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is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> Supernova Pointing Capabilities of DUNE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=DUNE+Collaboration"> DUNE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Abud%2C+A+A">A. Abed Abud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Abi%2C+B">B. Abi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adames%2C+M+R">M. R. Adames</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adamov%2C+G">G. Adamov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D">D. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adinolfi%2C+M">M. Adinolfi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adriano%2C+C">C. Adriano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aduszkiewicz%2C+A">A. Aduszkiewicz</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aguilar%2C+J">J. Aguilar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aimard%2C+B">B. Aimard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Akbar%2C+F">F. Akbar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Allison%2C+K">K. Allison</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Monsalve%2C+S+A">S. Alonso Monsalve</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alrashed%2C+M">M. Alrashed</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alton%2C+A">A. Alton</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alvarez%2C+R">R. Alvarez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alves%2C+T">T. Alves</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amar%2C+H">H. Amar</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Amedo%2C+P">P. Amedo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andrade%2C+D+A">D. A. Andrade</a> , et al. (1340 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2407.10339v1-abstract-short" style="display: inline;"> The determination of the direction of a stellar core collapse via its neutrino emission is crucial for the identification of the progenitor for a multimessenger follow-up. A highly effective method of reconstructing supernova directions within the Deep Underground Neutrino Experiment (DUNE) is introduced. The supernova neutrino pointing resolution is studied by simulating and reconstructing electr&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2407.10339v1-abstract-full').style.display = 'inline'; document.getElementById('2407.10339v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2407.10339v1-abstract-full" style="display: none;"> The determination of the direction of a stellar core collapse via its neutrino emission is crucial for the identification of the progenitor for a multimessenger follow-up. A highly effective method of reconstructing supernova directions within the Deep Underground Neutrino Experiment (DUNE) is introduced. The supernova neutrino pointing resolution is studied by simulating and reconstructing electron-neutrino charged-current absorption on $^{40}$Ar and elastic scattering of neutrinos on electrons. Procedures to reconstruct individual interactions, including a newly developed technique called ``brems flipping&#39;&#39;, as well as the burst direction from an ensemble of interactions are described. Performance of the burst direction reconstruction is evaluated for supernovae happening at a distance of 10 kpc for a specific supernova burst flux model. The pointing resolution is found to be 3.4 degrees at 68% coverage for a perfect interaction-channel classification and a fiducial mass of 40 kton, and 6.6 degrees for a 10 kton fiducial mass respectively. Assuming a 4% rate of charged-current interactions being misidentified as elastic scattering, DUNE&#39;s burst pointing resolution is found to be 4.3 degrees (8.7 degrees) at 68% coverage. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2407.10339v1-abstract-full').style.display = 'none'; document.getElementById('2407.10339v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 July, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">25 pages, 16 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-PUB-24-0319-LBNF </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2310.06082">arXiv:2310.06082</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2310.06082">pdf</a>, <a href="https://arxiv.org/format/2310.06082">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Measurement of nuclear effects in neutrino-argon interactions using generalized kinematic imbalance variables with the MicroBooNE detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=MicroBooNE+collaboration"> MicroBooNE collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Abratenko%2C+P">P. Abratenko</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alterkait%2C+O">O. Alterkait</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aldana%2C+D+A">D. Andrade Aldana</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Arellano%2C+L">L. Arellano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Asaadi%2C+J">J. Asaadi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ashkenazi%2C+A">A. Ashkenazi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balasubramanian%2C+S">S. Balasubramanian</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baller%2C+B">B. Baller</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barr%2C+G">G. Barr</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barrow%2C+D">D. Barrow</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barrow%2C+J">J. Barrow</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Basque%2C+V">V. Basque</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rodrigues%2C+O+B">O. Benevides Rodrigues</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berkman%2C+S">S. Berkman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bhanderi%2C+A">A. Bhanderi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bhat%2C+A">A. Bhat</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bhattacharya%2C+M">M. Bhattacharya</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bishai%2C+M">M. Bishai</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Blake%2C+A">A. Blake</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bogart%2C+B">B. Bogart</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bolton%2C+T">T. Bolton</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Book%2C+J+Y">J. Y. Book</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brunetti%2C+M+B">M. B. Brunetti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+L">L. Camilleri</a> , et al. (163 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2310.06082v4-abstract-short" style="display: inline;"> We present a set of new generalized kinematic imbalance variables that can be measured in neutrino scattering. These variables extend previous measurements of kinematic imbalance on the transverse plane, and are more sensitive to modeling of nuclear effects. We demonstrate the enhanced power of these variables using simulation, and then use the MicroBooNE detector to measure them for the first tim&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2310.06082v4-abstract-full').style.display = 'inline'; document.getElementById('2310.06082v4-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2310.06082v4-abstract-full" style="display: none;"> We present a set of new generalized kinematic imbalance variables that can be measured in neutrino scattering. These variables extend previous measurements of kinematic imbalance on the transverse plane, and are more sensitive to modeling of nuclear effects. We demonstrate the enhanced power of these variables using simulation, and then use the MicroBooNE detector to measure them for the first time. We report flux-integrated single- and double-differential measurements of charged-current muon neutrino scattering on argon using a topolgy with one muon and one proton in the final state as a function of these novel kinematic imbalance variables. These measurements allow us to demonstrate that the treatment of charged current quasielastic interactions in GENIE version 2 is inadequate to describe data. Further, they reveal tensions with more modern generator predictions particularly in regions of phase space where final state interactions are important. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2310.06082v4-abstract-full').style.display = 'none'; document.getElementById('2310.06082v4-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 May, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 9 October, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 109, 092007 (2024) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2008.06647">arXiv:2008.06647</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2008.06647">pdf</a>, <a href="https://arxiv.org/format/2008.06647">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Solar and Stellar Astrophysics">astro-ph.SR</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-021-09166-w">10.1140/epjc/s10052-021-09166-w <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=DUNE+collaboration"> DUNE collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Abi%2C+B">B. Abi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adamov%2C+G">G. Adamov</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D">D. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adinolfi%2C+M">M. Adinolfi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ahmed%2C+J">J. Ahmed</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Monsalve%2C+S+A">S. Alonso Monsalve</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alt%2C+C">C. Alt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andrews%2C+M+P">M. P. Andrews</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andrianala%2C+F">F. Andrianala</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andringa%2C+S">S. Andringa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Antonova%2C+M">M. Antonova</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Antusch%2C+S">S. Antusch</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Aranda-Fernandez%2C+A">A. Aranda-Fernandez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ariga%2C+A">A. Ariga</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Arnold%2C+L+O">L. O. Arnold</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Arroyave%2C+M+A">M. A. Arroyave</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Asaadi%2C+J">J. Asaadi</a> , et al. (949 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2008.06647v3-abstract-short" style="display: inline;"> The Deep Underground Neutrino Experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The gen&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2008.06647v3-abstract-full').style.display = 'inline'; document.getElementById('2008.06647v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2008.06647v3-abstract-full" style="display: none;"> The Deep Underground Neutrino Experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE&#39;s ability to constrain the $谓_e$ spectral parameters of the neutrino burst will be considered. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2008.06647v3-abstract-full').style.display = 'none'; document.getElementById('2008.06647v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 August, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">29 pages, 17 figures; paper based on DUNE Technical Design Report. arXiv admin note: substantial text overlap with arXiv:2002.03005</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-PUB-20-380-LBNF </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <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 class="nav-spaced"> <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 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