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data-tooltip="High Energy Physics - Experiment">hep-ex</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/10.1088/1748-0221/15/07/P07001">10.1088/1748-0221/15/07/P07001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Study of space charge in the ICARUS T600 detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bellini%2C+V">V. Bellini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bonesini%2C+M">M. Bonesini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bubak%2C+A">A. Bubak</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">K. Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dabrowska%2C+A">A. Dabrowska</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Falcone%2C+A">A. Falcone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gninenko%2C+S">S. Gninenko</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guglielmi%2C+A">A. Guglielmi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Haranczyk%2C+M">M. Haranczyk</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Holeczek%2C+J">J. Holeczek</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Kirsanov%2C+M">M. Kirsanov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Kisiel%2C+J">J. Kisiel</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Kochanek%2C+I">I. Kochanek</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Lagoda%2C+J">J. Lagoda</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Menegolli%2C+A">A. Menegolli</a> , et al. (23 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="2001.08934v3-abstract-short" style="display: inline;"> The accumulation of positive ions, produced by ionizing particles crossing Liquid Argon Time Projection Chambers (LAr-TPCs), may generate distortions of the electric drift field affecting the track reconstruction of the ionizing events. These effects could become relevant for large LAr-TPCs operating at surface or at shallow depth, where the detectors are exposed to a copious flux of cosmic rays.&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2001.08934v3-abstract-full').style.display = 'inline'; document.getElementById('2001.08934v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2001.08934v3-abstract-full" style="display: none;"> The accumulation of positive ions, produced by ionizing particles crossing Liquid Argon Time Projection Chambers (LAr-TPCs), may generate distortions of the electric drift field affecting the track reconstruction of the ionizing events. These effects could become relevant for large LAr-TPCs operating at surface or at shallow depth, where the detectors are exposed to a copious flux of cosmic rays. A detailed study of such possible field distortions in the ICARUS T600 LAr-TPC has been performed analyzing a sample of cosmic muon tracks recorded with one T600 module operated at surface in 2001. The maximum track distortion turns out to be of few mm in good agreement with the prediction by a numerical calculation. As a cross-check, the same analysis has been performed on a cosmic muon sample recorded during the ICARUS T600 run at the LNGS underground laboratory, where the cosmic ray flux was suppressed by a factor $\sim 10^6$ by 3400 m water equivalent shielding. No appreciable distortion has been observed, confirming that the effects measured on surface are actually due to ion space charge. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2001.08934v3-abstract-full').style.display = 'none'; document.getElementById('2001.08934v3-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> 28 May, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 January, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">16 pages, 11 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1807.10340">arXiv:1807.10340</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1807.10340">pdf</a>, <a href="https://arxiv.org/format/1807.10340">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> The DUNE Far Detector Interim Design Report, Volume 3: Dual-Phase Module </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=DUNE+Collaboration"> DUNE Collaboration</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Abi%2C+B">B. Abi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+D">D. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adinolfi%2C+M">M. Adinolfi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Soplin%2C+L+A">L. Aliaga Soplin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Monsalve%2C+S+A">S. Alonso Monsalve</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alrashed%2C+M">M. Alrashed</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alt%2C+C">C. Alt</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M+P">M. P. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R+A">R. A. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anthony%2C+J">J. Anthony</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonova%2C+M">M. Antonova</a> , et al. (1076 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="1807.10340v1-abstract-short" style="display: inline;"> The DUNE IDR describes the proposed physics program and technical designs of the DUNE far detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.10340v1-abstract-full').style.display = 'inline'; document.getElementById('1807.10340v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.10340v1-abstract-full" style="display: none;"> The DUNE IDR describes the proposed physics program and technical designs of the DUNE far detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 3 describes the dual-phase module&#39;s subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.10340v1-abstract-full').style.display = 'none'; document.getElementById('1807.10340v1-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> 26 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </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">280 pages, 109 figures. arXiv admin note: text overlap with arXiv:1807.10327</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Fermilab-Design-2018-04 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1807.10334">arXiv:1807.10334</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1807.10334">pdf</a>, <a href="https://arxiv.org/format/1807.10334">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> The DUNE Far Detector Interim Design Report Volume 1: Physics, Technology and Strategies </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=DUNE+Collaboration"> DUNE Collaboration</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Abi%2C+B">B. Abi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+D">D. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adinolfi%2C+M">M. Adinolfi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Soplin%2C+L+A">L. Aliaga Soplin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Monsalve%2C+S+A">S. Alonso Monsalve</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alrashed%2C+M">M. Alrashed</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alt%2C+C">C. Alt</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M+P">M. P. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R+A">R. A. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anthony%2C+J">J. Anthony</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonova%2C+M">M. Antonova</a> , et al. (1076 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="1807.10334v1-abstract-short" style="display: inline;"> The DUNE IDR describes the proposed physics program and technical designs of the DUNE Far Detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.10334v1-abstract-full').style.display = 'inline'; document.getElementById('1807.10334v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.10334v1-abstract-full" style="display: none;"> The DUNE IDR describes the proposed physics program and technical designs of the DUNE Far Detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 1 contains an executive summary that describes the general aims of this document. The remainder of this first volume provides a more detailed description of the DUNE physics program that drives the choice of detector technologies. It also includes concise outlines of two overarching systems that have not yet evolved to consortium structures: computing and calibration. Volumes 2 and 3 of this IDR describe, for the single-phase and dual-phase technologies, respectively, each detector module&#39;s subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.10334v1-abstract-full').style.display = 'none'; document.getElementById('1807.10334v1-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> 26 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </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">83 pages, 11 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Fermilab-Design-2018-02 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1807.10327">arXiv:1807.10327</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1807.10327">pdf</a>, <a href="https://arxiv.org/format/1807.10327">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> The DUNE Far Detector Interim Design Report, Volume 2: Single-Phase Module </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=DUNE+Collaboration"> DUNE Collaboration</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Abi%2C+B">B. Abi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+D">D. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adinolfi%2C+M">M. Adinolfi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Soplin%2C+L+A">L. Aliaga Soplin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Monsalve%2C+S+A">S. Alonso Monsalve</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alrashed%2C+M">M. Alrashed</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alt%2C+C">C. Alt</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M+P">M. P. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R+A">R. A. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anthony%2C+J">J. Anthony</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonova%2C+M">M. Antonova</a> , et al. (1076 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="1807.10327v1-abstract-short" style="display: inline;"> The DUNE IDR describes the proposed physics program and technical designs of the DUNE far detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.10327v1-abstract-full').style.display = 'inline'; document.getElementById('1807.10327v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.10327v1-abstract-full" style="display: none;"> The DUNE IDR describes the proposed physics program and technical designs of the DUNE far detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 2 describes the single-phase module&#39;s subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.10327v1-abstract-full').style.display = 'none'; document.getElementById('1807.10327v1-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> 26 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </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">324 pages, 130 figures. arXiv admin note: text overlap with arXiv:1807.10340</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> Fermilab-Design-2018-03 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1706.07081">arXiv:1706.07081</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1706.07081">pdf</a>, <a href="https://arxiv.org/format/1706.07081">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> The Single-Phase ProtoDUNE Technical Design Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Abi%2C+B">B. Abi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+D+L">D. L. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adinolfi%2C+M">M. Adinolfi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M+P">M. P. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R+A">R. A. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anjos%2C+J+d">J. dos Anjos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anthony%2C+J">J. Anthony</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fernandez%2C+A+A">A. Aranda Fernandez</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+A">A. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+T">T. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Diaz%2C+E+A">E. Arrieta Diaz</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Asaadi%2C+J">J. Asaadi</a> , et al. (806 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="1706.07081v2-abstract-short" style="display: inline;"> ProtoDUNE-SP is the single-phase DUNE Far Detector prototype that is under construction and will be operated at the CERN Neutrino Platform (NP) starting in 2018. ProtoDUNE-SP, a crucial part of the DUNE effort towards the construction of the first DUNE 10-kt fiducial mass far detector module (17 kt total LAr mass), is a significant experiment in its own right. With a total liquid argon (LAr) mass&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1706.07081v2-abstract-full').style.display = 'inline'; document.getElementById('1706.07081v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1706.07081v2-abstract-full" style="display: none;"> ProtoDUNE-SP is the single-phase DUNE Far Detector prototype that is under construction and will be operated at the CERN Neutrino Platform (NP) starting in 2018. ProtoDUNE-SP, a crucial part of the DUNE effort towards the construction of the first DUNE 10-kt fiducial mass far detector module (17 kt total LAr mass), is a significant experiment in its own right. With a total liquid argon (LAr) mass of 0.77 kt, it represents the largest monolithic single-phase LArTPC detector to be built to date. It&#39;s technical design is given in this report. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1706.07081v2-abstract-full').style.display = 'none'; document.getElementById('1706.07081v2-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> 27 July, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 June, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2017. </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">165 pages, fix references, author list and minor numbers</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1612.07715">arXiv:1612.07715</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1612.07715">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</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/10.1088/1748-0221/12/04/P04010">10.1088/1748-0221/12/04/P04010 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Muon momentum measurement in ICARUS-T600 LAr-TPC via multiple scattering in few-GeV range </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">Maddalena Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">Bagdat Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bellini%2C+V">Vincenzo Bellini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Benetti%2C+P+A">Pietro Angelo Benetti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">Fabrizio Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bubak%2C+A">Arkadiusz Bubak</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">Elio Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">Sandro Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cervi%2C+T">Tommaso Cervi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">Alessandra Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">Krzysztof Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">Alfredo G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dabrowska%2C+A">Anna Dabrowska</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">Alexander Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Falcone%2C+A">Andrea Falcone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">Christian Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">Angela Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">Alfredo Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">Daniele Gibin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gninenko%2C+S">Sergei Gninenko</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guglielmi%2C+A">Alberto Guglielmi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Haranczyk%2C+M">Malgorzata Haranczyk</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Holeczek%2C+J">Jacek Holeczek</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Janik%2C+M">Michal Janik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Kirsanov%2C+M">Mikhail Kirsanov</a> , et al. (32 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="1612.07715v2-abstract-short" style="display: inline;"> The measurement of muon momentum by Multiple Coulomb Scattering is a crucial ingredient to the reconstruction of 谓渭 CC events in the ICARUS-T600 liquid argon TPC in absence of magnetic field, as in the search for sterile neutrinos at Fermilab where ICARUS will be exposed to ~1 GeV Booster neutrino beam. A sample of ~1000 stopping muons produced by charged current interactions of CNGS 谓渭 in the sur&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.07715v2-abstract-full').style.display = 'inline'; document.getElementById('1612.07715v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1612.07715v2-abstract-full" style="display: none;"> The measurement of muon momentum by Multiple Coulomb Scattering is a crucial ingredient to the reconstruction of 谓渭 CC events in the ICARUS-T600 liquid argon TPC in absence of magnetic field, as in the search for sterile neutrinos at Fermilab where ICARUS will be exposed to ~1 GeV Booster neutrino beam. A sample of ~1000 stopping muons produced by charged current interactions of CNGS 谓渭 in the surrounding rock at the INFN Gran Sasso underground Laboratory provides an ideal benchmark in the few-GeV range since their momentum can be directly and independently obtained by the calorimetric measurement. Stopping muon momentum in the 0.5- 4.5 GeV/c range has been reconstructed via Multiple Coulomb Scattering with resolution ranging from 10 to 25 % depending on muon energy, track length and uniformity of the electric field in the drift volume. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1612.07715v2-abstract-full').style.display = 'none'; document.getElementById('1612.07715v2-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> 28 February, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 22 December, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2016. </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">20 pages, 20 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1601.05471">arXiv:1601.05471</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1601.05471">pdf</a>, <a href="https://arxiv.org/format/1601.05471">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 1: The LBNF and DUNE Projects </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adhikari%2C+S">S. Adhikari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Amador%2C+E">E. Amador</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M">M. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R">R. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anghel%2C+I">I. Anghel</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anjos%2C+J+d">J. d. Anjos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=ArandaFernandez%2C+A">A. ArandaFernandez</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+A">A. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+T">T. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Aristizabal%2C+D">D. Aristizabal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Arrieta-Diaz%2C+E">E. Arrieta-Diaz</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Aryal%2C+K">K. Aryal</a> , et al. (780 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="1601.05471v1-abstract-short" style="display: inline;"> This document presents the Conceptual Design Report (CDR) put forward by an international neutrino community to pursue the Deep Underground Neutrino Experiment at the Long-Baseline Neutrino Facility (LBNF/DUNE), a groundbreaking science experiment for long-baseline neutrino oscillation studies and for neutrino astrophysics and nucleon decay searches. The DUNE far detector will be a very large modu&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.05471v1-abstract-full').style.display = 'inline'; document.getElementById('1601.05471v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.05471v1-abstract-full" style="display: none;"> This document presents the Conceptual Design Report (CDR) put forward by an international neutrino community to pursue the Deep Underground Neutrino Experiment at the Long-Baseline Neutrino Facility (LBNF/DUNE), a groundbreaking science experiment for long-baseline neutrino oscillation studies and for neutrino astrophysics and nucleon decay searches. The DUNE far detector will be a very large modular liquid argon time-projection chamber (LArTPC) located deep underground, coupled to the LBNF multi-megawatt wide-band neutrino beam. DUNE will also have a high-resolution and high-precision near detector. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.05471v1-abstract-full').style.display = 'none'; document.getElementById('1601.05471v1-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> 20 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1601.02984">arXiv:1601.02984</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1601.02984">pdf</a>, <a href="https://arxiv.org/format/1601.02984">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNF </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adhikari%2C+S">S. Adhikari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Amador%2C+E">E. Amador</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M">M. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R">R. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anghel%2C+I">I. Anghel</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anjos%2C+J+d">J. d. Anjos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=ArandaFernandez%2C+A">A. ArandaFernandez</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+A">A. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+T">T. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Aristizabal%2C+D">D. Aristizabal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Arrieta-Diaz%2C+E">E. Arrieta-Diaz</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Aryal%2C+K">K. Aryal</a> , et al. (779 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="1601.02984v1-abstract-short" style="display: inline;"> A description of the proposed detector(s) for DUNE at LBNF </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.02984v1-abstract-full" style="display: none;"> A description of the proposed detector(s) for DUNE at LBNF <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.02984v1-abstract-full').style.display = 'none'; document.getElementById('1601.02984v1-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> 12 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2016. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1512.06148">arXiv:1512.06148</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1512.06148">pdf</a>, <a href="https://arxiv.org/format/1512.06148">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 2: The Physics Program for DUNE at LBNF </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=DUNE+Collaboration"> DUNE Collaboration</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamowski%2C+M">M. Adamowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adamson%2C+P">P. Adamson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adhikari%2C+S">S. Adhikari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ahmad%2C+Z">Z. Ahmad</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">T. Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Amador%2C+E">E. Amador</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+J">J. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">K. Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M">M. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+R">R. Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anghel%2C+I">I. Anghel</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anjos%2C+J+d">J. d. Anjos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A">A. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=ArandaFernandez%2C+A">A. ArandaFernandez</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+A">A. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ariga%2C+T">T. Ariga</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Aristizabal%2C+D">D. Aristizabal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Arrieta-Diaz%2C+E">E. Arrieta-Diaz</a> , et al. (780 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="1512.06148v2-abstract-short" style="display: inline;"> The Physics Program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neutrino Facility (LBNF) is described. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1512.06148v2-abstract-full" style="display: none;"> The Physics Program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neutrino Facility (LBNF) is described. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1512.06148v2-abstract-full').style.display = 'none'; document.getElementById('1512.06148v2-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> 22 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 18 December, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2015. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1504.01556">arXiv:1504.01556</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1504.01556">pdf</a>, <a href="https://arxiv.org/format/1504.01556">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</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/10.1088/1748-0221/10/12/P12004">10.1088/1748-0221/10/12/P12004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Operation and performance of the ICARUS-T600 cryogenic plant at Gran Sasso underground Laboratory </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Aprili%2C+P">P. Aprili</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bubak%2C+A">A. Bubak</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">E. Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Canci%2C+N">N. Canci</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">A. Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cie%C5%9Blik%2C+K">K. Cie艣lik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cline%2C+D+B">D. B. Cline</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dabrowski%2C+A">A. Dabrowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Disdier%2C+J+M">J. M. Disdier</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Falcone%2C+A">A. Falcone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gninenko%2C+S">S. Gninenko</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guglielmi%2C+A">A. Guglielmi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Haranczyk%2C+M">M. Haranczyk</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Holeczek%2C+J">J. Holeczek</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ivashkin%2C+A">A. Ivashkin</a> , et al. (33 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="1504.01556v3-abstract-short" style="display: inline;"> ICARUS T600 liquid argon time projection chamber is the first large mass electronic detector of a new generation able to combine the imaging capabilities of the old bubble chambers with the excellent calorimetric energy measurement. After the three months demonstration run on surface in Pavia during 2001, the T600 cryogenic plant was significantly revised, in terms of reliability and safety, in vi&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1504.01556v3-abstract-full').style.display = 'inline'; document.getElementById('1504.01556v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1504.01556v3-abstract-full" style="display: none;"> ICARUS T600 liquid argon time projection chamber is the first large mass electronic detector of a new generation able to combine the imaging capabilities of the old bubble chambers with the excellent calorimetric energy measurement. After the three months demonstration run on surface in Pavia during 2001, the T600 cryogenic plant was significantly revised, in terms of reliability and safety, in view of its long-term operation in an underground environment. The T600 detector was activated in Hall B of the INFN Gran Sasso Laboratory during Spring 2010, where it was operated without interruption for about three years, taking data exposed to the CERN to Gran Sasso long baseline neutrino beam and cosmic rays. In this paper the T600 cryogenic plant is described in detail together with the commissioning procedures that lead to the successful operation of the detector shortly after the end of the filling with liquid Argon. Overall plant performance and stability during the long-term underground operation are discussed. Finally, the decommissioning procedures, carried out about six months after the end of the CNGS neutrino beam operation, are reported. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1504.01556v3-abstract-full').style.display = 'none'; document.getElementById('1504.01556v3-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> 22 April, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 7 April, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2015. </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">27 pages; corrected typos; added references and reshuffled reference list (not in order of citation in previous version) 26 pages; forced figures within section; corrected typos</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1503.01520">arXiv:1503.01520</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1503.01520">pdf</a>, <a href="https://arxiv.org/format/1503.01520">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> A Proposal for a Three Detector Short-Baseline Neutrino Oscillation Program in the Fermilab Booster Neutrino Beam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Acciarri%2C+R">R. Acciarri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">C. Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=An%2C+R">R. An</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">C. Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ankowski%2C+A+M">A. M. Ankowski</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Asaadi%2C+J">J. Asaadi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Badgett%2C+W">W. Badgett</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bagby%2C+L">L. Bagby</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baller%2C+B">B. Baller</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barr%2C+G">G. Barr</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barros%2C+N">N. Barros</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bass%2C+M">M. Bass</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bellini%2C+V">V. Bellini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Benetti%2C+P">P. Benetti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bertolucci%2C+S">S. Bertolucci</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Biery%2C+K">K. Biery</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bilokon%2C+H">H. Bilokon</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bishai%2C+M">M. Bishai</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bitadze%2C+A">A. Bitadze</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Blake%2C+A">A. Blake</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bolton%2C+T">T. Bolton</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bonesini%2C+M">M. Bonesini</a> , et al. (199 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="1503.01520v1-abstract-short" style="display: inline;"> A Short-Baseline Neutrino (SBN) physics program of three LAr-TPC detectors located along the Booster Neutrino Beam (BNB) at Fermilab is presented. This new SBN Program will deliver a rich and compelling physics opportunity, including the ability to resolve a class of experimental anomalies in neutrino physics and to perform the most sensitive search to date for sterile neutrinos at the eV mass-sca&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1503.01520v1-abstract-full').style.display = 'inline'; document.getElementById('1503.01520v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1503.01520v1-abstract-full" style="display: none;"> A Short-Baseline Neutrino (SBN) physics program of three LAr-TPC detectors located along the Booster Neutrino Beam (BNB) at Fermilab is presented. This new SBN Program will deliver a rich and compelling physics opportunity, including the ability to resolve a class of experimental anomalies in neutrino physics and to perform the most sensitive search to date for sterile neutrinos at the eV mass-scale through both appearance and disappearance oscillation channels. Using data sets of 6.6e20 protons on target (P.O.T.) in the LAr1-ND and ICARUS T600 detectors plus 13.2e20 P.O.T. in the MicroBooNE detector, we estimate that a search for muon neutrino to electron neutrino appearance can be performed with ~5 sigma sensitivity for the LSND allowed (99% C.L.) parameter region. In this proposal for the SBN Program, we describe the physics analysis, the conceptual design of the LAr1-ND detector, the design and refurbishment of the T600 detector, the necessary infrastructure required to execute the program, and a possible reconfiguration of the BNB target and horn system to improve its performance for oscillation searches. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1503.01520v1-abstract-full').style.display = 'none'; document.getElementById('1503.01520v1-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> 4 March, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2015. </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">209 pages, 129 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1405.7591">arXiv:1405.7591</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1405.7591">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</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/10.1088/1748-0221/9/08/P08003">10.1088/1748-0221/9/08/P08003 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The trigger system of the ICARUS experiment for the CNGS beam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Benetti%2C+P">P. Benetti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bubak%2C+A">A. Bubak</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">E. Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">A. Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">K. Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cline%2C+D+B">D. B. Cline</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dabrowska%2C+A">A. Dabrowska</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dequal%2C+D">D. Dequal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dolfini%2C+R">R. Dolfini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Falcone%2C+A">A. Falcone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fiorillo%2C+G">G. Fiorillo</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gninenko%2C+S">S. Gninenko</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guglielmi%2C+A">A. Guglielmi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Haranczyk%2C+M">M. Haranczyk</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Holeczek%2C+J">J. Holeczek</a> , et al. (34 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="1405.7591v2-abstract-short" style="display: inline;"> The ICARUS T600 detector, with its 470 tons of active mass, is the largest liquid Argon TPC ever built. Operated for three years in the LNGS underground laboratory, it has collected thousands of CNGS neutrino beam interactions and cosmic ray events with energy spanning from tens of MeV to tens of GeV, with a trigger system based on scintillation light, charge signal on TPC wires and time informati&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1405.7591v2-abstract-full').style.display = 'inline'; document.getElementById('1405.7591v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1405.7591v2-abstract-full" style="display: none;"> The ICARUS T600 detector, with its 470 tons of active mass, is the largest liquid Argon TPC ever built. Operated for three years in the LNGS underground laboratory, it has collected thousands of CNGS neutrino beam interactions and cosmic ray events with energy spanning from tens of MeV to tens of GeV, with a trigger system based on scintillation light, charge signal on TPC wires and time information (for beam related events only). The performance of trigger system in terms of efficiency, background and live-time as a function of the event energy for the CNGS data taking is presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1405.7591v2-abstract-full').style.display = 'none'; document.getElementById('1405.7591v2-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> 8 August, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 May, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2014. </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">23 pages, 23 figures. Published as M Antonello et al 2014 JINST 9 P08003</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1307.7335">arXiv:1307.7335</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1307.7335">pdf</a>, <a href="https://arxiv.org/format/1307.7335">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="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</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"> The Long-Baseline Neutrino Experiment: Exploring Fundamental Symmetries of the Universe </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=LBNE+Collaboration"> LBNE Collaboration</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+C">Corey Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Adams%2C+D">David Adams</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Akiri%2C+T">Tarek Akiri</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Alion%2C+T">Tyler Alion</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anderson%2C+K">Kris Anderson</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andreopoulos%2C+C">Costas Andreopoulos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Andrews%2C+M">Mike Andrews</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anghel%2C+I">Ioana Anghel</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Anjos%2C+J+C+C+d">Jo茫o Carlos Costa dos Anjos</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">Maddalena Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Arrieta-Diaz%2C+E">Enrique Arrieta-Diaz</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Artuso%2C+M">Marina Artuso</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Asaadi%2C+J">Jonathan Asaadi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bai%2C+X">Xinhua Bai</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">Bagdat Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baird%2C+M">Michael Baird</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Balantekin%2C+B">Baha Balantekin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baller%2C+B">Bruce Baller</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baptista%2C+B">Brian Baptista</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barker%2C+D">D&#39;Ann Barker</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barker%2C+G">Gary Barker</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barletta%2C+W+A">William A. Barletta</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Barr%2C+G">Giles Barr</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bartoszek%2C+L">Larry Bartoszek</a> , et al. (461 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="1307.7335v3-abstract-short" style="display: inline;"> The preponderance of matter over antimatter in the early Universe, the dynamics of the supernova bursts that produced the heavy elements necessary for life and whether protons eventually decay --- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our Universe, its current state and its eventual fate. The Long-Baseline Neutrino Exp&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.7335v3-abstract-full').style.display = 'inline'; document.getElementById('1307.7335v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1307.7335v3-abstract-full" style="display: none;"> The preponderance of matter over antimatter in the early Universe, the dynamics of the supernova bursts that produced the heavy elements necessary for life and whether protons eventually decay --- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our Universe, its current state and its eventual fate. The Long-Baseline Neutrino Experiment (LBNE) represents an extensively developed plan for a world-class experiment dedicated to addressing these questions. LBNE is conceived around three central components: (1) a new, high-intensity neutrino source generated from a megawatt-class proton accelerator at Fermi National Accelerator Laboratory, (2) a near neutrino detector just downstream of the source, and (3) a massive liquid argon time-projection chamber deployed as a far detector deep underground at the Sanford Underground Research Facility. This facility, located at the site of the former Homestake Mine in Lead, South Dakota, is approximately 1,300 km from the neutrino source at Fermilab -- a distance (baseline) that delivers optimal sensitivity to neutrino charge-parity symmetry violation and mass ordering effects. This ambitious yet cost-effective design incorporates scalability and flexibility and can accommodate a variety of upgrades and contributions. With its exceptional combination of experimental configuration, technical capabilities, and potential for transformative discoveries, LBNE promises to be a vital facility for the field of particle physics worldwide, providing physicists from around the globe with opportunities to collaborate in a twenty to thirty year program of exciting science. In this document we provide a comprehensive overview of LBNE&#39;s scientific objectives, its place in the landscape of neutrino physics worldwide, the technologies it will incorporate and the capabilities it will possess. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.7335v3-abstract-full').style.display = 'none'; document.getElementById('1307.7335v3-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> 22 April, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 28 July, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2013. </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">Major update of previous version. This is the reference document for LBNE science program and current status. Chapters 1, 3, and 9 provide a comprehensive overview of LBNE&#39;s scientific objectives, its place in the landscape of neutrino physics worldwide, the technologies it will incorporate and the capabilities it will possess. 288 pages, 116 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> BNL-101354-2014-JA, FERMILAB-PUB-14-022, LA-UR-14-20881 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1307.4699">arXiv:1307.4699</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1307.4699">pdf</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 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/s10052-013-2599-z">10.1140/epjc/s10052-013-2599-z <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for anomalies in the 谓e appearance from a 谓渭 beam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Benetti%2C+P">P. Benetti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bubak%2C+A">A. Bubak</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">E. Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Canci%2C+N">N. Canci</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">A. Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">K. Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cline%2C+D+B">D. B. Cline</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dabrowska%2C+A">A. Dabrowska</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dequal%2C+D">D. Dequal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dolfini%2C+R">R. Dolfini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Falcone%2C+A">A. Falcone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fiorillo%2C+G">G. Fiorillo</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gninenko%2C+S">S. Gninenko</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guglielmi%2C+A">A. Guglielmi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Haranczyk%2C+M">M. Haranczyk</a> , et al. (35 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="1307.4699v3-abstract-short" style="display: inline;"> We report an updated result from the ICARUS experiment on the search for 谓渭 -&gt;谓e anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and travelling 730 km to the Gran Sasso Laboratory. The present analysis is based on a total sample of 1995 events of CNGS neutrino interactions, which corresponds to an almost doubled sample with respect to the previously published result&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.4699v3-abstract-full').style.display = 'inline'; document.getElementById('1307.4699v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1307.4699v3-abstract-full" style="display: none;"> We report an updated result from the ICARUS experiment on the search for 谓渭 -&gt;谓e anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and travelling 730 km to the Gran Sasso Laboratory. The present analysis is based on a total sample of 1995 events of CNGS neutrino interactions, which corresponds to an almost doubled sample with respect to the previously published result. Four clear 谓e events have been visually identified over the full sample, compared with an expectation of 6.4 +- 0.9 events from conventional sources. The result is compatible with the absence of additional anomalous contributions. At 90% and 99% confidence levels the limits to possible oscillated events are 3.7 and 8.3 respectively. The corresponding limit to oscillation probability becomes consequently 3.4 x 10-3 and 7.6 x 10-3 respectively. The present result confirms, with an improved sensitivity, the early result already published by the ICARUS collaboration. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.4699v3-abstract-full').style.display = 'none'; document.getElementById('1307.4699v3-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> 7 August, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 July, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2013. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1208.2629">arXiv:1208.2629</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1208.2629">pdf</a>, <a href="https://arxiv.org/format/1208.2629">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> </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/10.1007/JHEP11(2012)049">10.1007/JHEP11(2012)049 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Precision measurement of the neutrino velocity with the ICARUS detector in the CNGS beam </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Benetti%2C+P">P. Benetti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">E. Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Canci%2C+N">N. Canci</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">A. Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">K. Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cline%2C+D+B">D. B. Cline</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dabrowska%2C+A">A. Dabrowska</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dequal%2C+D">D. Dequal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dolfini%2C+R">R. Dolfini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fiorillo%2C+G">G. Fiorillo</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gninenko%2C+S">S. Gninenko</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Guglielmi%2C+A">A. Guglielmi</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Haranczyk%2C+M">M. Haranczyk</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Holeczek%2C+J">J. Holeczek</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ivashkin%2C+A">A. Ivashkin</a> , et al. (46 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="1208.2629v2-abstract-short" style="display: inline;"> During May 2012, the CERN-CNGS neutrino beam has been operated for two weeks for a total of 1.8 10^17 pot in bunched mode, with a 3 ns narrow width proton beam bunches, separated by 100 ns. This tightly bunched beam structure allows a very accurate time of flight measurement of neutrinos from CERN to LNGS on an event-by-event basis. Both the ICARUS-T600 PMT-DAQ and the CERN-LNGS timing synchroniza&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1208.2629v2-abstract-full').style.display = 'inline'; document.getElementById('1208.2629v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1208.2629v2-abstract-full" style="display: none;"> During May 2012, the CERN-CNGS neutrino beam has been operated for two weeks for a total of 1.8 10^17 pot in bunched mode, with a 3 ns narrow width proton beam bunches, separated by 100 ns. This tightly bunched beam structure allows a very accurate time of flight measurement of neutrinos from CERN to LNGS on an event-by-event basis. Both the ICARUS-T600 PMT-DAQ and the CERN-LNGS timing synchronization have been substantially improved for this campaign, taking ad-vantage of additional independent GPS receivers, both at CERN and LNGS as well as of the deployment of the &#34;White Rabbit&#34; protocol both at CERN and LNGS. The ICARUS-T600 detector has collected 25 beam-associated events; the corresponding time of flight has been accurately evaluated, using all different time synchronization paths. The measured neutrino time of flight is compatible with the arrival of all events with speed equivalent to the one of light: the difference between the expected value based on the speed of light and the measured value is tof_c - tof_nu = (0.10 \pm 0.67stat. \pm 2.39syst.) ns. This result is in agreement with the value previously reported by the ICARUS collaboration, tof_c - tof_nu = (0.3 \pm 4.9stat. \pm 9.0syst.) ns, but with improved statistical and systematic errors. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1208.2629v2-abstract-full').style.display = 'none'; document.getElementById('1208.2629v2-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> 26 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 13 August, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2012. </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">21 pages, 13 figures, 1 table</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1208.0862">arXiv:1208.0862</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1208.0862">pdf</a>, <a href="https://arxiv.org/format/1208.0862">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey 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="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> Search for anomalies in the neutrino sector with muon spectrometers and large LArTPC imaging detectors at CERN </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bagliani%2C+D">D. Bagliani</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bilokon%2C+H">H. Bilokon</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bonesini%2C+M">M. Bonesini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">E. Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Canci%2C+N">N. Canci</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">A. Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">K. Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cline%2C+D+B">D. B. Cline</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dequal%2C+D">D. Dequal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dolfini%2C+R">R. Dolfini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=De+Gerone%2C+M">M. De Gerone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dussoni%2C+S">S. Dussoni</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fiorillo%2C+G">G. Fiorillo</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Garvey%2C+G+T">G. T. Garvey</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gatti%2C+F">F. Gatti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a> , et al. (114 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="1208.0862v2-abstract-short" style="display: inline;"> A new experiment with an intense ~2 GeV neutrino beam at CERN SPS is proposed in order to definitely clarify the possible existence of additional neutrino states, as pointed out by neutrino calibration source experiments, reactor and accelerator experiments and measure the corresponding oscillation parameters. The experiment is based on two identical LAr-TPCs complemented by magnetized spectromete&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1208.0862v2-abstract-full').style.display = 'inline'; document.getElementById('1208.0862v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1208.0862v2-abstract-full" style="display: none;"> A new experiment with an intense ~2 GeV neutrino beam at CERN SPS is proposed in order to definitely clarify the possible existence of additional neutrino states, as pointed out by neutrino calibration source experiments, reactor and accelerator experiments and measure the corresponding oscillation parameters. The experiment is based on two identical LAr-TPCs complemented by magnetized spectrometers detecting electron and muon neutrino events at Far and Near positions, 1600 m and 300 m from the proton target, respectively. The ICARUS T600 detector, the largest LAr-TPC ever built with a size of about 600 ton of imaging mass, now running in the LNGS underground laboratory, will be moved at the CERN Far position. An additional 1/4 of the T600 detector (T150) will be constructed and located in the Near position. Two large area spectrometers will be placed downstream of the two LAr-TPC detectors to perform charge identification and muon momentum measurements from sub-GeV to several GeV energy range, greatly complementing the physics capabilities. This experiment will offer remarkable discovery potentialities, collecting a very large number of unbiased events both in the neutrino and antineutrino channels, largely adequate to definitely settle the origin of the observed neutrino-related anomalies. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1208.0862v2-abstract-full').style.display = 'none'; document.getElementById('1208.0862v2-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> 28 September, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 3 August, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2012. </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">Contribution to the European Strategy for Particle Physics - Open Symposium Preparatory Group, Kracow 10-12 September 2012</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1203.3432">arXiv:1203.3432</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1203.3432">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</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"> Search for &#34;anomalies&#34; from neutrino and anti-neutrino oscillations at Delta_m^2 ~ 1eV^2 with muon spectrometers and large LAr-TPC imaging detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ex?searchtype=author&amp;query=Antonello%2C+M">M. Antonello</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bagliani%2C+D">D. Bagliani</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Baibussinov%2C+B">B. Baibussinov</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bilokon%2C+H">H. Bilokon</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Boffelli%2C+F">F. Boffelli</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Bonesini%2C+M">M. Bonesini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Calligarich%2C+E">E. Calligarich</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Canci%2C+N">N. Canci</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Centro%2C+S">S. Centro</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cesana%2C+A">A. Cesana</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cieslik%2C+K">K. Cieslik</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cline%2C+D+B">D. B. Cline</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Cocco%2C+A+G">A. G. Cocco</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dequal%2C+D">D. Dequal</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dermenev%2C+A">A. Dermenev</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dolfini%2C+R">R. Dolfini</a>, <a href="/search/hep-ex?searchtype=author&amp;query=De+Gerone%2C+M">M. De Gerone</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Dussoni%2C+S">S. Dussoni</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Farnese%2C+C">C. Farnese</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fava%2C+A">A. Fava</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Ferrari%2C+A">A. Ferrari</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Fiorillo%2C+G">G. Fiorillo</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Garvey%2C+G+T">G. T. Garvey</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gatti%2C+F">F. Gatti</a>, <a href="/search/hep-ex?searchtype=author&amp;query=Gibin%2C+D">D. Gibin</a> , et al. (114 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="1203.3432v2-abstract-short" style="display: inline;"> This proposal describes an experimental search for sterile neutrinos beyond the Standard Model with a new CERN-SPS neutrino beam. The experiment is based on two identical LAr-TPC&#39;s followed by magnetized spectrometers, observing the electron and muon neutrino events at 1600 and 300 m from the proton target. This project will exploit the ICARUS T600, moved from LNGS to the CERN &#34;Far&#34; position. An a&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.3432v2-abstract-full').style.display = 'inline'; document.getElementById('1203.3432v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1203.3432v2-abstract-full" style="display: none;"> This proposal describes an experimental search for sterile neutrinos beyond the Standard Model with a new CERN-SPS neutrino beam. The experiment is based on two identical LAr-TPC&#39;s followed by magnetized spectrometers, observing the electron and muon neutrino events at 1600 and 300 m from the proton target. This project will exploit the ICARUS T600, moved from LNGS to the CERN &#34;Far&#34; position. An additional 1/4 of the T600 detector will be constructed and located in the &#34;Near&#34; position. Two spectrometers will be placed downstream of the two LAr-TPC detectors to greatly complement the physics capabilities. Spectrometers will exploit a classical dipole magnetic field with iron slabs, and a new concept air-magnet, to perform charge identification and muon momentum measurements in a wide energy range over a large transverse area. In the two positions, the radial and energy spectra of the nu_e beam are practically identical. Comparing the two detectors, in absence of oscillations, all cross sections and experimental biases cancel out, and the two experimentally observed event distributions must be identical. Any difference of the event distributions at the locations of the two detectors might be attributed to the possible existence of 谓-oscillations, presumably due to additional neutrinos with a mixing angle sin^2(2theta_new) and a larger mass difference Delta_m^2_new. The superior quality of the LAr imaging TPC, in particular its unique electron-pi_zero discrimination allows full rejection of backgrounds and offers a lossless nu_e detection capability. The determination of the muon charge with the spectrometers allows the full separation of nu_mu from anti-nu_mu and therefore controlling systematics from muon mis-identification largely at high momenta. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.3432v2-abstract-full').style.display = 'none'; document.getElementById('1203.3432v2-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 March, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 15 March, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2012. </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">Experiment proposal</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CERN-SPSC-2012-010 and SPSC-P-347 </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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