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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" dtd-version="1.4" xml:lang="en">
  <front>
    <journal-meta>
      <journal-id journal-id-type="publisher-id">ojmsi</journal-id>
      <journal-title-group>
        <journal-title>Open Journal of Modelling and Simulation</journal-title>
      </journal-title-group>
      <issn pub-type="epub">2327-4026</issn>
      <issn pub-type="ppub">2327-4018</issn>
      <publisher>
        <publisher-name>Scientific Research Publishing</publisher-name>
      </publisher>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.4236/ojmsi.2026.143005</article-id>
      <article-id pub-id-type="publisher-id">ojmsi-151184</article-id>
      <article-categories>
        <subj-group>
          <subject>Article</subject>
        </subj-group>
        <subj-group>
          <subject>Physics</subject>
          <subject>Mathematics</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title>Conservation of Energy in a Closed Universe and the Kinematic Illusion of Dark Energy</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <contrib-id contrib-id-type="orcid">0000-0001-5807-9821</contrib-id>
          <name name-style="western">
            <surname>Steynberg</surname>
            <given-names>André P.</given-names>
          </name>
          <xref ref-type="aff" rid="aff1">1</xref>
        </contrib>
      </contrib-group>
      <aff id="aff1"><label>1</label> Dublin, OH, USA </aff>
      <author-notes>
        <fn fn-type="conflict" id="fn-conflict">
          <p>The author declares no conflicts of interest regarding the publication of this paper.</p>
        </fn>
      </author-notes>
      <pub-date pub-type="epub">
        <day>09</day>
        <month>05</month>
        <year>2026</year>
      </pub-date>
      <pub-date pub-type="collection">
        <month>05</month>
        <year>2026</year>
      </pub-date>
      <volume>14</volume>
      <issue>03</issue>
      <fpage>73</fpage>
      <lpage>83</lpage>
      <history>
        <date date-type="received">
          <day>30</day>
          <month>03</month>
          <year>2026</year>
        </date>
        <date date-type="accepted">
          <day>06</day>
          <month>05</month>
          <year>2026</year>
        </date>
        <date date-type="published">
          <day>09</day>
          <month>05</month>
          <year>2026</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>© 2026 by the authors and Scientific Research Publishing Inc.</copyright-statement>
        <copyright-year>2026</copyright-year>
        <license license-type="open-access">
          <license-p> This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license ( <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link> ). </license-p>
        </license>
      </permissions>
      <self-uri content-type="doi" xlink:href="https://doi.org/10.4236/ojmsi.2026.143005">https://doi.org/10.4236/ojmsi.2026.143005</self-uri>
      <abstract>
        <p>We explore the thermodynamic lifecycle and macroscopic topology of a closed, temporally bifurcated spacetime manifold by applying the First Law of Thermodynamics and the Principle of Least Action to the primordial photon field. Utilizing a dimensionless equation linking the cosmic scale to the Planck scale, we demonstrate a linear geometric ratio mirroring the Schwarzschild geometry, necessitating a total invariant mass of <inline-formula><mml:math></mml:math></inline-formula></p>
        <p>2</p>
        <p>M</p>
        <p>u</p>
        <p>. To explain this physically, we propose a temporally bifurcated universe originating from a shared 5D torsion axis, which strictly separates a matter hemisphere from an equal antimatter hemisphere, thereby structurally bypassing the need for the Sakharov conditions to resolve Baryon Asymmetry. By evaluating the isotropic radiation pressure of the CMB traversing lines of zero spacetime interval, we offer a mathematical consistency argument—supported by the Isaacson effective stress-energy formulation—that the energy lost by the photon field is conserved as the mechanical work required to drive spherical volume expansion against the 5D Planck Stiffness (<inline-formula><mml:math></mml:math></inline-formula></p>
        <p>κ</p>
        <p>T</p>
        <p>=</p>
        <p>c</p>
        <p>4</p>
        <p>/G</p>
        <p>). Finally, we establish a temporal and spatial boundary (<inline-formula><mml:math></mml:math></inline-formula></p>
        <p>z≥1</p>
        <p>) for the application of this pure global expansion. At later historical times, isotropic expansion is superseded by localized gravitational clustering. By analyzing the Milky Way’s vantage point near the boundary of the Local Void, we provide quantitative scale checks demonstrating that the apparent “accelerated expansion” of nearby supernovae is a localized kinematic artifact—a bulk flow phenomenon—rendering the hypothesis of Dark Energy unnecessary.</p>
      </abstract>
      <kwd-group kwd-group-type="author-generated" xml:lang="en">
        <kwd>Geometric Monism</kwd>
        <kwd>Baryon Asymmetry</kwd>
        <kwd>Closed Universe</kwd>
        <kwd>Action Principle</kwd>
        <kwd>Dark Energy</kwd>
        <kwd>Local Void</kwd>
        <kwd>Type Ia Supernovae</kwd>
        <kwd>Bulk Flow</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec1">
      <title>1. Introduction: The Dimensionless Geometric Ratio</title>
      <p>The macroscopic topology of the universe can be formally constrained by a unified 5D Planck Stiffness (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> κ </mml:mi><mml:mi> T </mml:mi></mml:msub><mml:mo> = </mml:mo><mml:mrow><mml:mrow><mml:msup><mml:mi> c </mml:mi><mml:mn> 4 </mml:mn></mml:msup></mml:mrow><mml:mo> / </mml:mo><mml:mi> G </mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> ) [<xref ref-type="bibr" rid="B1">1</xref>]. To complete this physical framework, the microscopic topological constraints must be formally reconciled with the macroscopic boundary conditions of the universe. In earlier work, a dimensionless equation was derived linking the maximum parameters of a closed, finite spacetime manifold to the minimum Planck units [<xref ref-type="bibr" rid="B2">2</xref>]: </p>
      <disp-formula id="FD1">
        <label>(1)</label>
        <mml:math>
          <mml:mrow>
            <mml:mfrac>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>M</mml:mi>
                  <mml:mi>u</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>m</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>t</mml:mi>
                  <mml:mi>m</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mrow>
                <mml:mi>π</mml:mi>
                <mml:msub>
                  <mml:mi>t</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>l</mml:mi>
                  <mml:mi>m</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mrow>
                <mml:mi>π</mml:mi>
                <mml:msub>
                  <mml:mi>l</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>where <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> M </mml:mi><mml:mi> u </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mass of the observable universe, <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> t </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the maximum time dimension, and <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> l </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the maximum photon distance.</p>
      <p>The appearance of <inline-formula><mml:math><mml:mi> π </mml:mi></mml:math></inline-formula> in Equation (1) is an artifact of mapping a linear measurement to the spherical geometry of a 3-sphere manifold. When we compare the radial geometry directly, the maximum radius of the finite manifold <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> relates to the maximum time <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> t </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> via the circumference (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mi> m </mml:mi></mml:msub><mml:mo> = </mml:mo><mml:mrow><mml:mrow><mml:mn> 2 </mml:mn><mml:mi> c </mml:mi><mml:msub><mml:mi> t </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow><mml:mo> / </mml:mo><mml:mi> π </mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> ). By isolating <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> t </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from Equation (1) and substituting it into this geometric relation, the <inline-formula><mml:math><mml:mi> π </mml:mi></mml:math></inline-formula> terms cleanly cancel. Because the Planck length <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> l </mml:mi><mml:mi> P </mml:mi></mml:msub><mml:mo> = </mml:mo><mml:mi> c </mml:mi><mml:msub><mml:mi> t </mml:mi><mml:mi> P </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> , we derive the exact ratio between the radius of the macroscopic spacetime manifold and the Planck-scale torsion element: </p>
      <disp-formula id="FD2">
        <label>(2)</label>
        <mml:math>
          <mml:mrow>
            <mml:mfrac>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>R</mml:mi>
                  <mml:mi>m</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>l</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>=</mml:mo>
            <mml:mn>2</mml:mn>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mfrac>
                  <mml:mrow>
                    <mml:msub>
                      <mml:mi>M</mml:mi>
                      <mml:mi>u</mml:mi>
                    </mml:msub>
                  </mml:mrow>
                  <mml:mrow>
                    <mml:msub>
                      <mml:mi>m</mml:mi>
                      <mml:mi>P</mml:mi>
                    </mml:msub>
                  </mml:mrow>
                </mml:mfrac>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>The emergence of the factor of 2 is the exact geometric signature of the macroscopic Schwarzschild radius (<inline-formula><mml:math><mml:mrow><mml:mi> R </mml:mi><mml:mo> = </mml:mo><mml:mrow><mml:mrow><mml:mn> 2 </mml:mn><mml:mi> G </mml:mi><mml:mi> M </mml:mi></mml:mrow><mml:mo> / </mml:mo><mml:mrow><mml:msup><mml:mi> c </mml:mi><mml:mn> 2 </mml:mn></mml:msup></mml:mrow></mml:mrow></mml:mrow></mml:math></inline-formula> ). As formally proven in <bold>Appen</bold><bold>dix A</bold>, this is not an invalid application of a local static vacuum metric, but the strict analytical limit of the Friedmann equation evaluated at the global spatial maximum expansion (<inline-formula><mml:math><mml:mrow><mml:mover accent="true"><mml:mi> R </mml:mi><mml:mo> ˙ </mml:mo></mml:mover><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ).</p>
    </sec>
    <sec id="sec2">
      <title>2. The Antimatter Hemisphere and Temporal Bifurcation</title>
      <p>Standard cosmology is plagued by the Baryon Asymmetry problem. Standard baryogenesis models require the Sakharov conditions (baryon number violation, CP violation, and thermal non-equilibrium) to dynamically generate an imbalance from an initially mixed bath of matter and antimatter occupying the same 4D spatial volume.</p>
      <p>Geometric Monism offers a topological resolution that is consistent with Equation (2) while offering a topological alternative to these fine-tuned microphysical requirements. We hypothesize that the universe operates as a strictly closed system with a total mass of <inline-formula><mml:math><mml:mrow><mml:mn> 2 </mml:mn><mml:msub><mml:mi> M </mml:mi><mml:mi> u </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> , containing exactly equal quantities of matter and antimatter.</p>
      <sec id="sec2dot1">
        <title>
          The 5D Emergence Poles and the Shared Torsion Axis (
          <inline-formula>
            <mml:math>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>r</mml:mi>
                  <mml:mrow>
                    <mml:mi>m</mml:mi>
                    <mml:mi>i</mml:mi>
                    <mml:mi>n</mml:mi>
                  </mml:mrow>
                </mml:msub>
                <mml:mo>=</mml:mo>
                <mml:msub>
                  <mml:mi>l</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:math>
          </inline-formula>
          )
        </title>
        <p>At the conclusion of the previous spatial contraction cycle, the total energy of the universe is compressed into a primordial matter quark-gluon plasma and an equal antimatter quark-gluon plasma. These states are connected exclusively through a shared 5D torsion axis of radius <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> r </mml:mi><mml:mrow><mml:mi> min </mml:mi></mml:mrow></mml:msub><mml:mo> = </mml:mo><mml:msub><mml:mi> l </mml:mi><mml:mi> P </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> . This absolute minimum geometric boundary physically prevents an infinite-density singularity.</p>
        <p>At this temporal origin, the macroscopic matter and antimatter universes do not occupy the same 4D spatial volume; rather, they share the common central axis and immediately traverse in opposite temporal directions (<inline-formula><mml:math><mml:mrow><mml:mo> + </mml:mo><mml:mi> t </mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math><mml:mrow><mml:mo> − </mml:mo><mml:mi> t </mml:mi></mml:mrow></mml:math></inline-formula> ). Because they are topologically separated at emergence, their inverted chiralities never destructively interfere within the same 4D spacetime, geometrically preventing immediate total annihilation, as illustrated in <xref ref-type="fig" rid="fig1">Figure 1</xref>. The observed “asymmetry” is merely a local illusion resulting from our confinement entirely within the <inline-formula><mml:math><mml:mrow><mml:mo> + </mml:mo><mml:mi> t </mml:mi></mml:mrow></mml:math></inline-formula> temporal hemisphere.</p>
        <fig id="fig1">
          <label>Figure 1</label>
          <graphic xlink:href="https://html.scirp.org/file/2860345-rId65.jpeg?20260509023919" />
        </fig>
        <p><bold>Figure 1</bold><bold>.</bold>Temporal bifurcation on a truncated spacetime manifold (simplified by showing only one of the three identical space dimensions). The matter and antimatter hemispheres traverse opposite temporal longitudes until reaching the maximum spatial equator (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ), which enforces a gravitational turnaround.</p>
      </sec>
    </sec>
    <sec id="sec3">
      <title>3. Foundational Thermodynamic Assumptions</title>
      <p>Standard cosmology relies on the Friedmann equations, where redshifted photon energy is purportedly lost to “metric expansion” because global energy conservation cannot be formally defined in a non-stationary FLRW spacetime [<xref ref-type="bibr" rid="B3">3</xref>]. However, this limitation arises from a geometric asymmetry: standard models treat space as curved and potentially closed, while treating time as an infinite, uncurved coordinate.</p>
      <p>The present framework adopts the simplest symmetric assumption: time possesses exactly equal curvature to space. By modeling the universe as a fully closed <inline-formula><mml:math><mml:mrow><mml:msup><mml:mi> S </mml:mi><mml:mn> 3 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> manifold embedded within a 5D bulk, metric expansion is not a passive coordinate scaling, but a physical stretching of the manifold. Integrating the local covariant conservation law (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mo> ∇ </mml:mo><mml:mi> μ </mml:mi></mml:msub><mml:msup><mml:mi> T </mml:mi><mml:mrow><mml:mi> μ </mml:mi><mml:mi> ν </mml:mi></mml:mrow></mml:msup><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ) over this strictly finite volume yields a globally conserved quantity. We establish the following assumptions: </p>
      <p>1) <bold>Total Mass Conservation:</bold> The universe maintains a strictly conserved total invariant mass of <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> M </mml:mi><mml:mrow><mml:mi> t </mml:mi><mml:mi> o </mml:mi><mml:mi> t </mml:mi><mml:mi> a </mml:mi><mml:mi> l </mml:mi></mml:mrow></mml:msub><mml:mo> = </mml:mo><mml:mn> 2 </mml:mn><mml:msub><mml:mi> M </mml:mi><mml:mi> u </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> , defined exactly at the primordial temporal pole prior to expansion. </p>
      <p>2) <bold>Thermodynamic Isolation:</bold> The 3-sphere is perfectly adiabatic (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:mi> Q </mml:mi><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ). Energy is exclusively transferred between the internal radiation field and the geometric curvature of the manifold, without exchanging heat with the 5D bulk. </p>
      <p>3) <bold>Strict</bold><bold>Zero-Interval Propagation:</bold> The spatial traversal of photons (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:mi> x </mml:mi></mml:mrow></mml:math></inline-formula> ) is exactly bounded by their temporal traversal (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:mi> t </mml:mi></mml:mrow></mml:math></inline-formula> ), guaranteeing isotropic radiation pressure enforces spherical volume expansion. </p>
    </sec>
    <sec id="sec4">
      <title>4. Thermodynamic Work and the Adiabatic Expansion of Space</title>
      <p>Because the manifold is thermodynamically isolated (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:mi> Q </mml:mi><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ), the First Law of Thermodynamics dictates that any change in the internal energy (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:mi> U </mml:mi></mml:mrow></mml:math></inline-formula> ) of the primordial photons must be offset by the mechanical work done by the system: </p>
      <disp-formula id="FD3">
        <label>(3)</label>
        <mml:math>
          <mml:mrow>
            <mml:mi>d</mml:mi>
            <mml:mi>U</mml:mi>
            <mml:mo>+</mml:mo>
            <mml:mi>p</mml:mi>
            <mml:mi>d</mml:mi>
            <mml:mi>V</mml:mi>
            <mml:mo>=</mml:mo>
            <mml:mn>0</mml:mn>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>For relativistic photons (<inline-formula><mml:math><mml:mrow><mml:mi> p </mml:mi><mml:mo> = </mml:mo><mml:mrow><mml:mi> U </mml:mi><mml:mo> / </mml:mo><mml:mrow><mml:mn> 3 </mml:mn><mml:mi> V </mml:mi></mml:mrow></mml:mrow></mml:mrow></mml:math></inline-formula> ), integrating this relationship yields <inline-formula><mml:math><mml:mrow><mml:mi> U </mml:mi><mml:mo> ∝ </mml:mo><mml:msup><mml:mi> V </mml:mi><mml:mrow><mml:mo> − </mml:mo><mml:mrow><mml:mn> 1 </mml:mn><mml:mo> / </mml:mo><mml:mn> 3 </mml:mn></mml:mrow></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> . Because the spatial volume of a 3-sphere is proportional to the cube of its radius (<inline-formula><mml:math><mml:mrow><mml:mi> V </mml:mi><mml:mo> ∝ </mml:mo><mml:msup><mml:mi> R </mml:mi><mml:mn> 3 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> ), we find: </p>
      <disp-formula id="FD4">
        <label>(4)</label>
        <mml:math>
          <mml:mrow>
            <mml:mi>U</mml:mi>
            <mml:mo>∝</mml:mo>
            <mml:mfrac>
              <mml:mn>1</mml:mn>
              <mml:mi>R</mml:mi>
            </mml:mfrac>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>The macroscopic wavelength of the primordial photon field must scale linearly with the radius of the universe. The energy lost by the CMB photons is perfectly conserved as the mechanical work required to expand the spatial fabric of the manifold.</p>
      <sec id="sec4dot1">
        <title>The Energy Equivalence of Planck Stiffness</title>
        <p>Treating the geometric expansion of spacetime as mechanical work against a structural stiffness is not a Newtonian analogy, but a rigorous feature of relativistic continuum mechanics explicitly established by the Isaacson equation for gravitational waves [<xref ref-type="bibr" rid="B4">4</xref>]. The effective stress-energy tensor of a geometric metric perturbation (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> h </mml:mi><mml:mrow><mml:mi> α </mml:mi><mml:mi> β </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> ) is defined as: </p>
        <disp-formula id="FD5">
          <label>(5)</label>
          <mml:math>
            <mml:mrow>
              <mml:msubsup>
                <mml:mi>T</mml:mi>
                <mml:mrow>
                  <mml:mi>μ</mml:mi>
                  <mml:mi>ν</mml:mi>
                </mml:mrow>
                <mml:mrow>
                  <mml:mrow>
                    <mml:mo>(</mml:mo>
                    <mml:mrow>
                      <mml:mi>G</mml:mi>
                      <mml:mi>W</mml:mi>
                    </mml:mrow>
                    <mml:mo>)</mml:mo>
                  </mml:mrow>
                </mml:mrow>
              </mml:msubsup>
              <mml:mo>=</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>c</mml:mi>
                    <mml:mn>4</mml:mn>
                  </mml:msup>
                </mml:mrow>
                <mml:mrow>
                  <mml:mn>32</mml:mn>
                  <mml:mi>π</mml:mi>
                  <mml:mi>G</mml:mi>
                </mml:mrow>
              </mml:mfrac>
              <mml:mrow>
                <mml:mo>〈</mml:mo>
                <mml:mrow>
                  <mml:msub>
                    <mml:mo>∂</mml:mo>
                    <mml:mi>μ</mml:mi>
                  </mml:msub>
                  <mml:msub>
                    <mml:mi>h</mml:mi>
                    <mml:mrow>
                      <mml:mi>α</mml:mi>
                      <mml:mi>β</mml:mi>
                    </mml:mrow>
                  </mml:msub>
                  <mml:msub>
                    <mml:mo>∂</mml:mo>
                    <mml:mi>ν</mml:mi>
                  </mml:msub>
                  <mml:msup>
                    <mml:mi>h</mml:mi>
                    <mml:mrow>
                      <mml:mi>α</mml:mi>
                      <mml:mi>β</mml:mi>
                    </mml:mrow>
                  </mml:msup>
                </mml:mrow>
                <mml:mo>〉</mml:mo>
              </mml:mrow>
            </mml:mrow>
          </mml:math>
        </disp-formula>
        <p>This demonstrates that General Relativity natively translates geometric metric evolution into physical thermodynamic energy by multiplying the squared geometric gradient by the absolute Planck Stiffness (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> κ </mml:mi><mml:mi> T </mml:mi></mml:msub><mml:mo> = </mml:mo><mml:mrow><mml:mrow><mml:msup><mml:mi> c </mml:mi><mml:mn> 4 </mml:mn></mml:msup></mml:mrow><mml:mo> / </mml:mo><mml:mi> G </mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> ). In a finite, closed 3-sphere, the macroscopic expansion acts as a global geometric deformation. Therefore, the radiation pressure of the CMB performs tangible mechanical work (<inline-formula><mml:math><mml:mrow><mml:mo> − </mml:mo><mml:mi> p </mml:mi><mml:mi> d </mml:mi><mml:mi> V </mml:mi></mml:mrow></mml:math></inline-formula> ) against this exact relativistic stiffness to drive the metric expansion.</p>
      </sec>
    </sec>
    <sec id="sec5">
      <title>5. Pseudo-Riemannian Geometry and Null Geodesics</title>
      <p>To visualize how the radiation pressure enforces a perfectly isotropic spherical expansion, we must review the invariant spacetime interval (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:msup><mml:mi> s </mml:mi><mml:mn> 2 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> ), defined by the metric tensor <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> g </mml:mi><mml:mrow><mml:mi> μ </mml:mi><mml:mi> ν </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> : </p>
      <disp-formula id="FD6">
        <label>(6)</label>
        <mml:math>
          <mml:mrow>
            <mml:mi>d</mml:mi>
            <mml:msup>
              <mml:mi>s</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mo>=</mml:mo>
            <mml:msub>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msub>
            <mml:mi>d</mml:mi>
            <mml:msup>
              <mml:mi>x</mml:mi>
              <mml:mi>μ</mml:mi>
            </mml:msup>
            <mml:mi>d</mml:mi>
            <mml:msup>
              <mml:mi>x</mml:mi>
              <mml:mi>ν</mml:mi>
            </mml:msup>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>For a massless particle such as a photon, the trajectory is a null geodesic (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:msup><mml:mi> s </mml:mi><mml:mn> 2 </mml:mn></mml:msup><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ). In conformally flat space, this reduces Equation (6) to: </p>
      <disp-formula id="FD7">
        <label>(7)</label>
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>c</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mi>d</mml:mi>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mo>−</mml:mo>
            <mml:mi>d</mml:mi>
            <mml:msup>
              <mml:mi>x</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mo>=</mml:mo>
            <mml:mn>0</mml:mn>
            <mml:mo>⇒</mml:mo>
            <mml:mi>d</mml:mi>
            <mml:mi>x</mml:mi>
            <mml:mo>=</mml:mo>
            <mml:mi>c</mml:mi>
            <mml:mi>d</mml:mi>
            <mml:mi>t</mml:mi>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>This invariant zero interval is visualized in <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p>
      <fig id="fig2">
        <label>Figure 2</label>
        <graphic xlink:href="https://html.scirp.org/file/2860345-rId112.jpeg?20260509023919" />
      </fig>
      <p><bold>Figure 2</bold><bold>.</bold>A 1 + 1D pseudo-Riemannian spacetime diagram. The invariant zero interval (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:msup><mml:mi> s </mml:mi><mml:mn> 2 </mml:mn></mml:msup><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ) of the photon explicitly geometrically bounds the maximum spatial traversal (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:mi> x </mml:mi></mml:mrow></mml:math></inline-formula> ) to the temporal traversal (<inline-formula><mml:math><mml:mrow><mml:mi> c </mml:mi><mml:mi> d </mml:mi><mml:mi> t </mml:mi></mml:mrow></mml:math></inline-formula> ).</p>
      <p>In our closed, temporally bifurcated 3-sphere, Equation (7) ensures that spatial expansion is intrinsically bound to temporal traversal. As the initial expansion begins, each fundamental element of matter traces its own distinct temporal path. These individual timelike worldlines are geometrically represented as distinct lines of longitude tracing the surface of the expanding 3-sphere.</p>
      <p>While massive particles trace these distinct longitudinal worldlines, the primary photon paths traverse both longitude and latitude at an equal metric rate. This invariant zero interval causes the photon trajectories to act as rigid geometric boundaries, carving the surface of the 3-sphere into expanding operational quadrants, as depicted in <xref ref-type="fig" rid="fig3">Figure 3</xref>.</p>
    </sec>
    <sec id="sec6">
      <title>6. The Ultimate Dimensionless Symmetry and Action Formulation</title>
      <p>We can unify this entire lifecycle using the Principle of Least Action (<inline-formula><mml:math><mml:mrow><mml:mi> δ </mml:mi><mml:mi> S </mml:mi><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ). The total action <inline-formula><mml:math><mml:mi> S </mml:mi></mml:math></inline-formula> for our closed universe system can be expressed as: </p>
      <disp-formula id="FD8">
        <label>(8)</label>
        <mml:math>
          <mml:mrow>
            <mml:mi>S</mml:mi>
            <mml:mo>=</mml:mo>
            <mml:mstyle displaystyle="true">
              <mml:mrow>
                <mml:mo>∫</mml:mo>
                <mml:mrow>
                  <mml:mrow>
                    <mml:mo>(</mml:mo>
                    <mml:mrow>
                      <mml:mfrac>
                        <mml:mrow>
                          <mml:msub>
                            <mml:mi>κ</mml:mi>
                            <mml:mi>T</mml:mi>
                          </mml:msub>
                        </mml:mrow>
                        <mml:mrow>
                          <mml:mn>16</mml:mn>
                          <mml:mi>π</mml:mi>
                        </mml:mrow>
                      </mml:mfrac>
                      <mml:mi>R</mml:mi>
                      <mml:mo>+</mml:mo>
                      <mml:msub>
                        <mml:mi>ℒ</mml:mi>
                        <mml:mrow>
                          <mml:mi>r</mml:mi>
                          <mml:mi>a</mml:mi>
                          <mml:mi>d</mml:mi>
                        </mml:mrow>
                      </mml:msub>
                    </mml:mrow>
                    <mml:mo>)</mml:mo>
                  </mml:mrow>
                  <mml:msqrt>
                    <mml:mrow>
                      <mml:mo>−</mml:mo>
                      <mml:mi>g</mml:mi>
                    </mml:mrow>
                  </mml:msqrt>
                  <mml:mtext>
                     
                  </mml:mtext>
                  <mml:msup>
                    <mml:mtext>d</mml:mtext>
                    <mml:mn>4</mml:mn>
                  </mml:msup>
                  <mml:mi>x</mml:mi>
                </mml:mrow>
              </mml:mrow>
            </mml:mstyle>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>where <inline-formula><mml:math><mml:mi> R </mml:mi></mml:math></inline-formula> is the Ricci scalar curvature and <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> ℒ </mml:mi><mml:mrow><mml:mi> r </mml:mi><mml:mi> a </mml:mi><mml:mi> d </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the Lagrangian density of the primordial radiation field. By varying this action with respect to the metric tensor, the geometric curvature of the manifold (<inline-formula><mml:math><mml:mi> R </mml:mi></mml:math></inline-formula> ) is forced into strict dynamical equilibrium with the stress-energy tensor of the photons.</p>
      <fig id="fig3">
        <label>Figure 3</label>
        <graphic xlink:href="https://html.scirp.org/file/2860345-rId131.jpeg?20260509023920" />
      </fig>
      <p><bold>Figure 3</bold><bold>.</bold> Macroscopic mapping of the matter hemisphere. The four distinct primordial photon paths (<inline-formula><mml:math><mml:mrow><mml:mi> d </mml:mi><mml:msup><mml:mi> s </mml:mi><mml:mn> 2 </mml:mn></mml:msup><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ) propagate outward, carving the expanding 3-sphere into distinct operational quadrants until the longitudinal traversal halts at the spatial equator (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ).</p>
      <p>By defining the total mass of the initial state as <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> M </mml:mi><mml:mrow><mml:mi> t </mml:mi><mml:mi> o </mml:mi><mml:mi> t </mml:mi><mml:mi> a </mml:mi><mml:mi> l </mml:mi></mml:mrow></mml:msub><mml:mo> = </mml:mo><mml:mn> 2 </mml:mn><mml:msub><mml:mi> M </mml:mi><mml:mi> u </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> , we substitute this into our radial ratio (Equation (2)): </p>
      <disp-formula id="FD9">
        <label>(9)</label>
        <mml:math>
          <mml:mrow>
            <mml:mfrac>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>R</mml:mi>
                  <mml:mi>m</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>l</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>M</mml:mi>
                  <mml:mrow>
                    <mml:mi>t</mml:mi>
                    <mml:mi>o</mml:mi>
                    <mml:mi>t</mml:mi>
                    <mml:mi>a</mml:mi>
                    <mml:mi>l</mml:mi>
                  </mml:mrow>
                </mml:msub>
              </mml:mrow>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>m</mml:mi>
                  <mml:mi>P</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>At this spatial equator, the macroscopic radius (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mi> m </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ) is exactly the fundamental torsion radius (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> l </mml:mi><mml:mi> P </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ) scaled linearly by the ratio of the universe’s total mass to the Planck mass.</p>
      <p>At this critical boundary, the gravitational potential of the <inline-formula><mml:math><mml:mrow><mml:mn> 2 </mml:mn><mml:msub><mml:mi> M </mml:mi><mml:mi> u </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> total mass exactly equals the kinetic energy of the expansion, overcoming the diminished radiation pressure. This equator acts as a macroscopic Schwarzschild reflection limit, enforcing a gravitational turnaround and initiating the spatial contraction cycle. Because the matter and antimatter hemispheres are separated temporally rather than spatially, no spatial annihilation boundary exists across the observable universe, natively explaining the lack of gamma-ray annihilation signatures.</p>
    </sec>
    <sec id="sec7">
      <title>7. The Breakdown of Isotropic Kinematics</title>
      <p>The single-parameter closed universe model provides a geometric fit for cosmic expansion in the early universe, consistent with reported JWST observations of massive galaxies at extreme redshifts (<inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> ≥ </mml:mo><mml:mn> 15 </mml:mn></mml:mrow></mml:math></inline-formula> ) [<xref ref-type="bibr" rid="B5">5</xref>]. During the early universe (<inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> ≫ </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> ), the global matter distribution was highly uniform, and spatial expansion was purely adiabatic, driven uniformly by the isotropic radiation pressure against the 5D Planck Stiffness.</p>
      <p>The model defines redshift as: </p>
      <disp-formula id="FD10">
        <mml:math>
          <mml:mrow>
            <mml:mn>1</mml:mn>
            <mml:mo>+</mml:mo>
            <mml:mi>z</mml:mi>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:mi>sin</mml:mi>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mrow>
                        <mml:mn>13.8</mml:mn>
                      </mml:mrow>
                      <mml:mi>T</mml:mi>
                    </mml:mfrac>
                    <mml:mo>⋅</mml:mo>
                    <mml:mfrac>
                      <mml:mi>π</mml:mi>
                      <mml:mn>2</mml:mn>
                    </mml:mfrac>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mrow>
                <mml:mi>sin</mml:mi>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mi>t</mml:mi>
                      <mml:mi>T</mml:mi>
                    </mml:mfrac>
                    <mml:mo>⋅</mml:mo>
                    <mml:mfrac>
                      <mml:mi>π</mml:mi>
                      <mml:mn>2</mml:mn>
                    </mml:mfrac>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
            </mml:mfrac>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>This assumes that the Big Bang (time zero) was 13.8 billion years ago.</p>
      <p>The scale factor is: </p>
      <disp-formula id="FD11">
        <mml:math>
          <mml:mrow>
            <mml:mi>a</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mi>sin</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mfrac>
                  <mml:mrow>
                    <mml:mi>π</mml:mi>
                    <mml:mi>t</mml:mi>
                  </mml:mrow>
                  <mml:mrow>
                    <mml:mn>2</mml:mn>
                    <mml:mi>T</mml:mi>
                  </mml:mrow>
                </mml:mfrac>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>At <inline-formula><mml:math><mml:mrow><mml:mi> t </mml:mi><mml:mo> = </mml:mo><mml:mi> T </mml:mi></mml:mrow></mml:math></inline-formula> , <inline-formula><mml:math><mml:mrow><mml:mi> a </mml:mi><mml:mo> = </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> , and the 3-sphere’s radius is: </p>
      <disp-formula id="FD12">
        <mml:math>
          <mml:mrow>
            <mml:msub>
              <mml:mi>R</mml:mi>
              <mml:mi>m</mml:mi>
            </mml:msub>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:mn>2</mml:mn>
                <mml:mi>T</mml:mi>
              </mml:mrow>
              <mml:mi>π</mml:mi>
            </mml:mfrac>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>However, at a critical epoch, localized gravitational attraction began to overpower this uniform thermodynamic expansion, leading to the formation of the “cosmic web” and the evacuation of vast cosmic voids. To preserve the mathematical rigor of cosmic expansion models, data fitting for pure isotropic expansion must be restricted to redshifts <inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> ≥ </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> .</p>
      <p>This boundary is supported by large-scale structure formation literature. In N-body simulations (e.g., the Millennium Simulation), the epoch around <inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> ≈ </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> marks the critical transition where non-linear structure formation begins to radically dominate the universe’s matter distribution [<xref ref-type="bibr" rid="B6">6</xref>]. For observational data closer to the present time (<inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> &lt; </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> ), non-linear void evacuation and supercluster virialization dominate, and peculiar velocities of bulk flows become a significant, contaminating fraction of the measured recession velocity.</p>
    </sec>
    <sec id="sec8">
      <title>8. Re-Evaluating Late-Stage Redshift Data</title>
      <sec id="sec8dot1">
        <title>8.1. Methodology and Target Observables</title>
        <p>The foundational evidence for an accelerating universe—and consequently, Dark Energy—relies primarily on the luminosity-distance residuals of Type Ia Supernovae (SNe Ia) located at relatively low redshifts (<inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> &lt; </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> ). Standard models fit these observables to a Hubble diagram, assuming deviations from a linear Hubble law result from a changing global expansion rate (Λ). To extract this global metric, peculiar-velocity corrections are applied to subtract local kinematic motion.</p>
        <p>The methodology of this framework involves testing whether the peculiar-velocity corrections applied to <inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> &lt; </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> SNe Ia datasets are fundamentally contaminated by the Milky Way’s specific kinematic environment, mapped by recent large-scale cosmography surveys.</p>
      </sec>
      <sec id="sec8dot2">
        <title>8.2. Quantitative Scale Check of Kinematic Contamination</title>
        <p>At a benchmark redshift of <inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> ≈ </mml:mo><mml:mn> 0.05 </mml:mn></mml:mrow></mml:math></inline-formula> , the deviation from a linear Hubble flow required to fit the ΛCDM model corresponds to a distance modulus residual of approximately ~0.05 to 0.1 magnitudes [<xref ref-type="bibr" rid="B7">7</xref>][<xref ref-type="bibr" rid="B8">8</xref>]. Kinematically, this translates to an apparent excess recession velocity of roughly <inline-formula><mml:math><mml:mrow><mml:mi> Δ </mml:mi><mml:msub><mml:mi> v </mml:mi><mml:mi> Λ </mml:mi></mml:msub><mml:mo> ≈ </mml:mo><mml:mn> 200 </mml:mn><mml:mtext>   </mml:mtext><mml:mtext> - </mml:mtext><mml:mtext>   </mml:mtext><mml:mn> 400 </mml:mn></mml:mrow></mml:math></inline-formula> km/s.</p>
        <p>The Milky Way does not reside in a region of uniform density; we are located on the edge of the vast Local Void, deeply embedded within the branching structure of the massive Laniakea Supercluster [<xref ref-type="bibr" rid="B9">9</xref>][<xref ref-type="bibr" rid="B10">10</xref>]. The measured peculiar velocity of the Local Group—driven by gravitational repulsion from the void and attraction toward Shapley—is empirically established at approximately <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> v </mml:mi><mml:mrow><mml:mi> p </mml:mi><mml:mi> e </mml:mi><mml:mi> c </mml:mi></mml:mrow></mml:msub><mml:mo> ≈ </mml:mo><mml:mn> 630 </mml:mn></mml:mrow></mml:math></inline-formula> km/s [<xref ref-type="bibr" rid="B11">11</xref>].</p>
        <p>This numerical scale check demonstrates that the amplitude of our localized macroscopic bulk flow (&gt;600 km/s) is greater than the velocity residual attributed to Dark Energy at these redshifts. If cosmological fits systematically underestimate this coherent bulk flow, the uncorrected kinematic drift will organically reproduce the observational signature of an accelerating spatial expansion of the universe.</p>
      </sec>
    </sec>
    <sec id="sec9">
      <title>9. Kinematic Monopoles, Dipoles, and Apparent Isotropy</title>
      <p>A common defense of Dark Energy is the apparent isotropy of the acceleration signal. If the Milky Way is subject to a directional bulk flow toward Laniakea, one might expect a purely dipole acceleration signature. However, this expectation overlooks the dual kinematic nature of our environment.</p>
      <p>The Milky Way is embedded on the boundary of the Local Void. A cosmic void evacuates matter radially outward, generating a localized kinematic “bubble” characterized by a monopole expansion. Consequently, nearby galaxies in nearly all directions are pushed away from the void’s center, receding faster than the baseline global Hubble flow.</p>
      <p>When standard models spherically average SNe Ia calibrators, the directional dipole is smeared, and the localized monopole is mathematically misinterpreted as a uniform global acceleration (Λ). Furthermore, when SNe Ia data is analyzed without assuming strict isotropy, the acceleration signal is significantly anisotropic. Colin <italic>et al</italic>. (2019) demonstrated a pronounced dipole in the deceleration parameter (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> q </mml:mi><mml:mn> 0 </mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ), with the axis of maximum apparent acceleration aligning directly with our local bulk flow [<xref ref-type="bibr" rid="B12">12</xref>]. This strongly supports the hypothesis that the Dark Energy signal is deeply contaminated by localized kinematics.</p>
    </sec>
    <sec id="sec10">
      <title>10. Consistency with CMB and BAO Probes</title>
      <p>Standard cosmology cross-validates Dark Energy using the Cosmic Microwave Background (CMB) and Baryon Acoustic Oscillations (BAO). In ΛCDM, Dark Energy (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> Ω </mml:mi><mml:mi> Λ </mml:mi></mml:msub><mml:mo> ≈ </mml:mo><mml:mn> 0.68 </mml:mn></mml:mrow></mml:math></inline-formula> ) is mathematically required to bring the total energy density to exactly <inline-formula><mml:math><mml:mrow><mml:mi> Ω </mml:mi><mml:mo> = </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> , yielding a flat geometry that fits the angular position of the CMB’s first acoustic peak.</p>
      <p>However, in a natively closed 3-sphere (<inline-formula><mml:math><mml:mrow><mml:mi> k </mml:mi><mml:mo> = </mml:mo><mml:mo> + </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> ), spatial curvature intrinsically shifts the angular scale, satisfying the position of the acoustic peak without requiring an arbitrary Λ term to pad the energy density. Recent analyses of Planck data have independently highlighted that a closed universe provides a highly consistent fit to the CMB power spectrum [<xref ref-type="bibr" rid="B13">13</xref>].</p>
      <p>Furthermore, as mathematically detailed in <bold>Appendix B</bold>, when local bulk-flow kinematics are subtracted from low-redshift BAO anchoring data, and the transverse distance is modeled via the native <inline-formula><mml:math><mml:mrow><mml:msup><mml:mi> S </mml:mi><mml:mn> 3 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> trigonometric projection, apparent BAO acceleration anomalies natively resolve into the static geometric curvature of the closed manifold.</p>
    </sec>
    <sec id="sec11">
      <title>11. The Minor Thermodynamic Contribution of Galactic Photons</title>
      <p>While macroscopic expansion is overwhelmingly driven by the isotropic radiation pressure of the CMB, the cumulative emission of stellar photons (Extragalactic Background Light) introduces a supplementary thermodynamic variable. Because these galactic photons increase the total internal energy (<inline-formula><mml:math><mml:mi> U </mml:mi></mml:math></inline-formula> ) of the closed manifold, they exert an additional fractional radiation pressure against the 5D Planck Stiffness.</p>
      <p>However, the absolute maximum number of photons that galaxies can inject is dwarfed by the primordial CMB photon-to-baryon ratio (<inline-formula><mml:math><mml:mrow><mml:mi> η </mml:mi><mml:mo> ≈ </mml:mo><mml:msup><mml:mrow><mml:mn> 10 </mml:mn></mml:mrow><mml:mn> 9 </mml:mn></mml:msup><mml:mo> : </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> ). Therefore, while the EBL provides a minor supplementary thermodynamic pressure—contributing to a slight enhancement in the expansion of space relative to the pure CMB baseline—it is historically negligible compared to the primary driver.</p>
    </sec>
    <sec id="sec12">
      <title>12. Conclusions</title>
      <p>By synthesizing finite cosmological boundaries with the thermodynamic rules of a perfectly adiabatic system, we argue that the universe possesses strict geometric and temporal symmetry. The dimensionless ratio predicts a temporally bifurcated <inline-formula><mml:math><mml:mrow><mml:mn> 2 </mml:mn><mml:msub><mml:mi> M </mml:mi><mml:mi> u </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mass geometry, elegantly resolving the Baryon Asymmetry problem without unobserved microphysics.</p>
      <p>The macroscopic lifecycle guarantees global energy conservation, while establishing a firm temporal threshold (<inline-formula><mml:math><mml:mrow><mml:mi> z </mml:mi><mml:mo> = </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> ) for pure isotropic thermodynamics. The late-time enhanced separation of galaxies observed from Earth is the deterministic kinematic result of non-linear macroscopic clustering. By recognizing our specific vantage point on the edge of the Local Void, we provide a strongly competitive theoretical alternative to the Dark Energy hypothesis, preserving a conserved-energy interpretation to cosmological mechanics.</p>
    </sec>
    <sec id="sec13">
      <title>Appendix</title>
      <sec id="sec13dot1">
        <title>A. Friedmann Boundary Condition at Maximum Expansion</title>
        <p>To demonstrate that the factor of 2 in our dimensionless framework is an intrinsic property of a closed universe, we analyze the standard Friedmann equation for a <inline-formula><mml:math><mml:mrow><mml:mi> k </mml:mi><mml:mo> = </mml:mo><mml:mo> + </mml:mo><mml:mn> 1 </mml:mn></mml:mrow></mml:math></inline-formula> geometry: </p>
        <disp-formula id="FD13">
          <label>(10)</label>
          <mml:math>
            <mml:mrow>
              <mml:msup>
                <mml:mrow>
                  <mml:mrow>
                    <mml:mo>(</mml:mo>
                    <mml:mrow>
                      <mml:mfrac>
                        <mml:mover accent="true">
                          <mml:mi>R</mml:mi>
                          <mml:mo>˙</mml:mo>
                        </mml:mover>
                        <mml:mi>R</mml:mi>
                      </mml:mfrac>
                    </mml:mrow>
                    <mml:mo>)</mml:mo>
                  </mml:mrow>
                </mml:mrow>
                <mml:mn>2</mml:mn>
              </mml:msup>
              <mml:mo>=</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:mn>8</mml:mn>
                  <mml:mi>π</mml:mi>
                  <mml:mi>G</mml:mi>
                  <mml:mi>ρ</mml:mi>
                </mml:mrow>
                <mml:mn>3</mml:mn>
              </mml:mfrac>
              <mml:mo>−</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>c</mml:mi>
                    <mml:mn>2</mml:mn>
                  </mml:msup>
                </mml:mrow>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>R</mml:mi>
                    <mml:mn>2</mml:mn>
                  </mml:msup>
                </mml:mrow>
              </mml:mfrac>
            </mml:mrow>
          </mml:math>
        </disp-formula>
        <p>Substituting the volumetric mass density (<inline-formula><mml:math><mml:mrow><mml:mi> ρ </mml:mi><mml:mo> = </mml:mo><mml:mrow><mml:mrow><mml:mn> 3 </mml:mn><mml:mi> M </mml:mi></mml:mrow><mml:mo> / </mml:mo><mml:mrow><mml:mn> 4 </mml:mn><mml:mi> π </mml:mi><mml:msup><mml:mi> R </mml:mi><mml:mn> 3 </mml:mn></mml:msup></mml:mrow></mml:mrow></mml:mrow></mml:math></inline-formula> ): </p>
        <disp-formula id="FD14">
          <label>(11)</label>
          <mml:math>
            <mml:mrow>
              <mml:msup>
                <mml:mrow>
                  <mml:mrow>
                    <mml:mo>(</mml:mo>
                    <mml:mrow>
                      <mml:mfrac>
                        <mml:mover accent="true">
                          <mml:mi>R</mml:mi>
                          <mml:mo>˙</mml:mo>
                        </mml:mover>
                        <mml:mi>R</mml:mi>
                      </mml:mfrac>
                    </mml:mrow>
                    <mml:mo>)</mml:mo>
                  </mml:mrow>
                </mml:mrow>
                <mml:mn>2</mml:mn>
              </mml:msup>
              <mml:mo>=</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:mn>2</mml:mn>
                  <mml:mi>G</mml:mi>
                  <mml:mi>M</mml:mi>
                </mml:mrow>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>R</mml:mi>
                    <mml:mn>3</mml:mn>
                  </mml:msup>
                </mml:mrow>
              </mml:mfrac>
              <mml:mo>−</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>c</mml:mi>
                    <mml:mn>2</mml:mn>
                  </mml:msup>
                </mml:mrow>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>R</mml:mi>
                    <mml:mn>2</mml:mn>
                  </mml:msup>
                </mml:mrow>
              </mml:mfrac>
              <mml:mo>⇒</mml:mo>
              <mml:msup>
                <mml:mover accent="true">
                  <mml:mi>R</mml:mi>
                  <mml:mo>˙</mml:mo>
                </mml:mover>
                <mml:mn>2</mml:mn>
              </mml:msup>
              <mml:mo>=</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:mn>2</mml:mn>
                  <mml:mi>G</mml:mi>
                  <mml:mi>M</mml:mi>
                </mml:mrow>
                <mml:mi>R</mml:mi>
              </mml:mfrac>
              <mml:mo>−</mml:mo>
              <mml:msup>
                <mml:mi>c</mml:mi>
                <mml:mn>2</mml:mn>
              </mml:msup>
            </mml:mrow>
          </mml:math>
        </disp-formula>
        <p>At the spatial “equator” (global maximum expansion limit), macroscopic expansion must momentarily halt (<inline-formula><mml:math><mml:mrow><mml:mover accent="true"><mml:mi> R </mml:mi><mml:mo> ˙ </mml:mo></mml:mover><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula> ). This evaluates the strict boundary condition: </p>
        <disp-formula id="FD15">
          <label>(12)</label>
          <mml:math>
            <mml:mrow>
              <mml:mn>0</mml:mn>
              <mml:mo>=</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:mn>2</mml:mn>
                  <mml:mi>G</mml:mi>
                  <mml:mi>M</mml:mi>
                </mml:mrow>
                <mml:mrow>
                  <mml:msub>
                    <mml:mi>R</mml:mi>
                    <mml:mrow>
                      <mml:mi>max</mml:mi>
                    </mml:mrow>
                  </mml:msub>
                </mml:mrow>
              </mml:mfrac>
              <mml:mo>−</mml:mo>
              <mml:msup>
                <mml:mi>c</mml:mi>
                <mml:mn>2</mml:mn>
              </mml:msup>
              <mml:mo>⇒</mml:mo>
              <mml:msub>
                <mml:mi>R</mml:mi>
                <mml:mrow>
                  <mml:mi>max</mml:mi>
                </mml:mrow>
              </mml:msub>
              <mml:mo>=</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:mn>2</mml:mn>
                  <mml:mi>G</mml:mi>
                  <mml:mi>M</mml:mi>
                </mml:mrow>
                <mml:mrow>
                  <mml:msup>
                    <mml:mi>c</mml:mi>
                    <mml:mn>2</mml:mn>
                  </mml:msup>
                </mml:mrow>
              </mml:mfrac>
            </mml:mrow>
          </mml:math>
        </disp-formula>
        <p>This confirms that a closed universe natively recovers the exact mathematical signature of the Schwarzschild radius at its maximum expansion limit.</p>
      </sec>
      <sec id="sec13dot2">
        <title>B. Kinematic Calibration and the Geometric Resolution of BAO Anomalies</title>
        <p>The observed redshift (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> z </mml:mi><mml:mrow><mml:mi> o </mml:mi><mml:mi> b </mml:mi><mml:mi> s </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> ) of a low-redshift BAO calibrator galaxy is a composite of its cosmological metric redshift (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> z </mml:mi><mml:mi> c </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ) and its peculiar kinematic velocity (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> v </mml:mi><mml:mrow><mml:mi> p </mml:mi><mml:mi> e </mml:mi><mml:mi> c </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> ): </p>
        <disp-formula id="FD16">
          <label>(13)</label>
          <mml:math>
            <mml:mrow>
              <mml:msub>
                <mml:mi>z</mml:mi>
                <mml:mrow>
                  <mml:mi>o</mml:mi>
                  <mml:mi>b</mml:mi>
                  <mml:mi>s</mml:mi>
                </mml:mrow>
              </mml:msub>
              <mml:mo>≈</mml:mo>
              <mml:msub>
                <mml:mi>z</mml:mi>
                <mml:mi>c</mml:mi>
              </mml:msub>
              <mml:mo>+</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:msub>
                    <mml:mi>v</mml:mi>
                    <mml:mrow>
                      <mml:mi>p</mml:mi>
                      <mml:mi>e</mml:mi>
                      <mml:mi>c</mml:mi>
                    </mml:mrow>
                  </mml:msub>
                </mml:mrow>
                <mml:mi>c</mml:mi>
              </mml:mfrac>
            </mml:mrow>
          </mml:math>
        </disp-formula>
        <p>As established in Section 8.2, an uncorrected bulk flow of <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> v </mml:mi><mml:mrow><mml:mi> p </mml:mi><mml:mi> e </mml:mi><mml:mi> c </mml:mi></mml:mrow></mml:msub><mml:mo> ≈ </mml:mo><mml:mn> 630 </mml:mn></mml:mrow></mml:math></inline-formula> km/s introduces a systemic kinematic error of <inline-formula><mml:math><mml:mrow><mml:mtext> Δ </mml:mtext><mml:msub><mml:mi> z </mml:mi><mml:mrow><mml:mi> k </mml:mi><mml:mi> i </mml:mi><mml:mi> n </mml:mi></mml:mrow></mml:msub><mml:mo> ≈ </mml:mo><mml:mn> 0.002 </mml:mn></mml:mrow></mml:math></inline-formula> . Because the local Hubble constant is calibrated as <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> H </mml:mi><mml:mn> 0 </mml:mn></mml:msub><mml:mo> ≈ </mml:mo><mml:mrow><mml:mrow><mml:mi> c </mml:mi><mml:msub><mml:mi> z </mml:mi><mml:mrow><mml:mi> o </mml:mi><mml:mi> b </mml:mi><mml:mi> s </mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mo> / </mml:mo><mml:mi> D </mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> , artificially inflating <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> z </mml:mi><mml:mrow><mml:mi> o </mml:mi><mml:mi> b </mml:mi><mml:mi> s </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> systematically overestimates the global expansion rate (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> H </mml:mi><mml:mn> 0 </mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ).</p>
        <p>When standard ΛCDM applies this overestimated <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> H </mml:mi><mml:mn> 0 </mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to high-redshift BAO data, the theoretical distance falls short. In the single-parameter closed universe, the transverse comoving distance <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> D </mml:mi><mml:mi> M </mml:mi></mml:msub><mml:mrow><mml:mo> ( </mml:mo><mml:mi> z </mml:mi><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> must be geometrically projected across the curvature of the 3-sphere radius (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mn> 0 </mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ): </p>
        <disp-formula id="FD17">
          <label>(14)</label>
          <mml:math>
            <mml:mrow>
              <mml:msub>
                <mml:mi>D</mml:mi>
                <mml:mi>M</mml:mi>
              </mml:msub>
              <mml:mrow>
                <mml:mo>(</mml:mo>
                <mml:mi>z</mml:mi>
                <mml:mo>)</mml:mo>
              </mml:mrow>
              <mml:mo>=</mml:mo>
              <mml:msub>
                <mml:mi>R</mml:mi>
                <mml:mn>0</mml:mn>
              </mml:msub>
              <mml:mi>sin</mml:mi>
              <mml:mrow>
                <mml:mo>(</mml:mo>
                <mml:mrow>
                  <mml:mfrac>
                    <mml:mrow>
                      <mml:mi>χ</mml:mi>
                      <mml:mrow>
                        <mml:mo>(</mml:mo>
                        <mml:mi>z</mml:mi>
                        <mml:mo>)</mml:mo>
                      </mml:mrow>
                    </mml:mrow>
                    <mml:mrow>
                      <mml:msub>
                        <mml:mi>R</mml:mi>
                        <mml:mn>0</mml:mn>
                      </mml:msub>
                    </mml:mrow>
                  </mml:mfrac>
                </mml:mrow>
                <mml:mo>)</mml:mo>
              </mml:mrow>
              <mml:mo>≈</mml:mo>
              <mml:mi>χ</mml:mi>
              <mml:mrow>
                <mml:mo>(</mml:mo>
                <mml:mi>z</mml:mi>
                <mml:mo>)</mml:mo>
              </mml:mrow>
              <mml:mo>−</mml:mo>
              <mml:mfrac>
                <mml:mrow>
                  <mml:mi>χ</mml:mi>
                  <mml:msup>
                    <mml:mrow>
                      <mml:mrow>
                        <mml:mo>(</mml:mo>
                        <mml:mi>z</mml:mi>
                        <mml:mo>)</mml:mo>
                      </mml:mrow>
                    </mml:mrow>
                    <mml:mn>3</mml:mn>
                  </mml:msup>
                </mml:mrow>
                <mml:mrow>
                  <mml:mn>6</mml:mn>
                  <mml:msubsup>
                    <mml:mi>R</mml:mi>
                    <mml:mn>0</mml:mn>
                    <mml:mn>2</mml:mn>
                  </mml:msubsup>
                </mml:mrow>
              </mml:mfrac>
            </mml:mrow>
          </mml:math>
        </disp-formula>
        <p>When the baseline expansion rate (<inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> H </mml:mi><mml:mn> 0 </mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ) is correctly reduced by subtracting the local macroscopic bulk flow, and the transverse distance is modeled via the native <inline-formula><mml:math><mml:mrow><mml:msup><mml:mi> S </mml:mi><mml:mn> 3 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> trigonometric projection (<inline-formula><mml:math><mml:mrow><mml:mtext> sin </mml:mtext><mml:mrow><mml:mo> ( </mml:mo><mml:mrow><mml:mrow><mml:mi> χ </mml:mi><mml:mo> / </mml:mo><mml:mrow><mml:msub><mml:mi> R </mml:mi><mml:mn> 0 </mml:mn></mml:msub></mml:mrow></mml:mrow></mml:mrow><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> ), the apparent BAO acceleration anomaly is absorbed entirely by the static spatial curvature.</p>
      </sec>
    </sec>
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    <ref-list>
      <title>References</title>
      <ref id="B1">
        <label>1.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Steynberg, A.P. (2026) Geometric Monism: A 5-Dimensional Torsion-Based Calculation of Rest Mass for the Standard Model Spectrum. Zenodo. https://doi.org/10.5281/zenodo.18940793 <pub-id pub-id-type="doi">10.5281/zenodo.18940793</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.5281/zenodo.18940793">https://doi.org/10.5281/zenodo.18940793</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Steynberg, A.P.</string-name>
            </person-group>
            <year>2026</year>
            <article-title>Geometric Monism: A 5-Dimensional Torsion-Based Calculation of Rest Mass for the Standard Model Spectrum</article-title>
            <pub-id pub-id-type="doi">10.5281/zenodo.18940793</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B2">
        <label>2.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Steynberg, A.P. (2022) A Dimensionless Equation Linking the Maximum and Minimum Values for Mass (or Energy) and Time (or Length). <italic>Global Journal of Science Frontier Research</italic>, 22, 1-3.</mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Steynberg, A.P.</string-name>
            </person-group>
            <year>2022</year>
            <article-title>A Dimensionless Equation Linking the Maximum and Minimum Values for Mass (or Energy) and Time (or Length)</article-title>
            <source>Global Journal of Science Frontier Research</source>
            <volume>22</volume>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B3">
        <label>3.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Misner, C.W., Thorne, K.S. and Wheeler, J.A. (1973) Gravitation. W. H. Freeman and Company.</mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Misner, C.W.</string-name>
              <string-name>Thorne, K.S.</string-name>
              <string-name>Wheeler, J.A.</string-name>
            </person-group>
            <year>1973</year>
            <article-title>Gravitation</article-title>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B4">
        <label>4.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Isaacson, R.A. (1968) Gravitational Radiation in the Limit of High Frequency. II. Nonlinear Terms and the Effective Stress Tensor. <italic>Physical Review</italic>, 166, 1272-1280. https://doi.org/10.1103/PhysRev.166.1272 <pub-id pub-id-type="doi">10.1103/PhysRev.166.1272</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1103/PhysRev.166.1272">https://doi.org/10.1103/PhysRev.166.1272</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Isaacson, R.A.</string-name>
            </person-group>
            <year>1968</year>
            <article-title>Gravitational Radiation in the Limit of High Frequency</article-title>
            <source>II. Nonlinear Terms and the Effective Stress Tensor. Physical Review</source>
            <volume>166</volume>
            <pub-id pub-id-type="doi">10.1103/PhysRev.166.1272</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B5">
        <label>5.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Steynberg, A.P. (2025) Single Parameter Model for Cosmic Scale Photon Redshift in a Closed Universe Applied to Data from JWST. <italic>Open Journal of Modelling and Simu</italic><italic>lation</italic>, 13, 204-210. https://doi.org/10.4236/ojmsi.2025.134012 <pub-id pub-id-type="doi">10.4236/ojmsi.2025.134012</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.4236/ojmsi.2025.134012">https://doi.org/10.4236/ojmsi.2025.134012</ext-link></mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Steynberg, A.P.</string-name>
            </person-group>
            <year>2025</year>
            <article-title>Single Parameter Model for Cosmic Scale Photon Redshift in a Closed Universe Applied to Data from JWST</article-title>
            <source>Open Journal of Modelling and Simulation</source>
            <volume>13</volume>
            <pub-id pub-id-type="doi">10.4236/ojmsi.2025.134012</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B6">
        <label>6.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Springel, V., White, S.D.M., Jenkins, A., Frenk, C.S., Yoshida, N., Gao, L., <italic>et al</italic>. (2005) Simulations of the Formation, Evolution and Clustering of Galaxies and Quasars. <italic>Nature</italic>, 435, 629-636. https://doi.org/10.1038/nature03597 <pub-id pub-id-type="doi">10.1038/nature03597</pub-id><pub-id pub-id-type="pmid">15931216</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1038/nature03597">https://doi.org/10.1038/nature03597</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Springel, V.</string-name>
              <string-name>White, S.D.M.</string-name>
              <string-name>Jenkins, A.</string-name>
              <string-name>Frenk, C.S.</string-name>
              <string-name>Yoshida, N.</string-name>
              <string-name>Gao, L.</string-name>
              <string-name>Formation, E</string-name>
            </person-group>
            <year>2005</year>
            <article-title>Simulations of the Formation, Evolution and Clustering of Galaxies and Quasars</article-title>
            <source>Nature</source>
            <volume>435</volume>
            <pub-id pub-id-type="doi">10.1038/nature03597</pub-id>
            <pub-id pub-id-type="pmid">15931216</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B7">
        <label>7.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Riess, A.G., Filippenko, A.V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P.M., <italic>et al</italic>. (1998) Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant. <italic>The Astronomical Journal</italic>, 116, 1009-1038. https://doi.org/10.1086/300499 <pub-id pub-id-type="doi">10.1086/300499</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1086/300499">https://doi.org/10.1086/300499</ext-link></mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Riess, A.G.</string-name>
              <string-name>Filippenko, A.V.</string-name>
              <string-name>Challis, P.</string-name>
              <string-name>Clocchiatti, A.</string-name>
              <string-name>Diercks, A.</string-name>
              <string-name>Garnavich, P.M.</string-name>
            </person-group>
            <year>1998</year>
            <article-title>Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant</article-title>
            <source>The Astronomical Journal</source>
            <volume>116</volume>
            <pub-id pub-id-type="doi">10.1086/300499</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B8">
        <label>8.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R.A., Nugent, P., Castro, P.G., <italic>et al</italic>. (1999) Measurements of <italic>ω</italic> and <italic>λ</italic> from 42 High-Redshift Supernovae. <italic>The Astrophysical Journal</italic>, 517, 565-586. https://doi.org/10.1086/307221 <pub-id pub-id-type="doi">10.1086/307221</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1086/307221">https://doi.org/10.1086/307221</ext-link></mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Perlmutter, S.</string-name>
              <string-name>Aldering, G.</string-name>
              <string-name>Goldhaber, G.</string-name>
              <string-name>Knop, R.A.</string-name>
              <string-name>Nugent, P.</string-name>
              <string-name>Castro, P.G.</string-name>
            </person-group>
            <year>1999</year>
            <article-title>Measurements of ω and λ from 42 High-Redshift Supernovae</article-title>
            <source>The Astrophysical Journal</source>
            <volume>517</volume>
            <pub-id pub-id-type="doi">10.1086/307221</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B9">
        <label>9.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Tully, R.B., Courtois, H., Hoffman, Y. and Pomarède, D. (2014) The Laniakea Supercluster of Galaxies. <italic>Nature</italic>, 513, 71-73. https://doi.org/10.1038/nature13674 <pub-id pub-id-type="doi">10.1038/nature13674</pub-id><pub-id pub-id-type="pmid">25186900</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1038/nature13674">https://doi.org/10.1038/nature13674</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Tully, R.B.</string-name>
              <string-name>Courtois, H.</string-name>
              <string-name>Hoffman, Y.</string-name>
            </person-group>
            <year>2014</year>
            <article-title>The Laniakea Supercluster of Galaxies</article-title>
            <source>Nature</source>
            <volume>513</volume>
            <pub-id pub-id-type="doi">10.1038/nature13674</pub-id>
            <pub-id pub-id-type="pmid">25186900</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B10">
        <label>10.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Keenan, R.C., Barger, A.J. and Cowie, L.L. (2013) Evidence for a ~300 Mpc Scale Under-Density in the Local Galaxy Distribution. <italic>The Astrophysical Journal</italic>, 775, Article 62. https://doi.org/10.1088/0004-637X/775/1/62 <pub-id pub-id-type="doi">10.1088/0004-637X/775/1/62</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1088/0004-637X/775/1/62">https://doi.org/10.1088/0004-637X/775/1/62</ext-link></mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Keenan, R.C.</string-name>
              <string-name>Barger, A.J.</string-name>
              <string-name>Cowie, L.L.</string-name>
            </person-group>
            <year>2013</year>
            <article-title>Evidence for a ~300 Mpc Scale Under-Density in the Local Galaxy Distribution</article-title>
            <source>The Astrophysical Journal</source>
            <volume>775</volume>
            <elocation-id>62</elocation-id>
            <pub-id pub-id-type="doi">10.1088/0004-637X/775/1/62</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B11">
        <label>11.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Hoffman, Y., Pomarède, D., Tully, R.B. and Courtois, H.M. (2017) The Dipole Repeller. <italic>Nature Astronomy</italic>, 1, Article No. 0036. https://doi.org/10.1038/s41550-016-0036 <pub-id pub-id-type="doi">10.1038/s41550-016-0036</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1038/s41550-016-0036">https://doi.org/10.1038/s41550-016-0036</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Hoffman, Y.</string-name>
              <string-name>Tully, R.B.</string-name>
              <string-name>Courtois, H.M.</string-name>
            </person-group>
            <year>2017</year>
            <article-title>The Dipole Repeller</article-title>
            <source>Nature Astronomy</source>
            <volume>1</volume>
            <elocation-id>No</elocation-id>
            <pub-id pub-id-type="doi">10.1038/s41550-016-0036</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B12">
        <label>12.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Colin, J., Mohayaee, R., Rameez, M. and Sarkar, S. (2019) Evidence for Anisotropy of Cosmic Acceleration. <italic>Astronomy &amp; Astrophysics</italic>, 631, Article No. L13. https://doi.org/10.1051/0004-6361/201936373 <pub-id pub-id-type="doi">10.1051/0004-6361/201936373</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1051/0004-6361/201936373">https://doi.org/10.1051/0004-6361/201936373</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Colin, J.</string-name>
              <string-name>Mohayaee, R.</string-name>
              <string-name>Rameez, M.</string-name>
              <string-name>Sarkar, S.</string-name>
            </person-group>
            <year>2019</year>
            <article-title>Evidence for Anisotropy of Cosmic Acceleration</article-title>
            <source>Astronomy &amp; Astrophysics</source>
            <volume>631</volume>
            <elocation-id>No</elocation-id>
            <pub-id pub-id-type="doi">10.1051/0004-6361/201936373</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B13">
        <label>13.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Di Valentino, E., Melchiorri, A. and Silk, J. (2019) Planck Evidence for a Closed Universe and a Possible Crisis for Cosmology. <italic>Nature Astronomy</italic>, 4, 196-203. https://doi.org/10.1038/s41550-019-0906-9 <pub-id pub-id-type="doi">10.1038/s41550-019-0906-9</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1038/s41550-019-0906-9">https://doi.org/10.1038/s41550-019-0906-9</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Valentino, E.</string-name>
              <string-name>Melchiorri, A.</string-name>
              <string-name>Silk, J.</string-name>
            </person-group>
            <year>2019</year>
            <article-title>Planck Evidence for a Closed Universe and a Possible Crisis for Cosmology</article-title>
            <source>Nature Astronomy</source>
            <volume>4</volume>
            <pub-id pub-id-type="doi">10.1038/s41550-019-0906-9</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
    </ref-list>
  </back>
</article>