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entries per page: <a href=/list/hep-ex/new?skip=0&show=1000 rel="nofollow"> fewer</a> | <span style="color: #454545">more</span> | <span style="color: #454545">all</span> </div> <dl id='articles'> <h3>New submissions (showing 2 of 2 entries)</h3> <dt> <a name='item1'>[1]</a> <a href ="/abs/2503.16070" title="Abstract" id="2503.16070"> arXiv:2503.16070 </a> [<a href="/pdf/2503.16070" title="Download PDF" id="pdf-2503.16070" aria-labelledby="pdf-2503.16070">pdf</a>, <a href="https://arxiv.org/html/2503.16070v1" title="View HTML" id="html-2503.16070" aria-labelledby="html-2503.16070" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.16070" title="Other formats" id="oth-2503.16070" aria-labelledby="oth-2503.16070">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Search for the radiative leptonic decay $D^+\to纬e^+谓_e$ with Deep Learning </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=BESIII+Collaboration">BESIII Collaboration</a>: <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ablikim,+M">M. Ablikim</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Achasov,+M+N">M. N. Achasov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adlarson,+P">P. Adlarson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ai,+X+C">X. C. Ai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aliberti,+R">R. Aliberti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Amoroso,+A">A. Amoroso</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=An,+Q">Q. An</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bai,+Y">Y. Bai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bakina,+O">O. Bakina</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ban,+Y">Y. Ban</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bao,+H">H.-R. Bao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Batozskaya,+V">V. Batozskaya</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Begzsuren,+K">K. Begzsuren</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Berger,+N">N. Berger</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Berlowski,+M">M. Berlowski</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertani,+M">M. Bertani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bettoni,+D">D. Bettoni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bianchi,+F">F. Bianchi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bianco,+E">E. Bianco</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bortone,+A">A. Bortone</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Boyko,+I">I. Boyko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Briere,+R+A">R. A. Briere</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brueggemann,+A">A. Brueggemann</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cai,+H">H. Cai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cai,+M+H">M. H. Cai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cai,+X">X. Cai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Calcaterra,+A">A. Calcaterra</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cao,+G+F">G. F. Cao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cao,+N">N. Cao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cetin,+S+A">S. A. Cetin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chai,+X+Y">X. Y. Chai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chang,+J+F">J. F. Chang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Che,+G+R">G. R. Che</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Che,+Y+Z">Y. Z. Che</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chelkov,+G">G. Chelkov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+C">C. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+C+H">C. H. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+C">Chao Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+G">G. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+H+S">H. S. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+H+Y">H. Y. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+M+L">M. L. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+S+J">S. J. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+S+L">S. L. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+S+M">S. M. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+T">T. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+X+R">X. R. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+X+T">X. T. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Y+B">Y. B. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Y+Q">Y. Q. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Z+J">Z. J. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Z+K">Z. K. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choi,+S+K">S. K. Choi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chu,+X">X. Chu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cibinetto,+G">G. Cibinetto</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cossio,+F">F. Cossio</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cui,+J+J">J. J. Cui</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dai,+H+L">H. L. Dai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dai,+J+P">J. P. Dai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dbeyssi,+A">A. Dbeyssi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=de+Boer,+R+E">R. E. de Boer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dedovich,+D">D. Dedovich</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Deng,+C+Q">C. Q. Deng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Deng,+Z+Y">Z. Y. Deng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Denig,+A">A. Denig</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Denysenko,+I">I. Denysenko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Destefanis,+M">M. Destefanis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=DeMori,+F">F. DeMori</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+B">B. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+X+X">X. X. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+Y">Y. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+Y">Y. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+Y+X">Y. X. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+J">J. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+L+Y">L. Y. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+M+Y">M. Y. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+X">X. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Du,+M+C">M. C. Du</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Du,+S+X">S. X. Du</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Duan,+Y+Y">Y. Y. Duan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Duan,+Z+H">Z. H. Duan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Egorov,+P">P. Egorov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fan,+G+F">G. F. Fan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fan,+J+J">J. J. Fan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fan,+Y+H">Y. H. Fan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+J">J. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+J">J. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+S+S">S. S. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+W+X">W. X. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+Y+Q">Y. Q. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Farinelli,+R">R. Farinelli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fava,+L">L. Fava</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feldbauer,+F">F. Feldbauer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Felici,+G">G. Felici</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feng,+C+Q">C. Q. Feng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feng,+J+H">J. H. Feng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feng,+Y+T">Y. T. Feng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fritsch,+M">M. Fritsch</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fu,+C+D">C. D. Fu</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 15 pages, 6 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span>; High Energy Physics - Phenomenology (hep-ph) </div> <p class='mathjax'> Using 20.3$~\rm fb^{-1}$ of $e^+e^-$ annihilation data collected at a center-of-mass energy of 3.773$~\rm GeV$ with the BESIII detector, we report an improved search for the radiative leptonic decay $D^+\to\gamma e^+\nu_e$. An upper limit on its partial branching fraction for photon energies $E_\gamma>10~\rm MeV$ is determined to be $1.2\times10^{-5}$ at 90\% confidence level, which excludes most current theoretical predictions. A sophisticated deep learning approach with thorough validation, based on the Transformer architecture, is implemented to efficiently distinguish the signal from massive backgrounds. </p> </div> </dd> <dt> <a name='item2'>[2]</a> <a href ="/abs/2503.16213" title="Abstract" id="2503.16213"> arXiv:2503.16213 </a> [<a href="/pdf/2503.16213" title="Download PDF" id="pdf-2503.16213" aria-labelledby="pdf-2503.16213">pdf</a>, <a href="/format/2503.16213" title="Other formats" id="oth-2503.16213" aria-labelledby="oth-2503.16213">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Search for heavy neutral leptons in decays of W bosons using leptonic and semi-leptonic displaced vertices in $\sqrt{s} = 13$ TeV $pp$ collisions with the ATLAS detector </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=ATLAS+Collaboration">ATLAS Collaboration</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> Comments: 51 pages in total, author list starting page 33, 7 figures, 6 tables, submitted to JHEP. All figures including auxiliary figures are available at <a href="https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/EXOT-2022-12/" rel="external noopener nofollow" class="link-external link-https">this https URL</a> </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span> </div> <p class='mathjax'> A search is performed for long-lived heavy neutral leptons (HNLs), produced through the decay of a $W$ boson along with a muon or electron. Two channels are explored: a leptonic channel, in which the HNL decays into two leptons and a neutrino, and a semi-leptonic channel, in which the HNL decays into a lepton and a charged pion. The search is performed with 140~fb$^{-1}$ of $\sqrt{s} = 13$ TeV proton--proton collision data collected by ATLAS during Run 2 of the Large Hadron Collider. No excess of events is observed; Dirac-like and Majorana-like HNLs with masses below 14.5 GeV and mixing coefficients as small as 10$^{-7}$ are excluded at the 95% confidence level. The results are interpreted under different assumptions on the flavour of the leptons from the HNL decays. </p> </div> </dd> </dl> <dl id='articles'> <h3>Cross submissions (showing 8 of 8 entries)</h3> <dt> <a name='item3'>[3]</a> <a href ="/abs/2503.10825" title="Abstract" id="2503.10825"> arXiv:2503.10825 </a> (cross-list from hep-ph) [<a href="/pdf/2503.10825" title="Download PDF" id="pdf-2503.10825" aria-labelledby="pdf-2503.10825">pdf</a>, <a href="/format/2503.10825" title="Other formats" id="oth-2503.10825" aria-labelledby="oth-2503.10825">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> On Gauge Theories of Neutrino Masses and Dark Matter </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Debnath,+H">Hridoy Debnath</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Perez,+P+F">Pavel Fileviez Perez</a></div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Phenomenology (hep-ph)</span>; Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> We discuss the predictions in the simplest theory for neutrino masses based on the spontaneous breaking of local lepton number. This theory provides a simple theoretical framework to understand the possible relation between the origin of neutrino masses and the nature of the dark matter. In this theory, one of the fields needed for anomaly cancellation is a dark matter candidate and the local lepton number is broken at the low scale. We discuss in great detail the dark matter properties showing the allowed parameter space by the relic density bounds and the predictions for direct detection. The predictions for gamma and neutrino lines from dark matter annihilation are investigated. In the case of Dirac neutrinos, the bound on the effective number of relativistic degrees of freedom plays an important role and the predictions for gamma lines could be tested in the near future. We discuss the predictions in the case of Majorana neutrinos where the dark matter candidate has extra annihilation channels and compare all the predictions to the case with Dirac neutrinos. </p> </div> </dd> <dt> <a name='item4'>[4]</a> <a href ="/abs/2503.15616" title="Abstract" id="2503.15616"> arXiv:2503.15616 </a> (cross-list from physics.ins-det) [<a href="/pdf/2503.15616" title="Download PDF" id="pdf-2503.15616" aria-labelledby="pdf-2503.15616">pdf</a>, <a href="https://arxiv.org/html/2503.15616v1" title="View HTML" id="html-2503.15616" aria-labelledby="html-2503.15616" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.15616" title="Other formats" id="oth-2503.15616" aria-labelledby="oth-2503.15616">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Energy Response and Resolution to Positrons in a Capillary-Tube Dual-Readout Calorimeter </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Albergo,+S+F">Sebastiano Francesco Albergo</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Braghieri,+A">Alessandro Braghieri</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Burdyko,+A">Alexander Burdyko</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Cai,+Y">Yuchen Cai</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Carminati,+L">Leonardo Carminati</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Delfrate,+E">Eleonora Delfrate</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Falchieri,+D">Davide Falchieri</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Ferrari,+R">Roberto Ferrari</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Gaudio,+G">Gabriella Gaudio</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Giacomelli,+P">Paolo Giacomelli</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Centeno,+A+L">Andreas Loeschcke Centeno</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Mazzeo,+E">Elena Mazzeo</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Millesoli,+S">Samuele Millesoli</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Nasella,+L">Laura Nasella</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Negri,+A">Andrea Negri</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Pareti,+A">Andrea Pareti</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Persiani,+R">Rino Persiani</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Pezzotti,+L">Lorenzo Pezzotti</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Polesello,+G">Giacomo Polesello</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Salvatore,+P+F">Pasquale Fabrizio Salvatore</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Santoro,+R">Romualdo Santoro</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Tacchini,+L+D">Luca Davide Tacchini</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Turra,+R">Ruggero Turra</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Valle,+N">Nicolo' Valle</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Vivarelli,+I">Iacopo Vivarelli</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 16 pages, 10 Figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Instrumentation and Detectors (physics.ins-det)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> We present the results of a test beam campaign on a capillary-tube fibre-based dual-readout calorimeter, designed for precise hadronic and electromagnetic energy measurements in future collider experiments. The calorimeter prototype consists of nine modules, each composed of brass capillary tubes housing scintillating and Cherenkov optical fibres, read out using silicon photomultipliers for the central module and photomultiplier tubes for the outer modules. The performance of the detector was assessed using a positron beam with energies ranging from 10 to 120 GeV at the CERN SPS H8 beamline. The prototype is characterised in terms of the linearity and resolution of its energy response to positrons. The results confirm the feasibility of the capillary-tube mechanical design for large-scale dual-readout calorimetry and provide a benchmark for future detector development within the HiDRa project. </p> </div> </dd> <dt> <a name='item5'>[5]</a> <a href ="/abs/2503.16060" title="Abstract" id="2503.16060"> arXiv:2503.16060 </a> (cross-list from cond-mat.mtrl-sci) [<a href="/pdf/2503.16060" title="Download PDF" id="pdf-2503.16060" aria-labelledby="pdf-2503.16060">pdf</a>, <a href="https://arxiv.org/html/2503.16060v1" title="View HTML" id="html-2503.16060" aria-labelledby="html-2503.16060" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.16060" title="Other formats" id="oth-2503.16060" aria-labelledby="oth-2503.16060">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> A Novel Tool for Advanced Analysis of Geant4 Simulations of Charged Particles Interactions in Oriented Crystals </div> <div class='list-authors'><a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Negrello,+R">R. Negrello</a> (1,2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Bandiera,+L">L. Bandiera</a> (2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Canale,+N">N. Canale</a> (2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Fedeli,+P">P. Fedeli</a> (1,2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Guidi,+V">V. Guidi</a> (1,2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Haurylavets,+V+V">V. V. Haurylavets</a>, <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Mazzolari,+A">A. Mazzolari</a> (2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Patern%C3%B2,+G">G. Patern貌</a> (2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Romagnoni,+M">M. Romagnoni</a> (2), <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Tikhomirov,+V+V">V. V. Tikhomirov</a>, <a href="https://arxiv.org/search/cond-mat?searchtype=author&query=Sytov,+A">A. Sytov</a> (2) ((1) Department of Physics and Earth Science, University of Ferrara, Via Saragat 1, 44122 Ferrara, Italy,(2) INFN Section of Ferrara, Via Saragat 1, 44122 Ferrara, Italy)</div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2025 </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Materials Science (cond-mat.mtrl-sci)</span>; High Energy Physics - Experiment (hep-ex); Data Analysis, Statistics and Probability (physics.data-an) </div> <p class='mathjax'> We present a novel Python tool for the analysis of Geant4 simulations that enhances our understanding of coherent phenomena occurring during the interaction of charged particles with crystal planes. This tool compares the total energy of particles with the potential energy inside crystal channels, enabling a complete examination of coherent effects. By tracking the particle trajectory and classifying the dynamics at each simulation step, it provides deeper insights into how different phenomena contribute to both radiation and particle deflection. This tool can be used to improve crystal-based extraction methods and the development of gamma-ray sources using crystals. </p> </div> </dd> <dt> <a name='item6'>[6]</a> <a href ="/abs/2503.16097" title="Abstract" id="2503.16097"> arXiv:2503.16097 </a> (cross-list from hep-ph) [<a href="/pdf/2503.16097" title="Download PDF" id="pdf-2503.16097" aria-labelledby="pdf-2503.16097">pdf</a>, <a href="https://arxiv.org/html/2503.16097v1" title="View HTML" id="html-2503.16097" aria-labelledby="html-2503.16097" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.16097" title="Other formats" id="oth-2503.16097" aria-labelledby="oth-2503.16097">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> NLO corrections and factorization for transverse single-spin asymmetries </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Rein,+D">Daniel Rein</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Schlegel,+M">Marc Schlegel</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Tollk%C3%BChn,+P">Patrick Tollk眉hn</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Vogelsang,+W">Werner Vogelsang</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 7 pages, 4 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Phenomenology (hep-ph)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> We present next-to-leading order QCD corrections for the cross sections for $\ell p^\uparrow\to hX$, $\ell p^\uparrow\to {\mathrm{jet}}X$ with transversely polarized initial protons. These cross sections are known to be power-suppressed in QCD and probe twist-3 parton correlation functions in the proton. Our calculation exhibits the full complexity of a perturbative QCD analysis beyond leading power, involving in particular various derivatives of the parton correlation functions. We demonstrate that collinear factorization for these single-spin observables holds at one loop. We also present exploratory phenomenological results for the NLO single-spin asymmetry in $ep^\uparrow\to hX$ and compare to data from the HERMES experiment. </p> </div> </dd> <dt> <a name='item7'>[7]</a> <a href ="/abs/2503.16119" title="Abstract" id="2503.16119"> arXiv:2503.16119 </a> (cross-list from hep-ph) [<a href="/pdf/2503.16119" title="Download PDF" id="pdf-2503.16119" aria-labelledby="pdf-2503.16119">pdf</a>, <a href="/format/2503.16119" title="Other formats" id="oth-2503.16119" aria-labelledby="oth-2503.16119">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Transverse Nucleon Single-Spin Asymmetry for Single-Inclusive Hadron and Jet Production at NLO Accuracy </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Rein,+D">Daniel Rein</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Schlegel,+M">Marc Schlegel</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Tollk%C3%BChn,+P">Patrick Tollk眉hn</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Vogelsang,+W">Werner Vogelsang</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 79 pages, 27 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Phenomenology (hep-ph)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> We investigate the single-spin asymmetry for the single-inclusive production of hadrons and jets in collisions of transversely polarized nucleons and unpolarized leptons, $\ell N^\uparrow \to (h\,\mathrm{or\,jet})X$. We compute the spin-dependent cross section within collinear twist-3 factorization in perturbative QCD at next-to-leading order (NLO) accuracy. In this approach, multiparton correlations generate a non-vanishing effect. For the present paper, we focus on correlations in the nucleon initial-state rather than in the fragmentation process. We explicitly verify that collinear twist-3 factorization is valid at the one-loop level. Our analytical results show that at NLO the relevant multiparton correlation functions in the nucleon are probed on their full support in momentum fractions. Our numerical analysis for collisions at the Electron-Ion Collider indicates that the NLO corrections can be large and are sensitive to the functional form of the twist-3 correlation functions. </p> </div> </dd> <dt> <a name='item8'>[8]</a> <a href ="/abs/2503.16124" title="Abstract" id="2503.16124"> arXiv:2503.16124 </a> (cross-list from hep-ph) [<a href="/pdf/2503.16124" title="Download PDF" id="pdf-2503.16124" aria-labelledby="pdf-2503.16124">pdf</a>, <a href="https://arxiv.org/html/2503.16124v1" title="View HTML" id="html-2503.16124" aria-labelledby="html-2503.16124" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.16124" title="Other formats" id="oth-2503.16124" aria-labelledby="oth-2503.16124">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Effects of tau-neutrino detection on non-standard interactions at DUNE with a short discussion on the nature of neutrino mixing </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Yu,+X+Y">Xin Yue Yu</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Guan,+Z">Zishen Guan</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Dallaway,+W">William Dallaway</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Rahaman,+U">Ushak Rahaman</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ilic,+N">Nikolina Ilic</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 33 pages, 19 figures, 2 tables </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Phenomenology (hep-ph)</span>; High Energy Physics - Experiment (hep-ex); High Energy Physics - Theory (hep-th) </div> <p class='mathjax'> In this paper, we investigate the effects of $\nu_\tau$ and $\bar{\nu}_\tau$ detection at the DUNE far detector on the experiment's sensitivity to Non-Standard Interactions (NSI) in neutrino propagation. We show that the strongest observable NSI effect in the $\nu_\tau$ and $\bar{\nu}_\tau$ appearance probabilities arises from $\epsilon_{\mu\tau}$. We have studied the hierarchy sensitivity, CP violation sensitivity and octant sensitivity of DUNE from $\nu_\tau$ and $\bar{\nu}_\tau$ appearance channels in presence of NSI. We have also studied the detection sensitivity of NSI phases and the future constaints on NSI parameters from the tau neutrino appearance channels in DUNE. Additionally, we examine the role of $\nu_\tau$ detection in constraining the unitary nature of the PMNS matrix. These studies emphasize the importance of incorporating $\nu_\tau$ detection in long-baseline neutrino experiments such as DUNE. </p> </div> </dd> <dt> <a name='item9'>[9]</a> <a href ="/abs/2503.16173" title="Abstract" id="2503.16173"> arXiv:2503.16173 </a> (cross-list from astro-ph.HE) [<a href="/pdf/2503.16173" title="Download PDF" id="pdf-2503.16173" aria-labelledby="pdf-2503.16173">pdf</a>, <a href="https://arxiv.org/html/2503.16173v1" title="View HTML" id="html-2503.16173" aria-labelledby="html-2503.16173" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.16173" title="Other formats" id="oth-2503.16173" aria-labelledby="oth-2503.16173">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Precision cross-sections for advancing cosmic-ray physics and other applications: a comprehensive programme for the next decade </div> <div class='list-authors'><a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Maurin,+D">D. Maurin</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Audouin,+L">L. Audouin</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Berti,+E">E. Berti</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Coppin,+P">P. Coppin</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Di+Mauro,+M">M. Di Mauro</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=von+Doetinchem,+P">P. von Doetinchem</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Donato,+F">F. Donato</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Evoli,+C">C. Evoli</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=G%C3%A9nolini,+Y">Y. G茅nolini</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Ghosh,+P">P. Ghosh</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Leya,+I">I. Leya</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Losekamm,+M+J">M. J. Losekamm</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Mariani,+S">S. Mariani</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Norbury,+J+W">J. W. Norbury</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Orusa,+L">L. Orusa</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Paniccia,+M">M. Paniccia</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Poeschl,+T">T. Poeschl</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Serpico,+P+D">P. D. Serpico</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Tykhonov,+A">A. Tykhonov</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Unger,+M">M. Unger</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Vanstalle,+M">M. Vanstalle</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Zhao,+M">M.-J. Zhao</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Boncioli,+D">D. Boncioli</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Chiosso,+M">M. Chiosso</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Giordano,+D">D. Giordano</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Coral,+D+M+G">D. M. Gomez Coral</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Graziani,+G">G. Graziani</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Lucarelli,+C">C. Lucarelli</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Maestro,+P">P. Maestro</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Mahlein,+M">M. Mahlein</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Morejon,+L">L. Morejon</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Ocampo-Peleteiro,+J">J. Ocampo-Peleteiro</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Oliva,+A">A. Oliva</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Pierog,+T">T. Pierog</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=%C5%A0erk%C5%A1nyt%C4%97,+L">L. 艩erk拧nyt臈</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 103 pages, 24 figures, 8 tables (submitted to Physics Report) </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Astrophysical Phenomena (astro-ph.HE)</span>; High Energy Physics - Experiment (hep-ex); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th) </div> <p class='mathjax'> Cosmic-ray physics in the GeV-to-TeV energy range has entered a precision era thanks to recent data from space-based experiments. However, the poor knowledge of nuclear reactions, in particular for the production of antimatter and secondary nuclei, limits the information that can be extracted from these data, such as source properties, transport in the Galaxy and indirect searches for particle dark matter. The Cross-Section for Cosmic Rays at CERN workshop series has addressed the challenges encountered in the interpretation of high-precision cosmic-ray data, with the goal of strengthening emergent synergies and taking advantage of the complementarity and know-how in different communities, from theoretical and experimental astroparticle physics to high-energy and nuclear physics. In this paper, we present the outcomes of the third edition of the workshop that took place in 2024. We present the current state of cosmic-ray experiments and their perspectives, and provide a detailed road map to close the most urgent gaps in cross-section data, in order to efficiently progress on many open physics cases, which are motivated in the paper. Finally, with the aim of being as exhaustive as possible, this report touches several other fields -- such as cosmogenic studies, space radiation protection and hadrontherapy -- where overlapping and specific new cross-section measurements, as well as nuclear code improvement and benchmarking efforts, are also needed. We also briefly highlight further synergies between astroparticle and high-energy physics on the question of cross-sections. </p> </div> </dd> <dt> <a name='item10'>[10]</a> <a href ="/abs/2503.16269" title="Abstract" id="2503.16269"> arXiv:2503.16269 </a> (cross-list from physics.acc-ph) [<a href="/pdf/2503.16269" title="Download PDF" id="pdf-2503.16269" aria-labelledby="pdf-2503.16269">pdf</a>, <a href="https://arxiv.org/html/2503.16269v1" title="View HTML" id="html-2503.16269" aria-labelledby="html-2503.16269" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.16269" title="Other formats" id="oth-2503.16269" aria-labelledby="oth-2503.16269">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Coherent radiation in axially oriented industrial-grade tungsten crystals: A viable path for an innovative 纬-rays and positron sources </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Canale,+N">N. Canale</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Romagnoni,+M">M. Romagnoni</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Sytov,+A">A. Sytov</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Alharthi,+F">F. Alharthi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bertelli,+S">S. Bertelli</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Carsi,+S">S. Carsi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Chaikovska,+I">I. Chaikovska</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Chehab,+R">R. Chehab</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=De+Salvador,+D">D. De Salvador</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Fedeli,+P">P. Fedeli</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Guidi,+V">V. Guidi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Haurylavets,+V">V. Haurylavets</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Lezzani,+G">G. Lezzani</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Malagutti,+L">L. Malagutti</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Mangiacavalli,+S">S. Mangiacavalli</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Mazzolari,+A">A. Mazzolari</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Monti-Guarnieri,+P">P. Monti-Guarnieri</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Negrello,+R">R. Negrello</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Patern%C3%B2,+G">G. Patern貌</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Perna,+L">L. Perna</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Bandiera,+L">L. Bandiera</a></div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Volume 1075, June 2025, 170342 </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Accelerator Physics (physics.acc-ph)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> It is known that the alignment of an high-energy e- beam with specific crystal directions leads to a significant increase of the coherent radiation emission. This enhancement can be exploited to create an intense photon source. An elective application is an innovative positron source design for future lepton colliders. Such scheme takes advantage of lattice coherent effects by employing a high-Z crystalline radiator, followed by an amorphous metallic converter, to generate positrons via a two-step electromagnetic process. Additional applications can be in neutron production through photo-transmutation and radionuclide generation via photo-nuclear reactions. In this work, we present experimental results obtained from beam tests at CERN's PS facility using commercial industrial-grade tungsten crystals. The obtained results demonstrate the robust performance of industrial-grade radiators, even with their inherent imperfections, suggesting that it is possible to simplify the supply process and it is not strictly necessary to rely on highly specialized research infrastructures. </p> </div> </dd> </dl> <dl id='articles'> <h3>Replacement submissions (showing 6 of 6 entries)</h3> <dt> <a name='item11'>[11]</a> <a href ="/abs/2410.05526" title="Abstract" id="2410.05526"> arXiv:2410.05526 </a> (replaced) [<a href="/pdf/2410.05526" title="Download PDF" id="pdf-2410.05526" aria-labelledby="pdf-2410.05526">pdf</a>, <a href="https://arxiv.org/html/2410.05526v3" title="View HTML" id="html-2410.05526" aria-labelledby="html-2410.05526" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2410.05526" title="Other formats" id="oth-2410.05526" aria-labelledby="oth-2410.05526">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Measurement of d2sigma/d|q|dEavail in charged current neutrino-nucleus interactions at <Ev> = 1.86 GeV using the NOvA Near Detector </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Acero,+M+A">M. A. Acero</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Acharya,+B">B. Acharya</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adamson,+P">P. Adamson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aliaga,+L">L. Aliaga</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Anfimov,+N">N. Anfimov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Antoshkin,+A">A. Antoshkin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Arrieta-Diaz,+E">E. Arrieta-Diaz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Asquith,+L">L. Asquith</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aurisano,+A">A. Aurisano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Back,+A">A. Back</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Balashov,+N">N. Balashov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Baldi,+P">P. Baldi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bambah,+B+A">B. A. Bambah</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bannister,+E">E. Bannister</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barros,+A">A. Barros</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bashar,+S">S. Bashar</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bat,+A">A. Bat</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bays,+K">K. Bays</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bernstein,+R">R. Bernstein</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bezerra,+T+J+C">T. J. C. Bezerra</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bhatnagar,+V">V. Bhatnagar</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bhattarai,+D">D. Bhattarai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bhuyan,+B">B. Bhuyan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bian,+J">J. Bian</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Booth,+A+C">A. C. Booth</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bowles,+R">R. Bowles</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brahma,+B">B. Brahma</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bromberg,+C">C. Bromberg</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Buchanan,+N">N. Buchanan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Butkevich,+A">A. Butkevich</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Calvez,+S">S. Calvez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Carroll,+T+J">T. J. Carroll</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Catano-Mur,+E">E. Catano-Mur</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cesar,+J+P">J. P. Cesar</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chatla,+A">A. Chatla</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chirco,+R">R. Chirco</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choudhary,+B+C">B. C. Choudhary</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Christensen,+A">A. Christensen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cicala,+M+F">M. F. Cicala</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Coan,+T+E">T. E. Coan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cooleybeck,+A">A. Cooleybeck</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cortes-Parra,+C">C. Cortes-Parra</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Coveyou,+D">D. Coveyou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cremonesi,+L">L. Cremonesi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Davies,+G+S">G. S. Davies</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Derwent,+P+F">P. F. Derwent</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+P">P. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Djurcic,+Z">Z. Djurcic</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dobbs,+K">K. Dobbs</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dolce,+M">M. Dolce</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Doyle,+D">D. Doyle</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Tonguino,+D+D">D. Duenas Tonguino</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dukes,+E+C">E. C. Dukes</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dye,+A">A. Dye</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ehrlich,+R">R. Ehrlich</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ewart,+E">E. Ewart</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Filip,+P">P. Filip</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Frank,+M+J">M. J. Frank</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gallagher,+H+R">H. R. Gallagher</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gao,+F">F. Gao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Giri,+A">A. Giri</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gomes,+R+A">R. A. Gomes</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Goodman,+M+C">M. C. Goodman</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Groh,+M">M. Groh</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=R.+Group">R. Group</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Habig,+A">A. Habig</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hakl,+F">F. Hakl</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hartnell,+J">J. Hartnell</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hatcher,+R">R. Hatcher</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=He,+M">M. He</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Heller,+K">K. Heller</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hewes,+V">V Hewes</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Himmel,+A">A. Himmel</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Horoho,+T">T. Horoho</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ivaneev,+Y">Y. Ivaneev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ivanova,+A">A. Ivanova</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Jargowsky,+B">B. Jargowsky</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Jarosz,+J">J. Jarosz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Johnson,+C">C. Johnson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Judah,+M">M. Judah</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kakorin,+I">I. Kakorin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kaplan,+D+M">D. M. Kaplan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kalitkina,+A">A. Kalitkina</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kirezli-Ozdemir,+B">B. Kirezli-Ozdemir</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kleykamp,+J">J. Kleykamp</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Klimov,+O">O. Klimov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Koerner,+L+W">L. W. Koerner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kolupaeva,+L">L. Kolupaeva</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kralik,+R">R. Kralik</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kumar,+A">A. Kumar</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kuruppu,+C+D">C. D. Kuruppu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kus,+V">V. Kus</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lackey,+T">T. Lackey</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lang,+K">K. Lang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lesmeister,+J">J. Lesmeister</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lister,+A">A. Lister</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Liu,+J">J. Liu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lock,+J+A">J. A. Lock</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lokajicek,+M">M. Lokajicek</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=MacMahon,+M">M. MacMahon</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 20 pages, 15 figures </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Phys. Rev. D 111, 052009 (2025) </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span> </div> <p class='mathjax'> Double- and single-differential cross sections for inclusive charged-current neutrino-nucleus scattering are reported for the kinematic domain 0 to 2 GeV/c in three-momentum transfer and 0 to 2 GeV in available energy, at a mean muon-neutrino energy of 1.86 GeV. The measurements are based on an estimated 995,760 muon-neutrino CC interactions in the scintillator medium of the NOvA Near Detector. The subdomain populated by 2-particle-2-hole reactions is identified by the cross-section excess relative to predictions for neutrino-nucleus scattering that are constrained by a data control sample. Models for 2-particle-2- hole processes are rated by chi-square comparisons of the predicted-versus-measured muon-neutrino CC inclusive cross section over the full phase space and in the restricted subdomain. Shortfalls are observed in neutrino generator predictions obtained using the theory-based Val`encia and SuSAv2 2p2h models. </p> </div> </dd> <dt> <a name='item12'>[12]</a> <a href ="/abs/2410.08603" title="Abstract" id="2410.08603"> arXiv:2410.08603 </a> (replaced) [<a href="/pdf/2410.08603" title="Download PDF" id="pdf-2410.08603" aria-labelledby="pdf-2410.08603">pdf</a>, <a href="https://arxiv.org/html/2410.08603v2" title="View HTML" id="html-2410.08603" aria-labelledby="html-2410.08603" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2410.08603" title="Other formats" id="oth-2410.08603" aria-labelledby="oth-2410.08603">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Observation of $D^+\to畏^\prime渭^+谓_渭$ and First Study of $D^+\to 畏^\prime \ell^+谓_\ell$ Decay Dynamics </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=BESIII+Collaboration">BESIII Collaboration</a>: <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ablikim,+M">M. Ablikim</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Achasov,+M+N">M. N. Achasov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adlarson,+P">P. Adlarson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Afedulidis,+O">O. Afedulidis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ai,+X+C">X. C. Ai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aliberti,+R">R. Aliberti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Amoroso,+A">A. Amoroso</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=An,+Q">Q. An</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bai,+Y">Y. Bai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bakina,+O">O. Bakina</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Balossino,+I">I. Balossino</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ban,+Y">Y. Ban</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bao,+H">H.-R. Bao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Batozskaya,+V">V. Batozskaya</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Begzsuren,+K">K. Begzsuren</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Berger,+N">N. Berger</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Berlowski,+M">M. Berlowski</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertani,+M">M. Bertani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bettoni,+D">D. Bettoni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bianchi,+F">F. Bianchi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bianco,+E">E. Bianco</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bortone,+A">A. Bortone</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Boyko,+I">I. Boyko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Briere,+R+A">R. A. Briere</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brueggemann,+A">A. Brueggemann</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cai,+H">H. Cai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cai,+X">X. Cai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Calcaterra,+A">A. Calcaterra</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cao,+G+F">G. F. Cao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cao,+N">N. Cao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cetin,+S+A">S. A. Cetin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chang,+J+F">J. F. Chang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Che,+G+R">G. R. Che</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chelkov,+G">G. Chelkov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+C">C. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+C+H">C. H. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+C">Chao Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+G">G. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+H+S">H. S. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+H+Y">H. Y. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+M+L">M. L. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+S+J">S. J. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+S+L">S. L. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+S+M">S. M. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+T">T. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+X+R">X. R. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+X+T">X. T. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Y+B">Y. B. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Y+Q">Y. Q. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Z+J">Z. J. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+Z+Y">Z. Y. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choi,+S+K">S. K. Choi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cibinetto,+G">G. Cibinetto</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cossio,+F">F. Cossio</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cui,+J+J">J. J. Cui</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dai,+H+L">H. L. Dai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dai,+J+P">J. P. Dai</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dbeyssi,+A">A. Dbeyssi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=de+Boer,+R+E">R. E. de Boer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dedovich,+D">D. Dedovich</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Deng,+C+Q">C. Q. Deng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Deng,+Z+Y">Z. Y. Deng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Denig,+A">A. Denig</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Denysenko,+I">I. Denysenko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Destefanis,+M">M. Destefanis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Mori,+F">F. De Mori</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+B">B. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+X+X">X. X. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+Y">Y. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ding,+Y">Y. Ding</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+J">J. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+L+Y">L. Y. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+M+Y">M. Y. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+X">X. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Du,+M+C">M. C. Du</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Du,+S+X">S. X. Du</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Duan,+Y+Y">Y. Y. Duan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Duan,+Z+H">Z. H. Duan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Egorov,+P">P. Egorov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fan,+Y+H">Y. H. Fan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+J">J. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+J">J. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+S+S">S. S. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+W+X">W. X. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+Y">Y. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fang,+Y+Q">Y. Q. Fang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Farinelli,+R">R. Farinelli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fava,+L">L. Fava</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feldbauer,+F">F. Feldbauer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Felici,+G">G. Felici</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feng,+C+Q">C. Q. Feng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feng,+J+H">J. H. Feng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feng,+Y+T">Y. T. Feng</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fritsch,+M">M. Fritsch</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fu,+C+D">C. D. Fu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fu,+J+L">J. L. Fu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fu,+Y+W">Y. W. Fu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gao,+H">H. Gao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gao,+X+B">X. B. Gao</a></div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Phys. Rev. Lett. 134, 111801 (2025) </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span> </div> <p class='mathjax'> Using $20.3\,\rm fb^{-1}$ of $e^+e^-$ collision data collected at the center-of-mass energy 3.773\,GeV with the BESIII detector, we report the first observation of the semileptonic decay $D^+\to \eta^\prime \mu^+\nu_\mu$ with significance of $8.6\sigma$ including systematic uncertainties, and an improved measurement of $D^+\to \eta^\prime e^+\nu_e$. The branching fractions of $D^+\to \eta^\prime \mu^+\nu_\mu$ and $D^+\to \eta^\prime e^+\nu_e$ are determined to be $(1.92\pm0.28_{\rm stat}\pm 0.08_{\rm syst})\times 10^{-4}$ and $(1.79\pm0.19_{\rm stat}\pm 0.07_{\rm syst})\times 10^{-4}$, respectively. The ratio of the two branching fractions is determined to be ${\mathcal R}_{\mu/e}=1.07\pm0.19_{\rm stat}\pm 0.03_{\rm syst}$, which agrees with the theoretical expectation of lepton flavor universality within the Standard <a href="http://Model.From" rel="external noopener nofollow" class="link-external link-http">this http URL</a> an analysis of the $D^+\to \eta^\prime \ell^+\nu_\ell$ decay dynamics, the product of the hadronic form factor $f_+^{\eta^{\prime}}(0)$ and the CKM matrix element $|V_{cd}|$ is measured for the first time, giving $f^{\eta^\prime}_+(0)|V_{cd}| = (5.92\pm0.56_{\rm stat}\pm0.13_{\rm syst})\times 10^{-2}$. The $\eta-\eta^\prime$ mixing angle in the quark flavor basis is determined to be $\phi_{\rm P} =(39.8\pm0.8_{\rm stat}\pm0.3_{\rm syst})^\circ$. </p> </div> </dd> <dt> <a name='item13'>[13]</a> <a href ="/abs/2503.15247" title="Abstract" id="2503.15247"> arXiv:2503.15247 </a> (replaced) [<a href="/pdf/2503.15247" title="Download PDF" id="pdf-2503.15247" aria-labelledby="pdf-2503.15247">pdf</a>, <a href="https://arxiv.org/html/2503.15247v2" title="View HTML" id="html-2503.15247" aria-labelledby="html-2503.15247" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2503.15247" title="Other formats" id="oth-2503.15247" aria-labelledby="oth-2503.15247">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Classification of Electron and Muon Neutrino Events for the ESS$谓$SB Near Water Cherenkov Detector using Graph Neural Networks </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aguilar,+J">J. Aguilar</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Anastasopoulos,+M">M. Anastasopoulos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bar%C4%8Dot,+D">D. Bar膷ot</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Baussan,+E">E. Baussan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bhattacharyya,+A">A.K. Bhattacharyya</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bignami,+A">A. Bignami</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Blennow,+M">M. Blennow</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bogomilov,+M">M. Bogomilov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bolling,+B">B. Bolling</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bouquerel,+E">E. Bouquerel</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bramati,+F">F. Bramati</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Branca,+A">A. Branca</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brunetti,+G">G. Brunetti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bustinduy,+I">I. Bustinduy</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Carlile,+C">C.J. Carlile</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cederkall,+J">J. Cederkall</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choi,+T+W">T. W. Choi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choubey,+S">S. Choubey</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Christiansen,+P">P. Christiansen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Collins,+M">M. Collins</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Morales,+E+C">E. Cristaldo Morales</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cupia%C5%82,+P">P. Cupia艂</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=D'Ago,+D">D. D'Ago</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Danared,+H">H. Danared</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=de+Andr%C3%A9,+J+P+A+M">J. P. A. M. de Andr茅</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dracos,+M">M. Dracos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Efthymiopoulos,+I">I. Efthymiopoulos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ekel%C3%B6f,+T">T. Ekel枚f</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Eshraqi,+M">M. Eshraqi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fanourakis,+G">G. Fanourakis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Farricker,+A">A. Farricker</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fasoula,+E">E. Fasoula</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fukuda,+T">T. Fukuda</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Garc%C3%ADa-Marcos,+J">J. Garc铆a-Marcos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gazis,+N">N. Gazis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Geralis,+T">Th. Geralis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ghosh,+M">M. Ghosh</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Giarnetti,+A">A. Giarnetti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gokbulut,+G">G. Gokbulut</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hagner,+C">C. Hagner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hali%C4%87,+L">L. Hali膰</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hooft,+M">M. Hooft</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Iversen,+K+E">K. E. Iversen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Jachowicz,+N">N. Jachowicz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Jenssen,+M">M. Jenssen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Johansson,+R">R. Johansson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Karakoulias,+I">I. Karakoulias</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kasimi,+E">E. Kasimi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Topaksu,+A+K">A. Kayis Topaksu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kildetoft,+B">B. Kildetoft</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kli%C4%8Dek,+B">B. Kli膷ek</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kordas,+K">K. Kordas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Leisos,+A">A. Leisos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lindroos,+M">M. Lindroos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Longhin,+A">A. Longhin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Maiano,+C">C. Maiano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Marangoni,+S">S. Marangoni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Marrelli,+C">C. Marrelli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Meloni,+D">D. Meloni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Mezzetto,+M">M. Mezzetto</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Milas,+N">N. Milas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Mu%C3%B1oz,+J">J.L. Mu帽oz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Niewczas,+K">K. Niewczas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Oglakci,+M">M. Oglakci</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ohlsson,+T">T. Ohlsson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Olveg%C3%A5rd,+M">M. Olveg氓rd</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pari,+M">M. Pari</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Patrzalek,+D">D. Patrzalek</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Petkov,+G">G. Petkov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Petridou,+C">Ch. Petridou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Poussot,+P">P. Poussot</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Psallidas,+A">A. Psallidas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pupilli,+F">F. Pupilli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Saiang,+D">D. Saiang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Sampsonidis,+D">D. Sampsonidis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Schwab,+C">C. Schwab</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Sordo,+F">F. Sordo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Sosa,+A">A. Sosa</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Stavropoulos,+G">G. Stavropoulos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Stip%C4%8Devi%C4%87,+M">M. Stip膷evi膰</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Tarkeshian,+R">R. Tarkeshian</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Terranova,+F">F. Terranova</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Tolba,+T">T. Tolba</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Trachanas,+E">E. Trachanas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Tsenov,+R">R. Tsenov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Tsirigotis,+A">A. Tsirigotis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Tzamarias,+S+E">S. E. Tzamarias</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Vanderpoorten,+M">M. Vanderpoorten</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Vankova-Kirilova,+G">G. Vankova-Kirilova</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Vassilopoulos,+N">N. Vassilopoulos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Vihonen,+S">S. Vihonen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Wurtz,+J">J. Wurtz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Zeter,+V">V. Zeter</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Zormpa,+O">O. Zormpa</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 22 pages, 19 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span>; Instrumentation and Detectors (physics.ins-det) </div> <p class='mathjax'> In the effort to obtain a precise measurement of leptonic CP-violation with the ESS$\nu$SB experiment, accurate and fast reconstruction of detector events plays a pivotal role. In this work, we examine the possibility of replacing the currently proposed likelihood-based reconstruction method with an approach based on Graph Neural Networks (GNNs). As the likelihood-based reconstruction method is reasonably accurate but computationally expensive, one of the benefits of a Machine Learning (ML) based method is enabling fast event reconstruction in the detector development phase, allowing for easier investigation of the effects of changes to the detector design. Focusing on classification of flavour and interaction type in muon and electron events and muon- and electron neutrino interaction events, we demonstrate that the GNN reconstructs events with greater accuracy than the likelihood method for events with greater complexity, and with increased speed for all events. Additionally, we investigate the key factors impacting reconstruction performance, and demonstrate how separation of events by pion production using another GNN classifier can benefit flavour classification. </p> </div> </dd> <dt> <a name='item14'>[14]</a> <a href ="/abs/2408.07336" title="Abstract" id="2408.07336"> arXiv:2408.07336 </a> (replaced) [<a href="/pdf/2408.07336" title="Download PDF" id="pdf-2408.07336" aria-labelledby="pdf-2408.07336">pdf</a>, <a href="https://arxiv.org/html/2408.07336v3" title="View HTML" id="html-2408.07336" aria-labelledby="html-2408.07336" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2408.07336" title="Other formats" id="oth-2408.07336" aria-labelledby="oth-2408.07336">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Performance study of a bakelite RPC prototype built by new technique of linseed oil coating </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Sen,+A">A. Sen</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Mandal,+S">S. Mandal</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Chatterjee,+S">S. Chatterjee</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Gope,+S">S. Gope</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Das,+S">S. Das</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Biswas,+S">S. Biswas</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 16 pages, 14 figures; Accepted in JINST on 28 February 2025 </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Instrumentation and Detectors (physics.ins-det)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> Resistive Plate Chamber (RPC) is one of the most commonly used detectors in high energy physics experiments for triggering and tracking because of its good efficiency ($\textgreater$~90\%) and time resolution ($\sim$~1-2~ns). Generally, bakelite which is one of the most commonly used materials as electrode plates in RPC, sometimes suffers from surface roughness issues. If the surface is not smooth, the probability of micro discharges and spurious pulses increase, which leads to the deterioration in the performance of the detector. We have developed a new method of linseed oil coating for the bakelite based detectors to avoid the surface roughness issue. The detector is characterised with Tetrafluoroethane (R134a) based gas mixture. The detector is also tested with a high rate of gamma radiation environment in the laboratory for the radiation hardness test. The detailed measurement procedure and test results are presented in this article. </p> </div> </dd> <dt> <a name='item15'>[15]</a> <a href ="/abs/2410.21404" title="Abstract" id="2410.21404"> arXiv:2410.21404 </a> (replaced) [<a href="/pdf/2410.21404" title="Download PDF" id="pdf-2410.21404" aria-labelledby="pdf-2410.21404">pdf</a>, <a href="https://arxiv.org/html/2410.21404v3" title="View HTML" id="html-2410.21404" aria-labelledby="html-2410.21404" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2410.21404" title="Other formats" id="oth-2410.21404" aria-labelledby="oth-2410.21404">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Effective field theory for radiative corrections to charged-current processes II: Axial-vector coupling </div> <div class='list-authors'><a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Cirigliano,+V">Vincenzo Cirigliano</a>, <a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Dekens,+W">Wouter Dekens</a>, <a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Mereghetti,+E">Emanuele Mereghetti</a>, <a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Tomalak,+O">Oleksandr Tomalak</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 53 pages, 3 figures, version published in Physical Review D, references added, minor changes in text </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Nuclear Theory (nucl-th)</span>; High Energy Physics - Experiment (hep-ex); High Energy Physics - Phenomenology (hep-ph); Nuclear Experiment (nucl-ex) </div> <p class='mathjax'> We discuss the hadronic structure-dependent radiative corrections to the axial-vector coupling that controls single-nucleon weak charged-current processes -- commonly denoted by $g_A$. We match the Standard Model at the GeV scale onto chiral perturbation theory at next-to-leading order in the one-nucleon sector, in the presence of electromagnetic and weak interactions. As a result, we provide a representation for the corrections to $g_A$ in terms of infrared finite convolutions of simple kernels with the single-nucleon matrix elements of time-ordered products of two and three quark bilinears (vector, axial-vector, and pseudoscalar). We discuss strategies to determine the required non-perturbative input from data, lattice-QCD (+QED), and possibly hadronic models. This work paves the way for a precise comparison of the values of the ratio $g_A/g_V$ extracted from experiment and from lattice-QCD, which constrain physics beyond the Standard Model. </p> </div> </dd> <dt> <a name='item16'>[16]</a> <a href ="/abs/2411.19836" title="Abstract" id="2411.19836"> arXiv:2411.19836 </a> (replaced) [<a href="/pdf/2411.19836" title="Download PDF" id="pdf-2411.19836" aria-labelledby="pdf-2411.19836">pdf</a>, <a href="https://arxiv.org/html/2411.19836v2" title="View HTML" id="html-2411.19836" aria-labelledby="html-2411.19836" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19836" title="Other formats" id="oth-2411.19836" aria-labelledby="oth-2411.19836">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Searching for MeV-mass neutrinophilic Dark Matter with Large Scale Dark Matter Detectors </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Suliga,+A+M">Anna M. Suliga</a> (New York University), <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Fuller,+G+M">George M. Fuller</a> (University of California San Diego)</div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 7 pages, 2 figures. Clarifying changes, matches version published in Phys. Rev. D </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Phys. Rev. D 111, 063052 (2025) </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Phenomenology (hep-ph)</span>; High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> The indirect detection of dark matter (DM) through its annihilation products is one of the primary strategies for DM detection. One of the least constrained classes of models is neutrinophilic DM, because the annihilation products, weakly interacting neutrinos, are challenging to observe. Here, we consider a scenario where MeV-mass DM exclusively annihilates to the third neutrino mass eigenstate, which is predominantly of tau and muon flavor. In such a scenario, the potential detection rate of the neutrinos originating from the DM annihilation in our Galaxy in the conventional detectors would be suppressed by up to approximately two orders of magnitude. This is because the best sensitivity of such detectors for neutrinos with energies below approximately 100 MeV is for electron neutrino flavor. In this work, we highlight the potential of large-scale DM detectors in uncovering such signals in the tens of MeV range of DM masses. In addition, we discuss how coincident signals in direct detection DM experiments and upcoming neutrino detectors such as DUNE, Hyper-Kamiokande, and JUNO could provide new perspectives on the DM problem. </p> </div> </dd> </dl> <div class='paging'>Total of 16 entries </div> <div class='morefewer'>Showing up to 2000 entries per page: <a href=/list/hep-ex/new?skip=0&show=1000 rel="nofollow"> fewer</a> | <span style="color: #454545">more</span> | <span style="color: #454545">all</span> </div> </div> </div> </div> </main> <footer style="clear: both;"> <div class="columns is-desktop" role="navigation" aria-label="Secondary" style="margin: -0.75em -0.75em 0.75em -0.75em">  <div class="column" style="padding: 0;"> <div class="columns"> <div class="column"> <ul style="list-style: none; line-height: 2;"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul style="list-style: none; line-height: 2;"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div>   <div class="column" style="padding: 0;"> <div class="columns"> <div class="column"> <ul style="list-style: none; 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