboration 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        H
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
     </mrow> 
    </math> constraints, such a dataset provides strong support for a 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        H
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
     </mrow> 
    </math> value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        H
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
      <mo>
       =
      </mo>
      <msubsup> 
       <mrow> 
        <mn>
         66.8943
        </mn>
       </mrow> 
       <mrow> 
        <mo>
         −
        </mo>
        <mn>
         0.0287
        </mn>
       </mrow> 
       <mrow> 
        <mo>
         +
        </mo>
        <mn>
         0.0287
        </mn>
       </mrow> 
      </msubsup> 
     </mrow> 
    </math> km/s/Mpc based on the Fixsen (2009) observation of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
        T
       </mi> 
       <mn>
        0
       </mn> 
      </msub> 
      <mo>
       =
      </mo>
      <msubsup> 
       <mrow> 
        <mn>
         2.72548
        </mn>
       </mrow> 
       <mrow> 
        <mo>
         −
        </mo>
        <mn>
         0.00057
        </mn>
       </mrow> 
       <mrow> 
        <mo>
         +
        </mo>
        <mn>
         0.00057
        </mn>
       </mrow> 
      </msubsup> 
      <mtext>
        
      </mtext>
      <mtext>
       K
      </mtext>
     </mrow> 
    </math> .
   </abstract>
   <kwd-group> 
    <kwd>
     Hubble Tension
    </kwd> 
    <kwd>
      Hubble Constant
    </kwd> 
    <kwd>
      Cosmological Redshift z
    </kwd> 
    <kwd>
      CMB Temperature
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>1. The CMB Temperature Prediction Formula</title>
   <p>Tatum et al. <xref ref-type="bibr" rid="scirp.140972-1">
     [1]
    </xref> presented the following formula for the Cosmic Microwave Background (CMB) temperature in 2015, a formula which has been discussed in more depth and derived from the Stefan-Boltzmann law <xref ref-type="bibr" rid="scirp.140972-2">
     [2]
    </xref> <xref ref-type="bibr" rid="scirp.140972-3">
     [3]
    </xref> recently by Haug and Wojnow <xref ref-type="bibr" rid="scirp.140972-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.140972-5">
     [5]
    </xref>:</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> 
        <mo>
          , 
        </mo> 
        <mn>
          0 
        </mn> 
       </mrow> 
      </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> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          ℏ 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
        </msub> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
          <mn>
            2 
          </mn> 
          <msub> 
           <mi>
             l 
           </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>
         k 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the Boltzmann constant, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> is the Hubble radius, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math> is the Newtonian gravitational constant, 
    <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> is the Planck length, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         m 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <mi>
            ℏ 
          </mi> 
          <mi>
            c 
          </mi> 
         </mrow> 
         <mi>
           G 
         </mi> 
        </mfrac> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> is the Planck mass, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       c 
     </mi> 
    </math> is the speed of light, and 
    <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> 
     </mrow> 
    </math> is the reduced Planck constant, also known as the Dirac constant. 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the current equivalent mass in the Hubble sphere, where we can use the critical Friedmann mass 
    <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>
           2 
         </mn> 
        </msup> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> as the mass now. One should be aware that, in recent years, it has been demonstrated that the Planck units can be found independent of knowing 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>. See, for example, Haug <xref ref-type="bibr" rid="scirp.140972-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.140972-6">
     [6]
    </xref>. This implies that the Schwarzschild radius in the critical Friedmann universe is identical to the Hubble radius, something that is well known (see <xref ref-type="bibr" rid="scirp.140972-7">
     [7]
    </xref> <xref ref-type="bibr" rid="scirp.140972-8">
     [8]
    </xref>); possible connections between the Hubble sphere and black holes have been discussed since at least 1972 (see <xref ref-type="bibr" rid="scirp.140972-9">
     [9]
    </xref>) and are actively discussed to this day (see <xref ref-type="bibr" rid="scirp.140972-10">
     [10]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-13">
     [13]
    </xref>). Despite its likely great potential significance, this formula (Equation (1)) has received little attention from the wider astrophysics community.</p>
   <p>The Stefan-Boltzmann law is valid for nearly perfect black bodies. Based on extensive studies made by the COBE satellite, Muller et al. <xref ref-type="bibr" rid="scirp.140972-14">
     [14]
    </xref> state (see also <xref ref-type="bibr" rid="scirp.140972-15">
     [15]
    </xref>):</p>
   <p>“Observations with the COBE satellite have demonstrated that the CMB corresponds to a nearly perfect black body, characterized by a temperature 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> at 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>, which is measured with very high accuracy, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2.72548 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.00057 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>.”</p>
   <p>Therefore, it should not be a surprise that the Stefan-Boltzmann law can be used to derive the CMB temperature. One may question whether this law was also valid during earlier epochs of the universe. With the ΛCDM model, this is unlikely; however, our CMB formula is consistent with 
    <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> cosmology, which we will discuss shortly.</p>
   <p>It is worth noting that Equation (1) looks quite similar to the Hawking black hole temperature formula <xref ref-type="bibr" rid="scirp.140972-16">
     [16]
    </xref> <xref ref-type="bibr" rid="scirp.140972-17">
     [17]
    </xref>: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          H 
        </mi> 
        <mi>
          w 
        </mi> 
       </mrow> 
      </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> 
        <mi>
          M 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>, except that one replaces 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       M 
     </mi> 
    </math> with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msqrt> 
       <mrow> 
        <msub> 
         <mi>
           M 
         </mi> 
         <mi>
           c 
         </mi> 
        </msub> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math>.</p>
   <p>Based on Equation (1), we can calculate the current CMB temperature using the current Hubble constant value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        67.4 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.5 
      </mn> 
     </mrow> 
    </math> km/s/Mpc as given by the Particle Data Group (PDG)<sup>1</sup> in their Astrophysical Constants and Parameters. From Equation (1), we obtain 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          2.7358 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0101 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0102 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>. This result shows that the constraint on the CMB temperature given by the PDG ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          2.7255 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0006 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0006 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>) is within our predicted range, indicating that our model is not in conflict with these established measurements.</p>
   <p>Our uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> is indeed larger than that given by the observational study cited by the PDG. The reason for this is that our CMB temperature is a predicted value based on a new mathematical relation between 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> (Equation (1)). When predicting 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> from 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, the uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> is inherently linked to the uncertainty in the observed 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. The Λ-CDM model, however, does not predict 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, making our approach noteworthy.</p>
   <p>There is a duality in our formula: a CMB temperature of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2.7255 
      </mn> 
     </mrow> 
    </math> K corresponds to 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        66.9 
      </mn> 
     </mrow> 
    </math> km/s/Mpc, and vice versa (we will soon come back to the confidence intervals based on measurement inputs and how they affect our model). In other words, both the current CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> in this duality fall well within the constraints set for these cosmological parameters by the Particle Data Group (PDG). The beauty of this new exact mathematical relation between CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> is that we can now rely on the most precisely measured of the two to predict the other one with high precision, something which will become more clear as one goes through this manuscript, as well as the papers referred to.</p>
   <p>Although Equation (1) has recently been demonstrated to be derivable from the Stefan-Boltzmann law <xref ref-type="bibr" rid="scirp.140972-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.140972-5">
     [5]
    </xref>, Haug and Tatum <xref ref-type="bibr" rid="scirp.140972-18">
     [18]
    </xref> have also derived the same formula from a geometric mathematical approach, demonstrating its consistency with a geometric mean temperature between the lowest and highest possible current temperatures in the Hubble sphere. We are not the first to use geometric means in thermodynamics; see also Henderson <xref ref-type="bibr" rid="scirp.140972-19">
     [19]
    </xref>. Even a third alternative and compatible way to derive Equation (1) exists, based on the fact that the minimum light bending is linked to the Planck scale; see <xref ref-type="bibr" rid="scirp.140972-20">
     [20]
    </xref>. These radically different approaches, in addition to the Stefan-Boltzmann derivation, suggest that Equation (1) has a solid physical foundation.</p>
   <p>All of these approaches seem to create a consistent and interesting framework, particularly in line with “growing black hole” models such as the FSC Schwarzschild metric model, but likely also other growing black hole models that can be built around other metrics, such as <xref ref-type="bibr" rid="scirp.140972-21">
     [21]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-24">
     [24]
    </xref>.</p>
   <p>An actively discussed class of cosmological models, for comparison to the Λ-CDM model, is the 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> models (see, for example, <xref ref-type="bibr" rid="scirp.140972-8">
     [8]
    </xref> <xref ref-type="bibr" rid="scirp.140972-25">
     [25]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-29">
     [29]
    </xref>). Naturally, there are also critics of the 
    <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, and such discussions are essential for progress in research. Lewis <xref ref-type="bibr" rid="scirp.140972-30">
     [30]
    </xref>, for example, has criticized the 
    <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> model for its “unphysical properties”; however, these claims have been refuted by Melia <xref ref-type="bibr" rid="scirp.140972-31">
     [31]
    </xref>. Melia <xref ref-type="bibr" rid="scirp.140972-32">
     [32]
    </xref> also published a study summarizing 18 observational tests comparing the 
    <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> model with the Λ-CDM model and showing that most of these tests actually favor 
    <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>. Despite this, there are ongoing criticisms of the 
    <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> model to this day, as seen in the recent paper by Panchal and Desai <xref ref-type="bibr" rid="scirp.140972-33">
     [33]
    </xref>.</p>
   <p>The FSC model, originating with the referenced Tatum et al.’s (2015) paper, falls within the category of growing black hole variants 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, which represent a subclass 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. Thus, there is also thermodynamics related to the current and past CMB temperature in this cosmological model. A generalized version of Formula (1) can be:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mrow> 
        <mi>
          C 
        </mi> 
        <mi>
          M 
        </mi> 
        <mi>
          B 
        </mi> 
       </mrow> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          ℏ 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           k 
         </mi> 
         <mi>
           b 
         </mi> 
        </msub> 
        <mn>
          4 
        </mn> 
        <mi>
          π 
        </mi> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
          <mn>
            2 
          </mn> 
          <msub> 
           <mi>
             l 
           </mi> 
           <mi>
             p 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (2)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the black hole radius at any stage in the growing black hole universe. In this model, the universe starts out with a Planck mass Schwarzschild radius of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         s 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          G 
        </mi> 
        <msub> 
         <mi>
           m 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <msub> 
       <mi>
         l 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math> and then expands one Planck length in radius per Planck time. Thus, one can also say that it increases by one-half a Planck mass per Planck time. Be aware the Planck units can be found independent of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       G 
     </mi> 
    </math>, as demonstrated by Haug <xref ref-type="bibr" rid="scirp.140972-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.140972-6">
     [6]
    </xref>.</p>
  </sec><sec id="s2">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>2. Cosmological Redshift from CMB Temperatures</title>
   <p>In general, for many cosmological models, we have:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          R 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           t 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (3)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        R 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> is the scale factor dependent on the cosmological model, and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> is the reference time, which is now. In the Λ-CDM model, light is redshifted based on the idea of the expansion of space and cosmic time. The redshifted wavelength can be treated as stretching as space-time expands. In the FSC Tatum et al. model, we have 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mi>
        R 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           t 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
     </mrow> 
    </math>, which is simply the Hubble radius 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> at present. The Hubble radius is the distance light that has traveled since the beginning of the black hole universe, which in the FSC model started as a Planck mass black hole and today is the Hubble sphere with mass equal to the mass in the critical Friedmann <xref ref-type="bibr" rid="scirp.140972-34">
     [34]
    </xref> universe 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         M 
       </mi> 
       <mi>
         c 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mi>
           c 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          G 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>.</p>
   <p>Melia <xref ref-type="bibr" rid="scirp.140972-35">
     [35]
    </xref> has pointed out that the cosmological redshift in the Friedmann-LeMaitre-Robertson-Walker (FLRW) metrics with constant space-time curvature, which he emphasizes must be the case when 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        a 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mi>
         t 
       </mi> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> in the 
    <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> universe, yields:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mi>
             e 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           t 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           t 
         </mi> 
         <mi>
           e 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mtext>
         e 
       </mtext> 
       <mi>
         X 
       </mi> 
      </msup> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (4)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
     </mrow> 
    </math> represents the emission time and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> represents the observation time. Since 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> and we also can have 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> in the 
    <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> universe, this implies that we also can have: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mi>
             e 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>. When we reconcile this with our equation for the CMB temperature (2), we obtain:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        1 
      </mn> 
      <mo>
        + 
      </mo> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <mi>
                ℏ 
              </mi> 
              <mi>
                c 
              </mi> 
             </mrow> 
             <mrow> 
              <msub> 
               <mi>
                 k 
               </mi> 
               <mi>
                 b 
               </mi> 
              </msub> 
              <mn>
                4 
              </mn> 
              <mi>
                π 
              </mi> 
              <msqrt> 
               <mrow> 
                <msub> 
                 <mi>
                   R 
                 </mi> 
                 <mi>
                   t 
                 </mi> 
                </msub> 
                <mn>
                  2 
                </mn> 
                <msub> 
                 <mi>
                   l 
                 </mi> 
                 <mi>
                   p 
                 </mi> 
                </msub> 
               </mrow> 
              </msqrt> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <mi>
                ℏ 
              </mi> 
              <mi>
                c 
              </mi> 
             </mrow> 
             <mrow> 
              <msub> 
               <mi>
                 k 
               </mi> 
               <mi>
                 b 
               </mi> 
              </msub> 
              <mn>
                4 
              </mn> 
              <mi>
                π 
              </mi> 
              <msqrt> 
               <mrow> 
                <msub> 
                 <mi>
                   R 
                 </mi> 
                 <mi>
                   H 
                 </mi> 
                </msub> 
                <mn>
                  2 
                </mn> 
                <msub> 
                 <mi>
                   l 
                 </mi> 
                 <mi>
                   p 
                 </mi> 
                </msub> 
               </mrow> 
              </msqrt> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           t 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mn>
           0 
         </mn> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (5)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>. Alternatively, we could write this as:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           λ 
         </mi> 
         <mrow> 
          <mtext>
            observed 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           λ 
         </mi> 
         <mrow> 
          <mtext>
            emitted 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           λ 
         </mi> 
         <mrow> 
          <mtext>
            emitted 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (6)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <mi>
                ℏ 
              </mi> 
              <mi>
                c 
              </mi> 
             </mrow> 
             <mrow> 
              <msub> 
               <mi>
                 k 
               </mi> 
               <mi>
                 b 
               </mi> 
              </msub> 
              <mn>
                4 
              </mn> 
              <mi>
                π 
              </mi> 
              <msqrt> 
               <mrow> 
                <msub> 
                 <mi>
                   R 
                 </mi> 
                 <mi>
                   t 
                 </mi> 
                </msub> 
                <mn>
                  2 
                </mn> 
                <msub> 
                 <mi>
                   l 
                 </mi> 
                 <mi>
                   p 
                 </mi> 
                </msub> 
               </mrow> 
              </msqrt> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mfrac> 
             <mrow> 
              <mi>
                ℏ 
              </mi> 
              <mi>
                c 
              </mi> 
             </mrow> 
             <mrow> 
              <msub> 
               <mi>
                 k 
               </mi> 
               <mi>
                 b 
               </mi> 
              </msub> 
              <mn>
                4 
              </mn> 
              <mi>
                π 
              </mi> 
              <msqrt> 
               <mrow> 
                <msub> 
                 <mi>
                   R 
                 </mi> 
                 <mi>
                   H 
                 </mi> 
                </msub> 
                <mn>
                  2 
                </mn> 
                <msub> 
                 <mi>
                   l 
                 </mi> 
                 <mi>
                   p 
                 </mi> 
                </msub> 
               </mrow> 
              </msqrt> 
             </mrow> 
            </mfrac> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mi>
           t 
         </mi> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
       <mrow> 
        <msubsup> 
         <mi>
           T 
         </mi> 
         <mn>
           0 
         </mn> 
         <mn>
           2 
         </mn> 
        </msubsup> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math> (7)</p>
   <p>Solving for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> gives:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mi>
          β 
        </mi> 
       </mrow> 
      </msup> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </msup> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (8)</p>
   <p>In the current paper we provide some details about its derivation and additional discussion. Tatum and Seshavatharam have acknowledged that the formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> is likely valid and have used it in a recent paper <xref ref-type="bibr" rid="scirp.140972-36">
     [36]
    </xref>. Observational studies strongly support 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (see <xref ref-type="bibr" rid="scirp.140972-37">
     [37]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-39">
     [39]
    </xref>). Therefore, a model consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> is likely incorrect. This strongly indicates that 
    <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 which rely on 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mn>
        1 
      </mn> 
      <mo>
        + 
      </mo> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mn>
             0 
           </mn> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msub> 
           <mi>
             t 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> are likely wrong or incomplete.</p>
   <p>It is also worth looking at the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> distance as a function of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> in the following way:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (9)</p>
   <p>So, the distance to the observed redshift is then:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (10)</p>
   <p>and solved for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, we have:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mi>
         d 
       </mi> 
      </mfrac> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (11)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        d 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the estimated distance to the object emitting the photons.</p>
   <p>When 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> we can use the first term of the Taylor series expansion which is:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (12)</p>
   <p>and naturally:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          d 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> (13)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        d 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> is the distance to the object emitting the photon, that is identical to the standard Λ-CDM cosmological redshift prediction formula typically used for low 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> values.</p>
  </sec><sec id="s3">
   <title>3. Comparison of 

    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
      <msub> 
   
       <mi>
        
    T
   
       </mi> 
   
       <mi>
        
    t
   
       </mi> 
  
      </msub> 
  
      <mo>
       
   =
  
      </mo>
  
      <msub> 
   
       <mi>
        
    T
   
       </mi> 
   
       <mn>
        
    0
   
       </mn> 
  
      </msub> 
  
      <msqrt> 
   
       <mrow> 
    
        <mn>
         
     1
    
        </mn>
    
        <mo>
         
     +
    
        </mo>
    
        <mi>
         
     z
    
        </mi>
   
       </mrow> 
  
      </msqrt> 
 
     </mrow>

    </math> versus 

    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
      <msub> 
   
       <mi>
        
    T
   
       </mi> 
   
       <mi>
        
    t
   
       </mi> 
  
      </msub> 
  
      <mo>
       
   =
  
      </mo>
  
      <msub> 
   
       <mi>
        
    T
   
       </mi> 
   
       <mn>
        
    0
   
       </mn> 
  
      </msub> 
  
      <mrow>
   
       <mo>
        
    (
   
       </mo> 
   
       <mrow> 
    
        <mn>
         
     1
    
        </mn>
    
        <mo>
         
     +
    
        </mo>
    
        <mi>
         
     z
    
        </mi>
   
       </mrow> 
   
       <mo>
        
    )
   
       </mo>
  
      </mrow>
 
     </mrow>

    </math></title>
   <p>The 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mtext>
       Λ 
     </mtext> 
    </math>-CDM model has, for many years, been using the following relation between CMB temperature and redshift:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (14)</p>
   <p>Since there has been some uncertainty as to whether this really is the best model of CMB temperature versus cosmological redshift 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math>, Lima et al. <xref ref-type="bibr" rid="scirp.140972-40">
     [40]
    </xref> suggested the following generalization of the formula:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mi>
          β 
        </mi> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> (15)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       β 
     </mi> 
    </math> is an unknown constant that, if set to zero, yields the standard formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>; however, it has also been suggested that 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       β 
     </mi> 
    </math> can be other than zero. Chluba <xref ref-type="bibr" rid="scirp.140972-41">
     [41]
    </xref> has suggested that: “decay of vacuum energy leads to ‘adiabatic’ photon production (or destruction), such that the CMB temperature scales like 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mi>
          β 
        </mi> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>”.</p>
   <p>Research based on observations has confirmed that 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       β 
     </mi> 
    </math> should be close to zero; see again <xref ref-type="bibr" rid="scirp.140972-37">
     [37]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-39">
     [39]
    </xref>. Thus, there is strong observational support for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>.</p>
   <p>If we set 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>, then we can “only”<sup>2</sup> make 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> compatible with CMB Equations (1) and (2) in the following manner:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           λ 
         </mi> 
         <mrow> 
          <mtext>
            observed 
          </mtext> 
         </mrow> 
        </msub> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           λ 
         </mi> 
         <mrow> 
          <mtext>
            emitted 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           λ 
         </mi> 
         <mrow> 
          <mtext>
            emitted 
          </mtext> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
        <mo>
          − 
        </mo> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> (16)</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              ℏ 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
           <mrow> 
            <msub> 
             <mi>
               k 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
            <msqrt> 
             <mrow> 
              <msub> 
               <mi>
                 R 
               </mi> 
               <mi>
                 t 
               </mi> 
              </msub> 
              <mn>
                2 
              </mn> 
              <msub> 
               <mi>
                 l 
               </mi> 
               <mi>
                 p 
               </mi> 
              </msub> 
             </mrow> 
            </msqrt> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              ℏ 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
           <mrow> 
            <msub> 
             <mi>
               k 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
            <msqrt> 
             <mrow> 
              <msub> 
               <mi>
                 R 
               </mi> 
               <mi>
                 H 
               </mi> 
              </msub> 
              <mn>
                2 
              </mn> 
              <msub> 
               <mi>
                 l 
               </mi> 
               <mi>
                 p 
               </mi> 
              </msub> 
             </mrow> 
            </msqrt> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           T 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math> (17)</p>
   <p>This means that we have 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        a 
      </mi> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msqrt> 
         <mi>
           t 
         </mi> 
        </msqrt> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mi>
          t 
        </mi> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> and 
    <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>, that again gives: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
               t 
             </mi> 
             <mn>
               0 
             </mn> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mi>
          a 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <msqrt> 
           <mrow> 
            <msub> 
             <mi>
               t 
             </mi> 
             <mi>
               e 
             </mi> 
            </msub> 
           </mrow> 
          </msqrt> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>, since 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         t 
       </mi> 
       <mi>
         e 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>. Even if the scale factor and cosmological redshift now are functions of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msqrt> 
       <mi>
         t 
       </mi> 
      </msqrt> 
     </mrow> 
    </math> rather than 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       t 
     </mi> 
    </math>, the Hubble radius is still a linear function of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       t 
     </mi> 
    </math>, namely still according to 
    <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>.</p>
   <p>In this case, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> will give the same prediction as in the previous section where we instead had 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, something that only can be true if we now also have 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
       </mrow> 
       <mrow> 
        <msqrt> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> rather than 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>. This new possibility of setting: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>, should be carefully investigated, as this potentially could have an impact on how one interprets space expansion in accordance with 
    <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 and also how this can be considered in relation to the Λ-CDM model.</p>
   <p>Riechers et al. <xref ref-type="bibr" rid="scirp.140972-39">
     [39]
    </xref> have reported the Cosmic Microwave Background (CMB) temperature from the cosmic epoch at 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        6.34 
      </mn> 
     </mrow> 
    </math>, resulting in a temperature range of 16.4 - 30.2 K within one standard deviation uncertainty. In other words, even the one standard deviation, which represents only about 68% probability for the CMB temperature to be inside that range, is very wide. The two-standard deviation CMB temperature range is much broader. Therefore, we can conclude that the formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> is not sufficiently well-tested, given the very large uncertainty. The formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
      </msqrt> 
     </mrow> 
    </math> predicts a CMB temperature of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2.725 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
      <msqrt> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mn>
          6.34 
        </mn> 
       </mrow> 
      </msqrt> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        7.4 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math> which is inside the 95% confidence interval of the above report (using two standard deviations); however, as we have also shown, the FSC framework at present also appears to be consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>. Only further investigation can help us to decide on the optimal choice, even if observations appear to currently favor 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>.</p>
   <p>It is also worth looking at the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> distance as a function of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> in the following way:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mi>
            z 
          </mi> 
          <mo>
            + 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           t 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           R 
         </mi> 
         <mi>
           H 
         </mi> 
        </msub> 
       </mrow> 
       <mrow> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (18)</p>
   <p>So, the distance to the observed redshift is then:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        − 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math></p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                1 
              </mn> 
              <mo>
                + 
              </mo> 
              <mi>
                z 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> (19)</p>
   <p>and naturally:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          c 
        </mi> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <msup> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mn>
                  1 
                </mn> 
                <mo>
                  + 
                </mo> 
                <mi>
                  z 
                </mi> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mi>
         D 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> (20)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        D 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math>, which is the distance between us and the object emitting the observed photons. When 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> we can use the first term of the first order Taylor series expansion and we get:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        D 
      </mi> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        − 
      </mo> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          c 
        </mi> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (21)</p>
   <p>that naturally gives:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          D 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (22)</p>
   <p>and naturally:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          z 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mi>
         D 
       </mi> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (23)</p>
   <p>This is indeed different from the standard redshift formulation. However, in this case, the distance 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       D 
     </mi> 
    </math> will also differ from the distance predicted by the standard formula. Therefore, only careful further investigation can determine whether it is superior to the standard formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          d 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
     </mrow> 
    </math> or not. First of all, it is important to be aware that we have:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          z 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mi>
         D 
       </mi> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          z 
        </mi> 
        <mi>
          c 
        </mi> 
       </mrow> 
       <mi>
         d 
       </mi> 
      </mfrac> 
      <mo>
        , 
      </mo> 
      <mtext>
          
      </mtext> 
      <mi>
        z 
      </mi> 
      <mo>
        ≈ 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          D 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <mi>
          c 
        </mi> 
       </mrow> 
      </mfrac> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mrow> 
        <mi>
          d 
        </mi> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mi>
         c 
       </mi> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (24)</p>
   <p>These two formulas give identical predictions for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> when dealing with short distances and low 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math>. The “2” in the numerator is offset exactly by the fact that 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        D 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        2 
      </mn> 
      <mi>
        d 
      </mi> 
     </mrow> 
    </math> in the denominator. This holds true when the distance is short ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>). Thus, when used to extract the Hubble constant from, for example, nearby supernovae, the estimated 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> or estimated 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> are identical. It is the distances that differ in the two approaches. However, when dealing with supernovae or other objects far from us, the estimated Hubble constant values will be different, as we then need to use the exact formulas, rather than convenient approximations. This implies that, in the standard Λ-CDM model, the value of the Hubble constant based on higher redshifts is likely overestimated.</p>
   <p>For redshift and Hubble constant analysis at short distances, we can say that the Λ-CDM model likely has two errors that cancel each other out: it has the wrong distance and also the wrong formula, which offsets the error in the wrong distance. Therefore, its predictions for redshift 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> at short distances will be correct and the same as in our model. However, at much larger distances, their model will not be fully accurate, which we believe has led to the Hubble tension problem. This issue is addressed with our new way of looking at redshifts, as will become clear from the remainder of our paper, particularly in the sections where we aim to resolve the Hubble tension, namely Sections 4 and 5.</p>
   <p>If this latter redshift formula is correct, then distances to astronomical objects based on redshift are likely off by as much as a factor of 2. This could explain why the Λ-CDM model must have an expansion of space faster than 
    <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. Once again, we believe that our new approach and explanation likely resolves the Hubble tension problem.</p>
   <p>If one is not deeply entrenched in the topic, it may be easy to assume that our redshift Equation (21) must be incorrect, given the highly precise measurements of distances to various astronomical objects through independent methods, such as parallax. However, supernova distances are never measured directly by a method as elementary as parallax. Establishing their distances requires a complex understanding of the astronomical distance ladder and the inherent uncertainties built into each rung of this ladder. Type Ia supernovae represent some of our most reliable standardized candles. Therefore, the most accurate method of determining their distance is likely through cosmological redshift, albeit this approach is naturally model-dependent. While our math, which suggests that the distance to the more remote supernovae is significantly greater than that predicted by the Λ-CDM model, may initially seem unfeasible, based on our current limited knowledge, it should not be immediately discounted. The above text following Equation (23) we believe to be the crux of this paper. We would welcome any compelling arguments against our findings, in particular after studying the rest of our paper.</p>
   <p>
    <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref> shows the predicted distances for the full 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> range in the PantheonPlusSH0ES supernova database. We have predicted the distances based on the two approximation formulas. The two approximation formulas are based on the first term of the Taylor series expansion and are, in reality, only good approximations when 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        ≪ 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>. This is why these approximations strongly overestimate the distances for high- 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> supernovae. The two exact solutions, based on the assumptions given in this paper, yield different values. The model consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> predicts a distance for each 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> as given by the red line. The model consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
      </msup> 
     </mrow> 
    </math> predicts a distance for each 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> as given by the blue line. We will soon come back to comparing these distances with what is predicted from the ΛCDM model. We incorporate the current value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> to make these distance approximations, which we take from the Particle Data Group (PDG) Astrophysical Constants and Parameters, which gives 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        67.4 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.5 
      </mn> 
     </mrow> 
    </math> km/s/Mpc.</p>
   <p>In <xref ref-type="fig" rid="fig2">
     Figure 2
    </xref>, we have removed the approximation models and we now focus on those models which are relatively more accurate at higher redshifts. This makes more obvious the difference between the model consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mrow> 
         <mn>
           1 
         </mn> 
         <mo>
           / 
         </mo> 
         <mn>
           2 
         </mn> 
        </mrow> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, and which we will now call Model A, and the model consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>, which we will now call Model B. Be aware that the Λ-CDM model predicts the same distances as the blue line, at least for low 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> values. The red line prediction is what likely is correct, however, as it is consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>, which we will show that observations seem to favor. This will become more clear in the next section. The green line represents 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mi>
         D 
       </mi> 
       <mo>
         / 
       </mo> 
       <mi>
         d 
       </mi> 
      </mrow> 
     </mrow> 
    </math>.</p>
   <fig id="fig1" position="float">
    <label>Figure 1</label>
    <caption>
     <title>Figure 1. This figure shows the predicted supernova distances for different redshift models. Two of the models employ first series Taylor approximations and only give reasonably accurate solutions when 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <mi>
         
   z
  
        </mi>
  
        <mo>
         
   ≪
  
        </mo>
  
        <mn>
         
   1
  
        </mn>
 
       </mrow>

      </math>.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId355.jpeg?20250228035726" />
   </fig>
   <fig id="fig2" position="float">
    <label>Figure 2</label>
    <caption>
     <title>Figure 2. This figure shows the predicted supernova distances for these distance-vs-redshift models in somewhat greater detail, and in comparison to the 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <mrow>
   
         <mi>
          
    D
   
         </mi>
   
         <mo>
          
    /
   
         </mo>
   
         <mi>
          
    d
   
         </mi>
  
        </mrow> 
 
       </mrow>

      </math> ratio.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId358.jpeg?20250228035726" />
   </fig>
   <p>In <xref ref-type="fig" rid="fig3">
     Figure 3
    </xref>, we compare the predicted distance in our model for a given redshift with the three distances predicted by the Λ-CDM model. In the new model described in this paper, the co-moving, luminosity, and angular diameter distances become identical—a concept discussed in more detail in our recent paper <xref ref-type="bibr" rid="scirp.140972-42">
     [42]
    </xref>. Importantly, our model fully complies with Etherington’s <xref ref-type="bibr" rid="scirp.140972-43">
     [43]
    </xref> reciprocity theorem, which is based primarily on solid geometry and also plays an important role in the Λ-CDM model. Since none of the three distances predicted by the Λ-CDM model match the distance predicted by our model, none of these Λ-CDM distances can be used to verify the accuracy of our predicted distance.</p>
   <p>The only independent method of distance determination potentially available is parallax. Parallax is highly robust and independent of any particular cosmological model; it is grounded in straightforward geometric principles but has, for practical reasons, been limited to very short cosmological distances. Hypothetically, parallax could be applied to distant galaxies and potentially also supernovae, but for such cases, standard parallax methods do not necessarily retain the same robustness. It is well known that standard parallax, if hypothetically applied to distant galaxies, would require redshift adjustments; thus, even parallax distance predictions for such distant objects would be influenced by the underlying model; see Hogg <xref ref-type="bibr" rid="scirp.140972-44">
     [44]
    </xref>.</p>
   <fig id="fig3" position="float">
    <label>Figure 3</label>
    <caption>
     <title>Figure 3. This figure shows the predicted distance in the new 

      <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> type cosmology model developed by Haug and Tatum versus the three distances to the same redshifted object predicted by the Λ-CDM model.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId361.jpeg?20250228035726" />
   </fig>
   <p>We propose that the Λ-CDM model’s likely inaccuracy in predicting distances is the fundamental cause of the Hubble tension. In our model, the co-moving, luminosity, and angular diameter distances are unified into a single distance, not by assumption, but from derivations <xref ref-type="bibr" rid="scirp.140972-42">
     [42]
    </xref>. This unified distance feature, together with the rest of our model, appears to resolve the Hubble tension. As we will demonstrate, our model’s ability to predict all SN Ia redshifts with only one Hubble parameter is likely the most compelling evidence that our model also predicts the correct distances.</p>
  </sec><sec id="s4">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>4. Extracting the Current CMB Temperature from 2287 Type Ia Supernovae</title>
   <p>Here, we use the observed redshifts from 2287 supernova data points in the PantheonPlusSH0ES database to determine the current CMB temperature ( 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math>). The methodology employed is as follows: from the cosmological redshifts, we first predict the CMB temperatures for each observed 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> value, by using the standard and well-known relation 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>. Since our goal is to find 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> a priori, we start with a wild guess. For instance, we might start with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        4 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>, or even 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        10 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>, which is naturally far off from the currently observed CMB temperature of approximately 2.725 K. We start with a wild guess because we will later use optimization to determine if there exists a 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> that leads to an estimation error near zero, using the redshift prediction formula 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>. This can be achieved using optimization algorithms such as the Newton-Raphson method or the bisection method.</p>
   <p>Next, we calculate the radius of the Hubble sphere going back in time for each 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> value. This is done by assuming a FSC-like 
    <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> cosmology and solving Equation (2) for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math>. This gives:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              ℏ 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
           <mrow> 
            <msub> 
             <mi>
               T 
             </mi> 
             <mi>
               t 
             </mi> 
            </msub> 
            <msub> 
             <mi>
               k 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <msub> 
         <mi>
           l 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> (25)</p>
   <p>and since we also have 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>, we can replace 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> with this and get:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mi>
              ℏ 
            </mi> 
            <mi>
              c 
            </mi> 
           </mrow> 
           <mrow> 
            <msub> 
             <mi>
               T 
             </mi> 
             <mn>
               0 
             </mn> 
            </msub> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mn>
                1 
              </mn> 
              <mo>
                + 
              </mo> 
              <mi>
                z 
              </mi> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
            <msub> 
             <mi>
               k 
             </mi> 
             <mi>
               b 
             </mi> 
            </msub> 
            <mn>
              4 
            </mn> 
            <mi>
              π 
            </mi> 
           </mrow> 
          </mfrac> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mn>
         2 
       </mn> 
      </msup> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mrow> 
        <mn>
          2 
        </mn> 
        <msub> 
         <mi>
           l 
         </mi> 
         <mi>
           p 
         </mi> 
        </msub> 
       </mrow> 
      </mfrac> 
      <mo>
        . 
      </mo> 
     </mrow> 
    </math> (26)</p>
   <p>Because we are assuming that we do not know 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, we will not rely upon measured CMB temperatures. However, we can now input this expression for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
     </mrow> 
    </math> into our redshift formula (Equation (17)) and we get:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mfrac> 
               <mrow> 
                <mi>
                  ℏ 
                </mi> 
                <mi>
                  c 
                </mi> 
               </mrow> 
               <mrow> 
                <msub> 
                 <mi>
                   T 
                 </mi> 
                 <mn>
                   0 
                 </mn> 
                </msub> 
                <mrow> 
                 <mo>
                   ( 
                 </mo> 
                 <mrow> 
                  <mn>
                    1 
                  </mn> 
                  <mo>
                    + 
                  </mo> 
                  <msub> 
                   <mi>
                     z 
                   </mi> 
                   <mrow> 
                    <mi>
                      o 
                    </mi> 
                    <mi>
                      b 
                    </mi> 
                    <mi>
                      s 
                    </mi> 
                   </mrow> 
                  </msub> 
                 </mrow> 
                 <mo>
                   ) 
                 </mo> 
                </mrow> 
                <msub> 
                 <mi>
                   k 
                 </mi> 
                 <mi>
                   b 
                 </mi> 
                </msub> 
                <mn>
                  4 
                </mn> 
                <mi>
                  π 
                </mi> 
               </mrow> 
              </mfrac> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <msub> 
             <mi>
               l 
             </mi> 
             <mi>
               p 
             </mi> 
            </msub> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math> (27)</p>
   <p>We can now minimize the errors between 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          b 
        </mi> 
        <mi>
          s 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> by adjusting the unknown 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> value. This can be accomplished through pure trial-and-error, or more efficiently by using “intelligent” trial-and-error systems such as the Newton-Raphson method or the bisection method. The results from these approaches are the same, except that, by naive trial-and-error, one will waste more time finding the optimal CMB temperature. To do this, we also need 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>, which is the current Hubble radius, and therefore, we also need the current value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, which we take from Particle Data Group (PDG) Astrophysical Constants and Parameters which gives 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        67.4 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.5 
      </mn> 
     </mrow> 
    </math> km/s/Mpc. Thus, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> affects the value; it is actually this relatively new theoretical relationship between the Hubble parameter and CMB temperature, first given by Tatum et al. <xref ref-type="bibr" rid="scirp.140972-1">
     [1]
    </xref> in 2015 and later proved to be derivable from the Stefan-Boltzmann law by Haug and Wojnow <xref ref-type="bibr" rid="scirp.140972-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.140972-5">
     [5]
    </xref>, that makes this method possible. We also need the Planck length in our formula, so we have used the NIST CODATA (2018) value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         l 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        1.616255 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          35 
        </mn> 
       </mrow> 
      </msup> 
      <mtext>
          
      </mtext> 
      <mtext>
        m 
      </mtext> 
     </mrow> 
    </math> (with standard uncertainty of 0.000018 × 10<sup>−</sup><sup>35</sup> m). This uncertainty is therefore reflected in the reported STD for both our predicted CMB temperature as well as our predicted 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> using the PantheonPlusSH0ES database.</p>
   <p>
    <xref ref-type="fig" rid="fig4">
     Figure 4
    </xref> best illustrates the trial-and-error procedure. Assume that we initially have guessed a CMB temperature of 4 K. This is the red line in the figure, that we see is far above the observed redshifts represented by the blue line. However, at least it looks like it correlates well, and the measured Pearson correlation is actually a perfect 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         ρ 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          b 
        </mi> 
        <mi>
          s 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math>. This should not come as a big surprise, since we claim to have developed exact relations between 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math>, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and the CMB temperature. However, the output prediction is no better than the input prediction; the guess of CMB temperature 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        4 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math> is way off. Given that the redshift predictions are proportional to the current CMB temperature, we must guess a lower CMB temperature. Assume that we now guess 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        1.5 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>; we then get the predictions presented by the purple line. It becomes obvious that our 1.5 K prediction is now too low compared to the observed redshifts. We now know that the CMB temperature needed in order to minimize the prediction errors must be between 4 K and 1.5 K. We, therefore, now guess 3 K, and the redshift predictions we get from this (the green line) are much closer to observed, but still too high.</p>
   <fig id="fig4" position="float">
    <label>Figure 4</label>
    <caption>
     <title>Figure 4. This figure shows observed redshift values from 2287 type Ia supernovae, sorted by redshift. In addition, it shows the predicted redshifts for various qualified guesses on the current CMB temperature. We note that the predictions and observations are highly correlated, but they do not match. The predicted redshifts are too high when using CMB temperatures 4 K and 3 K and too low when using 1.5 K. However, by using efficient trial-and-error algorithms, we can quickly find the current CMB temperature that gives the best fit, as shown in the next figure. See <xref ref-type="fig" rid="fig5">
       Figure 5
      </xref>.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId422.jpeg?20250228035727" />
   </fig>
   <p>We can continue “manually” like this, or we can resort to efficient search algorithms that are used for similar statistical problems in many scientific fields. Among the most commonly used algorithms are the Newton-Raphson method or the bisection method. One can also use the goal seek function in Excel, which is likely based on the bisection method. These trial-and-error methods are simply a form of calibration method. The question is whether there exists a single CMB temperature, denoted as 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, for the current epoch of the cosmos that can make our “CMB redshift prediction formula” match the observed redshifts with precision.</p>
   <p>Effectively, we are calibrating our new cosmological redshift prediction equation relative to the observed 2287 supernova redshifts by finding the value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> that minimizes our prediction error. Only one parameter is adjusted (optimized), namely the “unknown” current CMB temperature, so that the errors indicated by the sum of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle displaystyle="true"> 
       <msubsup> 
        <mo>
          ∑ 
        </mo> 
        <mi>
          i 
        </mi> 
        <mi>
          n 
        </mi> 
       </msubsup> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              p 
            </mi> 
            <mi>
              r 
            </mi> 
            <mi>
              e 
            </mi> 
            <mi>
              d 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            − 
          </mo> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              b 
            </mi> 
            <mi>
              s 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              b 
            </mi> 
            <mi>
              s 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </mstyle> 
     </mrow> 
    </math> are minimized. This means that the sum of all individual redshift predictions is minimized by changing only one parameter, which in this case is the current CMB temperature 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> in Equation (27). This could potentially lead to a scenario where only the average error is zero, with some errors being positive and others negative, canceling each other out. However, we can easily check this after the optimization has been done by comparing all predicted redshift values individually against their corresponding observations. This is demonstrated graphically in <xref ref-type="fig" rid="fig5">
     Figure 5
    </xref>, where we can see that all predictions match their observations based on using the same optimized 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> for all predictions. In other words, it is not only that the average error is low, but all of the individual errors are close to zero. That said, each prediction indirectly incorporates the observed redshift parameter, as can be seen from Equation (27), so this can indeed be labeled as a form of curve fitting. However, the important point is that our simple redshift function can easily match all observed redshifts using only a single free parameter, namely the CMB temperature in this case. Or, alternatively, we could choose the Hubble constant value as our free parameter (see below). This flexibility is based upon the duality we have discovered between 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> values.</p>
   <fig id="fig5" position="float">
    <label>Figure 5</label>
    <caption>
     <title>Figure 5. This figure shows observed redshift values from 2287 type Ia supernovae, sorted by redshift. We find that, by starting with the PDG Hubble constant value of 67.4 km/s/Mpc and then assuming a current CMB temperature of 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mo>
         
   ≈
  
        </mo>
  
        <mn>
         
   2.7358
  
        </mn>
  
        <mtext>
         
    
  
        </mtext>
  
        <mtext>
         
   K
  
        </mtext>
 
       </mrow>

      </math>, there is a nice match between observed redshifts (blue line) and our predicted redshifts (red line).</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId435.jpeg?20250228035727" />
   </fig>
   <p>To be even more precise on exactly how we minimize the errors, for all redshift observations we first calculate:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          i 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mfrac> 
               <mrow> 
                <mi>
                  ℏ 
                </mi> 
                <mi>
                  c 
                </mi> 
               </mrow> 
               <mrow> 
                <msub> 
                 <mi>
                   T 
                 </mi> 
                 <mn>
                   0 
                 </mn> 
                </msub> 
                <mrow> 
                 <mo>
                   ( 
                 </mo> 
                 <mrow> 
                  <mn>
                    1 
                  </mn> 
                  <mo>
                    + 
                  </mo> 
                  <msub> 
                   <mi>
                     z 
                   </mi> 
                   <mrow> 
                    <mi>
                      o 
                    </mi> 
                    <mi>
                      b 
                    </mi> 
                    <mi>
                      s 
                    </mi> 
                    <mo>
                      , 
                    </mo> 
                    <mi>
                      i 
                    </mi> 
                   </mrow> 
                  </msub> 
                 </mrow> 
                 <mo>
                   ) 
                 </mo> 
                </mrow> 
                <msub> 
                 <mi>
                   k 
                 </mi> 
                 <mi>
                   b 
                 </mi> 
                </msub> 
                <mn>
                  4 
                </mn> 
                <mi>
                  π 
                </mi> 
               </mrow> 
              </mfrac> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <msub> 
             <mi>
               l 
             </mi> 
             <mi>
               p 
             </mi> 
            </msub> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math> (28)</p>
   <p>where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          o 
        </mi> 
        <mi>
          b 
        </mi> 
        <mi>
          s 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          i 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> is the observed redshift combined with an initial “wild” guess for the CMB temperature 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. In addition, we need a measured 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> value if we try to find the CMB temperature; all other inputs are known constants: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         k 
       </mi> 
       <mi>
         b 
       </mi> 
      </msub> 
     </mrow> 
    </math>, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       c 
     </mi> 
    </math>, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       ℏ 
     </mi> 
    </math>, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         l 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math> (where we also take into account the uncertainty in the Planck length 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         l 
       </mi> 
       <mi>
         p 
       </mi> 
      </msub> 
     </mrow> 
    </math>). This leads to predictions of all our redshifts that are far away from observed redshifts (see again <xref ref-type="fig" rid="fig4">
     Figure 4
    </xref>). Then, for each predicted redshift, we calculate the percentage</p>
   <p>error relative to the observed: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <mi>
            p 
          </mi> 
          <mi>
            r 
          </mi> 
          <mi>
            e 
          </mi> 
          <mo>
            , 
          </mo> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            b 
          </mi> 
          <mi>
            s 
          </mi> 
          <mo>
            , 
          </mo> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            b 
          </mi> 
          <mi>
            s 
          </mi> 
          <mo>
            , 
          </mo> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>. Then we sum up all of the errors. By trial and error, we only change 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, and for each new intelligent guess on 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, we repeat the procedure of recalculating all of the errors 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mfrac> 
       <mrow> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <mi>
            p 
          </mi> 
          <mi>
            r 
          </mi> 
          <mi>
            e 
          </mi> 
          <mo>
            , 
          </mo> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          − 
        </mo> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            b 
          </mi> 
          <mi>
            s 
          </mi> 
          <mo>
            , 
          </mo> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
       <mrow> 
        <msub> 
         <mi>
           z 
         </mi> 
         <mrow> 
          <mi>
            o 
          </mi> 
          <mi>
            b 
          </mi> 
          <mi>
            s 
          </mi> 
          <mo>
            , 
          </mo> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math>. We continue this trial-and-error process until we cannot reduce the sum of errors any further, and with a very high precision.</p>
   <p>The only values we use from the PantheonPlusSH0ES SN Ia database are the redshifts. For each of the 2287 observed redshifts, we calculate 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
        <mo>
          , 
        </mo> 
        <mi>
          i 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> based on Equation (28) using a single guess of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, our free parameter in this case. We use the same guess of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> for all 2287 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
        <mi>
          d 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math>. All of the predicted values are then compared with the corresponding observed values. Statistically, for all 2287 predictions, we can then summarize the percentage error relative to the observations according to 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle displaystyle="true"> 
       <msubsup> 
        <mo>
          ∑ 
        </mo> 
        <mrow> 
         <mi>
           i 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           1 
         </mn> 
        </mrow> 
        <mrow> 
         <mn>
           2287 
         </mn> 
        </mrow> 
       </msubsup> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              p 
            </mi> 
            <mi>
              r 
            </mi> 
            <mi>
              e 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            − 
          </mo> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              b 
            </mi> 
            <mi>
              s 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              b 
            </mi> 
            <mi>
              s 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </mstyle> 
     </mrow> 
    </math>.</p>
   <p>As we can see from Equation (28), if we reduce the guess of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, the predicted redshift values will go down, and if we increase the guess of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, the predicted redshift values will go up. This helps us to determine the direction to adjust 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> to reduce the sum of errors 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mstyle displaystyle="true"> 
       <msubsup> 
        <mo>
          ∑ 
        </mo> 
        <mrow> 
         <mi>
           i 
         </mi> 
         <mo>
           = 
         </mo> 
         <mn>
           1 
         </mn> 
        </mrow> 
        <mrow> 
         <mn>
           2287 
         </mn> 
        </mrow> 
       </msubsup> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              p 
            </mi> 
            <mi>
              r 
            </mi> 
            <mi>
              e 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
          <mo>
            − 
          </mo> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              b 
            </mi> 
            <mi>
              s 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             z 
           </mi> 
           <mrow> 
            <mi>
              o 
            </mi> 
            <mi>
              b 
            </mi> 
            <mi>
              s 
            </mi> 
            <mo>
              , 
            </mo> 
            <mi>
              i 
            </mi> 
           </mrow> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </mstyle> 
     </mrow> 
    </math>. After making these adjustments several times, the errors are reduced to close to zero for all 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math> simultaneously. This means that there is one best-fit 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> value for all 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
       </mrow> 
      </msub> 
     </mrow> 
    </math>, which we now see in <xref ref-type="fig" rid="fig5">
     Figure 5
    </xref>. This result seems almost too good to be true. However, the reason that this is possible is that we are using a linear 
    <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> model, where there are linear relations over cosmic time, unlike the Λ-CDM model, which has highly non-linear relations and lacks a formula to predict the CMB temperature in this way. Using Equation (28) in this way, anyone should be able to recreate our findings by inputting only the 2287 redshift values in the PantheonPlusSH0ES database.</p>
   <p>This method does not in any way guarantee zero or close to zero error for any model. If the model is misspecified or simply not flexible enough to match all of the observed redshifts, then even after minimizing errors, there will be considerable error. This is clearly demonstrated in section 8 where we illustrate exactly this point.</p>
   <p>Of course, it is almost always possible to come up with a mathematical function with enough flexible variables that can be tweaked to match observations; this would be, in our view, pure curve fitting, which would obviously be of little value. On the other hand, our model is derived from foundational principles, such as the Stefan-Boltzmann law, and with no initial aim at matching observed redshifts. It is the CMB temperature formula of Equation (1), combined with the observable confirmed relation: 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>, that leads directly to our redshift prediction formula. We have not added additional factors in order to match redshifts. For example, one could have added extra parameters (extra degrees of freedom) to our model to allow for some form of dark energy. On the contrary, we find that our simple 
    <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> model does not need any extra freedom parameter in order to match the full distance ladder of redshifts, while simultaneously matching the CMB temperature and being fully consistent with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>.</p>
   <p>The approach of minimizing errors just described results in a predicted current CMB temperature 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        2.73576067604891 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math> from the 2287 supernova observations in the PantheonPlusSH0ES database. We are not claiming that the current CMB temperature is exactly this (although it could be); rather, this is what it appears to be, based on the observed supernova redshifts in combination with the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        67.4 
      </mn> 
     </mrow> 
    </math> km/s/Mpc. When we also take into account the uncertainty in the value of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> (67.4 ± 0.5 km/s/Mpc), as reported by the Particle Data Group (PDG) Astrophysical Constants and Parameters, we get a one Standard Deviation (STD) confidence interval range of 2.7256 K to 2.7459 K for the current CMB temperature; the 95% confidence interval is 2.7154 K to 2.7560 K. The reason we provide the numerous digits in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        2.73576067604891 
      </mn> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math> is simply to enable others to obtain the same value when utilizing 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        67.4 
      </mn> 
     </mrow> 
    </math> km/s/Mpc following the procedure outlined in this paper. This is not meant to imply that we can determine the CMB temperature with such high precision. The measured CMB temperature has a lower uncertainty compared to our predicted CMB temperature. Rather, what is important to understand here is that we have a model that directly links the current CMB temperature to the Hubble constant. To the best of our knowledge, the Λ-CDM model does not offer such a direct relationship between the current CMB temperature and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>As different Hubble constant measurement studies and methods yield considerable uncertainty in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>, this uncertainty could be even larger. Moreover, there is the heretofore unexplained Hubble tension problem; see for example <xref ref-type="bibr" rid="scirp.140972-45">
     [45]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-48">
     [48]
    </xref>. Nevertheless, using our new radically different theoretical approach, we can closely approximate the recent CMB temperature observations by <xref ref-type="bibr" rid="scirp.140972-49">
     [49]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-52">
     [52]
    </xref>.</p>
   <p>By assuming a current CMB temperature 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        2.7358 
      </mn> 
      <msubsup> 
       <mo>
         ± 
       </mo> 
       <mrow> 
        <mn>
          0.0102 
        </mn> 
       </mrow> 
       <mrow> 
        <mn>
          0.0101 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>, the predictions from Equation (27) are now almost perfectly aligned with the observational blue line in <xref ref-type="fig" rid="fig5">
     Figure 5
    </xref>. In other words, the redshift formula we have presented is now capable of matching observed cosmological redshifts, if we start out with a measured CMB-based Hubble constant value.</p>
   <p>It is interesting that, by incorporating only the current CMB temperature and Hubble constant value, our redshift prediction function can match observations. It is important to note that we are matching the same epochal 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> for all supernovae, rather than different 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> values for different supernovae. We must keep in mind that all such redshifts have been measured in the current CMB temperature epoch. This basically demonstrates that our framework is consistent and robust. Our findings are fully consistent with the empirically tested relation 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> and also with the FSC growing black hole variant 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> cosmology.</p>
  </sec><sec id="s5">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>5. Why We Think That We May Have Solved the Hubble Tension Problem</title>
   <p>In the section above, where we found the CMB temperature that optimally fits with the observed supernova redshifts, we had to know the Planck-derived Hubble constant value. Alternatively, one can use the observed CMB temperature to optimally fit a Hubble constant value for the same 2287 supernova redshifts. The CMB temperature has been extremely accurately measured in recent years, for example, by <xref ref-type="bibr" rid="scirp.140972-49">
     [49]
    </xref>-<xref ref-type="bibr" rid="scirp.140972-52">
     [52]
    </xref>.</p>
   <p>First, we will use the most recent measurement by Fixen (2009) <xref ref-type="bibr" rid="scirp.140972-50">
     [50]
    </xref>, a CMB temperature of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mrow> 
        <mn>
          2.72548 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.00057 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.00057 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>, which is also fully consistent with the Particle Data Group (PDG)<sup>3</sup> Astrophysical Constants and Parameters that suggest 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          2.7255 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0006 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0006 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>. We then start out by assuming that we know very little about the Hubble constant value. All we know is that many different studies have arrived at different values. So, we start with a qualified, but wild, guess that it must be in a range from 50 to 80 km/s/Mpc. We then ask if there is a single Hubble constant 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math> value that, when used in our new CMB redshift prediction formula, matches all of the observed supernova redshifts. So, we start with a guess of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        50 
      </mn> 
     </mrow> 
    </math> km/s/Mpc and use the same formula as in the previous section:</p>
   <p>
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         z 
       </mi> 
       <mrow> 
        <mi>
          p 
        </mi> 
        <mi>
          r 
        </mi> 
        <mi>
          e 
        </mi> 
       </mrow> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mfrac> 
               <mrow> 
                <mi>
                  ℏ 
                </mi> 
                <mi>
                  c 
                </mi> 
               </mrow> 
               <mrow> 
                <msub> 
                 <mi>
                   T 
                 </mi> 
                 <mn>
                   0 
                 </mn> 
                </msub> 
                <mrow> 
                 <mo>
                   ( 
                 </mo> 
                 <mrow> 
                  <mn>
                    1 
                  </mn> 
                  <mo>
                    + 
                  </mo> 
                  <msub> 
                   <mi>
                     z 
                   </mi> 
                   <mrow> 
                    <mi>
                      o 
                    </mi> 
                    <mi>
                      b 
                    </mi> 
                    <mi>
                      s 
                    </mi> 
                   </mrow> 
                  </msub> 
                 </mrow> 
                 <mo>
                   ) 
                 </mo> 
                </mrow> 
                <msub> 
                 <mi>
                   k 
                 </mi> 
                 <mi>
                   b 
                 </mi> 
                </msub> 
                <mn>
                  4 
                </mn> 
                <mi>
                  π 
                </mi> 
               </mrow> 
              </mfrac> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <msub> 
             <mi>
               l 
             </mi> 
             <mi>
               p 
             </mi> 
            </msub> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1. 
      </mn> 
     </mrow> 
    </math> (29)</p>
   <p>The only difference in our approach (compared to in the previous section) is that we now substitute the CMB temperature measured by Fixsen (2009) for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. In the previous example, we assumed that we knew 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and tried to find 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. We can now use 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
       <mi>
         H 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mi>
         c 
       </mi> 
       <mrow> 
        <msub> 
         <mi>
           H 
         </mi> 
         <mn>
           0 
         </mn> 
        </msub> 
       </mrow> 
      </mfrac> 
     </mrow> 
    </math> to solve for 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>In <xref ref-type="fig" rid="fig6">
     Figure 6
    </xref>, once again, the actual observed redshifts for all 2287 supernovae in the PantheonPlusSH0ES database are represented as the blue line. As we can see, the red line indicates that this was an underestimated Hubble constant value, as our redshift prediction formula is inversely related to 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>. Accordingly, we next guess a much higher Hubble constant value, for example 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        80 
      </mn> 
     </mrow> 
    </math> km/s/Mpc, which gives redshift predictions correlating to the green line. Now the redshift predictions are too low. By simple trial-and-error, or by “intelligent” trial-and-error methods, such as the Newton-Raphson method or the bisection method, we can find the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> that minimizes the errors between predicted and observed redshifts.</p>
   <fig id="fig6" position="float">
    <label>Figure 6</label>
    <caption>
     <title>Figure 6. This figure shows observed redshift values from 2287 type Ia supernovae, sorted by redshift (blue line). We find that, by assuming the measured CMB temperature by Fixen (2009) of 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msubsup> 
   
         <mrow> 
    
          <mn>
           
     2.72548
    
          </mn>
   
         </mrow> 
   
         <mrow> 
    
          <mo>
           
     −
    
          </mo>
    
          <mn>
           
     0.00057
    
          </mn>
   
         </mrow> 
   
         <mrow> 
    
          <mo>
           
     +
    
          </mo>
    
          <mn>
           
     0.00057
    
          </mn>
   
         </mrow> 
  
        </msubsup> 
  
        <mtext>
         
    
  
        </mtext>
  
        <mtext>
         
   K
  
        </mtext>
 
       </mrow>

      </math>, the red line represents our predictions based on a wild guess of 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    H
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <mn>
         
   50
  
        </mn>
 
       </mrow>

      </math> km/s/Mpc, and the green line represents predictions based on a wild guess of 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    H
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <mn>
         
   80
  
        </mn>
 
       </mrow>

      </math> km/s/Mpc.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId537.jpeg?20250228035728" />
   </fig>
   <fig id="fig7" position="float">
    <label>Figure 7</label>
    <caption>
     <title>Figure 7. This figure shows observed redshift values from 2287 type Ia supernovae, sorted by redshift (blue line). Based upon the measured CMB temperature by Fixen (2009) of 2.72548 K, the red line represents our predictions based on 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    H
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <mn>
         
   66.8943
  
        </mn>
 
       </mrow>

      </math> km/s/Mpc, which we extracted from the redshift data using our trial-and-error approach. So, we find that there is a match between observed and predicted redshifts. Remarkably, the same 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    H
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
 
       </mrow>

      </math> value was predicted in 2015 by Tatum et al., using only this Fixen CMB temperature.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId544.jpeg?20250228035728" />
   </fig>
   <p>
    <xref ref-type="fig" rid="fig7">
     Figure 7
    </xref> shows the end-result. Here we are using the Fixen (2009) CMB temperature of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msubsup> 
       <mrow> 
        <mn>
          2.72548 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.00057 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.00057 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>. From this, in combination with the 2287 supernovae PantheonPlusSH0ES redshift data, a best fit is achieved with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          66.8943 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
      </msubsup> 
     </mrow> 
    </math> km/s/Mpc (corresponding to a 1STD range of 66.8656 to 66.9230 km/s/Mpc). This is well inside the 95% confidence interval given by the Particle Data Group (PDG) Astrophysical Constants and Parameters, which gives 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        67.4 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> km/s/Mpc for the 95% confidence interval. This trial-and-error methodology has recently been validated with a closed form solution (see Haug <xref ref-type="bibr" rid="scirp.140972-53">
     [53]
    </xref>) to the Hubble tension based on the same underlying Haug and Tatum cosmology model presented herein. This gives us great confidence in our methodology and in an actual duality between 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math>.</p>
   <p>Here, it is important to be aware that we are able to achieve essentially a perfect fit with all of the PantheonPlusSH0ES database supernovae using either a single measured Hubble constant value or a single measured CMB temperature. This appears to us to solve the Hubble tension problem in favor of the Planck Collaboration Hubble constant determination. The Hubble constant value cannot be measured directly; it is the redshift that is measured in the incorporated type of Ia supernova studies. The Hubble constant is estimated, and therefore relies on a model-based definition of redshift. In this paper, we use a new redshift model rooted in our new understanding of the inter-relationships between the current CMB temperature, the current Hubble constant, and cosmological redshifts; see <xref ref-type="bibr" rid="scirp.140972-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.140972-4">
     [4]
    </xref> <xref ref-type="bibr" rid="scirp.140972-54">
     [54]
    </xref>. This approach is clearly consistent with black hole variants 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> cosmological models.</p>
   <p>Our results are also fully in-line with the recent findings of Tatum et al. <xref ref-type="bibr" rid="scirp.140972-55">
     [55]
    </xref> that one can accurately find 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> from knowing the current CMB temperature, or vice-versa, something which the Λ-CDM model cannot do at present, as far as we know. Herein, we have taken an additional step forward and linked these two cosmological parameters to cosmological redshift. These inter-relationships are consistent with core principles in such 
    <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> cosmology model variants in general, and FSC in particular.</p>
   <p>In retrospect, the PantheonPlusSH0ES dataset relied upon in this paper appears to be particularly useful in solving the Hubble tension problem. Firstly, it is a rich dataset of 2287 type Ia supernova redshifts spanning the astronomical distance ladder, all of which have been incorporated into our parameter-matching algorithm. Our use of so many data points, in conjunction with the modern precision in measuring the CMB temperature, undoubtedly contributes to the remarkably low uncertainty in the derived (i.e. matched) Hubble constant values given above. This speaks to the power of using a carefully designed method, as employed herein. Furthermore, it speaks to the robust nature of our methodology that we have used the “local universe” dataset of supernova redshifts to severely challenge the reliance of other recent local universe studies upon the remote astronomical distance ladder for Hubble constant determination. The Riess et al. SH0ES studies, for instance, have relied heavily on correct calibrations of the astronomical distance ladder for their Hubble constant determination accuracy. We believe that our Hubble constant, cosmological distance, and redshift formula comparisons in Sections 2 and 3, particularly with reference to Equation (9) of standard cosmology and Equation (18) derived within our 
    <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> cosmology subclass, have much to do with solving this tension. The text following Equation (23) and preceding the <xref ref-type="fig" rid="fig1">
     Figure 1
    </xref> description can be regarded as the crux of this paper.</p>
   <p>It is also important to ask what the dataset of Baryonic Acoustic Oscillations (BAO) might reveal with respect to our Hubble tension solution. With respect to BAO data, Melia has extensively evaluated different cosmological models in comparison to the linear 
    <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> model. His recent study <xref ref-type="bibr" rid="scirp.140972-56">
     [56]
    </xref> of BAOs in the Lyman-alpha forest at an effective redshift of 2.334 concludes that the results are “completely consistent with the cosmic geometry predicted by 
    <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>”. He further points out that the results also provide “strong evidence disfavoring the standard model”. Melia’s work has demonstrated other successes of linear 
    <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 in comparison to Λ-CDM with respect to observational data; see, for instance, <xref ref-type="bibr" rid="scirp.140972-57">
     [57]
    </xref>.</p>
   <p>In summary, we conclude that the Planck Collaboration Hubble constant value of 67.4 ± 0.5 km/s/Mpc <xref ref-type="bibr" rid="scirp.140972-58">
     [58]
    </xref> is strongly supported by the PantheonPlusSH0ES supernova redshift dataset. We also conclude that the Riess et al. SH0ES study Hubble constant value of 73.04 ± 1.04 km/s/Mpc <xref ref-type="bibr" rid="scirp.140972-59">
     [59]
    </xref> is strongly disfavored by the PantheonPlusSH0ES supernova redshift dataset, at least within 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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      <mo>
        = 
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      </mi> 
      <mi>
        t 
      </mi> 
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    </math> cosmology. Nevertheless, ongoing studies and comparisons of the different models are recommended. Murakami et al. <xref ref-type="bibr" rid="scirp.140972-60">
     [60]
    </xref> have recently improved their estimate of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> using the full distance ladder of Type Ia supernovae (SN Ia) to determine 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mn>
        73.01 
      </mn> 
      <mo>
        ± 
      </mo> 
      <mn>
        0.92 
      </mn> 
     </mrow> 
    </math> km/s/Mpc. Although this is impressive within the mathematical lens of the Λ-CDM model, we must conclude that our new approach to examining cosmological redshifts in relation to CMB temperature does not align with this value when also utilizing the full distance ladder of SN Ia redshifts in conjunction with our 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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      <mo>
        = 
      </mo> 
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        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> model. In sharp contrast, 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> 
      <msubsup> 
       <mrow> 
        <mn>
          66.8943 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
      </msubsup> 
     </mrow> 
    </math> km/s/Mpc. While we do not expect this to be automatically accepted, we hope that our results will encourage other research groups to closely examine our new cosmological model, which is consistent with the 
    <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> principle and seems to resolve the Hubble tension in addition to reducing uncertainty in the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> value compared to other models and methods.</p>
   <p>There are also other types of observations not discussed in this study. For example, de Jaeger et al. <xref ref-type="bibr" rid="scirp.140972-61">
     [61]
    </xref> also estimate 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> from SNe II. However, they have correctly pointed out that, unlike SN Ia, “the SNe II are not standard candles”, and therefore, they have to be standardized through theoretical or empirical methods, as pointed out by the authors of that study. A database of SNe II observations is clearly something that also could be of interest to explore within our model framework, but it falls outside the scope of our current paper, and we strongly doubt that it would change our conclusions, if pursued. However, we suggest it here as yet another dataset one could investigate using this method. We have first chosen SN Ia observations, simply because they are known as our best standardized candles, covering the full distance ladder.</p>
  </sec><sec id="s6">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>6. Cosmic Evolution</title>
   <p>Cosmic evolution in 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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        = 
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      <mi>
        t 
      </mi> 
     </mrow> 
    </math> cosmology has been discussed in considerable detail by Melia <xref ref-type="bibr" rid="scirp.140972-62">
     [62]
    </xref>. Melia points out that:</p>
   <p>“As of today, more than 27 different kinds of observation have been used in comparative studies between this model and Λ-CDM, at both high and low redshifts, employing a broad range of integrated and differential measures, such as the luminosity and angular diameter distances, the redshift-dependent expansion rate, and the redshift-age relationship. In all of the tests completed and published thus far, 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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         R 
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      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> has accounted for the data at least as well as the standard model, and often much better.”</p>
   <p>Melia <xref ref-type="bibr" rid="scirp.140972-63">
     [63]
    </xref> has recently noted that observations from the James Webb Space Telescope (JWST) strongly support the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> cosmology timeline and severely challenge the timeline predicted by Λ-CDM. Melia’s findings align well with the 
    <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 presented herein, which also predicts an age of the universe of 14.6 billion years <xref ref-type="bibr" rid="scirp.140972-64">
     [64]
    </xref>.</p>
   <p>In our solution to the Hubble tension under 
    <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> cosmology, we obtain 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          66.8943 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
      </msubsup> 
     </mrow> 
    </math> km/s/Mpc, which corresponds to an age of the universe of 14.6 billion years. This provides approximately 800 million years more than the Λ-CDM model, potentially explaining why early galaxies appear to be so well-formed at the great distances observed by the James Webb Space Telescope. For a detailed discussion, see Haug and Tatum <xref ref-type="bibr" rid="scirp.140972-65">
     [65]
    </xref>. The ongoing debate in the literature about the advantages and disadvantages of various cosmological models is essential for scientific progress. Given the recent developments, we believe that it is too early to draw definitive conclusions; further investigation is necessary. In this spirit, the present paper contributes additional insights into 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> models, specifically focusing on a promising version of the 
    <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> model which appears to resolve the Hubble tension.</p>
   <p>We have already derived quantities such as the radiation density from our model <xref ref-type="bibr" rid="scirp.140972-66">
     [66]
    </xref> and obtained 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         Ω 
       </mi> 
       <mi>
         γ 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <mrow> 
       <mrow> 
        <msub> 
         <mi>
           ρ 
         </mi> 
         <mi>
           γ 
         </mi> 
        </msub> 
       </mrow> 
       <mo>
         / 
       </mo> 
       <mrow> 
        <msub> 
         <mi>
           ρ 
         </mi> 
         <mrow> 
          <mi>
            c 
          </mi> 
          <mi>
            r 
          </mi> 
          <mi>
            i 
          </mi> 
          <mi>
            t 
          </mi> 
         </mrow> 
        </msub> 
       </mrow> 
      </mrow> 
      <mo>
        ≈ 
      </mo> 
      <mn>
        5.53 
      </mn> 
      <mo>
        × 
      </mo> 
      <msup> 
       <mrow> 
        <mn>
          10 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          5 
        </mn> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, which lies well within the 95% confidence interval for the radiation density reported by the Particle Data Group (PDG), where the 95% confidence interval is 5.08 × 10<sup>−</sup><sup>5</sup> to 5.68 × 10<sup>−</sup><sup>5</sup> (5.35 ± 0.15 × 10<sup>−</sup><sup>5</sup> for 1STD). Our radiation density value is derived from the Friedmann equation in its recent thermodynamic form (see again <xref ref-type="bibr" rid="scirp.140972-65">
     [65]
    </xref>) connected to our variant of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
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      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> model. Precisely how multiple new derivations from our model should be interpreted physically in cosmological evolution remains open to discussion, but the most important point at this stage is that the predictions from our model which we have examined so far appear to fit observations quite well. Although there are still open questions concerning our model, we believe that additional research with respect to our model should help to determine whether this model is truly preferable over others. So far, it appears to be extremely promising in addressing the Hubble tension and other problems, such as providing a possible explanation for the puzzling early galaxy formation observations made by JWST <xref ref-type="bibr" rid="scirp.140972-67">
     [67]
    </xref>.</p>
   <p>An open question within the 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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         R 
       </mi> 
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        = 
      </mo> 
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      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> model introduced in this paper, is the matter and energy content at different cosmic epochs. Whether these can be precisely predicted within our model remains unclear and requires further investigation. However, what we have examined so far in our model appears to be consistent with observational data. Recently, we published our predicted Hubble parameter evolution and cosmological distances covering the full distance ladder of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> values from 0 to 2. This was done in order to compare our predictions to observations within the six different redshift bins selected for the pending final DESI BAO study report; see Tatum and Haug <xref ref-type="bibr" rid="scirp.140972-68">
     [68]
    </xref> for more details.</p>
  </sec><sec id="s7">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>7. Has Our Solution to the Hubble Tension Provided Us with New Universal Laws of Cosmology?</title>
   <p>
    <xref ref-type="fig" rid="fig7">
     Figure 7
    </xref> seems almost too good to be true. There may be a tendency to react in such a way, but the math appears to indicate otherwise. One even wonders if there are “new universal laws of cosmology” revealed by such an approach, because there appear to be exact relationships between the Hubble constant, cosmological redshift and the CMB temperature, without requiring such concepts as dark energy acceleration and superluminal space-time expansion.</p>
   <p>Naturally, it is not for us to say whether we have discovered “new universal laws”. But we do wonder about this. Clearly, we have not simply found broad statistical correlations between these parameters, but rather very precise mathematical inter-relationships between them. If one knows any two of these cosmological parameters with high precision, one can automatically solve for the other with high precision. To take but one example, if one knows the CMB temperature and the Hubble constant, one can precisely estimate the cosmological redshift for a given cosmological distance. There is hardly any wiggle room. We find that a convenient way to illustrate this is in <xref ref-type="fig" rid="fig8">
     Figure 8
    </xref>.</p>
   <fig id="fig8" position="float">
    <label>Figure 8</label>
    <caption>
     <title>Figure 8. This figure highlights the key equations which we suggest will be important for future progress along the lines developed in this paper.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId595.jpeg?20250228035730" />
   </fig>
   <p>The formula in the middle of the triangle demonstrates that the Hubble constant and the CMB temperature are simply connected by a composite constant that we have called Upsilon (the Latin symbol for Upsilon<sup>4</sup>): 
    <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ℧ 
      </mi> 
      <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> 
     </mrow> 
    </math>. When we ponder these inter-relationships, we are left asking if the Lambda-CDM model can accommodate them, or whether they are appropriate for a new paradigm represented by such 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
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    </math> model variants in general, and the FSC model in particular. We leave this question for others to ponder as well. It is worth mentioning that our model framework here is also consistent with a new thermodynamic approach to rewriting the Friedmann equation, which is fully consistent with the general theory of relativity; see again <xref ref-type="bibr" rid="scirp.140972-65">
     [65]
    </xref> and also <xref ref-type="bibr" rid="scirp.140972-69">
     [69]
    </xref>.</p>
  </sec><sec id="s8">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>8. Additional Comments Concerning Models and Analytic Methods Used</title>
   <p>In addition to our particularly useful Model B, Model A can be similarly explored, but only if one accepts 
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      <mo>
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         <mrow> 
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          </mo> 
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           ) 
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        </mrow> 
       </mrow> 
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         </mn> 
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     </mrow> 
    </math>, which contradicts observational studies of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mi>
       z 
     </mi> 
    </math> versus CMB temperature.</p>
   <p>One could also consider a hypothetical case where 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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      </mi> 
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      </mo> 
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      <mo>
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      </mo> 
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      </mn> 
     </mrow> 
    </math> and 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
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       </mi> 
       <mi>
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       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
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       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>. <xref ref-type="fig" rid="fig9">
     Figure 9
    </xref> illustrates the observed versus predicted redshifts, when assuming this and the current observed CMB temperature of 2.72548 K from Fixsen (2009). Here, we no longer have exact relationships that hold in practice, but merely statistical relationships. The resulting Pearson correlation coefficient between predicted and observed temperatures is 0.99813, indicating a high correlation, but only a correlation and not an exact relationship. The actual match between observed and predicted values is now weak, as can be clearly seen in <xref ref-type="fig" rid="fig9">
     Figure 9
    </xref>. One could only resolve this by introducing an additional parameter, such as an accelerating dark energy. However, an accelerating dark energy is not necessary to achieve a perfect match between predicted and observed supernova redshifts when there is an exact mathematical inter-relationship between the CMB temperature and cosmological redshifts, as shown in the sections above.</p>
   <p>Furthermore, without these exact relationships, simple but powerful optimization methods such as Newton-Raphson or bisection would generally fail to find a perfect match. Regardless of the parameter optimization method used, there would likely be failure to match results in a simple way when such exact relationships do not actually exist.</p>
   <p>
    <xref ref-type="fig" rid="fig10">
     Figure 10
    </xref> presents a suboptimal 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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    </math> model where the redshift is defined as 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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      </mi> 
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      </mo> 
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    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
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        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>. The Pearson correlation between predicted and observed values is 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        ρ 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0.99211 
      </mn> 
     </mrow> 
    </math>, but achieving a “perfect” match, as we have demonstrated in previous sections, is unattainable because the model is inconsistent with reality. Without knowledge of better models, one might in this model be tempted to propose a new type of exotic energy which decelerates the universe to align with observations. This is in sharp contrast to the immediately preceding model. However, as we have clearly shown with our Model B in previous sections, such ad hoc adjustments are completely unnecessary. It appears that one can match the supernova redshifts perfectly if the model simply uses 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        z 
      </mi> 
      <mo>
        = 
      </mo> 
      <msqrt> 
       <mrow> 
        <mfrac> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
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             H 
           </mi> 
          </msub> 
         </mrow> 
         <mrow> 
          <msub> 
           <mi>
             R 
           </mi> 
           <mi>
             t 
           </mi> 
          </msub> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </msqrt> 
      <mo>
        − 
      </mo> 
      <mn>
        1 
      </mn> 
     </mrow> 
    </math> in combination with 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mrow> 
       <mo>
         ( 
       </mo> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          + 
        </mo> 
        <mi>
          z 
        </mi> 
       </mrow> 
       <mo>
         ) 
       </mo> 
      </mrow> 
     </mrow> 
    </math>, which we call Model B.</p>
   <fig id="fig9" position="float">
    <label>Figure 9</label>
    <caption>
     <title>Figure 9. This figure shows observed redshift values from 2287 type Ia supernovae, sorted by redshift (blue line). The red line shows predicted redshifts when using a CMB temperature of 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <mn>
         
   2.72548
  
        </mn>
  
        <mtext>
         
    
  
        </mtext>
  
        <mtext>
         
   K
  
        </mtext>
 
       </mrow>

      </math> and assuming a 

      <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> model with 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <mi>
         
   z
  
        </mi>
  
        <mo>
         
   =
  
        </mo>
  
        <msqrt> 
   
         <mrow> 
    
          <mfrac> 
     
           <mrow> 
            <msub> 
             <mi>
               R 
             </mi> 
             <mi>
               H 
             </mi> 
            </msub> 
           </mrow> 
     
           <mrow> 
            <msub> 
             <mi>
               R 
             </mi> 
             <mi>
               t 
             </mi> 
            </msub> 
           </mrow> 
    
          </mfrac> 
   
         </mrow> 
  
        </msqrt> 
  
        <mo>
         
   −
  
        </mo>
  
        <mn>
         
   1
  
        </mn>
 
       </mrow>

      </math> and 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mi>
          
    t
   
         </mi> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <msup> 
   
         <mrow> 
    
          <mrow>
     
           <mo>
             ( 
           </mo> 
     
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              + 
            </mo> 
            <mi>
              z 
            </mi> 
           </mrow> 
     
           <mo>
             ) 
           </mo>
    
          </mrow>
   
         </mrow> 
   
         <mrow> 
    
          <mfrac> 
     
           <mn>
             1 
           </mn> 
     
           <mn>
             2 
           </mn> 
    
          </mfrac> 
   
         </mrow> 
  
        </msup> 
 
       </mrow>

      </math>. We clearly see that there is no way for the predicted redshifts to match the observed redshifts. One solution might be to introduce a hypothesis of dark energy acceleration on top of the model, but this is not needed in our Model B when properly and consistently applied.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId619.jpeg?20250228035731" />
   </fig>
   <fig id="fig10" position="float">
    <label>Figure 10</label>
    <caption>
     <title>Figure 10. This figure shows observed redshift values from 2287 type Ia supernovae, sorted by redshift (blue line). The red line shows predicted redshifts when using a CMB temperature of 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <mn>
         
   2.72548
  
        </mn>
  
        <mtext>
         
    
  
        </mtext>
  
        <mtext>
         
   K
  
        </mtext>
 
       </mrow>

      </math> and assuming a 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
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         </mi> 
   
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        </mo>
  
        <mi>
         
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        </mi>
  
        <mi>
         
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        </mi>
 
       </mrow>

      </math> model with 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <mi>
         
   z
  
        </mi>
  
        <mo>
         
   =
  
        </mo>
  
        <mfrac> 
   
         <mrow> 
    
          <msub> 
     
           <mi>
             R 
           </mi> 
     
           <mi>
             H 
           </mi> 
    
          </msub> 
   
         </mrow> 
   
         <mrow> 
    
          <msub> 
     
           <mi>
             R 
           </mi> 
     
           <mi>
             t 
           </mi> 
    
          </msub> 
   
         </mrow> 
  
        </mfrac> 
  
        <mo>
         
   −
  
        </mo>
  
        <mn>
         
   1
  
        </mn>
 
       </mrow>

      </math> and 

      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mi>
          
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         </mi> 
  
        </msub> 
  
        <mo>
         
   =
  
        </mo>
  
        <msub> 
   
         <mi>
          
    T
   
         </mi> 
   
         <mn>
          
    0
   
         </mn> 
  
        </msub> 
  
        <mrow>
   
         <mo>
          
    (
   
         </mo> 
   
         <mrow> 
    
          <mn>
           
     1
    
          </mn>
    
          <mo>
           
     +
    
          </mo>
    
          <mi>
           
     z
    
          </mi>
   
         </mrow> 
   
         <mo>
          
    )
   
         </mo>
  
        </mrow>
 
       </mrow>

      </math>. We clearly see that there is no way for the predicted redshifts to match the observed redshifts without adding more assumptions on top of this particular model.</title>
    </caption>
    <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1724020-rId628.jpeg?20250228035731" />
   </fig>
  </sec><sec id="s9">
   <title>
    <xref ref-type="bibr" rid="scirp.140972-"></xref>9. Conclusions</title>
   <p>In the context of growing black hole 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         R 
       </mi> 
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      <mo>
        = 
      </mo> 
      <mi>
        c 
      </mi> 
      <mi>
        t 
      </mi> 
     </mrow> 
    </math> model variants, we now have a robust theoretical framework for predicting the Cosmic Microwave Background (CMB) temperature by using a known Hubble constant value or vice versa <xref ref-type="bibr" rid="scirp.140972-1">
     [1]
    </xref> <xref ref-type="bibr" rid="scirp.140972-5">
     [5]
    </xref> <xref ref-type="bibr" rid="scirp.140972-55">
     [55]
    </xref>. This can be done both for present and past cosmic epochs (presumably), as well as in relation to cosmological redshifts. This framework initially emerged from the FSC cosmological model proposed by Tatum et al. However, it is worth exploring whether it can also be applied to other 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> models. The theory appears to be compatible with the relationship 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mi>
         t 
       </mi> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <msup> 
       <mrow> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mi>
            z 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
       <mrow> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mi>
          β 
        </mi> 
       </mrow> 
      </msup> 
     </mrow> 
    </math>, but only when 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mn>
        0 
      </mn> 
     </mrow> 
    </math> or 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <mi>
        β 
      </mi> 
      <mo>
        = 
      </mo> 
      <mfrac> 
       <mn>
         1 
       </mn> 
       <mn>
         2 
       </mn> 
      </mfrac> 
     </mrow> 
    </math>. Although it appears that we are gaining a new perspective on understanding and investigating cosmological redshift, further theoretical and observational studies are needed in order to reach a final consensus. There is still much to be discovered.</p>
   <p>In this paper, we have demonstrated, from the observed redshifts of 2287 type Ia supernovae (the PantheonPlusSH0ES database), how to achieve a perfect match between a particular Hubble constant value 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> and a 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
     </mrow> 
    </math> value from a high-precision CMB study. We refined our predictions by minimizing errors in our redshift prediction formula relative to the observed redshifts from the same 2287 type Ia supernovae. To give a prime example, utilizing the CMB temperature from Fixen (2009) of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         T 
       </mi> 
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       </mn> 
      </msub> 
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        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          2.72548 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.00057 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.00057 
        </mn> 
       </mrow> 
      </msubsup> 
      <mtext>
          
      </mtext> 
      <mtext>
        K 
      </mtext> 
     </mrow> 
    </math>, we derive a Hubble constant value from the full supernova database of 
    <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
      <msub> 
       <mi>
         H 
       </mi> 
       <mn>
         0 
       </mn> 
      </msub> 
      <mo>
        = 
      </mo> 
      <msubsup> 
       <mrow> 
        <mn>
          66.8943 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          − 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
       <mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          0.0287 
        </mn> 
       </mrow> 
      </msubsup> 
     </mrow> 
    </math> km/s/Mpc. Remarkably, our redshift formula can accurately predict the redshift of every supernova in the PantheonPlusSH0ES supernova database after calibration for distance. While this process resembles curve-fitting, the only free parameters are either the Hubble constant or the CMB temperature, with one being derived from measurement and the other automatically determined as a result. These results are consistent with the predictive power mentioned in References <xref ref-type="bibr" rid="scirp.140972-54">
     [54]
    </xref> <xref ref-type="bibr" rid="scirp.140972-55">
     [55]
    </xref>. Accordingly, we believe that our new approach has likely resolved the Hubble tension problem in favor of the Planck-based CMB-derived Hubble constant value. Nevertheless, our work should undergo careful scrutiny by others before drawing any lasting conclusions.</p>
  </sec><sec id="s10">
   <title>Data Availability Statements</title>
   <p>The supernova PantheonPlusSH0ES database that we have used can be found here: <xref ref-type="bibr" rid="scirp.140972-https://github.com/PantheonPlusSH0ES/DataRelease/blob/main/Pantheon%2B_Data/1_DATA/all_redshifts_PVs.csv">
     https://github.com/PantheonPlusSH0ES/DataRelease/blob/main/Pantheon%2B_Data/1_DATA/all_redshifts_PVs.csv
    </xref>.</p>
  </sec><sec id="s11">
   <title>NOTES</title>
   <p><sup>1</sup><xref ref-type="bibr" rid="scirp.140972-https://pdg.lbl.gov/2023/reviews/rpp2023-rev-astrophysical-constants.pdf">
     https://pdg.lbl.gov/2023/reviews/rpp2023-rev-astrophysical-constants.pdf
    </xref>.</p>
   <p><sup>2</sup>There could naturally be additional methods not discovered here, for example based on new cosmology or other metrics.</p>
   <p><sup>3</sup><xref ref-type="bibr" rid="scirp.140972-https://pdg.lbl.gov/2023/reviews/rpp2023-rev-astrophysical-constants.pdf">
     https://pdg.lbl.gov/2023/reviews/rpp2023-rev-astrophysical-constants.pdf
    </xref>.</p>
   <p><sup>4</sup>In the first paper about this formula, we used the Greek symbol for Upsilon: Υ.</p>
  </sec>
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