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aria-labelledby="recent-hep-ex" href="/list/hep-ex/recent">recent</a> articles</p> <h3>Showing new listings for Monday, 2 December 2024</h3> <div class='paging'>Total of 35 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> <dl id='articles'> <h3>New submissions (showing 11 of 11 entries)</h3> <dt> <a name='item1'>[1]</a> <a href ="/abs/2411.18639" title="Abstract" id="2411.18639"> arXiv:2411.18639 </a> [<a href="/pdf/2411.18639" title="Download PDF" id="pdf-2411.18639" aria-labelledby="pdf-2411.18639">pdf</a>, <a href="/format/2411.18639" title="Other formats" id="oth-2411.18639" aria-labelledby="oth-2411.18639">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Averages of $b$-hadron, $c$-hadron, and $\tau$-lepton properties as of 2023 </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Banerjee,+S">Sw. Banerjee</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ben-Haim,+E">E. Ben-Haim</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bernlochner,+F">F. Bernlochner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertholet,+E">E. Bertholet</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bona,+M">M. Bona</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bozek,+A">A. Bozek</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bozzi,+C">C. Bozzi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brodzicka,+J">J. Brodzicka</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chobanova,+V">V. Chobanova</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chrzaszcz,+M">M. Chrzaszcz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Egede,+U">U. Egede</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gersabeck,+M">M. Gersabeck</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Goldenzweig,+P">P. Goldenzweig</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gharbi,+N">N. Gharbi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Grillo,+L">L. Grillo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hayasaka,+K">K. Hayasaka</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Humair,+T">T. Humair</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Johnson,+D">D. Johnson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kuhr,+T">T. Kuhr</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Leroy,+O">O. Leroy</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lusiani,+A">A. Lusiani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ma,+H">H.-L. Ma</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Margoni,+M">M. Margoni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Mizuk,+R">R. Mizuk</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Naik,+P">P. Naik</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Petri,+T+N">T. Nanut Petri</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Castro,+A+P">A. Pereiro Castro</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Prim,+M">M. Prim</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Roney,+M">M. Roney</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Rotondo,+M">M. Rotondo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Schneider,+O">O. Schneider</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Schwanda,+C">C. Schwanda</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Schwartz,+A+J">A. J. Schwartz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Serrano,+J">J. Serrano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Shwartz,+B">B. Shwartz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Soffer,+A">A. Soffer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Whitehead,+M">M. Whitehead</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Yelton,+J">J. Yelton</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 523 pages. arXiv admin note: substantial text overlap with <a href="https://arxiv.org/abs/2206.07501" data-arxiv-id="2206.07501" class="link-https">arXiv:2206.07501</a>, <a href="https://arxiv.org/abs/1909.12524" data-arxiv-id="1909.12524" class="link-https">arXiv:1909.12524</a>; text overlap with <a href="https://arxiv.org/abs/1612.07233" data-arxiv-id="1612.07233" class="link-https">arXiv:1612.07233</a>, <a href="https://arxiv.org/abs/1412.7515" data-arxiv-id="1412.7515" class="link-https">arXiv:1412.7515</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'> This paper reports world averages of measurements of $b$-hadron, $c$-hadron, and $\tau$-lepton properties obtained by the Heavy Flavour Averaging Group using results available before October 2023. In rare cases, significant results obtained several months later are also used. For the averaging, common input parameters used in the various analyses are adjusted (rescaled) to common values, and known correlations are taken into account. The averages include branching fractions, lifetimes, neutral meson mixing parameters, \CP~violation parameters, parameters of semileptonic decays, and Cabibbo-Kobayashi-Maskawa matrix elements. </p> </div> </dd> <dt> <a name='item2'>[2]</a> <a href ="/abs/2411.18641" title="Abstract" id="2411.18641"> arXiv:2411.18641 </a> [<a href="/pdf/2411.18641" title="Download PDF" id="pdf-2411.18641" aria-labelledby="pdf-2411.18641">pdf</a>, <a href="/format/2411.18641" title="Other formats" id="oth-2411.18641" aria-labelledby="oth-2411.18641">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> First constraints on the coherent elastic scattering of reactor antineutrinos off xenon nuclei </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Akimov,+D">D.Yu. Akimov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Alexandrov,+I">I.S. Alexandrov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Belov,+V">V.A. Belov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bolozdynya,+A">A.I. Bolozdynya</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Etenko,+A">A.V. Etenko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Galavanov,+A">A.V. Galavanov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gusakov,+Y">Yu.V. Gusakov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Khromov,+A">A.V. Khromov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Konovalov,+A">A.M. Konovalov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kornoukhov,+V">V.N. Kornoukhov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kovalenko,+A">A.G. Kovalenko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kozlova,+E">E.S. Kozlova</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kumpan,+A">A.V. Kumpan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lukyashin,+A">A.V. Lukyashin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pinchuk,+A">A.V. Pinchuk</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Razuvaeva,+O">O.E. Razuvaeva</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Rudik,+D">D.G. Rudik</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Shakirov,+A">A.V. Shakirov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Simakov,+G">G.E. Simakov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Sosnovstsev,+V">V.V. Sosnovstsev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Vasin,+A">A.A. Vasin</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'> RED-100 is a two-phase emission detector with an active volume containing 126~kg of liquid xenon. The detector was exposed to the antineutrino flux of about $1.4 \cdot 10^{13}~$cm$^{-2}$s$^{-1}$ at a distance of 19~m from the 3.1~GW Kalinin Nuclear Power Plant (KNPP) reactor core. The comparison of data from 331~kg$\cdot$days with the reactor on and 106~kg$\cdot$days with the reactor off shows no statistically significant excess and allows to put constraints on coherent elastic interactions of antineutrinos with xenon nuclei. </p> </div> </dd> <dt> <a name='item3'>[3]</a> <a href ="/abs/2411.18787" title="Abstract" id="2411.18787"> arXiv:2411.18787 </a> [<a href="/pdf/2411.18787" title="Download PDF" id="pdf-2411.18787" aria-labelledby="pdf-2411.18787">pdf</a>, <a href="https://arxiv.org/html/2411.18787v1" title="View HTML" id="html-2411.18787" aria-labelledby="html-2411.18787" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18787" title="Other formats" id="oth-2411.18787" aria-labelledby="oth-2411.18787">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Observation of collider neutrinos without final state muons with the SND@LHC experiment </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=SND@LHC+Collaboration">SND@LHC Collaboration</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 7 pages, 3 figures </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'> We report the observation of neutrino interactions without final state muons at the LHC, with a significance of 6.4$ \sigma$. A data set of proton-proton collisions at $\sqrt{s}= 13.6$ TeV collected by SND@LHC in 2022 and 2023 is used, corresponding to an integrated luminosity of 68.6 fb$^{-1}$. Neutrino interactions without a reconstructed muon are selected, resulting in an event sample consisting mainly of neutral-current and electron neutrino charged-current interactions in the detector. After selection cuts, 9 neutrino interaction candidate events are observed with an estimated background of 0.32 events. </p> </div> </dd> <dt> <a name='item4'>[4]</a> <a href ="/abs/2411.18976" title="Abstract" id="2411.18976"> arXiv:2411.18976 </a> [<a href="/pdf/2411.18976" title="Download PDF" id="pdf-2411.18976" aria-labelledby="pdf-2411.18976">pdf</a>, <a href="https://arxiv.org/html/2411.18976v1" title="View HTML" id="html-2411.18976" aria-labelledby="html-2411.18976" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18976" title="Other formats" id="oth-2411.18976" aria-labelledby="oth-2411.18976">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Precision measurement of the longitudinal double-spin asymmetry for dijet production at intermediate pseudorapidity in polarized $pp$ collisions at $\sqrt{s}$ = 200 GeV </div> <div class='list-authors'>The <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=STAR+Collaboration">STAR Collaboration</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 17 pages, 9 figures. Submit to PRD </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'> The STAR Collaboration reports precise measurements of the longitudinal double-spin asymmetry, $A_{LL}$, for dijet production with at least one jet at intermediate pseudorapidity $0.8 < \eta_{\rm jet} < 1.8$ in polarized proton-proton collisions at a center-of-mass energy of 200 GeV. This study explores partons scattered with a longitudinal momentum fraction ($x$) from 0.01 to 0.5, which are predominantly characterized by interactions between high-$x$ valence quarks and low-$x$ gluons. The results are in good agreement with previous measurements at 200 GeV with improved precision and are found to be consistent with the predictions of global analyses that find the gluon polarization to be positive. In contrast, the negative gluon polarization solution from the JAM Collaboration is found to be strongly disfavored. </p> </div> </dd> <dt> <a name='item5'>[5]</a> <a href ="/abs/2411.19078" title="Abstract" id="2411.19078"> arXiv:2411.19078 </a> [<a href="/pdf/2411.19078" title="Download PDF" id="pdf-2411.19078" aria-labelledby="pdf-2411.19078">pdf</a>, <a href="https://arxiv.org/html/2411.19078v1" title="View HTML" id="html-2411.19078" aria-labelledby="html-2411.19078" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19078" title="Other formats" id="oth-2411.19078" aria-labelledby="oth-2411.19078">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aiello,+S">S. Aiello</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Albert,+A">A. Albert</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Alhebsi,+A+R">A. R. Alhebsi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Alshamsi,+M">M. Alshamsi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Garre,+S+A">S. Alves Garre</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ambrosone,+A">A. Ambrosone</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ameli,+F">F. Ameli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andre,+M">M. Andre</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aphecetche,+L">L. Aphecetche</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ardid,+M">M. Ardid</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ardid,+S">S. Ardid</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aublin,+J">J. Aublin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Badaracco,+F">F. Badaracco</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bailly-Salins,+L">L. Bailly-Salins</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barda%C4%8Dov%C3%A1,+Z">Z. Barda膷ov谩</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Baret,+B">B. Baret</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bariego-Quintana,+A">A. Bariego-Quintana</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Becherini,+Y">Y. Becherini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bendahman,+M">M. Bendahman</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Benfenati,+F">F. Benfenati</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Benhassi,+M">M. Benhassi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bennani,+M">M. Bennani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Benoit,+D+M">D. M. Benoit</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Berbee,+E">E. Berbee</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertin,+V">V. Bertin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Biagi,+S">S. Biagi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Boettcher,+M">M. Boettcher</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bonanno,+D">D. Bonanno</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bouasla,+A+B">A. B. Bouasla</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Boumaaza,+J">J. Boumaaza</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bouta,+M">M. Bouta</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bouwhuis,+M">M. Bouwhuis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bozza,+C">C. Bozza</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bozza,+R+M">R. M. Bozza</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Br%C3%A2nz%C4%83%C5%9F,+H">H. Br芒nz膬艧</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bretaudeau,+F">F. Bretaudeau</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Breuhaus,+M">M. Breuhaus</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bruijn,+R">R. Bruijn</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brunner,+J">J. Brunner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bruno,+R">R. Bruno</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Buis,+E">E. Buis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Buompane,+R">R. Buompane</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Busto,+J">J. Busto</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Caiffi,+B">B. Caiffi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Calvo,+D">D. Calvo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Capone,+A">A. Capone</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Carenini,+F">F. Carenini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Carretero,+V">V. Carretero</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cartraud,+T">T. Cartraud</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Castaldi,+P">P. Castaldi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cecchini,+V">V. Cecchini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Celli,+S">S. Celli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cerisy,+L">L. Cerisy</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chabab,+M">M. Chabab</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chen,+A">A. Chen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cherubini,+S">S. Cherubini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chiarusi,+T">T. Chiarusi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Circella,+M">M. Circella</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Clark,+R">R. Clark</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cocimano,+R">R. Cocimano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Coelho,+J+A+B">J. A. B. Coelho</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Coleiro,+A">A. Coleiro</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Condorelli,+A">A. Condorelli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Coniglione,+R">R. Coniglione</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Coyle,+P">P. Coyle</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Creusot,+A">A. Creusot</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cuttone,+G">G. Cuttone</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dallier,+R">R. Dallier</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Benedittis,+A">A. De Benedittis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Martino,+B">B. De Martino</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Wasseige,+G">G. De Wasseige</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Decoene,+V">V. Decoene</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Del+Rosso,+I">I. Del Rosso</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Di+Mauro,+L+S">L. S. Di Mauro</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Di+Palma,+I">I. Di Palma</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=D%C3%ADaz,+A+F">A. F. D铆az</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Diego-Tortosa,+D">D. Diego-Tortosa</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Distefano,+C">C. Distefano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Domi,+A">A. Domi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Donzaud,+C">C. Donzaud</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dornic,+D">D. Dornic</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Drakopoulou,+E">E. Drakopoulou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Drouhin,+D">D. Drouhin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ducoin,+J">J.-G. Ducoin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dvornick%C3%BD,+R">R. Dvornick媒</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Eberl,+T">T. Eberl</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Eckerov%C3%A1,+E">E. Eckerov谩</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Eddymaoui,+A">A. Eddymaoui</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=van+Eeden,+T">T. van Eeden</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Eff,+M">M. Eff</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=van+Eijk,+D">D. van Eijk</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bojaddaini,+I+E">I. El Bojaddaini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hedri,+S+E">S. El Hedri</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ellajosyula,+V">V. Ellajosyula</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Enzenh%C3%B6fer,+A">A. Enzenh枚fer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ferrara,+G">G. Ferrara</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Filipovi%C4%87,+M+D">M. D. Filipovi膰</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Filippini,+F">F. Filippini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Franciotti,+D">D. Franciotti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fusco,+L+A">L. A. Fusco</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'> KM3NeT/ORCA is an underwater neutrino telescope under construction in the Mediterranean Sea. Its primary scientific goal is to measure the atmospheric neutrino oscillation parameters and to determine the neutrino mass ordering. ORCA can constrain the oscillation parameters $\Delta m^{2}_{31}$ and $\theta_{23}$ by reconstructing the arrival direction and energy of multi-GeV neutrinos crossing the Earth. Searches for deviations from the Standard Model of particle physics in the forward scattering of neutrinos inside Earth matter, produced by Non-Standard Interactions, can be conducted by investigating distortions of the standard oscillation pattern of neutrinos of all flavours. This work reports on the results of the search for non-standard neutrino interactions using the first six detection units of ORCA and 433 kton-years of exposure. No significant deviation from standard interactions was found in a sample of 5828 events reconstructed in the 1 GeV$-$1 TeV energy range. The flavour structure of the non-standard coupling was constrained at 90\% confidence level to be $|\varepsilon_{\mu\tau} | \leq 5.4 \times 10^{-3}$, $|\varepsilon_{e\tau} | \leq 7.4 \times 10^{-2}$, $|\varepsilon_{e\mu} | \leq 5.6 \times 10^{-2}$ and $-0.015 \leq \varepsilon_{\tau\tau} - \varepsilon_{\mu\mu} \leq 0.017$. The results are comparable to the current most stringent limits placed on the parameters by other experiments. </p> </div> </dd> <dt> <a name='item6'>[6]</a> <a href ="/abs/2411.19469" title="Abstract" id="2411.19469"> arXiv:2411.19469 </a> [<a href="/pdf/2411.19469" title="Download PDF" id="pdf-2411.19469" aria-labelledby="pdf-2411.19469">pdf</a>, <a href="https://arxiv.org/html/2411.19469v1" title="View HTML" id="html-2411.19469" aria-labelledby="html-2411.19469" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19469" title="Other formats" id="oth-2411.19469" aria-labelledby="oth-2411.19469">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Search for the Electric Dipole Moment of the Tau Lepton at the Super Tau-Charm Facility </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Sun,+X">Xulei Sun</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Zhou,+X">Xiaorong Zhou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Wu,+Y">Yongcheng Wu</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 14 pages, 10 figures </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'> This study investigates the intrinsic electric dipole moment (EDM) of the $\tau$ lepton, an important quantity in the search for physics beyond the Standard Model (BSM). In preparation for future measurements at the Super Tau-Charm Facility (STCF), this research uses Monte Carlo simulations of the $e^+e^- \rightarrow \tau^+\tau^-$ process and optimizes the methodologies needed to obtain the EDM. Machine learning techniques are utilized to effectively identify signal photons and events, resulting in a significant improvement in signal-to-noise ratio. The event selection algorithm is optimized, achieving signal purity of $80.0\%$ with an efficiency of $6.3\%$. Furthermore, an analytical approach is introduced to solve for the $\tau$ lepton momentum, and accordingly the squared spin density matrix and optimal observables are derived. The relationship between these observables and the EDM is established, with the estimated sensitivity from the $\pi\pi$ channel of $|d_\tau| < 3.49\times 10^{-18}\,e\,\mathrm{cm}$, laying the foundation for future experimental measurements of the $\tau$ lepton EDM in STCF experiments. </p> </div> </dd> <dt> <a name='item7'>[7]</a> <a href ="/abs/2411.19506" title="Abstract" id="2411.19506"> arXiv:2411.19506 </a> [<a href="/pdf/2411.19506" title="Download PDF" id="pdf-2411.19506" aria-labelledby="pdf-2411.19506">pdf</a>, <a href="https://arxiv.org/html/2411.19506v1" title="View HTML" id="html-2411.19506" aria-labelledby="html-2411.19506" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19506" title="Other formats" id="oth-2411.19506" aria-labelledby="oth-2411.19506">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Real-time Anomaly Detection at the L1 Trigger of CMS Experiment </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gandrakota,+A">Abhijith Gandrakota</a> (on behalf of CMS collaboration)</div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> Contribution to 42nd International Conference on High Energy Physics (ICHEP 2024) </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span>; Machine Learning (cs.LG); Data Analysis, Statistics and Probability (physics.data-an) </div> <p class='mathjax'> We present the preparation, deployment, and testing of an autoencoder trained for unbiased detection of new physics signatures in the CMS experiment Global Trigger (GT) test crate FPGAs during LHC Run 3. The GT makes the final decision whether to readout or discard the data from each LHC collision, which occur at a rate of 40 MHz, within a 50 ns latency. The Neural Network makes a prediction for each event within these constraints, which can be used to select anomalous events for further analysis. The GT test crate is a copy of the main GT system, receiving the same input data, but whose output is not used to trigger the readout of CMS, providing a platform for thorough testing of new trigger algorithms on live data, but without interrupting data taking. We describe the methodology to achieve ultra low latency anomaly detection, and present the integration of the DNN into the GT test crate, as well as the monitoring, testing, and validation of the algorithm during proton collisions. </p> </div> </dd> <dt> <a name='item8'>[8]</a> <a href ="/abs/2411.19642" title="Abstract" id="2411.19642"> arXiv:2411.19642 </a> [<a href="/pdf/2411.19642" title="Download PDF" id="pdf-2411.19642" aria-labelledby="pdf-2411.19642">pdf</a>, <a href="https://arxiv.org/html/2411.19642v1" title="View HTML" id="html-2411.19642" aria-labelledby="html-2411.19642" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19642" title="Other formats" id="oth-2411.19642" aria-labelledby="oth-2411.19642">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Measurement of the Inclusive Cross Sections of Prompt $J/\psi$ and $\psi(3686)$ Production in $e^{+}e^{-}$ Annihilation from $\sqrt{s}=3.808$ to $4.951$ GeV </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,+M+R">M. R. An</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=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=Chang,+T+T">T. T. Chang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chang,+W+L">W. L. 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">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,+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+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=Cheng,+W+S">W. S. Cheng</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=Coen,+S+C">S. C. Coen</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,+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,+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+Y">Y.H. Y. Fan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fan,+Y+L">Y. L. 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,+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=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=Fischer,+K">K Fischer</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=Fritzsch,+C">C. Fritzsch</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,+Y+N">Y. N. Gao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gao,+Y">Yang Gao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Garbolino,+S">S. Garbolino</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 20 pages, 6 figures </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'> The inclusive cross sections of prompt $J/\psi$ and $\psi(3686)$ production are measured at center-of-mass energies from 3.808 to 4.951 GeV. The dataset used is 22 fb$^{-1}$ of $e^{+}e^{-}$ annihilation data collected with the BESIII detector operating at the BEPCII storage ring. The results obtained are in agreement with the previous BESIII measurements of exclusive $J/\psi$ and $\psi(3686)$ production. The average values obtained for the cross sections measured in the center-of-mass energy ranges from 4.527 to 4.951 GeV for $J/\psi$ and from 4.843 to 4.951 GeV for $\psi(3686)$, where the impact of known resonances is negligible, are $14.0\pm1.7\pm3.1$ pb and $15.3\pm3.0$ pb, respectively. For $J/\psi$, the first and the second uncertainties are statistical and systematic, respectively. For $\psi(3686)$, the uncertainty is total. These values are useful for testing charmonium production models. </p> </div> </dd> <dt> <a name='item9'>[9]</a> <a href ="/abs/2411.19749" title="Abstract" id="2411.19749"> arXiv:2411.19749 </a> [<a href="/pdf/2411.19749" title="Download PDF" id="pdf-2411.19749" aria-labelledby="pdf-2411.19749">pdf</a>, <a href="https://arxiv.org/html/2411.19749v1" title="View HTML" id="html-2411.19749" aria-labelledby="html-2411.19749" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19749" title="Other formats" id="oth-2411.19749" aria-labelledby="oth-2411.19749">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Proton reconstruction with the TOTEM Roman pot detectors for high-$\beta^*$ LHC data </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=CMS+Collaboration">CMS Collaboration</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=TOTEM+Collaboration">TOTEM Collaboration</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> Submitted to the Journal of Instrumentation. All figures and tables can be found at <a href="http://cms-results.web.cern.ch/cms-results/public-results/publications/SMP-23-006" rel="external noopener nofollow" class="link-external link-http">this http URL</a> (CMS Public Pages) </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'> The TOTEM Roman pot detectors are used to reconstruct the transverse momentum of scattered protons and to estimate the transverse location of the primary interaction. This paper presents new methods of track reconstruction, measurements of strip-level detection efficiencies, cross-checks of the LHC beam optics, and detector alignment techniques, along with their application in the selection of signal collision events. The track reconstruction is performed by exploiting hit cluster information through a novel method using a common polygonal area in the intercept-slope plane. The technique is applied in the relative alignment of detector layers with $\mu$m precision. A tag-and-probe method is used to extract strip-level detection efficiencies. The alignment of the Roman pot system is performed through time-dependent adjustments, resulting in a position accuracy of 3 $\mu$m in the horizontal and 60 $\mu$m in the vertical directions. The goal is to provide an optimal reconstruction tool for central exclusive physics analyses based on the high-$\beta^*$ data-taking period at $\sqrt{s}$ = 13 TeV in 2018. </p> </div> </dd> <dt> <a name='item10'>[10]</a> <a href ="/abs/2411.19767" title="Abstract" id="2411.19767"> arXiv:2411.19767 </a> [<a href="/pdf/2411.19767" title="Download PDF" id="pdf-2411.19767" aria-labelledby="pdf-2411.19767">pdf</a>, <a href="https://arxiv.org/html/2411.19767v1" title="View HTML" id="html-2411.19767" aria-labelledby="html-2411.19767" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19767" title="Other formats" id="oth-2411.19767" aria-labelledby="oth-2411.19767">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Recent measurements of top cross sections at CMS </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=del+Riego,+J">Javier del Riego</a> (on behalf of the CMS Collaboration)</div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> Talk at the 17th International Workshop on Top Quark Physics (Top2024), 22-27 September 2024 </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'> This contribution presents recent cross section measurements for top quark pair production (tt) and single top quark production in association with a W boson (tW) in proton-proton collisions at the CMS experiment at LHC. For tt production, data from 2017 at a center-of-mass (CM) energy of 5.02 TeV with an integrated luminosity of 302 pb^-1 were analyzed, with a measured inclusive cross section of 62.3 +- 1.5 (stat) +- 2.4 (syst) +- 1.2 (lumi) pb, consistent with standard model (SM) predictions. The tW measurement was performed using data from 2022 with an integrated luminosity of 34.7 fb^-1 at a CM energy of 13.6 TeV, yielding a cross section of 82.3 +- 2.1 (stat) +9.9,-9.7 (syst) +- 3.3 (lumi) pb, in agreement with SM predictions. It includes also differential cross sections which are in good agreement with next-to-leading order in perturbative quantum chromodynamics. </p> </div> </dd> <dt> <a name='item11'>[11]</a> <a href ="/abs/2411.19781" title="Abstract" id="2411.19781"> arXiv:2411.19781 </a> [<a href="/pdf/2411.19781" title="Download PDF" id="pdf-2411.19781" aria-labelledby="pdf-2411.19781">pdf</a>, <a href="/format/2411.19781" title="Other formats" id="oth-2411.19781" aria-labelledby="oth-2411.19781">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Observation of the open-charm tetraquark state $T_{cs 0}^{*}(2870)^0$ in the $B^- \rightarrow D^- D^0 K_\mathrm{S}^0$ decay </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=LHCb+collaboration">LHCb collaboration</a>: <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aaij,+R">R. Aaij</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Abdelmotteleb,+A">A.S.W. Abdelmotteleb</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Beteta,+C+A">C. Abellan Beteta</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Abudin%C3%A9n,+F">F. Abudin茅n</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ackernley,+T">T. Ackernley</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adefisoye,+A+A">A. A. Adefisoye</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adeva,+B">B. Adeva</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adinolfi,+M">M. Adinolfi</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=Agapopoulou,+C">C. Agapopoulou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aidala,+C">C.A. Aidala</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ajaltouni,+Z">Z. Ajaltouni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Akar,+S">S. Akar</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Akiba,+K">K. Akiba</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Albicocco,+P">P. Albicocco</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Albrecht,+J">J. Albrecht</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Alessio,+F">F. Alessio</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Alexander,+M">M. Alexander</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aliouche,+Z">Z. Aliouche</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cartelle,+P+A">P. Alvarez Cartelle</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Amalric,+R">R. Amalric</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Amato,+S">S. Amato</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Amey,+J">J.L. Amey</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Amhis,+Y">Y. Amhis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=An,+L">L. An</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Anderlini,+L">L. Anderlini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andersson,+M">M. Andersson</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andreianov,+A">A. Andreianov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andreola,+P">P. Andreola</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andreotti,+M">M. Andreotti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andreou,+D">D. Andreou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Anelli,+A">A. Anelli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ao,+D">D. Ao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Archilli,+F">F. Archilli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Argenton,+M">M. Argenton</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cuendis,+S+A">S. Arguedas Cuendis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Artamonov,+A">A. Artamonov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Artuso,+M">M. Artuso</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aslanides,+E">E. Aslanides</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Da+Silva,+R+A">R. Ata铆de Da Silva</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Atzeni,+M">M. Atzeni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Audurier,+B">B. Audurier</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bacher,+D">D. Bacher</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Perea,+I+B">I. Bachiller Perea</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bachmann,+S">S. Bachmann</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bachmayer,+M">M. Bachmayer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Back,+J">J.J. Back</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Rodriguez,+P+B">P. Baladron Rodriguez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Balagura,+V">V. Balagura</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Balboni,+A">A. Balboni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Baldini,+W">W. Baldini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Balzani,+L">L. Balzani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bao,+H">H. Bao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=de+Souza+Leite,+J+B">J. Baptista de Souza Leite</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pretel,+C+B">C. Barbero Pretel</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barbetti,+M">M. Barbetti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barbosa,+I+R">I. R. Barbosa</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barlow,+R">R.J. Barlow</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barnyakov,+M">M. Barnyakov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barsuk,+S">S. Barsuk</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barter,+W">W. Barter</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bartolini,+M">M. Bartolini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bartz,+J">J. Bartz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Basels,+J">J.M. Basels</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bashir,+S">S. Bashir</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bassi,+G">G. Bassi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Batsukh,+B">B. Batsukh</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Battista,+P+B">P. B. Battista</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bay,+A">A. Bay</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Beck,+A">A. Beck</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Becker,+M">M. Becker</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bedeschi,+F">F. Bedeschi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bediaga,+I">I.B. Bediaga</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Behling,+N+A">N. A. Behling</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Belin,+S">S. Belin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Belous,+K">K. Belous</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Belov,+I">I. Belov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Belyaev,+I">I. Belyaev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Benane,+G">G. Benane</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bencivenni,+G">G. Bencivenni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ben-Haim,+E">E. Ben-Haim</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Berezhnoy,+A">A. Berezhnoy</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bernet,+R">R. Bernet</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Andres,+S+B">S. Bernet Andres</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertolin,+A">A. Bertolin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Betancourt,+C">C. Betancourt</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Betti,+F">F. Betti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bex,+J">J. Bex</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bezshyiko,+I">Ia. Bezshyiko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bhom,+J">J. Bhom</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bieker,+M">M.S. Bieker</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Biesuz,+N">N.V. Biesuz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Billoir,+P">P. Billoir</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Biolchini,+A">A. Biolchini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Birch,+M">M. Birch</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bishop,+F">F.C.R. Bishop</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bitadze,+A">A. Bitadze</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bizzeti,+A">A. Bizzeti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Blake,+T">T. Blake</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> All figures and tables, along with machine-readable versions and any supplementary material and information, are available at <a href="https://lbfence.cern.ch/alcm/public/analysis/full-details/3162/" rel="external noopener nofollow" class="link-external link-https">this https URL</a> (LHCb public pages) </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'> An amplitude analysis of $B^-\rightarrow D^- D^0 K_\mathrm{S}^0$ decays is performed using proton-proton collision data, corresponding to an integrated luminosity of $9\,\text{fb}^{-1}$, collected with the LHCb detector at center-of-mass energies of 7, 8, and 13$\mathrm{\,Te\kern -0.1em V}$. A resonant structure of spin-parity $0^+$ is observed in the $D^0 K_\mathrm{S}^0$ invariant-mass spectrum with a significance of $5.3\,\sigma$. The mass and width of the state, modeled with a Breit$-$Wigner lineshape, are determined to be $2883\pm11\pm6\mathrm{\,Me\kern -0.1em V\!/}c^2$ and $87_{-47}^{+22}\pm6\mathrm{\,Me\kern -0.1em V}$ respectively, where the first uncertainties are statistical and the second systematic. These properties and the quark content are consistent with those of the open-charm tetraquark state $T_{cs 0}^{*}(2870)^0$ observed previously in the $D^+ K^-$ final state of the $B^-\rightarrow D^- D^+ K^-$ decay. This result confirms the existence of the $T_{cs 0}^{*}(2870)^0$ state in a new decay mode. The $T_{cs1}^{*}(2900)^0$ state, reported in the $B^-\rightarrow D^- D^+ K^-$ decay, is also searched for in the $D^0 K_\mathrm{S}^0$ invariant-mass spectrum of the $B^- \rightarrow D^- D^0 K_\mathrm{S}^0$ decay, without finding evidence for it. </p> </div> </dd> </dl> <dl id='articles'> <h3>Cross submissions (showing 10 of 10 entries)</h3> <dt> <a name='item12'>[12]</a> <a href ="/abs/2411.18812" title="Abstract" id="2411.18812"> arXiv:2411.18812 </a> (cross-list from nucl-ex) [<a href="/pdf/2411.18812" title="Download PDF" id="pdf-2411.18812" aria-labelledby="pdf-2411.18812">pdf</a>, <a href="https://arxiv.org/html/2411.18812v1" title="View HTML" id="html-2411.18812" aria-labelledby="html-2411.18812" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18812" title="Other formats" id="oth-2411.18812" aria-labelledby="oth-2411.18812">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> New Limits on Coherent Neutrino Nucleus Elastic Scattering Cross Section at the Kuo-Sheng Reactor Neutrino Laboratory </div> <div class='list-authors'><a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=TEXONO+Collaboration">TEXONO Collaboration</a>: <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Karmakar,+S">S. Karmakar</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Singh,+M">M.K. Singh</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Sharma,+V">V. Sharma</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Wong,+H">H.T. Wong</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=C.,+G">Greeshma C.</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Li,+H">H.B. Li</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Singh,+L">L. Singh</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Agartioglu,+M">M. Agartioglu</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Chen,+J">J.H. Chen</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Chiang,+C">C.I. Chiang</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Deniz,+M">M. Deniz</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Hsu,+H">H.C. Hsu</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Karadag,+S">S. Karadag</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Kumar,+V">V. Kumar</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Leung,+C">C.H. Leung</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Li,+J">J. Li</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Lin,+F">F.K. Lin</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Lin,+S">S.T. Lin</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Liu,+S">S.K. Liu</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Ma,+H">H. Ma</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Saraswat,+K">K. Saraswat</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Singh,+M">M.K. Singh</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Singh,+V">V. Singh</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Tanabe,+D">D. Tanabe</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Wang,+J">J.S. Wang</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Yang,+L">L.T. Yang</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Yeh,+C">C.H. Yeh</a>, <a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=Yue,+Q">Q. Yue</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 6 pages, 4 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Nuclear Experiment (nucl-ex)</span>; High Energy Physics - Experiment (hep-ex); High Energy Physics - Phenomenology (hep-ph) </div> <p class='mathjax'> Neutrino nucleus elastic scattering ({\nu}Ael) with reactor neutrinos is an interaction under full quantum-mechanical coherence. It has not yet been experimentally observed. We present new results on the studies of {\nu}Ael cross section with an electro-cooled p-type point-contact germanium detector at the Kuo-Sheng Reactor Neutrino laboratory. A total of (242)357 kg-days of Reactor ON(OFF) data at a detector threshold of 200 eVee in electron equivalent unit are analyzed. The Lindhard model parametrized by a single variable k which characterizes the quenching function was used. Limits at 90% confidence level are derived on the ratio {\rho} relative to standard model (SM) cross section of {\rho}<4.7 at the predicted value of k=0.162, while k<0.285 at the SM-value of {\rho}=1. Prospects on future positive measurements are discussed. </p> </div> </dd> <dt> <a name='item13'>[13]</a> <a href ="/abs/2411.18914" title="Abstract" id="2411.18914"> arXiv:2411.18914 </a> (cross-list from astro-ph.CO) [<a href="/pdf/2411.18914" title="Download PDF" id="pdf-2411.18914" aria-labelledby="pdf-2411.18914">pdf</a>, <a href="https://arxiv.org/html/2411.18914v1" title="View HTML" id="html-2411.18914" aria-labelledby="html-2411.18914" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18914" title="Other formats" id="oth-2411.18914" aria-labelledby="oth-2411.18914">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Toward a practical haloscope for the post-inflation axion incorporating a photonic band gap structure </div> <div class='list-authors'><a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Goulart,+D">D. Goulart</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Sindhwad,+A">A.M. Sindhwad</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Jackson,+H">H.M. Jackson</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Kowitt,+N">N.I. Kowitt</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Dones,+K">K.A. Dones</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Basurto,+P+C">P. Casta帽o Basurto</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Dawes,+A">A. Dawes</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Lewis,+S">S.M. Lewis</a>, <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=van+Bibber,+K">K. van Bibber</a></div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Cosmology and Nongalactic Astrophysics (astro-ph.CO)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> Current and future searches for dark matter axions, based on their resonant conversion to photons in a magnetic field, span many orders of magnitude, from the very low mass GUT-scale axion to the very high mass post-inflation axion. The higher end of this range, 10 GHz and above is challenging for conventional microwave cavity-based experiments, owing to the steep drop-off in volume and thus conversion power with frequency. We present results on a first step towards a tunable microwave resonator that can be made suitably large and sufficiently high in frequency to begin probing the lower end of the post-inflation axion mass range. The design incorporates a tunable symmetric lattice and a photonic band gap structure that confines the TM$_{010}$ mode to which the axion couples, while suppressing all TE modes to which the axion does not. </p> </div> </dd> <dt> <a name='item14'>[14]</a> <a href ="/abs/2411.18927" title="Abstract" id="2411.18927"> arXiv:2411.18927 </a> (cross-list from physics.ins-det) [<a href="/pdf/2411.18927" title="Download PDF" id="pdf-2411.18927" aria-labelledby="pdf-2411.18927">pdf</a>, <a href="https://arxiv.org/html/2411.18927v1" title="View HTML" id="html-2411.18927" aria-labelledby="html-2411.18927" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18927" title="Other formats" id="oth-2411.18927" aria-labelledby="oth-2411.18927">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Beamtest of a Large Dynamic Range SiPM Readout ASIC MPT2321-B </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Qi,+B">Baohua Qi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Liu,+Y">Yong Liu</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Shi,+H">Huangchao Shi</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wang,+D">Danqi Wang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Zhao,+Z">Zhiyu Zhao</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Zhu,+H">Hongbo Zhu</a></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'> A front-end readout system with a large dynamic range is required for the high-granularity crystal ECAL at future Higgs factories. A new commercially available ASIC, MPT2321-B, which offers a significantly large dynamic range for the readout of the SiPM, has undergone initial tests both in the laboratory and at a beamtest facility. The fundamental performance metrics, including response linearity and single photon sensitivity, have been characterised. To quantitatively assess the dynamic range of the chip and evaluate its feasibility for SiPM readout in high-granularity crystal ECAL, a beamtest was conducted using scintillating crystals exposed to electron beams. Observations confirmed that the chip exhibits a signal-to-noise ratio sufficient for the operation of the detector and a satisfactory dynamic range, indicating significant potential for future applications. </p> </div> </dd> <dt> <a name='item15'>[15]</a> <a href ="/abs/2411.18962" title="Abstract" id="2411.18962"> arXiv:2411.18962 </a> (cross-list from hep-ph) [<a href="/pdf/2411.18962" title="Download PDF" id="pdf-2411.18962" aria-labelledby="pdf-2411.18962">pdf</a>, <a href="https://arxiv.org/html/2411.18962v1" title="View HTML" id="html-2411.18962" aria-labelledby="html-2411.18962" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18962" title="Other formats" id="oth-2411.18962" aria-labelledby="oth-2411.18962">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Simulating toponium formation signals at the LHC </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Fuks,+B">Benjamin Fuks</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hagiwara,+K">Kaoru Hagiwara</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ma,+K">Kai Ma</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Zheng,+Y">Ya-Juan Zheng</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 16 pages, 7 figures, related code available from <a href="https://github.com/BFuks/toponium" 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 - Phenomenology (hep-ph)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> We present a method to simulate toponium formation events at the LHC using the Green's function of non-relativistic QCD in the Coulomb gauge, which governs the momentum distribution of top quarks in the presence of the QCD potential. This Green's function can be employed to re-weight any matrix elements relevant for $t\bar{t}$ production and decay processes where a colour-singlet top-antitop pair is produced in the $S$-wave at threshold. As an example, we study the formation of $\eta_t$ toponium states in the gluon fusion channel at the LHC, combining the re-weighted matrix elements with parton showering. </p> </div> </dd> <dt> <a name='item16'>[16]</a> <a href ="/abs/2411.18988" title="Abstract" id="2411.18988"> arXiv:2411.18988 </a> (cross-list from astro-ph.IM) [<a href="/pdf/2411.18988" title="Download PDF" id="pdf-2411.18988" aria-labelledby="pdf-2411.18988">pdf</a>, <a href="https://arxiv.org/html/2411.18988v1" title="View HTML" id="html-2411.18988" aria-labelledby="html-2411.18988" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.18988" title="Other formats" id="oth-2411.18988" aria-labelledby="oth-2411.18988">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Ground electron calibration of the Gamma-ray Transient Monitor onboard DRO-A Satellite </div> <div class='list-authors'><a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Feng,+P">Pei-Yi Feng</a> (1, 2), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=An,+Z">Zheng-Hua An</a> (1), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Li,+Y">Yu-Hui Li</a> (3), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Le,+Q">Qi Le</a> (3), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Zhang,+D">Da-Li Zhang</a> (1), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Li,+X">Xin-Qiao Li</a> (1), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Xiong,+S">Shao-Lin Xiong</a> (1), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Liu,+C">Cong-Zhan Liu</a> (1), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Liu,+W">Wei-Bin Liu</a> (3), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Wang,+J">Jian-Li Wang</a> (3), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Deng,+B">Bing-Lin Deng</a> (3), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Xu,+H">He Xu</a> (4), <a href="https://arxiv.org/search/astro-ph?searchtype=author&query=Lu,+H">Hong Lu</a> (1) ((1) Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China, (2) University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, China, (3) Key Laboratory of Particle Acceleration Physics and Technology, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China, (4) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China)</div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 14 pages, 16 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Instrumentation and Methods for Astrophysics (astro-ph.IM)</span>; High Energy Physics - Experiment (hep-ex); Accelerator Physics (physics.acc-ph); Instrumentation and Detectors (physics.ins-det) </div> <p class='mathjax'> The Gamma-Ray Transient Monitor (GTM) is an all-sky monitor onboard the Distant Retrograde Orbit-A (DRO-A) satellite, with the scientific objective of detecting gamma-ray bursts in the energy range of 20 keV to 1 MeV. The GTM is equipped with five Gamma-Ray Transient Probes (GTPs), utilizing silicon photomultiplier (SiPM) arrays coupled with NaI(Tl) scintillators for signal readout. To test the performance of the GTP in detecting electrons, we independently developed a continuous-energy-tunable, low-current, quasi-single-electron accelerator, and used this facility for ground-based electron calibration of the GTP. This paper provides a detailed description of the operational principles of the unique electron accelerator and comprehensively presents the process and results of electron calibration for the GTP. The calibration results indicate that the dead time for normal signals is less than 4 $\mu$s, while for overflow signals, it is approximately 70 $\mu$s, consistent with the design specifications. The GTP's time-recording capability is working correctly, accurately recording overflow events. The GTP responds normally to electrons in the 0.4-1.4 MeV energy range. The ground-based electron calibration validates the design of the GTP and enhances the probe's mass model, laying the foundation for payload development, in-orbit observation strategies, and scientific data analysis. </p> </div> </dd> <dt> <a name='item17'>[17]</a> <a href ="/abs/2411.19170" title="Abstract" id="2411.19170"> arXiv:2411.19170 </a> (cross-list from hep-ph) [<a href="/pdf/2411.19170" title="Download PDF" id="pdf-2411.19170" aria-labelledby="pdf-2411.19170">pdf</a>, <a href="https://arxiv.org/html/2411.19170v1" title="View HTML" id="html-2411.19170" aria-labelledby="html-2411.19170" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19170" title="Other formats" id="oth-2411.19170" aria-labelledby="oth-2411.19170">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Prospects for detecting the rare heavy Higgs decay $H\to h\gamma\gamma$ at the LHC </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Arroyo-Ure%C3%B1a,+M+A">M. A. Arroyo-Ure帽a</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ibarra,+A">Alejandro Ibarra</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Roig,+P">Pablo Roig</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Valencia-P%C3%A9rez,+T">T. Valencia-P茅rez</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 23 pages, 5 figures, 4 tables and 3 appendices </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 study the decay of a heavy CP-even neutral Higgs into an on-shell Standard Model-like Higgs boson and two photons, $H\to h\gamma\gamma$, in the two-Higgs doublet model. We argue that the decay channel $H\to h\gamma\gamma$, followed by the decay of the Standard Model Higgs $h\rightarrow b\bar b$, could be observed at the 5$\sigma$ level at the High-Luminosity LHC for masses of the heavy Higgs up to 900 GeV for the type-II, 500 GeV for the Lepton Specific and the Flipped 2HDMs, and at 3 sigmas for the type-I, for masses up to 600 GeV. We also discuss the possible role of the decay $H\to h\gamma\gamma$ in discriminating among 2HDMs. </p> </div> </dd> <dt> <a name='item18'>[18]</a> <a href ="/abs/2411.19327" title="Abstract" id="2411.19327"> arXiv:2411.19327 </a> (cross-list from hep-ph) [<a href="/pdf/2411.19327" title="Download PDF" id="pdf-2411.19327" aria-labelledby="pdf-2411.19327">pdf</a>, <a href="https://arxiv.org/html/2411.19327v1" title="View HTML" id="html-2411.19327" aria-labelledby="html-2411.19327" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19327" title="Other formats" id="oth-2411.19327" aria-labelledby="oth-2411.19327">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Axion-induced pair production: a new strategy for axion detection </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Arias-Arag%C3%B3n,+F">Fernando Arias-Arag贸n</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Giannotti,+M">Maurizio Giannotti</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=di+Cortona,+G+G">Giovanni Grilli di Cortona</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Mescia,+F">Federico Mescia</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 13 pages, 6 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 revisit and update the axion-induced pair production process in a nuclear electric field mediated by the axion-electron coupling, $a+{{}^{A}_{Z}X} \rightarrow {{}^{A}_{Z}X} + e^{+} + e^{-}$. This process emerges as one of the most efficient channels for detecting axions with energies above a few MeV in large underground detectors. It is particularly relevant for detecting axions produced in nuclear reactions, such as the $p+d~\rightarrow~{ }^3 \mathrm{He}~+~a(5.5\,\mathrm{MeV})$ reaction in the solar pp-chain, and for axions originating in supernovae. Despite recent interest in detecting high-energy axions, the pair production process has received limited attention, even in scenarios where it is the dominant detection channel. This study fills this gap by demonstrating that pair production is a highly effective detection mechanism for high-energy axions. We apply our results to axions from supernovae and the solar 5.5 MeV line, recasting the current bounds of Borexino and comparing the detection capabilities of the JUNO and Hyper-Kamiokande detectors. </p> </div> </dd> <dt> <a name='item19'>[19]</a> <a href ="/abs/2411.19424" title="Abstract" id="2411.19424"> arXiv:2411.19424 </a> (cross-list from physics.atom-ph) [<a href="/pdf/2411.19424" title="Download PDF" id="pdf-2411.19424" aria-labelledby="pdf-2411.19424">pdf</a>, <a href="https://arxiv.org/html/2411.19424v1" title="View HTML" id="html-2411.19424" aria-labelledby="html-2411.19424" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19424" title="Other formats" id="oth-2411.19424" aria-labelledby="oth-2411.19424">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Nuclear and Particle Physics through Quantum Sensing Using Cold Atoms and Molecules </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Kawasaki,+A">Akio Kawasaki</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 29 pages, 10 figures </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Atomic Physics (physics.atom-ph)</span>; High Energy Physics - Experiment (hep-ex); Nuclear Experiment (nucl-ex) </div> <p class='mathjax'> As techniques for manipulating single atoms and molecules developed, quantum technologies witnessed drastic advancements. These technologies are now so mature that they can be applied to various fields. One of such fields is nuclear and particle physics, which were conventionally investigated with high energy accelerators. In general, quantum sensing enables high-precision measurements, opening ways to investigate high-energy phenomena that slightly modify energy levels of low-energy systems by higher-order perturbations. In other cases, such high-precision measurements are sensitive to faint low-energy interactions between the low-energy system and exotic fields. These measurements open new parameter spaces to explore in conventionally investigated topics, e.g., variations of fundamental constants, dark matter, fifth force, parity violation, CP-violation, supersymmetric theories, and other physics beyond the Standard Model. Additionally, such measurements can serve as confirmations for existing results from completely different systems, or surpass existing results using smaller-scale experiments. The field of atomic and molecular physics oriented to nuclear and particle physics motivations evolved significantly. This paper provides an overview of the field of nuclear and particle physics through high-precision quantum measurements using atoms and molecules. </p> </div> </dd> <dt> <a name='item20'>[20]</a> <a href ="/abs/2411.19836" title="Abstract" id="2411.19836"> arXiv:2411.19836 </a> (cross-list from hep-ph) [<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/2411.19836v1" 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> 6 pages, 2 figures. Comments are welcome! </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> <dt> <a name='item21'>[21]</a> <a href ="/abs/2411.19872" title="Abstract" id="2411.19872"> arXiv:2411.19872 </a> (cross-list from physics.atom-ph) [<a href="/pdf/2411.19872" title="Download PDF" id="pdf-2411.19872" aria-labelledby="pdf-2411.19872">pdf</a>, <a href="https://arxiv.org/html/2411.19872v1" title="View HTML" id="html-2411.19872" aria-labelledby="html-2411.19872" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.19872" title="Other formats" id="oth-2411.19872" aria-labelledby="oth-2411.19872">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Two-Photon Optical Ramsey-Doppler Spectroscopy of Positronium and Muonium </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Javary,+E">Evans Javary</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Thorpe-Woods,+E">Edward Thorpe-Woods</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Cortinovis,+I">Irene Cortinovis</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=M%C3%A4hring,+M">Marcus M盲hring</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=de+Sousa+Borges,+L">Lucas de Sousa Borges</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Crivelli,+P">Paolo Crivelli</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 15 pages, 9 figures, 2 tables prepared for the topical issue in EPJD of the PSAS 2024 conference </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Atomic Physics (physics.atom-ph)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> Positronium and muonium, as purely leptonic atoms without internal structure, provide ideal systems for high-precision tests of quantum electrodynamics (QED) and measurements of fundamental constants. However, the high velocities of these lightweight atoms complicate precision spectroscopy, particularly in the 1S-2S transition, due to transit time broadening and second-order Doppler shifts. To overcome these challenges, we propose a novel method combining two-photon Ramsey spectroscopy with a technique to correct the second-order Doppler shifts on an atom-by-atom basis. Additionally, this approach suppresses systematic effects of the AC Stark shift to a negligible level compared to the target precision. Simulations predict that for both positronium and muonium, this method could improve the measurement precision of the 1S-2S transition by more than two orders of magnitude compared to the current state of the art. This approach opens up new avenues for rigorous bound-state QED tests and searches for physics beyond the Standard Model. </p> </div> </dd> </dl> <dl id='articles'> <h3>Replacement submissions (showing 14 of 14 entries)</h3> <dt> <a name='item22'>[22]</a> <a href ="/abs/2306.00641" title="Abstract" id="2306.00641"> arXiv:2306.00641 </a> (replaced) [<a href="/pdf/2306.00641" title="Download PDF" id="pdf-2306.00641" aria-labelledby="pdf-2306.00641">pdf</a>, <a href="/format/2306.00641" title="Other formats" id="oth-2306.00641" aria-labelledby="oth-2306.00641">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Combination and summary of ATLAS dark matter searches interpreted in a 2HDM with a pseudo-scalar mediator using 139 fb$^{-1}$ of $\sqrt{s} = 13$ TeV $pp$ collision data </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> 63 pages in total, author list starting page 46, 9 figures, 4 tables, published in Science Bulletin. All figures including auxiliary figures are available at <a href="http://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/EXOT-2018-64" rel="external noopener nofollow" class="link-external link-http">this http URL</a> </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Science Bulletin 69 (2024) 3005 </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'> Results from a wide range of searches targeting different experimental signatures with and without missing transverse momentum ($E_{\mathrm{T}}^{\mathrm{miss}}$) are used to constrain a Two-Higgs-Doublet Model (2HDM) with an additional pseudo-scalar mediating the interaction between ordinary and dark matter (2HDM+$a$). The analyses use up to 139 fb$^{-1}$ of proton-proton collision data at a centre-of-mass energy $\sqrt{s}=13$ TeV recorded with the ATLAS detector at the Large Hadron Collider during 2015-2018. The results from three of the most sensitive searches are combined statistically. These searches target signatures with large $E_{\mathrm{T}}^{\mathrm{miss}}$ and a leptonically decaying $Z$ boson; large $E_{\mathrm{T}}^{\mathrm{miss}}$ and a Higgs boson decaying to bottom quarks; and production of charged Higgs bosons in final states with top and bottom quarks, respectively. Constraints are derived for several common and new benchmark scenarios in the 2HDM+$a$. </p> </div> </dd> <dt> <a name='item23'>[23]</a> <a href ="/abs/2405.07386" title="Abstract" id="2405.07386"> arXiv:2405.07386 </a> (replaced) [<a href="/pdf/2405.07386" title="Download PDF" id="pdf-2405.07386" aria-labelledby="pdf-2405.07386">pdf</a>, <a href="https://arxiv.org/html/2405.07386v2" title="View HTML" id="html-2405.07386" aria-labelledby="html-2405.07386" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2405.07386" title="Other formats" id="oth-2405.07386" aria-labelledby="oth-2405.07386">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Search for lepton-flavor-violating $\tau^- \to \mu^-\mu^+\mu^-$ decays at Belle II </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Belle+II+Collaboration">Belle II Collaboration</a>: <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Adachi,+I">I. Adachi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aggarwal,+L">L. Aggarwal</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aihara,+H">H. Aihara</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Akopov,+N">N. Akopov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aloisio,+A">A. Aloisio</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Althubiti,+N">N. Althubiti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ky,+N+A">N. Anh Ky</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Asner,+D+M">D. M. Asner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Atmacan,+H">H. Atmacan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aushev,+V">V. Aushev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Aversano,+M">M. Aversano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ayad,+R">R. Ayad</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Babu,+V">V. Babu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bae,+H">H. Bae</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bahinipati,+S">S. Bahinipati</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bambade,+P">P. Bambade</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Banerjee,+S">Sw. Banerjee</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bansal,+S">S. Bansal</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Barrett,+M">M. Barrett</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Baudot,+J">J. Baudot</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Baur,+A">A. Baur</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Beaubien,+A">A. Beaubien</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Becherer,+F">F. Becherer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Becker,+J">J. Becker</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bennett,+J+V">J. V. Bennett</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bernlochner,+F+U">F. U. Bernlochner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertacchi,+V">V. Bertacchi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertemes,+M">M. Bertemes</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bertholet,+E">E. Bertholet</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bessner,+M">M. Bessner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bettarini,+S">S. Bettarini</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=Bierwirth,+L">L. Bierwirth</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bilka,+T">T. Bilka</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Biswas,+D">D. Biswas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bobrov,+A">A. Bobrov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bodrov,+D">D. Bodrov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bolz,+A">A. Bolz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Borah,+J">J. Borah</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Boschetti,+A">A. Boschetti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bozek,+A">A. Bozek</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bra%C4%8Dko,+M">M. Bra膷ko</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Branchini,+P">P. Branchini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Browder,+T+E">T. E. Browder</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Budano,+A">A. Budano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Bussino,+S">S. Bussino</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Campagna,+Q">Q. Campagna</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Campajola,+M">M. Campajola</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cao,+L">L. Cao</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Casarosa,+G">G. Casarosa</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cecchi,+C">C. Cecchi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cerasoli,+J">J. Cerasoli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chang,+M">M.-C. Chang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chang,+P">P. Chang</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cheaib,+R">R. Cheaib</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cheema,+P">P. Cheema</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=Cheon,+B+G">B. G. Cheon</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chilikin,+K">K. Chilikin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chirapatpimol,+K">K. Chirapatpimol</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cho,+H">H.-E. Cho</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cho,+K">K. Cho</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cho,+S">S.-J. Cho</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choi,+S">S.-K. Choi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Choudhury,+S">S. Choudhury</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cochran,+J">J. Cochran</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Corona,+L">L. Corona</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cui,+J+X">J. X. Cui</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Das,+S">S. Das</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dattola,+F">F. Dattola</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+La+Cruz-Burelo,+E">E. De La Cruz-Burelo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+La+Motte,+S+A">S. A. De La Motte</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Nardo,+G">G. De Nardo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Nuccio,+M">M. De Nuccio</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=De+Pietro,+G">G. De Pietro</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=de+Sangro,+R">R. de Sangro</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=Dey,+S">S. Dey</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dhamija,+R">R. Dhamija</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Di+Canto,+A">A. Di Canto</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Di+Capua,+F">F. Di Capua</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dingfelder,+J">J. Dingfelder</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dole%C5%BEal,+Z">Z. Dole啪al</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Jim%C3%A9nez,+I+D">I. Dom铆nguez Jim茅nez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dong,+T+V">T. V. Dong</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dorigo,+M">M. Dorigo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dorner,+D">D. Dorner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dort,+K">K. Dort</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dossett,+D">D. Dossett</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dreyer,+S">S. Dreyer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dubey,+S">S. Dubey</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dugic,+K">K. Dugic</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dujany,+G">G. Dujany</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ecker,+P">P. Ecker</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Eliachevitch,+M">M. Eliachevitch</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Feichtinger,+P">P. Feichtinger</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ferber,+T">T. Ferber</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ferlewicz,+D">D. Ferlewicz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fillinger,+T">T. Fillinger</a></div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> J. High Energ. Phys. 2024, 62 (2024). </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'> We present the result of a search for the charged-lepton-flavor violating decay $\tau^- \to \mu^-\mu^+\mu^-$ using a $424fb^{-1}$ sample of data recorded by the Belle II experiment at the SuperKEKB $e^{-}e^{+}$ collider. The selection of $e^{-}e^{+}\to\tau^+\tau^-$ events is based on an inclusive reconstruction of the non-signal tau decay, and on a boosted decision tree to suppress background. We observe one signal candidate, which is compatible with the expectation from background processes. We set a $90\%$ confidence level upper limit of $1.9 \times 10^{-8}$ on the branching fraction of the \taumu decay, which is the most stringent bound to date. </p> </div> </dd> <dt> <a name='item24'>[24]</a> <a href ="/abs/2405.19862" title="Abstract" id="2405.19862"> arXiv:2405.19862 </a> (replaced) [<a href="/pdf/2405.19862" title="Download PDF" id="pdf-2405.19862" aria-labelledby="pdf-2405.19862">pdf</a>, <a href="/format/2405.19862" title="Other formats" id="oth-2405.19862" aria-labelledby="oth-2405.19862">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Search for pair-produced vector-like quarks coupling to light quarks in the lepton plus jets final state using 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> 41 pages in total, author list starting page 24, 6 figures, 4 tables, published in Phys. Rev. D 110 (2024) 052009. All figures including auxiliary figures are available at <a href="https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/EXOT-2021-35/" rel="external noopener nofollow" class="link-external link-https">this https URL</a> </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Phys. Rev. D 110 (2024) 052009 </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 presented for the pair-production of heavy vector-like quarks (VLQs) that each decay into a $W$ boson and a light quark. This study focuses on events where one $W$ boson decays into leptons and the other into hadrons. The search analyzed 140 fb$^{-1}$ of $pp$ collision data with $\sqrt{s} = 13$ TeV, recorded by the ATLAS detector from 2015 to 2018 during Run 2 of the Large Hadron Collider. The final state is characterized by a high-transverse-momentum isolated electron or muon, large missing transverse momentum, multiple small-radius jets, and a single large-radius jet identified as originating from the hadronic decay of a boosted $W$ boson. With higher center-of-mass energy and integrated luminosity than in the Run 1 search, and improved analysis tools, this analysis excludes VLQs ($Q$) with masses below 1530 GeV at 95% CL for the branching ratio ${{\cal B}(Q \to Wq)} = 1$, an improvement of 840 GeV on the previous ATLAS limit. </p> </div> </dd> <dt> <a name='item25'>[25]</a> <a href ="/abs/2411.13915" title="Abstract" id="2411.13915"> arXiv:2411.13915 </a> (replaced) [<a href="/pdf/2411.13915" title="Download PDF" id="pdf-2411.13915" aria-labelledby="pdf-2411.13915">pdf</a>, <a href="https://arxiv.org/html/2411.13915v2" title="View HTML" id="html-2411.13915" aria-labelledby="html-2411.13915" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2411.13915" title="Other formats" id="oth-2411.13915" aria-labelledby="oth-2411.13915">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> An accurate solar axions ray-tracing response of BabyIAXO </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ahyoune,+S">S. Ahyoune</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Altenmueller,+K">K. Altenmueller</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Antolin,+I">I. Antolin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Basso,+S">S. Basso</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Brun,+P">P. Brun</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Candon,+F+R">F. R. Candon</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Castel,+J+F">J. F. Castel</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cebrian,+S">S. Cebrian</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chouhan,+D">D. Chouhan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Della+Ceca,+R">R. Della Ceca</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cervera-Cortes,+M">M. Cervera-Cortes</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Chernov,+V">V. Chernov</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Civitani,+M+M">M. M. Civitani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cogollos,+C">C. Cogollos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Costa,+E">E. Costa</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Cotroneo,+V">V. Cotroneo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dafni,+T">T. Dafni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Derbin,+A">A. Derbin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Desch,+K">K. Desch</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Diaz-Martin,+M+C">M. C. Diaz-Martin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Diaz-Morcillo,+A">A. Diaz-Morcillo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Diez-Ibanez,+D">D. Diez-Ibanez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pardos,+C+D">C. Diez Pardos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dinter,+M">M. Dinter</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Doebrich,+B">B. Doebrich</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Drachnev,+I">I. Drachnev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Dudarev,+A">A. Dudarev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ezquerro,+A">A. Ezquerro</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fabiani,+S">S. Fabiani</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ferrer-Ribas,+E">E. Ferrer-Ribas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Finelli,+F">F. Finelli</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Fleck,+I">I. Fleck</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Galan,+J">J. Galan</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Galanti,+G">G. Galanti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Galaverni,+M">M. Galaverni</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Garcia,+J+A">J. A. Garcia</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Garcia-Barcelo,+J+M">J. M. Garcia-Barcelo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gastaldo,+L">L. Gastaldo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Giannotti,+M">M. Giannotti</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Giganon,+A">A. Giganon</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Goblin,+C">C. Goblin</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Goyal,+N">N. Goyal</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Gu,+Y">Y. Gu</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hagge,+L">L. Hagge</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Helary,+L">L. Helary</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hengstler,+D">D. Hengstler</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Heuchel,+D">D. Heuchel</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Hoof,+S">S. Hoof</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Iglesias-Marzoa,+R">R. Iglesias-Marzoa</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Iguaz,+F+J">F. J. Iguaz</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Iniguez,+C">C. Iniguez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Irastorza,+I+G">I. G. Irastorza</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Jakovcic,+K">K. Jakovcic</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kaefer,+D">D. Kaefer</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Kaminski,+J">J. Kaminski</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Karstensen,+S">S. Karstensen</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Law,+M">M. Law</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lindner,+A">A. Lindner</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Loidl,+M">M. Loidl</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Loiseau,+C">C. Loiseau</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lopez-Alegre,+G">G. Lopez-Alegre</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lozano-Guerrero,+A">A. Lozano-Guerrero</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Lubsandorzhiev,+B">B. Lubsandorzhiev</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Luzon,+G">G. Luzon</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Manthos,+I">I. Manthos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Margalejo,+C">C. Margalejo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Marin-Franch,+A">A. Marin-Franch</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Marques,+J">J. Marques</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Marutzky,+F">F. Marutzky</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Menneglier,+C">C. Menneglier</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Mentink,+M">M. Mentink</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Mertens,+S">S. Mertens</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Miralda-Escude,+J">J. Miralda-Escude</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Mirallas,+H">H. Mirallas</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Muleri,+F">F. Muleri</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Muratova,+V">V. Muratova</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Navarro-Madrid,+J+R">J. R. Navarro-Madrid</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Navick,+X+F">X. F. Navick</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Nikolopoulos,+K">K. Nikolopoulos</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Notari,+A">A. Notari</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Nozik,+A">A. Nozik</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Obis,+L">L. Obis</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ortiz-de-Solorzano,+A">A. Ortiz-de-Solorzano</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=O'Shea,+T">T. O'Shea</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=von+Oy,+J">J. von Oy</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pareschi,+G">G. Pareschi</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Papaevangelou,+T">T. Papaevangelou</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Perez,+K">K. Perez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Perez,+O">O. Perez</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Picatoste,+E">E. Picatoste</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Pivovaroff,+M+J">M. J. Pivovaroff</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Porron,+J">J. Porron</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Puyuelo,+M+J">M. J. Puyuelo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Quintana,+A">A. Quintana</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Redondo,+J">J. Redondo</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Reuther,+D">D. Reuther</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Ringwald,+A">A. Ringwald</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Rodrigues,+M">M. Rodrigues</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Rubini,+A">A. Rubini</a>, <a href="https://arxiv.org/search/hep-ex?searchtype=author&query=Rueda-Teruel,+S">S. Rueda-Teruel</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 36 pages, 18 figures, 4 tables, Submitted to JHEP </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Experiment (hep-ex)</span>; Instrumentation and Methods for Astrophysics (astro-ph.IM); Solar and Stellar Astrophysics (astro-ph.SR); Computational Physics (physics.comp-ph); Data Analysis, Statistics and Probability (physics.data-an) </div> <p class='mathjax'> BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. Its primary goal is the detection of solar axions following the axion helioscope technique. Axions are converted into photons in a large magnet that is pointing to the sun. The resulting X-rays are focused by appropriate X-ray optics and detected by sensitive low-background detectors placed at the focal spot. The aim of this article is to provide an accurate quantitative description of the different components (such as the magnet, optics, and X-ray detectors) involved in the detection of axions. Our efforts have focused on developing robust and integrated software tools to model these helioscope components, enabling future assessments of modifications or upgrades to any part of the IAXO axion helioscope and evaluating the potential impact on the experiment's sensitivity. In this manuscript, we demonstrate the application of these tools by presenting a precise signal calculation and response analysis of BabyIAXO's sensitivity to the axion-photon coupling. Though focusing on the Primakoff solar flux component, our virtual helioscope model can be used to test different production mechanisms, allowing for direct comparisons within a unified framework. </p> </div> </dd> <dt> <a name='item26'>[26]</a> <a href ="/abs/2203.08271" title="Abstract" id="2203.08271"> arXiv:2203.08271 </a> (replaced) [<a href="/pdf/2203.08271" title="Download PDF" id="pdf-2203.08271" aria-labelledby="pdf-2203.08271">pdf</a>, <a href="/format/2203.08271" title="Other formats" id="oth-2203.08271" aria-labelledby="oth-2203.08271">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> The strong coupling constant: State of the art and the decade ahead </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=d'Enterria,+D">D. d'Enterria</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kluth,+S">S. Kluth</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Zanderighi,+G">G. Zanderighi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ayala,+C">C. Ayala</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Benitez-Rathgeb,+M">M.A. Benitez-Rathgeb</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Bluemlein,+J">J. Bluemlein</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Boito,+D">D. Boito</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Brambilla,+N">N. Brambilla</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Britzger,+D">D. Britzger</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Camarda,+S">S. Camarda</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cooper-Sarkar,+A+M">A. M. Cooper-Sarkar</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cridge,+T">T. Cridge</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cvetic,+G">G. Cvetic</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Brida,+M+D">M. Dalla Brida</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Deur,+A">A. Deur</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Giuli,+F">F. Giuli</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Golterman,+M">M. Golterman</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hoang,+A">A.H. Hoang</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Huston,+J">J. Huston</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Jamin,+M">M. Jamin</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kotikov,+A+V">A. V. Kotikov</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Krivokhizhin,+V+G">V. G. Krivokhizhin</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kronfeld,+A">A.S. Kronfeld</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Leino,+V">V. Leino</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Lipka,+K">K. Lipka</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Makela,+T">T. Makela</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Malaescu,+B">B. Malaescu</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Maltman,+K">K. Maltman</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Marzani,+S">S. Marzani</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Mateu,+V">V. Mateu</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Moch,+S">S. Moch</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Monni,+P+F">P. F. Monni</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nadolsky,+P">P. Nadolsky</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nason,+P">P. Nason</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nesterenko,+A">A.V. Nesterenko</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Perez-Ramos,+R">R. Perez-Ramos</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Peris,+S">S. Peris</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Petreczky,+P">P. Petreczky</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Pich,+A">A. Pich</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Rabbertz,+K">K. Rabbertz</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ramos,+A">A. Ramos</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Reichelt,+D">D. Reichelt</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Rodriguez-Sanchez,+A">A. Rodriguez-Sanchez</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Rojo,+J">J. Rojo</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Saragnese,+M">M. Saragnese</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Sawyer,+L">L. Sawyer</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Schott,+M">M. Schott</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Schumann,+S">S. Schumann</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Shaikhatdenov,+B+G">B. G. Shaikhatdenov</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Sint,+S">S. Sint</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Soyez,+G">G. Soyez</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Teca,+D">D. Teca</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Vairo,+A">A. Vairo</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Vos,+M">M. Vos</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Waits,+C">C. Waits</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Weber,+J+H">J. H. Weber</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Wobisch,+M">M. Wobisch</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Xie,+K">K. Xie</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 135 pages, 45 figures. White paper for the "Energy Frontier Proceedings of the US Community Study on the Future of Particle Physics" (Snowmass 2021). Matches JPG published version </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> J.Phys.G 51 (2024) 9, 090501 </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 - Lattice (hep-lat) </div> <p class='mathjax'> Theoretical predictions for particle production cross sections and decays at colliders rely heavily on perturbative Quantum Chromodynamics (QCD) calculations, expressed as an expansion in powers of the strong coupling constant $\alpha_s$. The current $\mathcal{O}(1\%)$ uncertainty of the QCD coupling evaluated at the reference Z boson mass, $\alpha_s(m_Z) = 0.1179 \pm 0.0009$, is one of the limiting factors to more precisely describe multiple processes at current and future colliders. A reduction of this uncertainty is thus a prerequisite to perform precision tests of the Standard Model as well as searches for new physics. This report provides a comprehensive summary of the state-of-the-art, challenges, and prospects in the experimental and theoretical study of the strong coupling. The current $\alpha_s(m_Z)$ world average is derived from a combination of seven categories of observables: (i) lattice QCD, (ii) hadronic $\tau$ decays, (iii) deep-inelastic scattering and parton distribution functions fits, (iv) electroweak boson decays, hadronic final-states in (v) $e^+e^-$, (vi) e-p, and (vii) p-p collisions, and (viii) quarkonia decays and masses. We review the current status of each of these seven $\alpha_s(m_Z)$ extraction methods, discuss novel $\alpha_s$ determinations, and examine the averaging method used to obtain the world-average value. Each of the methods discussed provides a ``wish list'' of experimental and theoretical developments required in order to achieve the goal of a per-mille precision on $\alpha_s(m_Z)$ within the next decade. </p> </div> </dd> <dt> <a name='item27'>[27]</a> <a href ="/abs/2302.14676" title="Abstract" id="2302.14676"> arXiv:2302.14676 </a> (replaced) [<a href="/pdf/2302.14676" title="Download PDF" id="pdf-2302.14676" aria-labelledby="pdf-2302.14676">pdf</a>, <a href="https://arxiv.org/html/2302.14676v4" title="View HTML" id="html-2302.14676" aria-labelledby="html-2302.14676" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2302.14676" title="Other formats" id="oth-2302.14676" aria-labelledby="oth-2302.14676">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Zero Casimir Force in Axion Electrodynamics and the Search for a New Force </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ema,+Y">Yohei Ema</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hazumi,+M">Masashi Hazumi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Iizuka,+H">Hideo Iizuka</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Mukaida,+K">Kyohei Mukaida</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nakayama,+K">Kazunori Nakayama</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 29 pages, 9 figures; to appear in PRD; typos fixed </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">High Energy Physics - Phenomenology (hep-ph)</span>; Mesoscale and Nanoscale Physics (cond-mat.mes-hall); High Energy Physics - Experiment (hep-ex); Quantum Physics (quant-ph) </div> <p class='mathjax'> We point out that there is a stable configuration of metal plates where the Casimir force is vanishing in axion electrodynamics. We consider a concrete setup involving Weyl semimetals, which hosts an axion-like effect on the electromagnetism, towards the measurement of the axionic effect on the Casimir force. Our setup realizes zero Casimir force between metals and may be useful for the search for new force mediated by light particles at the micrometer scale. </p> </div> </dd> <dt> <a name='item28'>[28]</a> <a href ="/abs/2404.19123" title="Abstract" id="2404.19123"> arXiv:2404.19123 </a> (replaced) [<a href="/pdf/2404.19123" title="Download PDF" id="pdf-2404.19123" aria-labelledby="pdf-2404.19123">pdf</a>, <a href="https://arxiv.org/html/2404.19123v3" title="View HTML" id="html-2404.19123" aria-labelledby="html-2404.19123" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2404.19123" title="Other formats" id="oth-2404.19123" aria-labelledby="oth-2404.19123">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> CP Violation Problem </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Popov,+N">Nicolai Popov</a> (LMU), <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Briscoe,+W+J">William J. Briscoe</a> (GWU), <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Strakovsky,+I">Igor Strakovsky</a> (GWU)</div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 25 pages, 5 figures; we have revised the paper accordingly: 35 pages and 8 figures now </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); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th) </div> <p class='mathjax'> The strong CP violation problem has a long history emanating from its discovery 60 years ago in the decay of neutral kaons and subsequent experimental and theoretical studies over several decades. We review herein experimental data that observe indirect CP violation of the order of $\sim10^{-3}$, as well as the discovery of direct CP violation of the order of $\sim10^{-6}$. Despite improved experimental methods over the past half a century, the original CP violation numbers have remained the same. Verification of the CP violation in the decay of charged kaons was also observed. Data reflecting CP violation in the decays of $B$ and $D$ mesons have become very important and are also discussed in this review. The question of CP violation only with the participation of $s\bar{s}$, $c\bar{c}$, and $b\bar{b}$ quarks in the framework of the Standard Model or beyond it and its small magnitude remains open. </p> </div> </dd> <dt> <a name='item29'>[29]</a> <a href ="/abs/2405.05078" title="Abstract" id="2405.05078"> arXiv:2405.05078 </a> (replaced) [<a href="/pdf/2405.05078" title="Download PDF" id="pdf-2405.05078" aria-labelledby="pdf-2405.05078">pdf</a>, <a href="/format/2405.05078" title="Other formats" id="oth-2405.05078" aria-labelledby="oth-2405.05078">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Observation of $t\bar{t}$ production in the lepton+jets and dilepton channels in $p$+Pb collisions at $\sqrt{s_\mathrm{NN}}=8.16$ TeV with the ATLAS detector </div> <div class='list-authors'><a href="https://arxiv.org/search/nucl-ex?searchtype=author&query=ATLAS+Collaboration">ATLAS Collaboration</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 37 pages in total, author list starting page 20, 3 figures, 1 table, published in JHEP 11 (2024) 101. All figures including auxiliary figures are available at <a href="https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/TOPQ-2023-32/" rel="external noopener nofollow" class="link-external link-https">this https URL</a> </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> JHEP 11 (2024) 101 </div> <div class='list-subjects'><span class='descriptor'>Subjects:</span> <span class="primary-subject">Nuclear Experiment (nucl-ex)</span>; High Energy Physics - Experiment (hep-ex) </div> <p class='mathjax'> This paper reports the observation of top-quark pair production in proton-lead collisions in the ATLAS experiment at the Large Hadron Collider. The measurement is performed using 165 nb$^{-1}$ of $p$+Pb data collected at $\sqrt{s_\mathrm{NN}}=8.16$ TeV in 2016. Events are categorised in two analysis channels, consisting of either events with exactly one lepton (electron or muon) and at least four jets, or events with two opposite-charge leptons and at least two jets. In both channels at least one $b$-tagged jet is also required. Top-quark pair production is observed with a significance over five standard deviations in each channel. The top-quark pair production cross-section is measured to be $\sigma_{t\bar{t}}= 58.1\pm 2.0\;\mathrm{(stat.)\;^{+4.8}_{-4.4} \;\mathrm{(syst.)}}\;\mathrm{nb}$, with a total uncertainty of 9%. In addition, the nuclear modification factor is measured to be $R_{p\mathrm{A}} = 1.090\pm0.039\;(\mathrm{stat.})\;^{+0.094}_{-0.087}\;(\mathrm{syst.})$. The measurements are found to be in good agreement with theory predictions involving nuclear parton distribution functions. </p> </div> </dd> <dt> <a name='item30'>[30]</a> <a href ="/abs/2405.18720" title="Abstract" id="2405.18720"> arXiv:2405.18720 </a> (replaced) [<a href="/pdf/2405.18720" title="Download PDF" id="pdf-2405.18720" aria-labelledby="pdf-2405.18720">pdf</a>, <a href="https://arxiv.org/html/2405.18720v3" title="View HTML" id="html-2405.18720" aria-labelledby="html-2405.18720" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2405.18720" title="Other formats" id="oth-2405.18720" aria-labelledby="oth-2405.18720">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Machine-Learning based photon counting for PMT waveforms and its application to the improvement of the energy resolution in large liquid scintillator detectors </div> <div class='list-authors'><a href="https://arxiv.org/search/physics?searchtype=author&query=Jiang,+W">Wei Jiang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Huang,+G">Guihong Huang</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Liu,+Z">Zhen Liu</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Luo,+W">Wuming Luo</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Wen,+L">Liangjian Wen</a>, <a href="https://arxiv.org/search/physics?searchtype=author&query=Luo,+J">Jianyi Luo</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 10 pages, 9 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'> Photomultiplier tubes (PMTs) are widely used in particle experiments for photon detection. PMT waveform analysis is crucial for high-precision measurements of the position and energy of incident particles in liquid scintillator (LS) detectors. A key factor contributing to the energy resolution in large liquid scintillator detectors with PMTs is the charge smearing of PMTs. This paper presents a machine-learning-based photon counting method for PMT waveforms and its application to the energy reconstruction, using the JUNO experiment as an example. The results indicate that leveraging the photon counting information from the machine learning model can partially mitigate the impact of PMT charge smearing and lead to a relative 2.0% to 2.8% improvement on the energy resolution in the energy range of [1, 9] MeV. </p> </div> </dd> <dt> <a name='item31'>[31]</a> <a href ="/abs/2405.19419" title="Abstract" id="2405.19419"> arXiv:2405.19419 </a> (replaced) [<a href="/pdf/2405.19419" title="Download PDF" id="pdf-2405.19419" aria-labelledby="pdf-2405.19419">pdf</a>, <a href="https://arxiv.org/html/2405.19419v2" title="View HTML" id="html-2405.19419" aria-labelledby="html-2405.19419" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2405.19419" title="Other formats" id="oth-2405.19419" aria-labelledby="oth-2405.19419">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Supernova electron-neutrino interactions with xenon in the nEXO detector </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=nEXO+Collaboration">nEXO Collaboration</a>: <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hedges,+S">S. Hedges</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kharusi,+S+A">S. Al Kharusi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Angelico,+E">E. Angelico</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Brodsky,+J+P">J. P. Brodsky</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Richardson,+G">G. Richardson</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Wilde,+S">S. Wilde</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Amy,+A">A. Amy</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Anker,+A">A. Anker</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Arnquist,+I+J">I. J. Arnquist</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Arsenault,+P">P. Arsenault</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Atencio,+A">A. Atencio</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Badhrees,+I">I. Badhrees</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Bane,+J">J. Bane</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Belov,+V">V. Belov</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Bernard,+E+P">E. P. Bernard</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Bhatta,+T">T. Bhatta</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Bolotnikov,+A">A. Bolotnikov</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Breslin,+J">J. Breslin</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Breur,+P+A">P. A. Breur</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Brown,+E">E. Brown</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Brunner,+T">T. Brunner</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Caden,+E">E. Caden</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cao,+G+F">G. F. Cao</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cao,+L+Q">L. Q. Cao</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cesmecioglu,+D">D. Cesmecioglu</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Chambers,+E">E. Chambers</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Chana,+B">B. Chana</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Charlebois,+S+A">S. A. Charlebois</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Chernyak,+D">D. Chernyak</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Chiu,+M">M. Chiu</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Collister,+R">R. Collister</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Cvitan,+M">M. Cvitan</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Dalmasson,+J">J. Dalmasson</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Daniels,+T">T. Daniels</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Darroch,+L">L. Darroch</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=DeVoe,+R">R. DeVoe</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=di+Vacri,+M+L">M. L. di Vacri</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ding,+Y+Y">Y. Y. Ding</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Dolinski,+M+J">M. J. Dolinski</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Eckert,+B">B. Eckert</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Elbeltagi,+M">M. Elbeltagi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Elmansali,+R">R. Elmansali</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Fabris,+L">L. Fabris</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Fairbank,+W">W. Fairbank</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Farine,+J">J. Farine</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Fatemighomi,+N">N. Fatemighomi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Foust,+B">B. Foust</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Fu,+Y+S">Y. S. Fu</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gallacher,+D">D. Gallacher</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gallice,+N">N. Gallice</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gillis,+W">W. Gillis</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Goeldi,+D">D. Goeldi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gorham,+A">A. Gorham</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gornea,+R">R. Gornea</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gratta,+G">G. Gratta</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Guan,+Y+D">Y. D. Guan</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hardy,+C+A">C. A. Hardy</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Heffner,+M">M. Heffner</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hein,+E">E. Hein</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Holt,+J+D">J. D. Holt</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hoppe,+E+W">E. W. Hoppe</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=House,+A">A. House</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Hunt,+W">W. Hunt</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Iverson,+A">A. Iverson</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kachru,+P">P. Kachru</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Karelin,+A">A. Karelin</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Keblbeck,+D">D. Keblbeck</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kuchenkov,+A">A. Kuchenkov</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Kumar,+K+S">K. S. Kumar</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Larson,+A">A. Larson</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Latif,+M+B">M. B. Latif</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Leach,+K+G">K. G. Leach</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Lenardo,+B+G">B. G. Lenardo</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Leonard,+D+S">D. S. Leonard</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Lewis,+H">H. Lewis</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Li,+G">G. Li</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Li,+Z">Z. Li</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Licciardi,+C">C. Licciardi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Lindsay,+R">R. Lindsay</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=MacLellan,+R">R. MacLellan</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Majidi,+S">S. Majidi</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Malbrunot,+C">C. Malbrunot</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Martel-Dion,+P">P. Martel-Dion</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Masbou,+J">J. Masbou</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=McMichael,+K">K. McMichael</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Medina-Peregrina,+M">M. Medina-Peregrina</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Mong,+B">B. Mong</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Moore,+D+C">D. C. Moore</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nattress,+J">J. Nattress</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Natzke,+C+R">C. R. Natzke</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ngwadla,+X+E">X. E. Ngwadla</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ni,+K">K. Ni</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nolan,+A">A. Nolan</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Nowicki,+S+C">S. C. Nowicki</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ondze,+J+C+N">J. C. Nzobadila Ondze</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Orrell,+J+L">J. L. Orrell</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Ortega,+G+S">G. S. Ortega</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Overman,+C+T">C. T. Overman</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Pagani,+L">L. Pagani</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 17 pages, 16 figures </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Phys. Rev. D 110, 093002 (2024) </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); Nuclear Theory (nucl-th) </div> <p class='mathjax'> Electron-neutrino charged-current interactions with xenon nuclei were modeled in the nEXO neutrinoless double-$\beta$ decay detector (~5 metric ton, 90% ${}^{136}$Xe, 10% ${}^{134}$Xe) to evaluate its sensitivity to supernova neutrinos. Predictions for event rates and detectable signatures were modeled using the Model of Argon Reaction Low Energy Yields (MARLEY) event generator. We find good agreement between MARLEY's predictions and existing theoretical calculations of the inclusive cross sections at supernova neutrino energies. The interactions modeled by MARLEY were simulated within the nEXO simulation framework and were run through an example reconstruction algorithm to determine the detector's efficiency for reconstructing these events. The simulated data, incorporating the detector response, were used to study the ability of nEXO to reconstruct the incident electron-neutrino spectrum and these results were extended to a larger xenon detector of the same isotope enrichment. We estimate that nEXO will be able to observe electron-neutrino interactions with xenon from supernovae as far as 5-8 kpc from Earth, while the ability to reconstruct incident electron-neutrino spectrum parameters from observed interactions in nEXO is limited to closer supernovae. </p> </div> </dd> <dt> <a name='item32'>[32]</a> <a href ="/abs/2407.15065" title="Abstract" id="2407.15065"> arXiv:2407.15065 </a> (replaced) [<a href="/pdf/2407.15065" title="Download PDF" id="pdf-2407.15065" aria-labelledby="pdf-2407.15065">pdf</a>, <a href="https://arxiv.org/html/2407.15065v2" title="View HTML" id="html-2407.15065" aria-labelledby="html-2407.15065" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2407.15065" title="Other formats" id="oth-2407.15065" aria-labelledby="oth-2407.15065">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Anisotropic flow fluctuation as a possible signature of clustered nuclear geometry in O-O collisions at the Large Hadron Collider </div> <div class='list-authors'><a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Prasad,+S">Suraj Prasad</a>, <a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Mallick,+N">Neelkamal Mallick</a>, <a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Sahoo,+R">Raghunath Sahoo</a>, <a href="https://arxiv.org/search/nucl-th?searchtype=author&query=Barnaf%C3%B6ldi,+G+G">Gergely G谩bor Barnaf枚ldi</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 15 pages and 12 captioned figures, Same as the published version in Phys. Letts. B </div> <div class='list-journal-ref'><span class='descriptor'>Journal-ref:</span> Phys. Lett. B 860 (2025) 139145 </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'> Nuclei having $4n$ number of nucleons are theorized to possess clusters of $\alpha$ particles ($^4$He nucleus). The Oxygen nucleus ($^{16}$O) is a doubly magic nucleus, where the presence of an $\alpha$-clustered nuclear structure grants additional nuclear stability. In this study, we exploit the anisotropic flow coefficients to discern the effects of an $\alpha$-clustered nuclear geometry with respect to a Woods-Saxon nuclear distribution in O--O collisions at $\sqrt{s_{\rm NN}}=7$ TeV using a hybrid of IP-Glasma + MUSIC + iSS + UrQMD models. In addition, we use the multi-particle cumulants method to measure anisotropic flow coefficients, such as elliptic flow ($v_{2}$) and triangular flow ($v_{3}$), as a function of multiplicity class. Anisotropic flow fluctuations, which are expected to be larger in small collision systems, are also studied for the first time in O--O collisions. It is found that an $\alpha$-clustered nuclear distribution gives rise to an enhanced value of $v_{2}$ and $v_3$ for the low-multiplicity events. Consequently, a rise in $v_3/v_2$ is also observed for the 0--10\% multiplicity class. Further, for $\alpha$-clustered O--O collisions, fluctuations of $v_{2}$ are larger for the highest multiplicity events, which decrease as the final-state multiplicity decreases. In contrast, for a Woods-Saxon $^{16}$O nucleus, $v_{2}$ fluctuations show an opposite behavior with decreasing multiplicity. When confronted with experimental data, this study may reveal the importance of the nuclear density profile on the discussed observables and provide physics validation for the hybrid model discussed in this work. </p> </div> </dd> <dt> <a name='item33'>[33]</a> <a href ="/abs/2409.10503" title="Abstract" id="2409.10503"> arXiv:2409.10503 </a> (replaced) [<a href="/pdf/2409.10503" title="Download PDF" id="pdf-2409.10503" aria-labelledby="pdf-2409.10503">pdf</a>, <a href="https://arxiv.org/html/2409.10503v2" title="View HTML" id="html-2409.10503" aria-labelledby="html-2409.10503" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2409.10503" title="Other formats" id="oth-2409.10503" aria-labelledby="oth-2409.10503">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Improved $\pi^0,\eta,\eta^{\prime}$ transition form factors in resonance chiral theory and their $a_\mu^{\rm{HLbL}}$ contribution </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Estrada,+E+J">Emilio J. Estrada</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Gonz%C3%A0lez-Sol%C3%ADs,+S">Sergi Gonz脿lez-Sol铆s</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Guevara,+A">Adolfo Guevara</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Roig,+P">Pablo Roig</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 49 pages, 8 figures. The correlations between the pseudo-data points from Lattice QCD were considered and the Global Analysis was changed accordingly in this version. Furthermore, the high energy behavior was analyzed in the whole spectrum of asymmetries between the single virtual and the double virtual case </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 - Lattice (hep-lat) </div> <p class='mathjax'> Working with Resonance Chiral Theory, within the two resonance multiplets saturation scheme, we satisfy leading (and some subleading) chiral and asymptotic QCD constraints and accurately fit simultaneously the $\pi^{0},\eta,\eta^{\prime}$ transition form factors, for single and double virtuality. In the latter case, we supplement the few available measurements with lattice data to ensure a faithful description. Mainly due to the new results for the doubly virtual case, we improve over existing descriptions for the $\eta$ and $\eta^\prime$. Our evaluation of the corresponding pole contributions to the hadronic light-by-light piece of the muon $g-2$ read: $a_\mu^{\pi^{0}\text{-}\rm{pole}}=\left(61.9\pm0.6^{+2.4}_{-1.5}\right)\times10^{-11}$, $a_\mu^{\eta\text{-}\rm{pole}}=\left(15.2\pm0.5^{+1.1}_{-0.8}\right)\times10^{-11}$ and $a_\mu^{\eta^\prime\text{-}\rm{pole}}=\left(14.2\pm0.7^{+1.4}_{-0.9}\right)\times10^{-11}$, for a total of $a_\mu^{\pi^0+\eta+\eta^{\prime}\text{-}\rm{pole}}=\left(91.3\pm1.0^{+3.0}_{-1.9}\right)\times10^{-11}$, where the first and second errors are the statistical and systematic uncertainties, respectively. </p> </div> </dd> <dt> <a name='item34'>[34]</a> <a href ="/abs/2409.12070" title="Abstract" id="2409.12070"> arXiv:2409.12070 </a> (replaced) [<a href="/pdf/2409.12070" title="Download PDF" id="pdf-2409.12070" aria-labelledby="pdf-2409.12070">pdf</a>, <a href="https://arxiv.org/html/2409.12070v2" title="View HTML" id="html-2409.12070" aria-labelledby="html-2409.12070" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2409.12070" title="Other formats" id="oth-2409.12070" aria-labelledby="oth-2409.12070">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Fully charmed tetraquark production at the LHC experiments </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Belov,+I">Ilia Belov</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Giachino,+A">Alessandro Giachino</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Santopinto,+E">Elena Santopinto</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> Accepted by JHEP. 19 pages, 5 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 develop the formalism for production of a fully heavy tetraquark and apply it to the calculation of $pp\to T_{4c}+X$ cross-sections. We demonstrate that the production cross-section of a fully heavy tetraquark, even if it is a diquark-antidiquark cluster, can be obtained in the meson-like basis, for which the spin-color projection technique is well established. Prompted by the recent LHCb, ATLAS and CMS data, we perform a pQCD calculation of ${\cal O}(\alpha_s^5)$ short-distance factors in the dominant channel of gluon fusion, and match these to the four-body $T_{4c}$ wave functions in order to obtain the unpolarized $T_{4c}(0^{++},1^{+-},2^{++})$ cross-sections. The novelty in comparison with the recently published article~\cite{Feng:2023agq} lies in the fact that we predict the absolute values as well as the $d\sigma/dp_T$ spectra in the kinematic ranges accessible at the ongoing LHC experiments. From the comparison with the signal yield at LHCb we derive the constraints on the $\Phi\cdot\text{Br}(J/\psi\,J/\psi)$ (reduced wave function times branching) product for the $T_{4c}$ candidates for $X(6900)$ and observe that $X(6900)$ is compatible with a $2^{++}(2S)$ state. </p> </div> </dd> <dt> <a name='item35'>[35]</a> <a href ="/abs/2410.15339" title="Abstract" id="2410.15339"> arXiv:2410.15339 </a> (replaced) [<a href="/pdf/2410.15339" title="Download PDF" id="pdf-2410.15339" aria-labelledby="pdf-2410.15339">pdf</a>, <a href="https://arxiv.org/html/2410.15339v2" title="View HTML" id="html-2410.15339" aria-labelledby="html-2410.15339" rel="noopener noreferrer" target="_blank">html</a>, <a href="/format/2410.15339" title="Other formats" id="oth-2410.15339" aria-labelledby="oth-2410.15339">other</a>] </dt> <dd> <div class='meta'> <div class='list-title mathjax'><span class='descriptor'>Title:</span> Spectroscopic Properties of Double-Strangeness Molecular Tetraquarks </div> <div class='list-authors'><a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Wang,+F">Fu-Lai Wang</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Luo,+S">Si-Qiang Luo</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Qian,+R">Ri-Qing Qian</a>, <a href="https://arxiv.org/search/hep-ph?searchtype=author&query=Liu,+X">Xiang Liu</a></div> <div class='list-comments mathjax'><span class='descriptor'>Comments:</span> 16 pages, 4 figures, and 5 tables. Accepted by Physical Review D </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 - Lattice (hep-lat) </div> <p class='mathjax'> Inspired by recent advances in the study of the $K^{(*)} \bar K^{(*)}$ molecular tetraquarks and the $H$-dibaryon, we focus on the spectroscopic properties of the $\bar K^{(*)} \bar K^{(*)}$ systems, which exhibit exotic flavor quantum number of $ss\bar q \bar q$. A dynamical analysis is performed using the one-boson-exchange model to describe the effective interactions for these systems, accounting for both $S$-$D$ wave mixing and coupled-channel effects. By solving the coupled-channel Schr$\ddot{\rm o}$dinger equation, we identify the $I(J^P)=0(1^+)$ $\bar K \bar K^*$ and $I(J^P)=0(1^+)$ $\bar K^* \bar K^*$ states as the most likely candidates for double-strangeness molecular tetraquarks. Furthermore, we estimate their strong decay behaviors based on the effective Lagrangian approach, with several channels exhibiting considerable decay widths. Meanwhile, we investigate their magnetic moments and M1 radiative decay widths, shedding light on their inner structures, within the constituent quark model. Finally, we encourage experimentalists to focus on these predicted double-strangeness molecular tetraquark candidates, particularly in $B$ meson decays. Such efforts could pave the way for establishing the molecular tetraquark states in the light-quark sector. </p> </div> </dd> </dl> <div class='paging'>Total of 35 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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