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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="Nuclear Theory">nucl-th</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/10.1103/PhysRevD.110.093002">10.1103/PhysRevD.110.093002 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Supernova electron-neutrino interactions with xenon in the nEXO detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&amp;query=nEXO+Collaboration"> nEXO Collaboration</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Hedges%2C+S">S. Hedges</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Kharusi%2C+S+A">S. Al Kharusi</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Angelico%2C+E">E. Angelico</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Brodsky%2C+J+P">J. P. Brodsky</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Richardson%2C+G">G. Richardson</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Wilde%2C+S">S. Wilde</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Amy%2C+A">A. Amy</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Anker%2C+A">A. Anker</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Arnquist%2C+I+J">I. J. Arnquist</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Arsenault%2C+P">P. Arsenault</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Atencio%2C+A">A. Atencio</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Badhrees%2C+I">I. Badhrees</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bane%2C+J">J. Bane</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Belov%2C+V">V. Belov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bernard%2C+E+P">E. P. Bernard</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bhatta%2C+T">T. Bhatta</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bolotnikov%2C+A">A. Bolotnikov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Breslin%2C+J">J. Breslin</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Breur%2C+P+A">P. A. Breur</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Brown%2C+E">E. Brown</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Brunner%2C+T">T. Brunner</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Caden%2C+E">E. Caden</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cao%2C+G+F">G. F. Cao</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cao%2C+L+Q">L. Q. Cao</a> , et al. (122 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="2405.19419v2-abstract-short" style="display: inline;"> Electron-neutrino charged-current interactions with xenon nuclei were modeled in the nEXO neutrinoless double-$尾$ decay detector (~5 metric ton, 90% ${}^{136}$Xe, 10% ${}^{134}$Xe) to evaluate its sensitivity to supernova neutrinos. Predictions for event rates and detectable signatures were modeled using the Model of Argon Reaction Low Energy Yields (MARLEY) event generator. We find good agreement&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.19419v2-abstract-full').style.display = 'inline'; document.getElementById('2405.19419v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2405.19419v2-abstract-full" style="display: none;"> Electron-neutrino charged-current interactions with xenon nuclei were modeled in the nEXO neutrinoless double-$尾$ decay detector (~5 metric ton, 90% ${}^{136}$Xe, 10% ${}^{134}$Xe) to evaluate its sensitivity to supernova neutrinos. Predictions for event rates and detectable signatures were modeled using the Model of Argon Reaction Low Energy Yields (MARLEY) event generator. We find good agreement between MARLEY&#39;s predictions and existing theoretical calculations of the inclusive cross sections at supernova neutrino energies. The interactions modeled by MARLEY were simulated within the nEXO simulation framework and were run through an example reconstruction algorithm to determine the detector&#39;s efficiency for reconstructing these events. The simulated data, incorporating the detector response, were used to study the ability of nEXO to reconstruct the incident electron-neutrino spectrum and these results were extended to a larger xenon detector of the same isotope enrichment. We estimate that nEXO will be able to observe electron-neutrino interactions with xenon from supernovae as far as 5-8 kpc from Earth, while the ability to reconstruct incident electron-neutrino spectrum parameters from observed interactions in nEXO is limited to closer supernovae. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.19419v2-abstract-full').style.display = 'none'; document.getElementById('2405.19419v2-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 November, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 May, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">17 pages, 16 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> LLNL-JRNL-864783 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 110, 093002 (2024) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2203.07361">arXiv:2203.07361</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2203.07361">pdf</a>, <a href="https://arxiv.org/format/2203.07361">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 - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&amp;query=Abdullah%2C+M">M. Abdullah</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Abele%2C+H">H. Abele</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Akimov%2C+D">D. Akimov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Angloher%2C+G">G. Angloher</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Aristizabal-Sierra%2C+D">D. Aristizabal-Sierra</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Balantekin%2C+A+B">A. B. Balantekin</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Balogh%2C+L">L. Balogh</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Barbeau%2C+P+S">P. S. Barbeau</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Baudis%2C+L">L. Baudis</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Baxter%2C+A+L">A. L. Baxter</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Beaufort%2C+C">C. Beaufort</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Beaulieu%2C+G">G. Beaulieu</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Belov%2C+V">V. Belov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bento%2C+A">A. Bento</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Berge%2C+L">L. Berge</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bernardi%2C+I+A">I. A. Bernardi</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bolozdynya%2C+A">A. Bolozdynya</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bonhomme%2C+A">A. Bonhomme</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bres%2C+G">G. Bres</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bret%2C+J+L">J-. L. Bret</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Broniatowski%2C+A">A. Broniatowski</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Brossard%2C+A">A. Brossard</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Buck%2C+C">C. Buck</a> , et al. (250 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="2203.07361v1-abstract-short" style="display: inline;"> Coherent elastic neutrino-nucleus scattering (CE$谓$NS) is a process in which neutrinos scatter on a nucleus which acts as a single particle. Though the total cross section is large by neutrino standards, CE$谓$NS has long proven difficult to detect, since the deposited energy into the nucleus is $\sim$ keV. In 2017, the COHERENT collaboration announced the detection of CE$谓$NS using a stopped-pion&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.07361v1-abstract-full').style.display = 'inline'; document.getElementById('2203.07361v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2203.07361v1-abstract-full" style="display: none;"> Coherent elastic neutrino-nucleus scattering (CE$谓$NS) is a process in which neutrinos scatter on a nucleus which acts as a single particle. Though the total cross section is large by neutrino standards, CE$谓$NS has long proven difficult to detect, since the deposited energy into the nucleus is $\sim$ keV. In 2017, the COHERENT collaboration announced the detection of CE$谓$NS using a stopped-pion source with CsI detectors, followed up the detection of CE$谓$NS using an Ar target. The detection of CE$谓$NS has spawned a flurry of activities in high-energy physics, inspiring new constraints on beyond the Standard Model (BSM) physics, and new experimental methods. The CE$谓$NS process has important implications for not only high-energy physics, but also astrophysics, nuclear physics, and beyond. This whitepaper discusses the scientific importance of CE$谓$NS, highlighting how present experiments such as COHERENT are informing theory, and also how future experiments will provide a wealth of information across the aforementioned fields of physics. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.07361v1-abstract-full').style.display = 'none'; document.getElementById('2203.07361v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 March, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2022. </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 Snowmasss 2021. Contact authors: P. S. Barbeau, R. Strauss, L. E. Strigari</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1708.01294">arXiv:1708.01294</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1708.01294">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <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="Nuclear Theory">nucl-th</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/10.1126/science.aao0990">10.1126/science.aao0990 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Observation of Coherent Elastic Neutrino-Nucleus Scattering </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&amp;query=Akimov%2C+D">D. Akimov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Albert%2C+J+B">J. B. Albert</a>, <a href="/search/hep-ph?searchtype=author&amp;query=An%2C+P">P. An</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Awe%2C+C">C. Awe</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Barbeau%2C+P+S">P. S. Barbeau</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Becker%2C+B">B. Becker</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Belov%2C+V">V. Belov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Brown%2C+A">A. Brown</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Bolozdynya%2C+A">A. Bolozdynya</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cabrera-Palmer%2C+B">B. Cabrera-Palmer</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cervantes%2C+M">M. Cervantes</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Collar%2C+J+I">J. I. Collar</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cooper%2C+R+J">R. J. Cooper</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cooper%2C+R+L">R. L. Cooper</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cuesta%2C+C">C. Cuesta</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Dean%2C+D+J">D. J. Dean</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Detwiler%2C+J+A">J. A. Detwiler</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Eberhardt%2C+A">A. Eberhardt</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Efremenko%2C+Y">Y. Efremenko</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Elliott%2C+S+R">S. R. Elliott</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Erkela%2C+E+M">E. M. Erkela</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Fabris%2C+L">L. Fabris</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Febbraro%2C+M">M. Febbraro</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Fields%2C+N+E">N. E. Fields</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Fox%2C+W">W. Fox</a> , et al. (56 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="1708.01294v1-abstract-short" style="display: inline;"> The coherent elastic scattering of neutrinos off nuclei has eluded detection for four decades, even though its predicted cross-section is the largest by far of all low-energy neutrino couplings. This mode of interaction provides new opportunities to study neutrino properties, and leads to a miniaturization of detector size, with potential technological applications. We observe this process at a 6.&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1708.01294v1-abstract-full').style.display = 'inline'; document.getElementById('1708.01294v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1708.01294v1-abstract-full" style="display: none;"> The coherent elastic scattering of neutrinos off nuclei has eluded detection for four decades, even though its predicted cross-section is the largest by far of all low-energy neutrino couplings. This mode of interaction provides new opportunities to study neutrino properties, and leads to a miniaturization of detector size, with potential technological applications. We observe this process at a 6.7-sigma confidence level, using a low-background, 14.6-kg CsI[Na] scintillator exposed to the neutrino emissions from the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory. Characteristic signatures in energy and time, predicted by the Standard Model for this process, are observed in high signal-to-background conditions. Improved constraints on non-standard neutrino interactions with quarks are derived from this initial dataset. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1708.01294v1-abstract-full').style.display = 'none'; document.getElementById('1708.01294v1-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> 3 August, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2017. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1601.07266">arXiv:1601.07266</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1601.07266">pdf</a>, <a href="https://arxiv.org/format/1601.07266">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</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/10.1103/PhysRevD.93.072001">10.1103/PhysRevD.93.072001 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First Search for Lorentz and CPT Violation in Double Beta Decay with EXO-200 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&amp;query=Collaboration%2C+E">EXO-200 Collaboration</a>, <a href="/search/hep-ph?searchtype=author&amp;query=%3A"> :</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Albert%2C+J+B">J. B. Albert</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Barbeau%2C+P+S">P. S. Barbeau</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Beck%2C+D">D. Beck</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Belov%2C+V">V. Belov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Breidenbach%2C+M">M. Breidenbach</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Brunner%2C+T">T. Brunner</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Burenkov%2C+A">A. Burenkov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cao%2C+G+F">G. F. Cao</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Chambers%2C+C">C. Chambers</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Cleveland%2C+B">B. Cleveland</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Coon%2C+M">M. Coon</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Craycraft%2C+A">A. Craycraft</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Daniels%2C+T">T. Daniels</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Danilov%2C+M">M. Danilov</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Daugherty%2C+S+J">S. J. Daugherty</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Davis%2C+C+G">C. G. Davis</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Davis%2C+J">J. Davis</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Delaquis%2C+S">S. Delaquis</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Der+Mesrobian-Kabakian%2C+A">A. Der Mesrobian-Kabakian</a>, <a href="/search/hep-ph?searchtype=author&amp;query=DeVoe%2C+R">R. DeVoe</a>, <a href="/search/hep-ph?searchtype=author&amp;query=D%C3%ADaz%2C+J+S">J. S. D铆az</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Didberidze%2C+T">T. Didberidze</a>, <a href="/search/hep-ph?searchtype=author&amp;query=Dilling%2C+J">J. Dilling</a> , et al. (65 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="1601.07266v2-abstract-short" style="display: inline;"> A search for Lorentz- and CPT-violating signals in the double beta decay spectrum of $^{136}$Xe has been performed using an exposure of 100 kg$\cdot$yr with the EXO-200 detector. No significant evidence of the spectral modification due to isotropic Lorentz-violation was found, and a two-sided limit of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.07266v2-abstract-full').style.display = 'inline'; document.getElementById('1601.07266v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1601.07266v2-abstract-full" style="display: none;"> A search for Lorentz- and CPT-violating signals in the double beta decay spectrum of $^{136}$Xe has been performed using an exposure of 100 kg$\cdot$yr with the EXO-200 detector. No significant evidence of the spectral modification due to isotropic Lorentz-violation was found, and a two-sided limit of $-2.65 \times 10^{-5 } \; \textrm{GeV} &lt; \mathring{a}^{(3)}_{\text{of}} &lt; 7.60 \times 10^{-6} \; \textrm{GeV}$ (90% C.L.) is placed on the relevant coefficient within the Standard-Model Extension (SME). This is the first experimental study of the effect of the SME-defined oscillation-free and momentum-independent neutrino coupling operator on the double beta decay process. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1601.07266v2-abstract-full').style.display = 'none'; document.getElementById('1601.07266v2-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> 3 April, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 January, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">6 pages, 3 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 93, 072001 (2016) </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 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div> <!-- end MetaColumn 1 --> <!-- MetaColumn 2 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/license/index.html">Copyright</a></li> <li><a href="https://info.arxiv.org/help/policies/privacy_policy.html">Privacy Policy</a></li> </ul> </div> <div class="column sorry-app-links"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/web_accessibility.html">Web Accessibility Assistance</a></li> <li> <p class="help"> <a class="a11y-main-link" href="https://status.arxiv.org" target="_blank">arXiv Operational Status <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 256 512" class="icon filter-dark_grey" role="presentation"><path d="M224.3 273l-136 136c-9.4 9.4-24.6 9.4-33.9 0l-22.6-22.6c-9.4-9.4-9.4-24.6 0-33.9l96.4-96.4-96.4-96.4c-9.4-9.4-9.4-24.6 0-33.9L54.3 103c9.4-9.4 24.6-9.4 33.9 0l136 136c9.5 9.4 9.5 24.6.1 34z"/></svg></a><br> Get status notifications via <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/email/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg>email</a> or <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/slack/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 448 512" class="icon filter-black" role="presentation"><path d="M94.12 315.1c0 25.9-21.16 47.06-47.06 47.06S0 341 0 315.1c0-25.9 21.16-47.06 47.06-47.06h47.06v47.06zm23.72 0c0-25.9 21.16-47.06 47.06-47.06s47.06 21.16 47.06 47.06v117.84c0 25.9-21.16 47.06-47.06 47.06s-47.06-21.16-47.06-47.06V315.1zm47.06-188.98c-25.9 0-47.06-21.16-47.06-47.06S139 32 164.9 32s47.06 21.16 47.06 47.06v47.06H164.9zm0 23.72c25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06H47.06C21.16 243.96 0 222.8 0 196.9s21.16-47.06 47.06-47.06H164.9zm188.98 47.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06h-47.06V196.9zm-23.72 0c0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06V79.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06V196.9zM283.1 385.88c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06v-47.06h47.06zm0-23.72c-25.9 0-47.06-21.16-47.06-47.06 0-25.9 21.16-47.06 47.06-47.06h117.84c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06H283.1z"/></svg>slack</a> </p> </li> </ul> </div> </div> </div> <!-- end MetaColumn 2 --> </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

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