<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.4 20241031//EN" "JATS-journalpublishing1-4.dtd">
<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">jhepgc</journal-id>
      <journal-title-group>
        <journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title>
      </journal-title-group>
      <issn pub-type="epub">2380-4335</issn>
      <issn pub-type="ppub">2380-4327</issn>
      <publisher>
        <publisher-name>Scientific Research Publishing</publisher-name>
      </publisher>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.4236/jhepgc.2026.122063</article-id>
      <article-id pub-id-type="publisher-id">jhepgc-151049</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>A First Order Wave Equation Composed of a Curved Spacetime Metric</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <contrib-id contrib-id-type="orcid">0009-0001-1513-4605</contrib-id>
          <name name-style="western">
            <surname>Poon</surname>
            <given-names>Gary</given-names>
          </name>
          <xref ref-type="aff" rid="aff1">1</xref>
        </contrib>
      </contrib-group>
      <aff id="aff1"><label>1</label> Division of Mathematics, Sciences and Engineering, Rio Hondo College, Whittier, CA, 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>01</day>
        <month>04</month>
        <year>2026</year>
      </pub-date>
      <pub-date pub-type="collection">
        <month>04</month>
        <year>2026</year>
      </pub-date>
      <volume>12</volume>
      <issue>02</issue>
      <fpage>1210</fpage>
      <lpage>1217</lpage>
      <history>
        <date date-type="received">
          <day>20</day>
          <month>01</month>
          <year>2026</year>
        </date>
        <date date-type="accepted">
          <day>26</day>
          <month>04</month>
          <year>2026</year>
        </date>
        <date date-type="published">
          <day>29</day>
          <month>04</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/jhepgc.2026.122063">https://doi.org/10.4236/jhepgc.2026.122063</self-uri>
      <abstract>
        <p>The ultimate quest of field theory is to pursue a fundamental law that can address both micro and macro issues, namely quantum entanglement and the inflationary universe, respectively. Here in this paper, a wave equation revealing the causality of a de-Sitter Space explains the so-called spooky action at a distance and the expansion of the universe within a single theory, quantum field theory on curved spacetime. An Astrophysical aspect of the theory is pursued at the end. Historic Background of Quantum Field Theory in Curved Spacetime: A century ago, there were two theories in physics that split the universe into aspects: the quantum theory dealing with microscopic world and the theory of general relativity dealing with macroscopic world. From the development of physics, we started with global phenomena like Newton’s gravitation law and came down to local phenomenon like particle wave duality in early twentieth century. Gravity was a well-known phenomenon since Newton’s time and reformulated by Einstein as general theory of relativity. There is no doubt that gravity expressed by the general theory of relativity coincides with the observational astronomy like gravitational wave, gravitational lensing and blackhole dynamics. At the same time, it is well tested by high energy physics that quantum mechanics is the fundamental theory for particle physics. It would be wrong to favor one over the other. Therefore I propose that the dual aspect of universe respecting both quantum and classical physics is simply expressed by one fundamental law. The appropriate candidate is Quantum Field Theory in Curved Spacetime. Working towards a unified theory for four fundamental forces, namely gravitation, electromagnetic force, strong and weak. Three out of the four, except for gravitation, can be explained by quantum mechanics. People are challenged to quantize gravity based on their mathematical skills, like gauge theory or string theory but still cannot escape the consequence of mathematical remedial technique—renormalization of the loops. They may be successful in one-loop renormalization but keep on renormalizing the subsequent loops without ending. If the theory does not make mathematical sense, it is a sign we should reconsider all the other possible ones. Here quantum field theory in curved space is studied [<xref ref-type="bibr" rid="B1">1</xref>]-[<xref ref-type="bibr" rid="B3">3</xref>].</p>
      </abstract>
      <kwd-group kwd-group-type="author-generated" xml:lang="en">
        <kwd>Field Theory</kwd>
        <kwd>Curved Spacetime</kwd>
        <kwd>De-Sitter Space</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec1">
      <title>1. Introduction</title>
      <p>Quantum Field Theory in curved space brings the dynamics to a quantum ensemble by introducing the classical spacetime manifold, a 4 × 4 metric to the wave equation [<xref ref-type="bibr" rid="B4">4</xref>]. The 4 × 4 metric is a signature of the curved spacetime manifold determined by Einstein Field Equation [<xref ref-type="bibr" rid="B5">5</xref>], <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:mo> + </mml:mo><mml:mi> Λ </mml:mi><mml:msub><mml:mi> g </mml:mi><mml:mrow><mml:mi> μ </mml:mi><mml:mi> ν </mml:mi></mml:mrow></mml:msub><mml:mo> = </mml:mo><mml:mi> κ </mml:mi><mml:msub><mml:mi> T </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>
      <p>Originally, the cosmological term, <inline-formula><mml:math><mml:mrow><mml:mi> Λ </mml:mi><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> didn’t exist in the equation until the realization of the expansion of the universe was confirmed after Hubble with his constant <inline-formula><mml:math><mml:mrow><mml:mi> H </mml:mi><mml:mo> = </mml:mo><mml:mi> α </mml:mi><mml:msqrt><mml:mi> Λ </mml:mi></mml:msqrt><mml:mo> = </mml:mo><mml:mfrac><mml:mn> 1 </mml:mn><mml:mi> R </mml:mi></mml:mfrac></mml:mrow></mml:math></inline-formula> .</p>
      <p>Where Λ is the cosmological constant, <inline-formula><mml:math><mml:mi> α </mml:mi></mml:math></inline-formula> is a proportionality constant and <inline-formula><mml:math><mml:mi> R </mml:mi></mml:math></inline-formula> is the radius of curvature of the observable universe. The cosmological constant arises due to the hypothesis of dark energy that exists to explain the expansion of the universe. The values of the cosmological constant will not be discussed here since they are irrelevant to the quantum mechanical part of the theory. In the quantum part of the theory, gravity is expressed as the geometric (four dimensional) manifold from the theory of general relativity and it cannot be treated as a quantum field without running into the catastrophe of ultraviolet divergence [<xref ref-type="bibr" rid="B6">6</xref>]. The only way to avoid the endless cycle of renormalization is to rely on the quantum theory of field in curved space in which the electromagnetic, strong and weak forces are regarded as Klein-Gordon fields and gravity is regarded as classical field. Thus, string theory as a fundamental theory for unifying four fundamental forces is not essential since the quantum dynamics of fields in curved spacetime can serve the purpose of unification. That will be explored in sections 4, 5, 6 and 7.</p>
      <p>In my previous work, there is a mathematical concept stating that a Klein-Godon field can gain a scalar potential under a unitary transformation, <italic>i.e</italic>. time evolution on de-Sitter space [<xref ref-type="bibr" rid="B7">7</xref>]. First, Klein Gordon equation is invariant under a de-Sitter transformation, otherwise it is not a unitary transformation or Klein Gordon field is not a quantum field. Since, Klein Gordon equation yields quantum dynamics in curved spacetime, de-Sitter universe is regarded as the best approximation of the cosmological space [<xref ref-type="bibr" rid="B7">7</xref>]. Now we are ready to use the mathematics developed by Friedlander [<xref ref-type="bibr" rid="B4">4</xref>] to the content of this section. The divergence of a vector field on a spacetime manifold, M is a scalar field, a function on M see (1.1.24) in local coordinates [<xref ref-type="bibr" rid="B4">4</xref>],</p>
      <disp-formula id="FD1">
        <mml:math>
          <mml:mrow>
            <mml:mi>d</mml:mi>
            <mml:mi>i</mml:mi>
            <mml:mi>v</mml:mi>
            <mml:mtext>
               
            </mml:mtext>
            <mml:mi>v</mml:mi>
            <mml:mo>=</mml:mo>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>|</mml:mo>
                  <mml:mi>g</mml:mi>
                  <mml:mo>|</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mrow>
                <mml:mo>−</mml:mo>
                <mml:mfrac>
                  <mml:mn>1</mml:mn>
                  <mml:mn>2</mml:mn>
                </mml:mfrac>
              </mml:mrow>
            </mml:msup>
            <mml:mfrac>
              <mml:mo>∂</mml:mo>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:msup>
                  <mml:mrow>
                    <mml:mrow>
                      <mml:mo>|</mml:mo>
                      <mml:mi>g</mml:mi>
                      <mml:mo>|</mml:mo>
                    </mml:mrow>
                  </mml:mrow>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mn>1</mml:mn>
                      <mml:mn>2</mml:mn>
                    </mml:mfrac>
                  </mml:mrow>
                </mml:msup>
                <mml:msub>
                  <mml:mi>v</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi> g </mml:mi><mml:mo> = </mml:mo><mml:mi> det </mml:mi><mml:msub><mml:mi> g </mml:mi><mml:mrow><mml:mi> i </mml:mi><mml:mi> j </mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> . Now, suppose the vector field is replaced by a distribution, or a wavefunction on a manifold (1.1.26) [<xref ref-type="bibr" rid="B4">4</xref>] states that the linear differential operator up to second order on the distribution in the manifold equals to a scalar function in the manifold. Considering only the second order and the zeroth order terms with the first order term being omitted in (2.8.19) [<xref ref-type="bibr" rid="B4">4</xref>], along with the hypothesis (1.1.26) [<xref ref-type="bibr" rid="B4">4</xref>], we have the familiar Klein Gordon equation wave equation on Riemannian metric that has been studied [<xref ref-type="bibr" rid="B7">7</xref>]. Considering the first order term only, we have a first order linear differential equation expressing the wave mechanics in curved spacetime as follows in natural units <inline-formula><mml:math><mml:mrow><mml:mi> ℏ </mml:mi><mml:mo> = </mml:mo><mml:mi> c </mml:mi><mml:mo> = </mml:mo><mml:mn> 0 </mml:mn></mml:mrow></mml:math></inline-formula></p>
      <disp-formula id="FD2">
        <label>(1)</label>
        <mml:math>
          <mml:mrow>
            <mml:mo>−</mml:mo>
            <mml:mi>i</mml:mi>
            <mml:msub>
              <mml:mo>∂</mml:mo>
              <mml:mi>μ</mml:mi>
            </mml:msub>
            <mml:msup>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msup>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mi>ν</mml:mi>
            </mml:msub>
            <mml:mo>=</mml:mo>
            <mml:msub>
              <mml:mi>p</mml:mi>
              <mml:mi>μ</mml:mi>
            </mml:msub>
            <mml:msup>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msup>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mi>ν</mml:mi>
            </mml:msub>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>where <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> is a 4 × 4 metric tensor signifying the curvature of a curved manifold. The RHS of (1) can be understood as a scalar function which is an infinitely differentiable continuous function on the manifold, M or simply said as analytical. After the functional analysis of (2.8.19) [<xref ref-type="bibr" rid="B4">4</xref>] and (1.1.26) [<xref ref-type="bibr" rid="B4">4</xref>] in addition with the generalization to a vector field, <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> ψ </mml:mi><mml:mi> μ </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from a scalar Klein-Gordon field, <inline-formula><mml:math><mml:mi> ϕ </mml:mi></mml:math></inline-formula> and to a four momentum <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> p </mml:mi><mml:mi> μ </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as an operator, <inline-formula><mml:math><mml:mrow><mml:mo> − </mml:mo><mml:mi> i </mml:mi><mml:msub><mml:mo> ∂ </mml:mo><mml:mi> μ </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in configuration space, from a scalar potential V [<xref ref-type="bibr" rid="B7">7</xref>], we can write the wave equation on curved spacetime manifold as an eigenvalue equation (1). It is a wave equation in local coordinates, the Cauchy data defined on a global manifold, M (see Dimock) [<xref ref-type="bibr" rid="B8">8</xref>]. Please note that the 4 × 4 metric satisfies relativistic covariance as shown in the next section so that (1) is consistent with the principle of relativistic invariant.</p>
    </sec>
    <sec id="sec2">
      <title>2. De-Sitter Space</title>
      <p>The metrics are given by</p>
      <disp-formula id="FD3">
        <label>(2)</label>
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msup>
            <mml:mo>=</mml:mo>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mi>t</mml:mi>
                      <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:mtext>diag</mml:mtext>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mo>−</mml:mo>
                <mml:mn>1</mml:mn>
                <mml:mo>,</mml:mo>
                <mml:mn>1</mml:mn>
                <mml:mo>,</mml:mo>
                <mml:mn>1</mml:mn>
                <mml:mo>,</mml:mo>
                <mml:mn>1</mml:mn>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD4">
        <label>(3)</label>
        <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:mo>=</mml:mo>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mi>R</mml:mi>
                      <mml:mi>t</mml:mi>
                    </mml:mfrac>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mtext>diag</mml:mtext>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mo>−</mml:mo>
                <mml:mn>1</mml:mn>
                <mml:mo>,</mml:mo>
                <mml:mn>1</mml:mn>
                <mml:mo>,</mml:mo>
                <mml:mn>1</mml:mn>
                <mml:mo>,</mml:mo>
                <mml:mn>1</mml:mn>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>where <inline-formula><mml:math><mml:mrow><mml:mi> μ </mml:mi><mml:mo> = </mml:mo><mml:mi> ν </mml:mi><mml:mo> = </mml:mo><mml:mrow><mml:mo> ( </mml:mo><mml:mrow><mml:mn> 0 </mml:mn><mml:mo> , </mml:mo><mml:mn> 1 </mml:mn><mml:mo> , </mml:mo><mml:mn> 2 </mml:mn><mml:mo> , </mml:mo><mml:mn> 3 </mml:mn></mml:mrow><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> and <italic>R</italic> is the radius of the universe or the inverse of the Hubble constant.</p>
      <p>Embedded in five dimensions, de-Sitter universe is a highly symmetric manifold, a hyperbolic surface, <inline-formula><mml:math><mml:mrow><mml:msubsup><mml:mi> x </mml:mi><mml:mn> 0 </mml:mn><mml:mn> 2 </mml:mn></mml:msubsup><mml:mo> − </mml:mo><mml:msubsup><mml:mi> x </mml:mi><mml:mn> 1 </mml:mn><mml:mn> 2 </mml:mn></mml:msubsup><mml:mo> − </mml:mo><mml:msubsup><mml:mi> x </mml:mi><mml:mn> 2 </mml:mn><mml:mn> 2 </mml:mn></mml:msubsup><mml:mo> − </mml:mo><mml:msubsup><mml:mi> x </mml:mi><mml:mn> 3 </mml:mn><mml:mn> 2 </mml:mn></mml:msubsup><mml:mo> − </mml:mo><mml:msubsup><mml:mi> x </mml:mi><mml:mn> 4 </mml:mn><mml:mn> 2 </mml:mn></mml:msubsup><mml:mo> = </mml:mo><mml:mo> − </mml:mo><mml:msup><mml:mi> R </mml:mi><mml:mn> 2 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></p>
      <p>Where <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> x </mml:mi><mml:mn> 0 </mml:mn></mml:msub><mml:mo> = </mml:mo><mml:mi> t </mml:mi></mml:mrow></mml:math></inline-formula> , the other four components are spatial. It’s metric contains no matter and a constant curvature that explains the current state of inflationary universe or accelerating universe due to Euclidean vacuum [<xref ref-type="bibr" rid="B9">9</xref>]. It is the geometry of the large scale structure of the universe worth for studying because of the wave equation being analytical as will be seen below. The radius of the curvature R can tell the so-called the age of the universe according to Hubble’s constant. Hubble’s inference of the big bang theory was true provided time-like and light-like geodesics on the de-Sitter manifold in the intergalactic space or the large scale of the universe. What if the geodesics is spacelike causality upon the rate of expansion of the universe beyond the speed of light according to the steady state constant curvature of de-Sitter space. Then there is no time-like or light-like causality in the de-Sitter universe to connect the past event with the present event. Hubble’s idea of the origin of the big scale universe might not sound right. On the mathematical analysis, the hyperbola is intercepted by a flat space plane at 45 degrees under the Lorentzian transformation in 5 dimensions [<xref ref-type="bibr" rid="B10">10</xref>] as time goes back to infinite past, namely <italic>R</italic> = 0. Upon the symmetry breaking of the de-Sitter manifold, a wedge of the manifold cut, the manifold intercepted by the 45 degree plane has no origin. The origin of time doesn’t exist in de-Sitter hyperbola. No big bang occurred.</p>
    </sec>
    <sec id="sec3">
      <title>3. Wave Equation Solved in de-Sitter Space</title>
      <p>The metric (2) and (3) fulfill the principle of relativistic covariance such that</p>
      <disp-formula id="FD5">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msup>
            <mml:msub>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>ν</mml:mi>
                <mml:mi>σ</mml:mi>
              </mml:mrow>
            </mml:msub>
            <mml:mo>=</mml:mo>
            <mml:msubsup>
              <mml:mi>δ</mml:mi>
              <mml:mi>σ</mml:mi>
              <mml:mi>μ</mml:mi>
            </mml:msubsup>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD6">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:msup>
                <mml:mi>x</mml:mi>
                <mml:mo>′</mml:mo>
              </mml:msup>
              <mml:mi>μ</mml:mi>
            </mml:msup>
            <mml:mo>=</mml:mo>
            <mml:msup>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msup>
            <mml:msub>
              <mml:mi>x</mml:mi>
              <mml:mi>ν</mml:mi>
            </mml:msub>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>Considering</p>
      <disp-formula id="FD7">
        <mml:math>
          <mml:mtable>
            <mml:mtr>
              <mml:mtd>
                <mml:msup>
                  <mml:msup>
                    <mml:mi>x</mml:mi>
                    <mml:mo>′</mml:mo>
                  </mml:msup>
                  <mml:mi>μ</mml:mi>
                </mml:msup>
                <mml:msub>
                  <mml:msup>
                    <mml:mi>x</mml:mi>
                    <mml:mo>′</mml:mo>
                  </mml:msup>
                  <mml:mi>μ</mml:mi>
                </mml:msub>
                <mml:mo>=</mml:mo>
                <mml:msup>
                  <mml:mi>g</mml:mi>
                  <mml:mrow>
                    <mml:mi>μ</mml:mi>
                    <mml:mi>ν</mml:mi>
                  </mml:mrow>
                </mml:msup>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>ν</mml:mi>
                </mml:msub>
                <mml:msub>
                  <mml:mi>g</mml:mi>
                  <mml:mrow>
                    <mml:mi>μ</mml:mi>
                    <mml:mi>σ</mml:mi>
                  </mml:mrow>
                </mml:msub>
                <mml:msup>
                  <mml:mi>x</mml:mi>
                  <mml:mi>σ</mml:mi>
                </mml:msup>
              </mml:mtd>
            </mml:mtr>
            <mml:mtr>
              <mml:mtd>
                <mml:mo>=</mml:mo>
                <mml:msubsup>
                  <mml:mi>δ</mml:mi>
                  <mml:mi>σ</mml:mi>
                  <mml:mi>ν</mml:mi>
                </mml:msubsup>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>ν</mml:mi>
                </mml:msub>
                <mml:msup>
                  <mml:mi>x</mml:mi>
                  <mml:mi>σ</mml:mi>
                </mml:msup>
              </mml:mtd>
            </mml:mtr>
            <mml:mtr>
              <mml:mtd>
                <mml:mo>=</mml:mo>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>ν</mml:mi>
                </mml:msub>
                <mml:msup>
                  <mml:mi>x</mml:mi>
                  <mml:mi>ν</mml:mi>
                </mml:msup>
              </mml:mtd>
            </mml:mtr>
          </mml:mtable>
        </mml:math>
      </disp-formula>
      <p>Relativistic covariance was proved.</p>
      <p>We are now in the position to solve the equation (1) as follow</p>
      <disp-formula id="FD8">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>|</mml:mo>
                  <mml:mrow>
                    <mml:mi>det</mml:mi>
                    <mml:mrow>
                      <mml:mo>(</mml:mo>
                      <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:mo>)</mml:mo>
                    </mml:mrow>
                  </mml:mrow>
                  <mml:mo>|</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mrow>
                <mml:mfrac>
                  <mml:mn>1</mml:mn>
                  <mml:mn>2</mml:mn>
                </mml:mfrac>
              </mml:mrow>
            </mml:msup>
            <mml:mo>=</mml:mo>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mi>R</mml:mi>
                      <mml:mi>t</mml:mi>
                    </mml:mfrac>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mn>4</mml:mn>
            </mml:msup>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>(1) follows <inline-formula><mml:math><mml:mrow><mml:mstyle displaystyle="true"><mml:msub><mml:mo> ∑ </mml:mo><mml:mrow><mml:mi> μ </mml:mi><mml:mo> , </mml:mo><mml:mi> ν </mml:mi></mml:mrow></mml:msub><mml:mrow><mml:msup><mml:mrow><mml:mrow><mml:mo> | </mml:mo><mml:mrow><mml:mi> det </mml:mi><mml:mrow><mml:mo> ( </mml:mo><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:mo> ) </mml:mo></mml:mrow></mml:mrow><mml:mo> | </mml:mo></mml:mrow></mml:mrow><mml:mrow><mml:mo> − </mml:mo><mml:mfrac><mml:mn> 1 </mml:mn><mml:mn> 2 </mml:mn></mml:mfrac></mml:mrow></mml:msup><mml:mfrac><mml:mo> ∂ </mml:mo><mml:mrow><mml:mo> ∂ </mml:mo><mml:msub><mml:mi> x </mml:mi><mml:mi> μ </mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mrow><mml:mo> ( </mml:mo><mml:mrow><mml:msup><mml:mrow><mml:mrow><mml:mo> | </mml:mo><mml:mrow><mml:mi> det </mml:mi><mml:mrow><mml:mo> ( </mml:mo><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:mo> ) </mml:mo></mml:mrow></mml:mrow><mml:mo> | </mml:mo></mml:mrow></mml:mrow><mml:mrow><mml:mfrac><mml:mn> 1 </mml:mn><mml:mn> 2 </mml:mn></mml:mfrac></mml:mrow></mml:msup><mml:msup><mml:mi> g </mml:mi><mml:mrow><mml:mi> μ </mml:mi><mml:mi> ν </mml:mi></mml:mrow></mml:msup><mml:msub><mml:mi> ψ </mml:mi><mml:mi> ν </mml:mi></mml:msub></mml:mrow><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:mstyle><mml:mo> = </mml:mo><mml:mi> i </mml:mi><mml:msub><mml:mi> p </mml:mi><mml:mi> μ </mml:mi></mml:msub><mml:msup><mml:mi> g </mml:mi><mml:mrow><mml:mi> μ </mml:mi><mml:mi> ν </mml:mi></mml:mrow></mml:msup><mml:msub><mml:mi> ψ </mml:mi><mml:mi> ν </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></p>
      <disp-formula id="FD9">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>4</mml:mn>
            </mml:msup>
            <mml:mstyle displaystyle="true">
              <mml:msub>
                <mml:mo>∑</mml:mo>
                <mml:mrow>
                  <mml:mi>μ</mml:mi>
                  <mml:mo>,</mml:mo>
                  <mml:mi>ν</mml:mi>
                </mml:mrow>
              </mml:msub>
              <mml:mrow>
                <mml:mfrac>
                  <mml:mo>∂</mml:mo>
                  <mml:mrow>
                    <mml:mo>∂</mml:mo>
                    <mml:msub>
                      <mml:mi>x</mml:mi>
                      <mml:mi>μ</mml:mi>
                    </mml:msub>
                  </mml:mrow>
                </mml:mfrac>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:msup>
                      <mml:mi>t</mml:mi>
                      <mml:mrow>
                        <mml:mo>−</mml:mo>
                        <mml:mn>4</mml:mn>
                      </mml:mrow>
                    </mml:msup>
                    <mml:msup>
                      <mml:mi>g</mml:mi>
                      <mml:mrow>
                        <mml:mi>μ</mml:mi>
                        <mml:mi>ν</mml:mi>
                      </mml:mrow>
                    </mml:msup>
                    <mml:msub>
                      <mml:mi>ψ</mml:mi>
                      <mml:mi>ν</mml:mi>
                    </mml:msub>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
            </mml:mstyle>
            <mml:mo>=</mml:mo>
            <mml:mi>i</mml:mi>
            <mml:msub>
              <mml:mi>p</mml:mi>
              <mml:mi>μ</mml:mi>
            </mml:msub>
            <mml:msup>
              <mml:mi>g</mml:mi>
              <mml:mrow>
                <mml:mi>μ</mml:mi>
                <mml:mi>ν</mml:mi>
              </mml:mrow>
            </mml:msup>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mi>ν</mml:mi>
            </mml:msub>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD10">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>4</mml:mn>
            </mml:msup>
            <mml:mfrac>
              <mml:mo>∂</mml:mo>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:mi>t</mml:mi>
              </mml:mrow>
            </mml:mfrac>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mo>−</mml:mo>
                <mml:mfrac>
                  <mml:mn>1</mml:mn>
                  <mml:mrow>
                    <mml:msup>
                      <mml:mi>R</mml:mi>
                      <mml:mn>2</mml:mn>
                    </mml:msup>
                    <mml:msup>
                      <mml:mi>t</mml:mi>
                      <mml:mn>2</mml:mn>
                    </mml:msup>
                  </mml:mrow>
                </mml:mfrac>
                <mml:msub>
                  <mml:mi>ψ</mml:mi>
                  <mml:mn>0</mml:mn>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>+</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:msup>
                  <mml:mi>t</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:munderover>
              <mml:mstyle mathsize="140%" displaystyle="true">
                <mml:mo>∑</mml:mo>
              </mml:mstyle>
              <mml:mrow>
                <mml:mi>i</mml:mi>
                <mml:mo>=</mml:mo>
                <mml:mn>1</mml:mn>
              </mml:mrow>
              <mml:mn>3</mml:mn>
            </mml:munderover>
            <mml:mfrac>
              <mml:mo>∂</mml:mo>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
              </mml:mrow>
            </mml:mfrac>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mi>i</mml:mi>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mrow>
                <mml:mi>i</mml:mi>
                <mml:msup>
                  <mml:mi>t</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:mo>(</mml:mo>
              <mml:mrow>
                <mml:mstyle displaystyle="true">
                  <mml:msubsup>
                    <mml:mo>∑</mml:mo>
                    <mml:mrow>
                      <mml:mi>i</mml:mi>
                      <mml:mo>=</mml:mo>
                      <mml:mn>1</mml:mn>
                    </mml:mrow>
                    <mml:mn>3</mml:mn>
                  </mml:msubsup>
                  <mml:mrow>
                    <mml:msub>
                      <mml:mi>p</mml:mi>
                      <mml:mi>i</mml:mi>
                    </mml:msub>
                    <mml:msub>
                      <mml:mi>ψ</mml:mi>
                      <mml:mi>i</mml:mi>
                    </mml:msub>
                    <mml:mrow>
                      <mml:mo>(</mml:mo>
                      <mml:mrow>
                        <mml:msub>
                          <mml:mi>x</mml:mi>
                          <mml:mi>i</mml:mi>
                        </mml:msub>
                      </mml:mrow>
                      <mml:mo>)</mml:mo>
                    </mml:mrow>
                  </mml:mrow>
                </mml:mstyle>
                <mml:mo>−</mml:mo>
                <mml:mi>E</mml:mi>
                <mml:msub>
                  <mml:mi>ψ</mml:mi>
                  <mml:mn>0</mml:mn>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>Solving the temporary component and spatial components separately,</p>
      <disp-formula id="FD11">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>4</mml:mn>
            </mml:msup>
            <mml:mfrac>
              <mml:mo>∂</mml:mo>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:mi>t</mml:mi>
              </mml:mrow>
            </mml:mfrac>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mrow>
                <mml:mo>−</mml:mo>
                <mml:mn>2</mml:mn>
              </mml:mrow>
            </mml:msup>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mi>i</mml:mi>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mi>E</mml:mi>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD12">
        <mml:math>
          <mml:mrow>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mfrac>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:msub>
                  <mml:mi>ψ</mml:mi>
                  <mml:mn>0</mml:mn>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:mi>t</mml:mi>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>−</mml:mo>
            <mml:mn>2</mml:mn>
            <mml:mi>t</mml:mi>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mi>i</mml:mi>
            <mml:msup>
              <mml:mi>t</mml:mi>
              <mml:mn>2</mml:mn>
            </mml:msup>
            <mml:mi>E</mml:mi>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD13">
        <mml:math>
          <mml:mrow>
            <mml:mfrac>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:msub>
                  <mml:mi>ψ</mml:mi>
                  <mml:mn>0</mml:mn>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mrow>
                <mml:mo>∂</mml:mo>
                <mml:mi>t</mml:mi>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>=</mml:mo>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mfrac>
                  <mml:mn>2</mml:mn>
                  <mml:mi>t</mml:mi>
                </mml:mfrac>
                <mml:mo>+</mml:mo>
                <mml:mi>i</mml:mi>
                <mml:mi>E</mml:mi>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD14">
        <mml:math>
          <mml:mrow>
            <mml:mi>ln</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>ψ</mml:mi>
                  <mml:mn>0</mml:mn>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mi>i</mml:mi>
            <mml:mstyle displaystyle="true">
              <mml:mrow>
                <mml:mo>∫</mml:mo>
                <mml:mrow>
                  <mml:mi>E</mml:mi>
                  <mml:mtext>d</mml:mtext>
                  <mml:mi>t</mml:mi>
                </mml:mrow>
              </mml:mrow>
            </mml:mstyle>
            <mml:mo>+</mml:mo>
            <mml:mn>2</mml:mn>
            <mml:mi>ln</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>After putting back the natural units, we have the solutions</p>
      <disp-formula id="FD15">
        <label>(4)</label>
        <mml:math>
          <mml:mrow>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mrow>
                        <mml:mi>c</mml:mi>
                        <mml:mi>t</mml:mi>
                      </mml:mrow>
                      <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:mi>exp</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mi>i</mml:mi>
                <mml:mi>φ</mml:mi>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD16">
        <label>(5)</label>
        <mml:math>
          <mml:mrow>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mi>i</mml:mi>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mi>exp</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mi>i</mml:mi>
                <mml:msub>
                  <mml:mi>θ</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:msub>
                      <mml:mi>x</mml:mi>
                      <mml:mi>i</mml:mi>
                    </mml:msub>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD17">
        <mml:math>
          <mml:mrow>
            <mml:mi>φ</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mn>1</mml:mn>
              <mml:mi>ℏ</mml:mi>
            </mml:mfrac>
            <mml:mstyle displaystyle="true">
              <mml:mrow>
                <mml:mo>∫</mml:mo>
                <mml:mrow>
                  <mml:mi>E</mml:mi>
                  <mml:mtext>d</mml:mtext>
                  <mml:mi>t</mml:mi>
                </mml:mrow>
              </mml:mrow>
            </mml:mstyle>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <p>After normalization factor was recovered by integrating the wavefunctions (4) and (5) over the entire space and time, we have</p>
      <disp-formula id="FD18">
        <label>(6)</label>
        <mml:math>
          <mml:mrow>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mn>0</mml:mn>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mi>t</mml:mi>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mn>1</mml:mn>
              <mml:mrow>
                <mml:msqrt>
                  <mml:mrow>
                    <mml:mn>2</mml:mn>
                    <mml:mi>π</mml:mi>
                  </mml:mrow>
                </mml:msqrt>
              </mml:mrow>
            </mml:mfrac>
            <mml:mo>⋅</mml:mo>
            <mml:msup>
              <mml:mrow>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:mfrac>
                      <mml:mrow>
                        <mml:mi>c</mml:mi>
                        <mml:mi>t</mml:mi>
                      </mml:mrow>
                      <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:mi>exp</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mi>i</mml:mi>
                <mml:mi>φ</mml:mi>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mi>t</mml:mi>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
      <disp-formula id="FD19">
        <label>(7)</label>
        <mml:math>
          <mml:mrow>
            <mml:msub>
              <mml:mi>ψ</mml:mi>
              <mml:mi>i</mml:mi>
            </mml:msub>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:msub>
                  <mml:mi>x</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
            <mml:mo>=</mml:mo>
            <mml:mfrac>
              <mml:mn>1</mml:mn>
              <mml:mrow>
                <mml:msqrt>
                  <mml:mrow>
                    <mml:mn>2</mml:mn>
                    <mml:mi>π</mml:mi>
                  </mml:mrow>
                </mml:msqrt>
              </mml:mrow>
            </mml:mfrac>
            <mml:mi>exp</mml:mi>
            <mml:mrow>
              <mml:mo>(</mml:mo>
              <mml:mrow>
                <mml:mi>i</mml:mi>
                <mml:msub>
                  <mml:mi>θ</mml:mi>
                  <mml:mi>i</mml:mi>
                </mml:msub>
                <mml:mrow>
                  <mml:mo>(</mml:mo>
                  <mml:mrow>
                    <mml:msub>
                      <mml:mi>x</mml:mi>
                      <mml:mi>i</mml:mi>
                    </mml:msub>
                  </mml:mrow>
                  <mml:mo>)</mml:mo>
                </mml:mrow>
              </mml:mrow>
              <mml:mo>)</mml:mo>
            </mml:mrow>
          </mml:mrow>
        </mml:math>
      </disp-formula>
    </sec>
    <sec id="sec4">
      <title>4. Analysis of Solutions of the Wave Equation</title>
      <p>The expansion rate of the universe determined after Hubble constant, <italic>H =</italic>1/<italic>R</italic> brings global aspect to the local phenomenon (4) and (6). The wavefunction of (4) / (6) reveals the nature of inflationary universe. There is a correlation relationship between quantum entanglement and inflationary cosmology in [<xref ref-type="bibr" rid="B11">11</xref>]. The nature of quantum entanglement manifests since the wavefunction (6) is time dependent with a factor <inline-formula><mml:math><mml:mrow><mml:msup><mml:mrow><mml:mrow><mml:mo> ( </mml:mo><mml:mrow><mml:mfrac><mml:mrow><mml:mi> c </mml:mi><mml:mi> t </mml:mi></mml:mrow><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:mrow></mml:math></inline-formula> and the phase is a superposition of linearly independent energy eigenstates if the integral is replaced by an infinite sum. If the wavefunction is to remain fixed at an arbitrary time, <italic>t</italic> that means the distribution of energy <italic>E</italic>(<italic>t</italic>) has to change corresponding to the variation of any energy eigenstates in the distribution of energy at that arbitrary time. In other words, an energy eigenstate changes (maybe spin state), all the others change accordingly in order to preserve the phases, <inline-formula><mml:math><mml:mrow><mml:mi> φ </mml:mi><mml:mrow><mml:mo> ( </mml:mo><mml:mi> t </mml:mi><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> θ </mml:mi><mml:mi> i </mml:mi></mml:msub><mml:mrow><mml:mo> ( </mml:mo><mml:mrow><mml:msub><mml:mi> x </mml:mi><mml:mi> i </mml:mi></mml:msub></mml:mrow><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> and in turn the wavefunction (6) as a global phenomenon. Note that the distribution of energy varies independent with the de-Sitter manifold’s causal domains – timelike, spacelike or lightlike. Quantum entanglement can be observed over different cosmological causal domains. Therefore, it is a universal phenomenon over the three stages of cosmological expansions, timelike or lightlike relation <inline-formula><mml:math><mml:mrow><mml:mi> v </mml:mi><mml:mo> ≤ </mml:mo><mml:mi> c </mml:mi></mml:mrow></mml:math></inline-formula> as our current stage or spacelike relation <inline-formula><mml:math><mml:mrow><mml:mi> v </mml:mi><mml:mo> &gt; </mml:mo><mml:mi> c </mml:mi></mml:mrow></mml:math></inline-formula> in the future stage. This is a signature behavior of quantum fields in de-Sitter spacetime.</p>
      <p>Remark: The integral in the phases can be regarded as a Riemann sum of energy eigenstates in which one eigenstate varies, all the others follow so that the sum remains fixed.</p>
    </sec>
    <sec id="sec5">
      <title>5. De-Sitter Space to Minkowski Space</title>
      <p>Revisiting (6), at the limit <italic>ct = R</italic>, back to flat spacetime limit, we recover the plane wave solution of Schrödinger equation. Solution of the wave equation in Minkowski space or Schrödinger equation exists in the light cone of causality as a well known fact. So, quantum entanglement in Minkowski’s limit is restricted only valid in local coordinates, not in global manifold, M, like the one shown previously in de-Sitter space in section 3. Thus, it cannot be called spooky actions at a distance or quantum entanglement in global coordinates. In other words, Schrödinger equation, a local wave theory is just a special case (or the Minkowski’s limit), the temporary component of the solutions <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> ψ </mml:mi><mml:mi> μ </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> , of the general wave equation on curved spacetime (1).</p>
    </sec>
    <sec id="sec6">
      <title>6. Discussions on Dark Matter/Energy in the de-Sitter Universe</title>
      <p>Evidence, like Cosmic Background Radiation shows that our inflationary universe due to a positive value of cosmological constant is due to the existence of dark matter which has an energy called dark energy, comprising more than 90% of the energy of the universe. It is called dark energy because it is not measurable but determined from Einstein Field Equation in the observable universe and its existence was assumed after Hubble observation of the expanding universe. There is an interesting phenomenon, particles creation or annihilation can occur in de-Sitter universe regardless of the stages of evolution of the universe, accelerated or steady state [<xref ref-type="bibr" rid="B12">12</xref>]. This result signifies the existence of dark energy in de-Sitter universe as a pair of photons with cosmic background radiation energy 29.5 MeV that in turn gives rise to an electron-positron pair creation or annihilation (<inline-formula><mml:math><mml:mrow><mml:mi> γ </mml:mi><mml:mi> γ </mml:mi><mml:mo> → </mml:mo><mml:msup><mml:mi> e </mml:mi><mml:mo> − </mml:mo></mml:msup><mml:msup><mml:mi> e </mml:mi><mml:mo> + </mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> ) [<xref ref-type="bibr" rid="B12">12</xref>]. The missing mass 29.5 MeV of dark matter can be analysed through the conservation of four momentum, <inline-formula><mml:math><mml:mrow><mml:msup><mml:mi> p </mml:mi><mml:mi> μ </mml:mi></mml:msup><mml:msub><mml:mi> p </mml:mi><mml:mi> μ </mml:mi></mml:msub><mml:mo> = </mml:mo><mml:msup><mml:mi> m </mml:mi><mml:mn> 2 </mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> or simply as the particles on shell in local coordinates. The four momentum <inline-formula><mml:math><mml:mrow><mml:msup><mml:mi> p </mml:mi><mml:mi> μ </mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> here is the same as the one in (1) so the wavefuctions (6) and (7) both describe the behavior of dark matter as well as ordinary matter. Then integrals of energy and momentum in the phases <inline-formula><mml:math><mml:mrow><mml:mi> φ </mml:mi><mml:mrow><mml:mo> ( </mml:mo><mml:mi> t </mml:mi><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> θ </mml:mi><mml:mi> i </mml:mi></mml:msub><mml:mrow><mml:mo> ( </mml:mo><mml:mrow><mml:msub><mml:mi> x </mml:mi><mml:mi> i </mml:mi></mml:msub></mml:mrow><mml:mo> ) </mml:mo></mml:mrow></mml:mrow></mml:math></inline-formula> are the statistical values of energy and momentum for the ensemble. They are supposed to be the ones used in experimental work, roughly <italic>m</italic> = 29.5 MeV in the Planck scale.</p>
    </sec>
    <sec id="sec7">
      <title>7. Conclusion</title>
      <p>As shown up to this point, quantum field theory in flat space metric is only a partial truth of the one in curved space. Quantum entanglement was illustrated in global coordinates, <italic>t</italic> as well as the expansion of the universe manifested by the metric carrying the factor <italic>R =</italic> 1/<italic>H,</italic>both in the same wave equation<italic>.</italic>The wave equation, a local phenomenon, gauged by the global metric shows the transformation of the vector field through the differential operator <inline-formula><mml:math><mml:mrow><mml:msub><mml:mi> p </mml:mi><mml:mi> μ </mml:mi></mml:msub><mml:mo> = </mml:mo><mml:mo> − </mml:mo><mml:mi> i </mml:mi><mml:msub><mml:mo> ∂ </mml:mo><mml:mi> μ </mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> , in configuration space based on the mathematical concepts developed by Friedlander [<xref ref-type="bibr" rid="B4">4</xref>]. The philosophy of this theory is that quantum field dynamics is governed by causality, particularly in de-Sitter universe. This proves that the theory of general relativity can bring the role of gravity in the theory of quantum field. In the tradition of quantum field theory development, Klein-Gordon equation, Schrödinger equation, and Dirac equation are all good up to local phenomena, no gravitation is conceived if it is considered as a global field. However, in terms of global geometry, one has to rely upon the theory of quantum field on curved spacetime. The wave solutions (6) and (7) being consistent with the hypothesis of quantum entanglement and inflationary universe, address the skeptical question of public concern over the idea of quantizing gravity through the use of the metric of the space as a function of being turned into an operator. It is evident that quantizing gravity is not mathematically justified through the study of this paper, as discussed in section 1. This paper can also shed light on the hypothesis of dark matter as a further investigation on the existence of dark energy by looking at the solutions of the wave equation (1). It seems dark energy embedded with the background manifold like de-Sitter space and Schwarzschild blackhole satisfies Einstein field equation [<xref ref-type="bibr" rid="B13">13</xref>]. Interested researchers may study the field behaviors further, particularly with the metrics of Schwarzschild blackhole [<xref ref-type="bibr" rid="B13">13</xref>] or Kerr blackhole [<xref ref-type="bibr" rid="B14">14</xref>].</p>
    </sec>
    <sec id="sec8">
      <title>Acknowledgements</title>
      <p>I’d like to take this opportunity to show appreciation of my mentor, Dr Dimock with whom I learnt quantum mechanics and in turn quantum field theory on curved spacetime during my PhD dissertation writing times between 2007 and 2009 at University at Buffalo. He taught me the theories in the mathematics settings that form my research background in the current study of field theory. It is no surprise that I inherited his teaching and brought it to light in the two disciplines of physics—high energy physics and cosmology.</p>
    </sec>
  </body>
  <back>
    <ref-list>
      <title>References</title>
      <ref id="B1">
        <label>1.</label>
        <citation-alternatives>
          <mixed-citation publication-type="book">Birrell, N.D. and Davies, P.C.W. (2012) Quantum Fields in Curved Space. Cambridge University Press.</mixed-citation>
          <element-citation publication-type="book">
            <person-group person-group-type="author">
              <string-name>Birrell, N.D.</string-name>
              <string-name>Davies, P.C.W.</string-name>
            </person-group>
            <year>2012</year>
            <article-title>Quantum Fields in Curved Space</article-title>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B2">
        <label>2.</label>
        <citation-alternatives>
          <mixed-citation publication-type="book">Wald, R.M. (1994) Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics. University of Chicago Press.</mixed-citation>
          <element-citation publication-type="book">
            <person-group person-group-type="author">
              <string-name>Wald, R.M.</string-name>
            </person-group>
            <year>1994</year>
            <article-title>Quantum Field Theory in Curved Spacetime and Black Hole Thermodynamics</article-title>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B3">
        <label>3.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Preskill, J. (1990) Quantum Field Theory in Curved Spacetime. Springer.</mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Preskill, J.</string-name>
            </person-group>
            <year>1990</year>
            <article-title>Quantum Field Theory in Curved Spacetime</article-title>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B4">
        <label>4.</label>
        <citation-alternatives>
          <mixed-citation publication-type="book">Friedlander, F.G. (1975) The Wave Equation on a Curved Space-Time. Cambridge University Press.</mixed-citation>
          <element-citation publication-type="book">
            <person-group person-group-type="author">
              <string-name>Friedlander, F.G.</string-name>
            </person-group>
            <year>1975</year>
            <article-title>The Wave Equation on a Curved Space-Time</article-title>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B5">
        <label>5.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Einstein, A. (1916) Die Grundlage der allgemeinen Relativitätstheorie. <italic>Annalen der Physik</italic>, 354, 769-822. <underline> https://doi.org/10.1002/andp.19163540702 </underline><pub-id pub-id-type="doi">10.1002/andp.19163540702</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1002/andp.19163540702">https://doi.org/10.1002/andp.19163540702</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Einstein, A.</string-name>
            </person-group>
            <year>1916</year>
            <article-title>Die Grundlage der allgemeinen Relativitätstheorie</article-title>
            <source>Annalen der Physik</source>
            <volume>354</volume>
            <pub-id pub-id-type="doi">10.1002/andp.19163540702</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B6">
        <label>6.</label>
        <citation-alternatives>
          <mixed-citation publication-type="book">Scadron, M. (1990) Advanced Quantum Theory and Its Applications through Feynman Diagrams. 2nd Edition, Springer.</mixed-citation>
          <element-citation publication-type="book">
            <person-group person-group-type="author">
              <string-name>Scadron, M.</string-name>
              <string-name>Edition, S</string-name>
            </person-group>
            <year>1990</year>
            <article-title>Advanced Quantum Theory and Its Applications through Feynman Diagrams</article-title>
            <source>2nd Edition</source>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B7">
        <label>7.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Poon, G.K. (2010) Relative Unitary Implementability of Perturbed Quantum Field Dynamics on De Sitter Space. <italic>Journal of Mathematical Physics</italic>, 51, Article ID: 042503. <underline> https://doi.org/10.1063/1.3387251 </underline><pub-id pub-id-type="doi">10.1063/1.3387251</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1063/1.3387251">https://doi.org/10.1063/1.3387251</ext-link></mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Poon, G.K.</string-name>
            </person-group>
            <year>2010</year>
            <article-title>Relative Unitary Implementability of Perturbed Quantum Field Dynamics on De Sitter Space</article-title>
            <source>Journal of Mathematical Physics</source>
            <volume>51</volume>
            <fpage>042503</fpage>
            <elocation-id>ID</elocation-id>
            <pub-id pub-id-type="doi">10.1063/1.3387251</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B8">
        <label>8.</label>
        <citation-alternatives>
          <mixed-citation publication-type="book">Dimock, J. (2011) Quantum Mechanics and Quantum Field Theory: A Mathematical Primer. Cambridge University Press. <underline> https://doi.org/10.1017/cbo9780511793349 </underline><pub-id pub-id-type="doi">10.1017/cbo9780511793349</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1017/cbo9780511793349">https://doi.org/10.1017/cbo9780511793349</ext-link></mixed-citation>
          <element-citation publication-type="book">
            <person-group person-group-type="author">
              <string-name>Dimock, J.</string-name>
            </person-group>
            <year>2011</year>
            <article-title>Quantum Mechanics and Quantum Field Theory: A Mathematical Primer</article-title>
            <pub-id pub-id-type="doi">10.1017/cbo9780511793349</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B9">
        <label>9.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Allen, B. (1985) Vacuum States in de Sitter Space. <italic>Physical Review D</italic>, 32, 3136-3149. <underline> https://doi.org/10.1103/physrevd.32.3136 </underline><pub-id pub-id-type="doi">10.1103/physrevd.32.3136</pub-id><pub-id pub-id-type="pmid">9956107</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1103/physrevd.32.3136">https://doi.org/10.1103/physrevd.32.3136</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Allen, B.</string-name>
            </person-group>
            <year>1985</year>
            <article-title>Vacuum States in de Sitter Space</article-title>
            <source>Physical Review D</source>
            <volume>32</volume>
            <pub-id pub-id-type="doi">10.1103/physrevd.32.3136</pub-id>
            <pub-id pub-id-type="pmid">9956107</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B10">
        <label>10.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Norton, J.D. (2013) De Sitter Spacetime. University of Pittsburgh.</mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Norton, J.D.</string-name>
            </person-group>
            <year>2013</year>
            <article-title>De Sitter Spacetime</article-title>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B11">
        <label>11.</label>
        <citation-alternatives>
          <mixed-citation publication-type="journal">Koh, S., Lee, J.H., Park, C. and Ro, D. (2020) Quantum Entanglement in Inflationary Cosmology. <italic>The European Physical Journal C</italic>, 80, Article No. 724. <underline> https://doi.org/10.1140/epjc/s10052-020-8295-x </underline><pub-id pub-id-type="doi">10.1140/epjc/s10052-020-8295-x</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1140/epjc/s10052-020-8295-x">https://doi.org/10.1140/epjc/s10052-020-8295-x</ext-link></mixed-citation>
          <element-citation publication-type="journal">
            <person-group person-group-type="author">
              <string-name>Koh, S.</string-name>
              <string-name>Lee, J.H.</string-name>
              <string-name>Park, C.</string-name>
              <string-name>Ro, D.</string-name>
            </person-group>
            <year>2020</year>
            <article-title>Quantum Entanglement in Inflationary Cosmology</article-title>
            <source>The European Physical Journal C</source>
            <volume>80</volume>
            <elocation-id>No</elocation-id>
            <pub-id pub-id-type="doi">10.1140/epjc/s10052-020-8295-x</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B12">
        <label>12.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Alcántara-Pérez, Y.B., García-Aspeitia, M.A., Martínez-Huerta, H. and Hernández-Almada, A. (2023) Mev Dark Energy Emission from a De Sitter Universe. <italic>Universe</italic>, 9, Article 513. <underline> https://doi.org/10.3390/universe9120513 </underline><pub-id pub-id-type="doi">10.3390/universe9120513</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3390/universe9120513">https://doi.org/10.3390/universe9120513</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Aspeitia, M.A.</string-name>
              <string-name>Huerta, H.</string-name>
              <string-name>Almada, A.</string-name>
            </person-group>
            <year>2023</year>
            <article-title>Mev Dark Energy Emission from a De Sitter Universe</article-title>
            <source>Universe</source>
            <volume>9</volume>
            <elocation-id>513</elocation-id>
            <pub-id pub-id-type="doi">10.3390/universe9120513</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B13">
        <label>13.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Ishwarchandra, N., Ibohal, N. and Yugindro Singh, K. (2014) Schwarzschild Black Hole in Dark Energy Background. <italic>Astrophysics and Space Science</italic>, 353, 633-639. <underline> https://doi.org/10.1007/s10509-014-2071-z </underline><pub-id pub-id-type="doi">10.1007/s10509-014-2071-z</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1007/s10509-014-2071-z">https://doi.org/10.1007/s10509-014-2071-z</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Ishwarchandra, N.</string-name>
              <string-name>Ibohal, N.</string-name>
              <string-name>Singh, K.</string-name>
            </person-group>
            <year>2014</year>
            <article-title>Schwarzschild Black Hole in Dark Energy Background</article-title>
            <source>Astrophysics and Space Science</source>
            <volume>353</volume>
            <pub-id pub-id-type="doi">10.1007/s10509-014-2071-z</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
      <ref id="B14">
        <label>14.</label>
        <citation-alternatives>
          <mixed-citation publication-type="other">Jiménez Madrid, J.A. and González-Díaz, P.F. (2008) Evolution of a Kerr-Newman Black Hole in a Dark Energy Universe. <italic>Gravitation and Cosmology</italic>, 14, 213-225. <underline> https://doi.org/10.1134/s020228930803002x </underline><pub-id pub-id-type="doi">10.1134/s020228930803002x</pub-id><ext-link ext-link-type="uri" xlink:href="https://doi.org/10.1134/s020228930803002x">https://doi.org/10.1134/s020228930803002x</ext-link></mixed-citation>
          <element-citation publication-type="other">
            <person-group person-group-type="author">
              <string-name>Madrid, J.A.</string-name>
            </person-group>
            <year>2008</year>
            <article-title>Evolution of a Kerr-Newman Black Hole in a Dark Energy Universe</article-title>
            <source>Gravitation and Cosmology</source>
            <volume>14</volume>
            <pub-id pub-id-type="doi">10.1134/s020228930803002x</pub-id>
          </element-citation>
        </citation-alternatives>
      </ref>
    </ref-list>
  </back>
</article>