Physical Review D最新文献

{"title":"Scotogenic model with U(1) symmetry and a scalar dark matter","authors":"Anjan Kumar Barik, Najimuddin Khan, Santosh Kumar Rai","doi":"10.1103/physrevd.111.075023","DOIUrl":"https://doi.org/10.1103/physrevd.111.075023","url":null,"abstract":"We study a scotogenic model augmented with an additional U</a:mi>(</a:mo>1</a:mn>)</a:mo></a:math> gauge and a discrete <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:msub><e:mi>Z</e:mi><e:mn>2</e:mn></e:msub></e:math> symmetry. The lightest <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:msub><g:mi>Z</g:mi><g:mn>2</g:mn></g:msub></g:math>-odd particle in our model becomes the dark matter (DM) candidate while tiny neutrino masses are realized at one loop. We explore the parameter space of the model for which the DM relic density is satisfied, and the correct low-energy neutrino observables are reproduced. The extended gauge symmetry includes a beyond Standard Model (SM) particle spectrum consisting of vectorlike fermions and scalars. We also highlight possible collider signatures of these particles at the LHC. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"33 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143862284","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Implications of the first CONUS+ measurement of coherent elastic neutrino-nucleus scattering","authors":"V. De Romeri, D. K. Papoulias, G. Sanchez Garcia","doi":"10.1103/physrevd.111.075025","DOIUrl":"https://doi.org/10.1103/physrevd.111.075025","url":null,"abstract":"The CONUS</a:mi>+</a:mo></a:mrow></a:math> collaboration has reported their first observation of coherent elastic neutrino-nucleus scattering (<c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mrow><c:mi>CE</c:mi><c:mrow><c:mi>ν</c:mi></c:mrow><c:mi>NS</c:mi></c:mrow></c:math>). The experiment uses reactor electron antineutrinos and germanium detectors with recoil thresholds as low as <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mn>160</e:mn><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mrow><e:msub><e:mi>eV</e:mi><e:mi>ee</e:mi></e:msub></e:mrow></e:math>. With an exposure of <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mrow><g:mn>327</g:mn><g:mtext> </g:mtext><g:mtext> </g:mtext><g:mi>kg</g:mi><g:mo>×</g:mo><g:mi mathvariant=\"normal\">d</g:mi></g:mrow></g:math>, the measurement was made with a statistical significance of <j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><j:mn>3.7</j:mn><j:mi>σ</j:mi></j:math>. We explore several physics implications of this observation, both within the standard model and in the context of new physics. We focus on a determination of the weak mixing angle, nonstandard and generalized neutrino interactions both with heavy and light mediators, neutrino magnetic moments, and the up-scattering of neutrinos into sterile fermions through the sterile dipole portal and new mediators. Our results highlight the role of reactor-based <l:math xmlns:l=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><l:mrow><l:mi>CE</l:mi><l:mrow><l:mi>ν</l:mi></l:mrow><l:mi>NS</l:mi></l:mrow></l:math> experiments in probing a vast array of neutrino properties and new physics models. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"18 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143862321","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Estimate of the S -wave D*K scattering length in the isospin-0 channel from Belle and LHCb data","authors":"N. N. Achasov, G. N. Shestakov","doi":"10.1103/physrevd.111.076022","DOIUrl":"https://doi.org/10.1103/physrevd.111.076022","url":null,"abstract":"It is shown that the Belle and LHCb data on the interference of the amplitudes of the S&lt;/a:mi&gt;&lt;/a:mrow&gt;&lt;/a:math&gt; and &lt;c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;c:mrow&gt;&lt;c:mi&gt;D&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;/c:math&gt; partial waves in the decays &lt;e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;e:msub&gt;&lt;e:mi&gt;D&lt;/e:mi&gt;&lt;e:mrow&gt;&lt;e:mi&gt;s&lt;/e:mi&gt;&lt;e:mn&gt;1&lt;/e:mn&gt;&lt;/e:mrow&gt;&lt;/e:msub&gt;&lt;e:mo stretchy=\"false\"&gt;(&lt;/e:mo&gt;&lt;e:mn&gt;2536&lt;/e:mn&gt;&lt;e:msup&gt;&lt;e:mo stretchy=\"false\"&gt;)&lt;/e:mo&gt;&lt;e:mo&gt;+&lt;/e:mo&gt;&lt;/e:msup&gt;&lt;e:mo stretchy=\"false\"&gt;→&lt;/e:mo&gt;&lt;e:msup&gt;&lt;e:mi&gt;D&lt;/e:mi&gt;&lt;e:mrow&gt;&lt;e:mo&gt;*&lt;/e:mo&gt;&lt;e:mo&gt;+&lt;/e:mo&gt;&lt;/e:mrow&gt;&lt;/e:msup&gt;&lt;e:msubsup&gt;&lt;e:mi&gt;K&lt;/e:mi&gt;&lt;e:mi&gt;S&lt;/e:mi&gt;&lt;e:mn&gt;0&lt;/e:mn&gt;&lt;/e:msubsup&gt;&lt;/e:math&gt; and &lt;j:math xmlns:j=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;j:msub&gt;&lt;j:mi&gt;D&lt;/j:mi&gt;&lt;j:mrow&gt;&lt;j:mi&gt;s&lt;/j:mi&gt;&lt;j:mn&gt;1&lt;/j:mn&gt;&lt;/j:mrow&gt;&lt;/j:msub&gt;&lt;j:mo stretchy=\"false\"&gt;(&lt;/j:mo&gt;&lt;j:mn&gt;2536&lt;/j:mn&gt;&lt;j:msup&gt;&lt;j:mo stretchy=\"false\"&gt;)&lt;/j:mo&gt;&lt;j:mo&gt;−&lt;/j:mo&gt;&lt;/j:msup&gt;&lt;j:mo stretchy=\"false\"&gt;→&lt;/j:mo&gt;&lt;j:msup&gt;&lt;j:mover accent=\"true\"&gt;&lt;j:mi&gt;D&lt;/j:mi&gt;&lt;j:mo stretchy=\"false\"&gt;¯&lt;/j:mo&gt;&lt;/j:mover&gt;&lt;j:mrow&gt;&lt;j:mo&gt;*&lt;/j:mo&gt;&lt;j:mn&gt;0&lt;/j:mn&gt;&lt;/j:mrow&gt;&lt;/j:msup&gt;&lt;j:msup&gt;&lt;j:mi&gt;K&lt;/j:mi&gt;&lt;j:mo&gt;−&lt;/j:mo&gt;&lt;/j:msup&gt;&lt;/j:math&gt; allow us to obtain an estimate of the &lt;q:math xmlns:q=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;q:mrow&gt;&lt;q:mi&gt;S&lt;/q:mi&gt;&lt;/q:mrow&gt;&lt;/q:math&gt;-wave &lt;s:math xmlns:s=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;s:msup&gt;&lt;s:mi&gt;D&lt;/s:mi&gt;&lt;s:mo&gt;*&lt;/s:mo&gt;&lt;/s:msup&gt;&lt;s:mi&gt;K&lt;/s:mi&gt;&lt;/s:math&gt; scattering length in the channel with isospin &lt;u:math xmlns:u=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;u:mi&gt;I&lt;/u:mi&gt;&lt;u:mo&gt;=&lt;/u:mo&gt;&lt;u:mn&gt;0&lt;/u:mn&gt;&lt;/u:math&gt;: &lt;w:math xmlns:w=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;w:mo stretchy=\"false\"&gt;|&lt;/w:mo&gt;&lt;w:msubsup&gt;&lt;w:mi&gt;a&lt;/w:mi&gt;&lt;w:mrow&gt;&lt;w:msup&gt;&lt;w:mi&gt;D&lt;/w:mi&gt;&lt;w:mo&gt;*&lt;/w:mo&gt;&lt;/w:msup&gt;&lt;w:mi&gt;K&lt;/w:mi&gt;&lt;/w:mrow&gt;&lt;w:mrow&gt;&lt;w:mo stretchy=\"false\"&gt;(&lt;/w:mo&gt;&lt;w:mn&gt;0&lt;/w:mn&gt;&lt;w:mo stretchy=\"false\"&gt;)&lt;/w:mo&gt;&lt;/w:mrow&gt;&lt;/w:msubsup&gt;&lt;w:mo stretchy=\"false\"&gt;|&lt;/w:mo&gt;&lt;w:mo&gt;=&lt;/w:mo&gt;&lt;w:mo stretchy=\"false\"&gt;(&lt;/w:mo&gt;&lt;w:mn&gt;0.94&lt;/w:mn&gt;&lt;w:mo&gt;±&lt;/w:mo&gt;&lt;w:mn&gt;0.06&lt;/w:mn&gt;&lt;w:mo stretchy=\"false\"&gt;)&lt;/w:mo&gt;&lt;w:mtext&gt; &lt;/w:mtext&gt;&lt;w:mtext&gt; &lt;/w:mtext&gt;&lt;w:mi&gt;fm&lt;/w:mi&gt;&lt;/w:math&gt;. The possibility of explaining the found value by the contribution of the &lt;eb:math xmlns:eb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;eb:msub&gt;&lt;eb:mi&gt;D&lt;/eb:mi&gt;&lt;eb:mrow&gt;&lt;eb:mi&gt;s&lt;/eb:mi&gt;&lt;eb:mn&gt;1&lt;/eb:mn&gt;&lt;/eb:mrow&gt;&lt;/eb:msub&gt;&lt;eb:mo stretchy=\"false\"&gt;(&lt;/eb:mo&gt;&lt;eb:mn&gt;2460&lt;/eb:mn&gt;&lt;eb:mo stretchy=\"false\"&gt;)&lt;/eb:mo&gt;&lt;/eb:math&gt; resonance is discussed. The decay of &lt;ib:math xmlns:ib=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;ib:msub&gt;&lt;ib:mi&gt;B&lt;/ib:mi&gt;&lt;ib:mrow&gt;&lt;ib:mi&gt;s&lt;/ib:mi&gt;&lt;ib:mn&gt;1&lt;/ib:mn&gt;&lt;/ib:mrow&gt;&lt;/ib:msub&gt;&lt;ib:mo stretchy=\"false\"&gt;(&lt;/ib:mo&gt;&lt;ib:mn&gt;5830&lt;/ib:mn&gt;&lt;ib:mo stretchy=\"false\"&gt;)&lt;/ib:mo&gt;&lt;ib:mo stretchy=\"false\"&gt;→&lt;/ib:mo&gt;&lt;ib:msup&gt;&lt;ib:mi&gt;B&lt;/ib:mi&gt;&lt;ib:mo&gt;*&lt;/ib:mo&gt;&lt;/ib:msup&gt;&lt;ib:mover accent=\"true\"&gt;&lt;ib:mi&gt;K&lt;/ib:mi&gt;&lt;ib:mo stretchy=\"false\"&gt;¯&lt;/ib:mo&gt;&lt;/ib:mover&gt;&lt;/ib:math&gt; is also briefly discussed. &lt;jats:supplementa","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"25 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857664","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Collinear parton dynamics beyond Dokshitzer-Gribov-Lipatov-Altarelli-Parisi framework","authors":"Hao Chen, Max Jaarsma, Yibei Li, Ian Moult, Wouter J. Waalewijn, Hua Xing Zhu","doi":"10.1103/physrevd.111.076021","DOIUrl":"https://doi.org/10.1103/physrevd.111.076021","url":null,"abstract":"Renormalization group evolution equations describing the scale dependence of quantities in quantum chromodynamics play a central role in the interpretation of experimental data. Arguably the most important evolution equations for collider physics applications are the Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) equations, which describe the evolution of a quark or gluon fragmenting into hadrons, with only a hadron identified at a time. In recent years, the study of the correlations of energy flow within jets has come to play a central role at collider experiments, necessitating an understanding of correlations, going beyond the standard DGLAP paradigm. In this paper we derive a general renormalization group equation describing the collinear dynamics that account for correlations in the fragmentation. We compute the kernel of this evolution equation at next-to-leading order, where it involves the 1</a:mn>→</a:mo>3</a:mn></a:mrow></a:math> splitting functions, and develop techniques to solve it numerically. We show that our equation encompasses all previously known collinear evolution equations, namely DGLAP and the evolution of multihadron fragmentation functions. As an application of our results, we consider the phenomenologically relevant example of energy flow on charged particles, computing the energy fraction in charged particles in <d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:msup><d:mi>e</d:mi><d:mo>+</d:mo></d:msup><d:msup><d:mi>e</d:mi><d:mo>−</d:mo></d:msup><d:mo stretchy=\"false\">→</d:mo></d:math> hadrons at next-to-next-to-leading order. Our results are an important step toward improving the understanding of the collinear dynamics of jets, with broad applications in jet substructure, ranging from the study of multihadron correlations, to the description of inclusive (sub)jet production, and the advancement of modern parton showers. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"37 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857657","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"CPT symmetry and its breaking in the chiral fermion formalism","authors":"I. P-Castro, J. L. Díaz-Cruz, A. Pérez-Lorenzana","doi":"10.1103/physrevd.111.076023","DOIUrl":"https://doi.org/10.1103/physrevd.111.076023","url":null,"abstract":"In this paper, we review the fundamental aspects of N</a:mi>=</a:mo>1</a:mn></a:math> supergravity and employ the chiral formalism to describe spin-<d:math xmlns:d=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><d:mfrac><d:mn>3</d:mn><d:mn>2</d:mn></d:mfrac></d:math> fermions. Armed with this, we analyze the discrete symmetries of the graviton in the context of linearized gravity (LG) and Rarita-Schwinger (RS) fields, which include the description of the gravitino. Additionally, we highlight the advantages of the chiral formalism in classifying Lorentz and <f:math xmlns:f=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><f:mi>C</f:mi><f:mi>P</f:mi><f:mi>T</f:mi></f:math>-violating terms in RS theories, extending these models by including Lorentz-violating operators, as has been done in LG. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"7 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857658","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Cornering relative symmetry theories","authors":"Mirjam Cvetič, Ron Donagi, Jonathan J. Heckman, Max Hübner, Ethan Torres","doi":"10.1103/physrevd.111.085026","DOIUrl":"https://doi.org/10.1103/physrevd.111.085026","url":null,"abstract":"The symmetry data of a d</a:mi></a:math>-dimensional quantum field theory (QFT) can often be captured in terms of a higher-dimensional symmetry topological field theory. In top-down (i.e., stringy) realizations of this structure, the QFT in question is localized in a higher-dimensional bulk. In many cases of interest, however, the associated (<c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:mrow><c:mi>d</c:mi><c:mo>+</c:mo><c:mn>1</c:mn></c:mrow></c:math>)-dimensional bulk is not fully gapped and one must instead consider a filtration of theories to reach a gapped bulk in <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mi>D</e:mi><e:mo>=</e:mo><e:mi>d</e:mi><e:mo>+</e:mo><e:mi>m</e:mi></e:math> dimensions. Overall, this leads us to a nested structure of relative symmetry theories which descend to coupled edge modes, with the original QFT degrees of freedom localized at a corner of this <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mi>D</g:mi></g:math>-dimensional bulk system. We present a bottom-up characterization of this structure and also show how it naturally arises in a number of string-based constructions of QFTs with both finite and continuous symmetries. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"25 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857727","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Hidden charm Pcs(4338)0 production in baryonic B−→J/ψΛp¯ decay","authors":"Yu-Kuo Hsiao, Shu-Ting Cai, Yan-Li Wang","doi":"10.1103/physrevd.111.076020","DOIUrl":"https://doi.org/10.1103/physrevd.111.076020","url":null,"abstract":"We investigate the resonant baryonic B&lt;/a:mi&gt;&lt;/a:math&gt; decay &lt;c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;c:mrow&gt;&lt;c:msup&gt;&lt;c:mrow&gt;&lt;c:mi&gt;B&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;c:mrow&gt;&lt;c:mo&gt;−&lt;/c:mo&gt;&lt;/c:mrow&gt;&lt;/c:msup&gt;&lt;c:mo stretchy=\"false\"&gt;→&lt;/c:mo&gt;&lt;c:msubsup&gt;&lt;c:mrow&gt;&lt;c:mi mathvariant=\"script\"&gt;P&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;c:mrow&gt;&lt;c:mi&gt;c&lt;/c:mi&gt;&lt;c:mi&gt;s&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;c:mrow&gt;&lt;c:mn&gt;0&lt;/c:mn&gt;&lt;/c:mrow&gt;&lt;/c:msubsup&gt;&lt;c:mover accent=\"true\"&gt;&lt;c:mrow&gt;&lt;c:mi&gt;p&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;c:mrow&gt;&lt;c:mo stretchy=\"false\"&gt;¯&lt;/c:mo&gt;&lt;/c:mrow&gt;&lt;/c:mover&gt;&lt;c:mo&gt;,&lt;/c:mo&gt;&lt;c:msubsup&gt;&lt;c:mrow&gt;&lt;c:mi mathvariant=\"script\"&gt;P&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;c:mrow&gt;&lt;c:mi&gt;c&lt;/c:mi&gt;&lt;c:mi&gt;s&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;c:mrow&gt;&lt;c:mn&gt;0&lt;/c:mn&gt;&lt;/c:mrow&gt;&lt;/c:msubsup&gt;&lt;c:mo stretchy=\"false\"&gt;→&lt;/c:mo&gt;&lt;c:mi&gt;J&lt;/c:mi&gt;&lt;c:mo&gt;/&lt;/c:mo&gt;&lt;c:mi&gt;ψ&lt;/c:mi&gt;&lt;c:mi mathvariant=\"normal\"&gt;Λ&lt;/c:mi&gt;&lt;/c:mrow&gt;&lt;/c:math&gt;, where &lt;l:math xmlns:l=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;l:mrow&gt;&lt;l:msubsup&gt;&lt;l:mrow&gt;&lt;l:mi mathvariant=\"script\"&gt;P&lt;/l:mi&gt;&lt;/l:mrow&gt;&lt;l:mrow&gt;&lt;l:mi&gt;c&lt;/l:mi&gt;&lt;l:mi&gt;s&lt;/l:mi&gt;&lt;/l:mrow&gt;&lt;l:mrow&gt;&lt;l:mn&gt;0&lt;/l:mn&gt;&lt;/l:mrow&gt;&lt;/l:msubsup&gt;&lt;l:mo&gt;≡&lt;/l:mo&gt;&lt;l:msub&gt;&lt;l:mrow&gt;&lt;l:mi mathvariant=\"script\"&gt;P&lt;/l:mi&gt;&lt;/l:mrow&gt;&lt;l:mrow&gt;&lt;l:mi&gt;c&lt;/l:mi&gt;&lt;l:mi&gt;s&lt;/l:mi&gt;&lt;/l:mrow&gt;&lt;/l:msub&gt;&lt;l:mo stretchy=\"false\"&gt;(&lt;/l:mo&gt;&lt;l:mn&gt;4338&lt;/l:mn&gt;&lt;l:msup&gt;&lt;l:mrow&gt;&lt;l:mo stretchy=\"false\"&gt;)&lt;/l:mo&gt;&lt;/l:mrow&gt;&lt;l:mrow&gt;&lt;l:mn&gt;0&lt;/l:mn&gt;&lt;/l:mrow&gt;&lt;/l:msup&gt;&lt;/l:mrow&gt;&lt;/l:math&gt; is identified as a hidden charm pentaquark candidate with strangeness. By interpreting &lt;r:math xmlns:r=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;r:msubsup&gt;&lt;r:mi mathvariant=\"script\"&gt;P&lt;/r:mi&gt;&lt;r:mrow&gt;&lt;r:mi&gt;c&lt;/r:mi&gt;&lt;r:mi&gt;s&lt;/r:mi&gt;&lt;/r:mrow&gt;&lt;r:mn&gt;0&lt;/r:mn&gt;&lt;/r:msubsup&gt;&lt;/r:math&gt; as the &lt;u:math xmlns:u=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;u:msub&gt;&lt;u:mi mathvariant=\"normal\"&gt;Ξ&lt;/u:mi&gt;&lt;u:mi&gt;c&lt;/u:mi&gt;&lt;/u:msub&gt;&lt;u:mover accent=\"true\"&gt;&lt;u:mi&gt;D&lt;/u:mi&gt;&lt;u:mo stretchy=\"false\"&gt;¯&lt;/u:mo&gt;&lt;/u:mover&gt;&lt;/u:math&gt; molecule that strongly decays into &lt;z:math xmlns:z=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;z:mi&gt;J&lt;/z:mi&gt;&lt;z:mo&gt;/&lt;/z:mo&gt;&lt;z:mi&gt;ψ&lt;/z:mi&gt;&lt;z:mi mathvariant=\"normal\"&gt;Λ&lt;/z:mi&gt;&lt;/z:math&gt; and &lt;cb:math xmlns:cb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;cb:msub&gt;&lt;cb:mi&gt;η&lt;/cb:mi&gt;&lt;cb:mi&gt;c&lt;/cb:mi&gt;&lt;/cb:msub&gt;&lt;cb:mi mathvariant=\"normal\"&gt;Λ&lt;/cb:mi&gt;&lt;/cb:math&gt;, we discover a dominant triangle rescattering effect for &lt;fb:math xmlns:fb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;fb:mrow&gt;&lt;fb:msup&gt;&lt;fb:mrow&gt;&lt;fb:mi&gt;B&lt;/fb:mi&gt;&lt;/fb:mrow&gt;&lt;fb:mrow&gt;&lt;fb:mo&gt;−&lt;/fb:mo&gt;&lt;/fb:mrow&gt;&lt;/fb:msup&gt;&lt;fb:mo stretchy=\"false\"&gt;→&lt;/fb:mo&gt;&lt;fb:msubsup&gt;&lt;fb:mrow&gt;&lt;fb:mi mathvariant=\"script\"&gt;P&lt;/fb:mi&gt;&lt;/fb:mrow&gt;&lt;fb:mrow&gt;&lt;fb:mi&gt;c&lt;/fb:mi&gt;&lt;fb:mi&gt;s&lt;/fb:mi&gt;&lt;/fb:mrow&gt;&lt;fb:mrow&gt;&lt;fb:mn&gt;0&lt;/fb:mn&gt;&lt;/fb:mrow&gt;&lt;/fb:msubsup&gt;&lt;fb:mover accent=\"true\"&gt;&lt;fb:mrow&gt;&lt;fb:mi&gt;p&lt;/fb:mi&gt;&lt;/fb:mrow&gt;&lt;fb:mrow&gt;&lt;fb:mo stretchy=\"false\"&gt;¯&lt;/fb:mo&gt;&lt;/fb:mrow&gt;&lt;/fb:mover&gt;&lt;/fb:mrow&gt;&lt;/fb:math&gt;, initiated by &lt;lb:math xmlns:lb=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"&gt;&lt;lb:mrow&gt;&lt;lb:msup&gt;&lt;lb:mrow&gt;&lt;lb:mi&gt;B&lt;/lb:mi&gt;&lt;/lb:mrow&gt;&lt;lb:mrow&gt;&lt;lb:mo&gt;−&lt;/lb:mo&gt;&lt;/lb:mrow&gt;&lt;/lb:msup&gt;&lt;lb:mo stretchy=\"false\"&gt;→&lt;/lb:mo&gt;","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"85 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857660","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Role of the chiral anomaly in polarized deeply inelastic scattering. III. Wess-Zumino-Witten contributions and chiral Ward identities for finite quark mass","authors":"Andrey Tarasov, Raju Venugopalan","doi":"10.1103/physrevd.111.074027","DOIUrl":"https://doi.org/10.1103/physrevd.111.074027","url":null,"abstract":"We extend our prior results on the worldline computation of the axial vector-vector-vector (AVV) triangle anomaly in polarized deeply inelastic scattering (DIS) to the finite mass case by computing in addition the pseudoscalar-vector-vector (PVV) triangle graph. For the well-studied QED case, we show explicitly how the off-forward AVV pole exactly cancels an identical PVV pole. We then demonstrate the dramatic difference in QCD due to the chiral condensate, which qualitatively modifies anomalous Ward identities. As in the massless case, the anomaly pole in QCD is canceled by the dynamics of a primordial isosinglet pseudoscalar η</a:mi>¯</a:mo></a:mover></a:math>-meson, whose Wess-Zumino-Witten coupling to the topological charge density shifts the pole to the physical <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:msup><e:mi>η</e:mi><e:mo>′</e:mo></e:msup></e:math> mass, with the finite quark mass contribution differing by <g:math xmlns:g=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><g:mi>O</g:mi><g:mo stretchy=\"false\">(</g:mo><g:mn>10</g:mn><g:mo>%</g:mo><g:mo stretchy=\"false\">)</g:mo></g:math> from the Witten-Veneziano formula. We obtain a compact analytic expression for the finite mass corrections to Shore and Veneziano’s result that the proton’s net quark helicity <k:math xmlns:k=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><k:mi mathvariant=\"normal\">Δ</k:mi><k:mi mathvariant=\"normal\">Σ</k:mi><k:mo>∝</k:mo><k:msqrt><k:mrow><k:msubsup><k:mi>χ</k:mi><k:mi>QCD</k:mi><k:mo>′</k:mo></k:msubsup><k:msub><k:mo stretchy=\"false\">|</k:mo><k:mrow><k:mi>m</k:mi><k:mo>=</k:mo><k:mn>0</k:mn></k:mrow></k:msub><k:mo stretchy=\"false\">(</k:mo><k:mn>0</k:mn><k:mo stretchy=\"false\">)</k:mo></k:mrow></k:msqrt></k:math>, the forward slope of the topological susceptibility in the chiral limit, and show they are of the order of a few percentages. Our prior prediction that the polarized DIS structure function <r:math xmlns:r=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><r:msub><r:mi>g</r:mi><r:mn>1</r:mn></r:msub></r:math> is quenched by sphaleronlike topological transitions at small <t:math xmlns:t=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><t:mi>x</t:mi></t:math> is unaffected by quark mass effects. Our results illustrate how worldline computations of anomalous processes, in synergy with lattice computations and nonet chiral perturbation theory, can uncover novel nonperturbative features of QCD at the Electron-Ion Collider. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"52 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857659","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Identifying neutrino mass ordering with cosmic gravitational focusing","authors":"Shao-Feng Ge, Liang Tan","doi":"10.1103/physrevd.111.083539","DOIUrl":"https://doi.org/10.1103/physrevd.111.083539","url":null,"abstract":"The cosmic gravitational focusing (CGF) of relic neutrinos can provide an independent measurement of the absolute neutrino masses m</a:mi></a:mrow>i</a:mi></a:mrow></a:msub></a:mrow></a:math> with fourth-power dependence (<c:math xmlns:c=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><c:msubsup><c:mi>m</c:mi><c:mi>i</c:mi><c:mn>4</c:mn></c:msubsup></c:math>). We demonstrate in this paper for the first time how this can help identify the neutrino mass ordering, using the fact that total mass falling below the inverted ordering threshold allows the discrimination of inverted ordering. Upon incorporating the projected CGF sensitivity at DESI, the preference for the normal ordering with a prior <e:math xmlns:e=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><e:mo>∑</e:mo><e:msub><e:mi>m</e:mi><e:mi>i</e:mi></e:msub><e:mo>&gt;</e:mo><e:mn>0.059</e:mn><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mi>eV</e:mi></e:math> would increase from the original 89.9% of the existing matter clustering method with the DESI analysis to 98.2% while the inverted ordering is further disfavored from 10.1% to 1.8%. We also show how this can affect the prospects of the neutrinoless double beta and single beta decay measurements. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"108 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143857745","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Vortex state properties in multiphoton scalar pair production","authors":"Hong-Hao Fan, Cui-Wen Zhang, Suo Tang, Bai-Song Xie","doi":"10.1103/physrevd.111.076017","DOIUrl":"https://doi.org/10.1103/physrevd.111.076017","url":null,"abstract":"The vortex state properties of a pair of scalar particles produced in a strong circularly polarized electromagnetic standing wave field are investigated under the dipole approximation in the multiphoton regime. We find that vortex orientation is related to the intrinsic orbital angular momentum of created particles associating with the helicity of absorbed photons, while the magnitude of the orbital angular momentum, i.e., the topology charge, is determined by the number of absorbed photons. Moreover, the properties of particle creation and vortices formation can be understood by analyzing the pair production process in quasiparticle representation. This study provides new insights into the angular momentum transfer from field to particle in the scalar pair production process in vacuum. It is expected that there are similar findings about vortex features for different spin alignment in electron-positron pair production in strong fields via the topology charge as a new freedom. <jats:supplementary-material> <jats:copyright-statement>Published by the American Physical Society</jats:copyright-statement> <jats:copyright-year>2025</jats:copyright-year> </jats:permissions> </jats:supplementary-material>","PeriodicalId":20167,"journal":{"name":"Physical Review D","volume":"40 1","pages":""},"PeriodicalIF":5.0,"publicationDate":"2025-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143849437","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}