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href="https://doi.org/10.1103/PhysRevD.107.112013">10.1103/PhysRevD.107.112013 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Search for Low-mass Dark Matter via Bremsstrahlung Radiation and the Migdal Effect in SuperCDMS </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Albakry%2C+M+F">M. F. Albakry</a>, <a href="/search/hep-ph?searchtype=author&query=Alkhatib%2C+I">I. Alkhatib</a>, <a href="/search/hep-ph?searchtype=author&query=Alonso%2C+D">D. Alonso</a>, <a href="/search/hep-ph?searchtype=author&query=Amaral%2C+D+W+P">D. W. P. Amaral</a>, <a href="/search/hep-ph?searchtype=author&query=Aralis%2C+T">T. Aralis</a>, <a href="/search/hep-ph?searchtype=author&query=Aramaki%2C+T">T. Aramaki</a>, <a href="/search/hep-ph?searchtype=author&query=Arnquist%2C+I+J">I. J. Arnquist</a>, <a href="/search/hep-ph?searchtype=author&query=Langroudy%2C+I+A">I. Ataee Langroudy</a>, <a href="/search/hep-ph?searchtype=author&query=Azadbakht%2C+E">E. Azadbakht</a>, <a href="/search/hep-ph?searchtype=author&query=Banik%2C+S">S. Banik</a>, <a href="/search/hep-ph?searchtype=author&query=Bathurst%2C+C">C. Bathurst</a>, <a href="/search/hep-ph?searchtype=author&query=Bhattacharyya%2C+R">R. Bhattacharyya</a>, <a href="/search/hep-ph?searchtype=author&query=Brink%2C+P+L">P. L. Brink</a>, <a href="/search/hep-ph?searchtype=author&query=Bunker%2C+R">R. Bunker</a>, <a href="/search/hep-ph?searchtype=author&query=Cabrera%2C+B">B. Cabrera</a>, <a href="/search/hep-ph?searchtype=author&query=Calkins%2C+R">R. Calkins</a>, <a href="/search/hep-ph?searchtype=author&query=Cameron%2C+R+A">R. A. Cameron</a>, <a href="/search/hep-ph?searchtype=author&query=Cartaro%2C+C">C. Cartaro</a>, <a href="/search/hep-ph?searchtype=author&query=Cerde%C3%B1o%2C+D+G">D. G. Cerde帽o</a>, <a href="/search/hep-ph?searchtype=author&query=Chang%2C+Y+-">Y. -Y. Chang</a>, <a href="/search/hep-ph?searchtype=author&query=Chaudhuri%2C+M">M. Chaudhuri</a>, <a href="/search/hep-ph?searchtype=author&query=Chen%2C+R">R. Chen</a>, <a href="/search/hep-ph?searchtype=author&query=Chott%2C+N">N. Chott</a>, <a href="/search/hep-ph?searchtype=author&query=Cooley%2C+J">J. Cooley</a>, <a href="/search/hep-ph?searchtype=author&query=Coombes%2C+H">H. Coombes</a> , et al. (108 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="2302.09115v1-abstract-short" style="display: inline;"> We present a new analysis of previously published of SuperCDMS data using a profile likelihood framework to search for sub-GeV dark matter (DM) particles through two inelastic scattering channels: bremsstrahlung radiation and the Migdal effect. By considering these possible inelastic scattering channels, experimental sensitivity can be extended to DM masses that are undetectable through the DM-nuc… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.09115v1-abstract-full').style.display = 'inline'; document.getElementById('2302.09115v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2302.09115v1-abstract-full" style="display: none;"> We present a new analysis of previously published of SuperCDMS data using a profile likelihood framework to search for sub-GeV dark matter (DM) particles through two inelastic scattering channels: bremsstrahlung radiation and the Migdal effect. By considering these possible inelastic scattering channels, experimental sensitivity can be extended to DM masses that are undetectable through the DM-nucleon elastic scattering channel, given the energy threshold of current experiments. We exclude DM masses down to $220~\textrm{MeV}/c^2$ at $2.7 \times 10^{-30}~\textrm{cm}^2$ via the bremsstrahlung channel. The Migdal channel search provides overall considerably more stringent limits and excludes DM masses down to $30~\textrm{MeV}/c^2$ at $5.0 \times 10^{-30}~\textrm{cm}^2$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.09115v1-abstract-full').style.display = 'none'; document.getElementById('2302.09115v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 February, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2023. </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">Submitted to PRD</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> 112013 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 107, 2023 </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> [<a href="https://arxiv.org/pdf/2203.07361">pdf</a>, <a href="https://arxiv.org/format/2203.07361">other</a>] </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&query=Abdullah%2C+M">M. Abdullah</a>, <a href="/search/hep-ph?searchtype=author&query=Abele%2C+H">H. Abele</a>, <a href="/search/hep-ph?searchtype=author&query=Akimov%2C+D">D. Akimov</a>, <a href="/search/hep-ph?searchtype=author&query=Angloher%2C+G">G. Angloher</a>, <a href="/search/hep-ph?searchtype=author&query=Aristizabal-Sierra%2C+D">D. Aristizabal-Sierra</a>, <a href="/search/hep-ph?searchtype=author&query=Augier%2C+C">C. Augier</a>, <a href="/search/hep-ph?searchtype=author&query=Balantekin%2C+A+B">A. B. Balantekin</a>, <a href="/search/hep-ph?searchtype=author&query=Balogh%2C+L">L. Balogh</a>, <a href="/search/hep-ph?searchtype=author&query=Barbeau%2C+P+S">P. S. Barbeau</a>, <a href="/search/hep-ph?searchtype=author&query=Baudis%2C+L">L. Baudis</a>, <a href="/search/hep-ph?searchtype=author&query=Baxter%2C+A+L">A. L. Baxter</a>, <a href="/search/hep-ph?searchtype=author&query=Beaufort%2C+C">C. Beaufort</a>, <a href="/search/hep-ph?searchtype=author&query=Beaulieu%2C+G">G. Beaulieu</a>, <a href="/search/hep-ph?searchtype=author&query=Belov%2C+V">V. Belov</a>, <a href="/search/hep-ph?searchtype=author&query=Bento%2C+A">A. Bento</a>, <a href="/search/hep-ph?searchtype=author&query=Berge%2C+L">L. Berge</a>, <a href="/search/hep-ph?searchtype=author&query=Bernardi%2C+I+A">I. A. Bernardi</a>, <a href="/search/hep-ph?searchtype=author&query=Billard%2C+J">J. Billard</a>, <a href="/search/hep-ph?searchtype=author&query=Bolozdynya%2C+A">A. Bolozdynya</a>, <a href="/search/hep-ph?searchtype=author&query=Bonhomme%2C+A">A. Bonhomme</a>, <a href="/search/hep-ph?searchtype=author&query=Bres%2C+G">G. Bres</a>, <a href="/search/hep-ph?searchtype=author&query=Bret%2C+J+L">J-. L. Bret</a>, <a href="/search/hep-ph?searchtype=author&query=Broniatowski%2C+A">A. Broniatowski</a>, <a href="/search/hep-ph?searchtype=author&query=Brossard%2C+A">A. Brossard</a>, <a href="/search/hep-ph?searchtype=author&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… <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';">▽ 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';">△ 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/2011.09183">arXiv:2011.09183</a> <span> [<a href="https://arxiv.org/pdf/2011.09183">pdf</a>, <a href="https://arxiv.org/format/2011.09183">other</a>] </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="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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 - Phenomenology">hep-ph</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/10.1103/PhysRevLett.127.081802">10.1103/PhysRevLett.127.081802 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Constraints on Lightly Ionizing Particles from CDMSlite </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=SuperCDMS+Collaboration"> SuperCDMS Collaboration</a>, <a href="/search/hep-ph?searchtype=author&query=Alkhatib%2C+I">I. Alkhatib</a>, <a href="/search/hep-ph?searchtype=author&query=Amaral%2C+D+W+P">D. W. P. Amaral</a>, <a href="/search/hep-ph?searchtype=author&query=Aralis%2C+T">T. Aralis</a>, <a href="/search/hep-ph?searchtype=author&query=Aramaki%2C+T">T. Aramaki</a>, <a href="/search/hep-ph?searchtype=author&query=Arnquist%2C+I+J">I. J. Arnquist</a>, <a href="/search/hep-ph?searchtype=author&query=Langroudy%2C+I+A">I. Ataee Langroudy</a>, <a href="/search/hep-ph?searchtype=author&query=Azadbakht%2C+E">E. Azadbakht</a>, <a href="/search/hep-ph?searchtype=author&query=Banik%2C+S">S. Banik</a>, <a href="/search/hep-ph?searchtype=author&query=Barker%2C+D">D. Barker</a>, <a href="/search/hep-ph?searchtype=author&query=Bathurst%2C+C">C. Bathurst</a>, <a href="/search/hep-ph?searchtype=author&query=Bauer%2C+D+A">D. A. Bauer</a>, <a href="/search/hep-ph?searchtype=author&query=Bezerra%2C+L+V+S">L. V. S. Bezerra</a>, <a href="/search/hep-ph?searchtype=author&query=Bhattacharyya%2C+R">R. Bhattacharyya</a>, <a href="/search/hep-ph?searchtype=author&query=Bowles%2C+M+A">M. A. Bowles</a>, <a href="/search/hep-ph?searchtype=author&query=Brink%2C+P+L">P. L. Brink</a>, <a href="/search/hep-ph?searchtype=author&query=Bunker%2C+R">R. Bunker</a>, <a href="/search/hep-ph?searchtype=author&query=Cabrera%2C+B">B. Cabrera</a>, <a href="/search/hep-ph?searchtype=author&query=Calkins%2C+R">R. Calkins</a>, <a href="/search/hep-ph?searchtype=author&query=Cameron%2C+R+A">R. A. Cameron</a>, <a href="/search/hep-ph?searchtype=author&query=Cartaro%2C+C">C. Cartaro</a>, <a href="/search/hep-ph?searchtype=author&query=Cerde%C3%B1o%2C+D+G">D. G. Cerde帽o</a>, <a href="/search/hep-ph?searchtype=author&query=Chang%2C+Y+-">Y. -Y. Chang</a>, <a href="/search/hep-ph?searchtype=author&query=Chaudhuri%2C+M">M. Chaudhuri</a>, <a href="/search/hep-ph?searchtype=author&query=Chen%2C+R">R. Chen</a> , et al. (93 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="2011.09183v4-abstract-short" style="display: inline;"> The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to Lightly Ionizing Particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the v… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.09183v4-abstract-full').style.display = 'inline'; document.getElementById('2011.09183v4-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2011.09183v4-abstract-full" style="display: none;"> The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to Lightly Ionizing Particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically-produced LIPs with an electric charge smaller than $e/(3\times10^5$), as well as the strongest limits for charge $\leq e/160$, with a minimum vertical intensity of $1.36\times10^{-7}$\,cm$^{-2}$s$^{-1}$sr$^{-1}$ at charge $e/160$. These results apply over a wide range of LIP masses (5\,MeV/$c^2$ to 100\,TeV/$c^2$) and cover a wide range of $尾纬$ values (0.1 -- $10^6$), thus excluding non-relativistic LIPs with $尾纬$ as small as 0.1 for the first time. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.09183v4-abstract-full').style.display = 'none'; document.getElementById('2011.09183v4-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 February, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 18 November, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 127, 081802 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1708.08869">arXiv:1708.08869</a> <span> [<a href="https://arxiv.org/pdf/1708.08869">pdf</a>, <a href="https://arxiv.org/format/1708.08869">other</a>] </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> </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/PhysRevLett.120.061802">10.1103/PhysRevLett.120.061802 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Results from the Super Cryogenic Dark Matter Search (SuperCDMS) experiment at Soudan </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=SuperCDMS+Collaboration"> SuperCDMS Collaboration</a>, <a href="/search/hep-ph?searchtype=author&query=Agnese%2C+R">R. Agnese</a>, <a href="/search/hep-ph?searchtype=author&query=Aramaki%2C+T">T. Aramaki</a>, <a href="/search/hep-ph?searchtype=author&query=Arnquist%2C+I+J">I. J. Arnquist</a>, <a href="/search/hep-ph?searchtype=author&query=Baker%2C+W">W. Baker</a>, <a href="/search/hep-ph?searchtype=author&query=Balakishiyeva%2C+D">D. Balakishiyeva</a>, <a href="/search/hep-ph?searchtype=author&query=Banik%2C+S">S. Banik</a>, <a href="/search/hep-ph?searchtype=author&query=Barker%2C+D">D. Barker</a>, <a href="/search/hep-ph?searchtype=author&query=Thakur%2C+R+B">R. Basu Thakur</a>, <a href="/search/hep-ph?searchtype=author&query=Bauer%2C+D+A">D. A. Bauer</a>, <a href="/search/hep-ph?searchtype=author&query=Binder%2C+T">T. Binder</a>, <a href="/search/hep-ph?searchtype=author&query=Bowles%2C+M+A">M. A. Bowles</a>, <a href="/search/hep-ph?searchtype=author&query=Brink%2C+P+L">P. L. Brink</a>, <a href="/search/hep-ph?searchtype=author&query=Bunker%2C+R">R. Bunker</a>, <a href="/search/hep-ph?searchtype=author&query=Cabrera%2C+B">B. Cabrera</a>, <a href="/search/hep-ph?searchtype=author&query=Caldwell%2C+D+O">D. O. Caldwell</a>, <a href="/search/hep-ph?searchtype=author&query=Calkins%2C+R">R. Calkins</a>, <a href="/search/hep-ph?searchtype=author&query=Cartaro%2C+C">C. Cartaro</a>, <a href="/search/hep-ph?searchtype=author&query=Cerde%C3%B1o%2C+D+G">D. G. Cerde帽o</a>, <a href="/search/hep-ph?searchtype=author&query=Chang%2C+Y">Y. Chang</a>, <a href="/search/hep-ph?searchtype=author&query=Chen%2C+Y">Y. Chen</a>, <a href="/search/hep-ph?searchtype=author&query=Cooley%2C+J">J. Cooley</a>, <a href="/search/hep-ph?searchtype=author&query=Cornell%2C+B">B. Cornell</a>, <a href="/search/hep-ph?searchtype=author&query=Cushman%2C+P">P. Cushman</a>, <a href="/search/hep-ph?searchtype=author&query=Daal%2C+M">M. Daal</a> , et al. (79 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="1708.08869v1-abstract-short" style="display: inline;"> We report the result of a blinded search for Weakly Interacting Massive Particles (WIMPs) using the majority of the SuperCDMS Soudan dataset. With an exposure of 1690 kg days, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP--nucleon cross section of $1.4 \times 10^{-44}$ (… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1708.08869v1-abstract-full').style.display = 'inline'; document.getElementById('1708.08869v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1708.08869v1-abstract-full" style="display: none;"> We report the result of a blinded search for Weakly Interacting Massive Particles (WIMPs) using the majority of the SuperCDMS Soudan dataset. With an exposure of 1690 kg days, a single candidate event is observed, consistent with expected backgrounds. This analysis (combined with previous Ge results) sets an upper limit on the spin-independent WIMP--nucleon cross section of $1.4 \times 10^{-44}$ ($1.0 \times 10^{-44}$) cm$^2$ at 46 GeV/$c^2$. These results set the strongest limits for WIMP--germanium-nucleus interactions for masses $>$12 GeV/$c^2$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1708.08869v1-abstract-full').style.display = 'none'; document.getElementById('1708.08869v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 August, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2017. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 120, 061802 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1707.04591">arXiv:1707.04591</a> <span> [<a href="https://arxiv.org/pdf/1707.04591">pdf</a>, <a href="https://arxiv.org/format/1707.04591">other</a>] </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="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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"> US Cosmic Visions: New Ideas in Dark Matter 2017: Community Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Battaglieri%2C+M">Marco Battaglieri</a>, <a href="/search/hep-ph?searchtype=author&query=Belloni%2C+A">Alberto Belloni</a>, <a href="/search/hep-ph?searchtype=author&query=Chou%2C+A">Aaron Chou</a>, <a href="/search/hep-ph?searchtype=author&query=Cushman%2C+P">Priscilla Cushman</a>, <a href="/search/hep-ph?searchtype=author&query=Echenard%2C+B">Bertrand Echenard</a>, <a href="/search/hep-ph?searchtype=author&query=Essig%2C+R">Rouven Essig</a>, <a href="/search/hep-ph?searchtype=author&query=Estrada%2C+J">Juan Estrada</a>, <a href="/search/hep-ph?searchtype=author&query=Feng%2C+J+L">Jonathan L. Feng</a>, <a href="/search/hep-ph?searchtype=author&query=Flaugher%2C+B">Brenna Flaugher</a>, <a href="/search/hep-ph?searchtype=author&query=Fox%2C+P+J">Patrick J. Fox</a>, <a href="/search/hep-ph?searchtype=author&query=Graham%2C+P">Peter Graham</a>, <a href="/search/hep-ph?searchtype=author&query=Hall%2C+C">Carter Hall</a>, <a href="/search/hep-ph?searchtype=author&query=Harnik%2C+R">Roni Harnik</a>, <a href="/search/hep-ph?searchtype=author&query=Hewett%2C+J">JoAnne Hewett</a>, <a href="/search/hep-ph?searchtype=author&query=Incandela%2C+J">Joseph Incandela</a>, <a href="/search/hep-ph?searchtype=author&query=Izaguirre%2C+E">Eder Izaguirre</a>, <a href="/search/hep-ph?searchtype=author&query=McKinsey%2C+D">Daniel McKinsey</a>, <a href="/search/hep-ph?searchtype=author&query=Pyle%2C+M">Matthew Pyle</a>, <a href="/search/hep-ph?searchtype=author&query=Roe%2C+N">Natalie Roe</a>, <a href="/search/hep-ph?searchtype=author&query=Rybka%2C+G">Gray Rybka</a>, <a href="/search/hep-ph?searchtype=author&query=Sikivie%2C+P">Pierre Sikivie</a>, <a href="/search/hep-ph?searchtype=author&query=Tait%2C+T+M+P">Tim M. P. Tait</a>, <a href="/search/hep-ph?searchtype=author&query=Toro%2C+N">Natalia Toro</a>, <a href="/search/hep-ph?searchtype=author&query=Van+De+Water%2C+R">Richard Van De Water</a>, <a href="/search/hep-ph?searchtype=author&query=Weiner%2C+N">Neal Weiner</a> , et al. (226 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="1707.04591v1-abstract-short" style="display: inline;"> This white paper summarizes the workshop "U.S. Cosmic Visions: New Ideas in Dark Matter" held at University of Maryland on March 23-25, 2017. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1707.04591v1-abstract-full" style="display: none;"> This white paper summarizes the workshop "U.S. Cosmic Visions: New Ideas in Dark Matter" held at University of Maryland on March 23-25, 2017. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.04591v1-abstract-full').style.display = 'none'; document.getElementById('1707.04591v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 July, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">102 pages + references</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1608.08632">arXiv:1608.08632</a> <span> [<a href="https://arxiv.org/pdf/1608.08632">pdf</a>, <a href="https://arxiv.org/format/1608.08632">other</a>] </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="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Dark Sectors 2016 Workshop: Community Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Alexander%2C+J">Jim Alexander</a>, <a href="/search/hep-ph?searchtype=author&query=Battaglieri%2C+M">Marco Battaglieri</a>, <a href="/search/hep-ph?searchtype=author&query=Echenard%2C+B">Bertrand Echenard</a>, <a href="/search/hep-ph?searchtype=author&query=Essig%2C+R">Rouven Essig</a>, <a href="/search/hep-ph?searchtype=author&query=Graham%2C+M">Matthew Graham</a>, <a href="/search/hep-ph?searchtype=author&query=Izaguirre%2C+E">Eder Izaguirre</a>, <a href="/search/hep-ph?searchtype=author&query=Jaros%2C+J">John Jaros</a>, <a href="/search/hep-ph?searchtype=author&query=Krnjaic%2C+G">Gordan Krnjaic</a>, <a href="/search/hep-ph?searchtype=author&query=Mardon%2C+J">Jeremy Mardon</a>, <a href="/search/hep-ph?searchtype=author&query=Morrissey%2C+D">David Morrissey</a>, <a href="/search/hep-ph?searchtype=author&query=Nelson%2C+T">Tim Nelson</a>, <a href="/search/hep-ph?searchtype=author&query=Perelstein%2C+M">Maxim Perelstein</a>, <a href="/search/hep-ph?searchtype=author&query=Pyle%2C+M">Matt Pyle</a>, <a href="/search/hep-ph?searchtype=author&query=Ritz%2C+A">Adam Ritz</a>, <a href="/search/hep-ph?searchtype=author&query=Schuster%2C+P">Philip Schuster</a>, <a href="/search/hep-ph?searchtype=author&query=Shuve%2C+B">Brian Shuve</a>, <a href="/search/hep-ph?searchtype=author&query=Toro%2C+N">Natalia Toro</a>, <a href="/search/hep-ph?searchtype=author&query=Van+De+Water%2C+R+G">Richard G Van De Water</a>, <a href="/search/hep-ph?searchtype=author&query=Akerib%2C+D">Daniel Akerib</a>, <a href="/search/hep-ph?searchtype=author&query=An%2C+H">Haipeng An</a>, <a href="/search/hep-ph?searchtype=author&query=Aniol%2C+K">Konrad Aniol</a>, <a href="/search/hep-ph?searchtype=author&query=Arnquist%2C+I+J">Isaac J. Arnquist</a>, <a href="/search/hep-ph?searchtype=author&query=Asner%2C+D+M">David M. Asner</a>, <a href="/search/hep-ph?searchtype=author&query=Back%2C+H+O">Henning O. Back</a>, <a href="/search/hep-ph?searchtype=author&query=Baker%2C+K">Keith Baker</a> , et al. (179 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="1608.08632v1-abstract-short" style="display: inline;"> This report, based on the Dark Sectors workshop at SLAC in April 2016, summarizes the scientific importance of searches for dark sector dark matter and forces at masses beneath the weak-scale, the status of this broad international field, the important milestones motivating future exploration, and promising experimental opportunities to reach these milestones over the next 5-10 years. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1608.08632v1-abstract-full" style="display: none;"> This report, based on the Dark Sectors workshop at SLAC in April 2016, summarizes the scientific importance of searches for dark sector dark matter and forces at masses beneath the weak-scale, the status of this broad international field, the important milestones motivating future exploration, and promising experimental opportunities to reach these milestones over the next 5-10 years. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1608.08632v1-abstract-full').style.display = 'none'; document.getElementById('1608.08632v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 August, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 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">66 pages, 15 figures, 3 tables. Workshop website and agenda: http://www-conf.slac.stanford.edu/darksectors2016/ https://indico.cern.ch/event/507783/ Editors: J. Alexander, M. Battaglieri, B. Echenard, R. Essig, M. Graham, E. Izaguirre, J. Jaros, G. Krnjaic, J. Mardon, D. Morrissey, T. Nelson, M. Perelstein, M. Pyle, A. Ritz, P. Schuster, B. Shuve, N. Toro, R. Van De Water</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1505.08061">arXiv:1505.08061</a> <span> [<a href="https://arxiv.org/pdf/1505.08061">pdf</a>, <a href="https://arxiv.org/format/1505.08061">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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.92.063518">10.1103/PhysRevD.92.063518 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Readout strategies for directional dark matter detection beyond the neutrino background </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=O%27Hare%2C+C+A+J">Ciaran A. J. O'Hare</a>, <a href="/search/hep-ph?searchtype=author&query=Green%2C+A+M">Anne M. Green</a>, <a href="/search/hep-ph?searchtype=author&query=Billard%2C+J">Julien Billard</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">Enectali Figueroa-Feliciano</a>, <a href="/search/hep-ph?searchtype=author&query=Strigari%2C+L+E">Louis E. Strigari</a> </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="1505.08061v2-abstract-short" style="display: inline;"> The search for weakly interacting massive particles (WIMPs) by direct detection faces an encroaching background due to coherent neutrino-nucleus scattering. As the sensitivity of these experiments improves, the question of how to best distinguish a dark matter signal from neutrinos will become increasingly important. A proposed method of overcoming this so-called 'neutrino floor' is to utilize the… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1505.08061v2-abstract-full').style.display = 'inline'; document.getElementById('1505.08061v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1505.08061v2-abstract-full" style="display: none;"> The search for weakly interacting massive particles (WIMPs) by direct detection faces an encroaching background due to coherent neutrino-nucleus scattering. As the sensitivity of these experiments improves, the question of how to best distinguish a dark matter signal from neutrinos will become increasingly important. A proposed method of overcoming this so-called 'neutrino floor' is to utilize the directional signature that both neutrino and dark matter induced recoils possess. We show that directional experiments can indeed probe WIMP-nucleon cross-sections below the neutrino floor with little loss in sensitivity due to the neutrino background. In particular we find at low WIMP masses (around 6 GeV) the discovery limits for directional detectors penetrate below the non-directional limit by several orders of magnitude. For high WIMP masses (around 100 GeV), the non-directional limit is overcome by a factor of a few. Furthermore we show that even for directional detectors which can only measure 1- or 2-dimensional projections of the 3-dimensional recoil track, the discovery potential is only reduced by a factor of 3 at most. We also demonstrate that while the experimental limitations of directional detectors, such as sense recognition and finite angular resolution, have a detrimental effect on the discovery limits, it is still possible to overcome the ultimate neutrino background faced by non-directional detectors. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1505.08061v2-abstract-full').style.display = 'none'; document.getElementById('1505.08061v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 September, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 May, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 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">16 pages, 12 figures, published version</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 92, 063518 (2015) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1503.03379">arXiv:1503.03379</a> <span> [<a href="https://arxiv.org/pdf/1503.03379">pdf</a>, <a href="https://arxiv.org/format/1503.03379">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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 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.91.092004">10.1103/PhysRevD.91.092004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Dark matter effective field theory scattering in direct detection experiments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Schneck%2C+K">K. Schneck</a>, <a href="/search/hep-ph?searchtype=author&query=Cabrera%2C+B">B. Cabrera</a>, <a href="/search/hep-ph?searchtype=author&query=Cerdeno%2C+D+G">D. G. Cerdeno</a>, <a href="/search/hep-ph?searchtype=author&query=Mandic%2C+V">V. Mandic</a>, <a href="/search/hep-ph?searchtype=author&query=Rogers%2C+H+E">H. E. Rogers</a>, <a href="/search/hep-ph?searchtype=author&query=Agnese%2C+R">R. Agnese</a>, <a href="/search/hep-ph?searchtype=author&query=Anderson%2C+A+J">A. J. Anderson</a>, <a href="/search/hep-ph?searchtype=author&query=Asai%2C+M">M. Asai</a>, <a href="/search/hep-ph?searchtype=author&query=Balakishiyeva%2C+D">D. Balakishiyeva</a>, <a href="/search/hep-ph?searchtype=author&query=Barker%2C+D">D. Barker</a>, <a href="/search/hep-ph?searchtype=author&query=Thakur%2C+R+B">R. Basu Thakur</a>, <a href="/search/hep-ph?searchtype=author&query=Bauer%2C+D+A">D. A. Bauer</a>, <a href="/search/hep-ph?searchtype=author&query=Billard%2C+J">J. Billard</a>, <a href="/search/hep-ph?searchtype=author&query=Borgland%2C+A">A. Borgland</a>, <a href="/search/hep-ph?searchtype=author&query=Brandt%2C+D">D. Brandt</a>, <a href="/search/hep-ph?searchtype=author&query=Brink%2C+P+L">P. L. Brink</a>, <a href="/search/hep-ph?searchtype=author&query=Bunker%2C+R">R. Bunker</a>, <a href="/search/hep-ph?searchtype=author&query=Caldwell%2C+D+O">D. O. Caldwell</a>, <a href="/search/hep-ph?searchtype=author&query=Calkins%2C+R">R. Calkins</a>, <a href="/search/hep-ph?searchtype=author&query=Chagani%2C+H">H. Chagani</a>, <a href="/search/hep-ph?searchtype=author&query=Chen%2C+Y">Y. Chen</a>, <a href="/search/hep-ph?searchtype=author&query=Cooley%2C+J">J. Cooley</a>, <a href="/search/hep-ph?searchtype=author&query=Cornell%2C+B">B. Cornell</a>, <a href="/search/hep-ph?searchtype=author&query=Crewdson%2C+C+H">C. H. Crewdson</a>, <a href="/search/hep-ph?searchtype=author&query=Cushman%2C+P">P. Cushman</a> , et al. (62 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="1503.03379v3-abstract-short" style="display: inline;"> We examine the consequences of the effective field theory (EFT) of dark matter-nucleon scattering for current and proposed direct detection experiments. Exclusion limits on EFT coupling constants computed using the optimum interval method are presented for SuperCDMS Soudan, CDMS II, and LUX, and the necessity of combining results from multiple experiments in order to determine dark matter paramete… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1503.03379v3-abstract-full').style.display = 'inline'; document.getElementById('1503.03379v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1503.03379v3-abstract-full" style="display: none;"> We examine the consequences of the effective field theory (EFT) of dark matter-nucleon scattering for current and proposed direct detection experiments. Exclusion limits on EFT coupling constants computed using the optimum interval method are presented for SuperCDMS Soudan, CDMS II, and LUX, and the necessity of combining results from multiple experiments in order to determine dark matter parameters is discussed. We demonstrate that spectral differences between the standard dark matter model and a general EFT interaction can produce a bias when calculating exclusion limits and when developing signal models for likelihood and machine learning techniques. We also discuss the implications of the EFT for the next-generation (G2) direct detection experiments and point out regions of complementarity in the EFT parameter space. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1503.03379v3-abstract-full').style.display = 'none'; document.getElementById('1503.03379v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 August, 2016; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 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">Newest version includes erratum</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 91, 092004 (2015) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1409.0050">arXiv:1409.0050</a> <span> [<a href="https://arxiv.org/pdf/1409.0050">pdf</a>, <a href="https://arxiv.org/format/1409.0050">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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 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.91.095023">10.1103/PhysRevD.91.095023 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Solar neutrino physics with low-threshold dark matter detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Billard%2C+J">J. Billard</a>, <a href="/search/hep-ph?searchtype=author&query=Strigari%2C+L">L. Strigari</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a> </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="1409.0050v1-abstract-short" style="display: inline;"> Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent neutrino-nucleus scattering and neutrino electron elastic scattering. We establish an analysis method for extracting Solar model properties and neutrino properties from these measurements, including the possible effects of sterile neutrinos which have been hinted at by some reactor experiments and c… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1409.0050v1-abstract-full').style.display = 'inline'; document.getElementById('1409.0050v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1409.0050v1-abstract-full" style="display: none;"> Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent neutrino-nucleus scattering and neutrino electron elastic scattering. We establish an analysis method for extracting Solar model properties and neutrino properties from these measurements, including the possible effects of sterile neutrinos which have been hinted at by some reactor experiments and cosmological measurements. Even including sterile neutrinos, through the coherent scattering channel a 1 ton-year exposure with a low-threshold Germanium detector could improve on the current measurement of the normalization of the $^8$B Solar neutrino flux down to 3% or less. Combining with the elastic scattering data will provide constraints on both the high and low energy survival probability, and will improve on the uncertainty on the active-to-sterile mixing angle by a factor of two. This sensitivity to active-to-sterile transitions is competitive and complementary to forthcoming dedicated short baseline sterile neutrino searches with nuclear decays. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1409.0050v1-abstract-full').style.display = 'none'; document.getElementById('1409.0050v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 August, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 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">12 pages, 4 figures, 3 tables</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1408.3581">arXiv:1408.3581</a> <span> [<a href="https://arxiv.org/pdf/1408.3581">pdf</a>, <a href="https://arxiv.org/format/1408.3581">other</a>] </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="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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/10.1103/PhysRevD.90.083510">10.1103/PhysRevD.90.083510 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Complementarity of dark matter detectors in light of the neutrino background </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Ruppin%2C+F">F. Ruppin</a>, <a href="/search/hep-ph?searchtype=author&query=Billard%2C+J">J. Billard</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a>, <a href="/search/hep-ph?searchtype=author&query=Strigari%2C+L">L. Strigari</a> </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="1408.3581v1-abstract-short" style="display: inline;"> Direct detection dark matter experiments looking for WIMP-nucleus elastic scattering will soon be sensitive to an irreducible background from neutrinos which will drastically affect their discovery potential. Here we explore how the neutrino background will affect future ton-scale experiments considering both spin-dependent and spin-independent interactions. We show that combining data from experi… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1408.3581v1-abstract-full').style.display = 'inline'; document.getElementById('1408.3581v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1408.3581v1-abstract-full" style="display: none;"> Direct detection dark matter experiments looking for WIMP-nucleus elastic scattering will soon be sensitive to an irreducible background from neutrinos which will drastically affect their discovery potential. Here we explore how the neutrino background will affect future ton-scale experiments considering both spin-dependent and spin-independent interactions. We show that combining data from experiments using different targets can improve the dark matter discovery potential due to target complementarity. We find that in the context of spin-dependent interactions, combining results from several targets can greatly enhance the subtraction of the neutrino background for WIMP masses below 10 GeV/c$^2$ and therefore probe dark matter models to lower cross-sections. In the context of target complementarity, we also explore how one can tune the relative exposures of different target materials to optimize the WIMP discovery potential. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1408.3581v1-abstract-full').style.display = 'none'; document.getElementById('1408.3581v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 August, 2014; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 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">13 pages, 12 figures, 3 tables</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 90, 083510 (2014) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1310.0125">arXiv:1310.0125</a> <span> [<a href="https://arxiv.org/pdf/1310.0125">pdf</a>, <a href="https://arxiv.org/format/1310.0125">other</a>] </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="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> Coherent Scattering Investigations at the Spallation Neutron Source: a Snowmass White Paper </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Akimov%2C+D">D. Akimov</a>, <a href="/search/hep-ph?searchtype=author&query=Bernstein%2C+A">A. Bernstein</a>, <a href="/search/hep-ph?searchtype=author&query=Barbeau%2C+P">P. Barbeau</a>, <a href="/search/hep-ph?searchtype=author&query=Barton%2C+P">P. Barton</a>, <a href="/search/hep-ph?searchtype=author&query=Bolozdynya%2C+A">A. Bolozdynya</a>, <a href="/search/hep-ph?searchtype=author&query=Cabrera-Palmer%2C+B">B. Cabrera-Palmer</a>, <a href="/search/hep-ph?searchtype=author&query=Cavanna%2C+F">F. Cavanna</a>, <a href="/search/hep-ph?searchtype=author&query=Cianciolo%2C+V">V. Cianciolo</a>, <a href="/search/hep-ph?searchtype=author&query=Collar%2C+J">J. Collar</a>, <a href="/search/hep-ph?searchtype=author&query=Cooper%2C+R+J">R. J. Cooper</a>, <a href="/search/hep-ph?searchtype=author&query=Dean%2C+D">D. Dean</a>, <a href="/search/hep-ph?searchtype=author&query=Efremenko%2C+Y">Y. Efremenko</a>, <a href="/search/hep-ph?searchtype=author&query=Etenko%2C+A">A. Etenko</a>, <a href="/search/hep-ph?searchtype=author&query=Fields%2C+N">N. Fields</a>, <a href="/search/hep-ph?searchtype=author&query=Foxe%2C+M">M. Foxe</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a>, <a href="/search/hep-ph?searchtype=author&query=Fomin%2C+N">N. Fomin</a>, <a href="/search/hep-ph?searchtype=author&query=Gallmeier%2C+F">F. Gallmeier</a>, <a href="/search/hep-ph?searchtype=author&query=Garishvili%2C+I">I. Garishvili</a>, <a href="/search/hep-ph?searchtype=author&query=Gerling%2C+M">M. Gerling</a>, <a href="/search/hep-ph?searchtype=author&query=Green%2C+M">M. Green</a>, <a href="/search/hep-ph?searchtype=author&query=Greene%2C+G">G. Greene</a>, <a href="/search/hep-ph?searchtype=author&query=Hatzikoutelis%2C+A">A. Hatzikoutelis</a>, <a href="/search/hep-ph?searchtype=author&query=Henning%2C+R">R. Henning</a>, <a href="/search/hep-ph?searchtype=author&query=Hix%2C+R">R. Hix</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="1310.0125v1-abstract-short" style="display: inline;"> The Spallation Neutron Source (SNS) at Oak Ridge National Laboratory, Tennessee, provides an intense flux of neutrinos in the few tens-of-MeV range, with a sharply-pulsed timing structure that is beneficial for background rejection. In this white paper, we describe how the SNS source can be used for a measurement of coherent elastic neutrino-nucleus scattering (CENNS), and the physics reach of dif… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.0125v1-abstract-full').style.display = 'inline'; document.getElementById('1310.0125v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1310.0125v1-abstract-full" style="display: none;"> The Spallation Neutron Source (SNS) at Oak Ridge National Laboratory, Tennessee, provides an intense flux of neutrinos in the few tens-of-MeV range, with a sharply-pulsed timing structure that is beneficial for background rejection. In this white paper, we describe how the SNS source can be used for a measurement of coherent elastic neutrino-nucleus scattering (CENNS), and the physics reach of different phases of such an experimental program (CSI: Coherent Scattering Investigations at the SNS). <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1310.0125v1-abstract-full').style.display = 'none'; document.getElementById('1310.0125v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 September, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">Snowmass white paper</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1307.5458">arXiv:1307.5458</a> <span> [<a href="https://arxiv.org/pdf/1307.5458">pdf</a>, <a href="https://arxiv.org/ps/1307.5458">ps</a>, <a href="https://arxiv.org/format/1307.5458">other</a>] </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="Astrophysics of Galaxies">astro-ph.GA</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.89.023524">10.1103/PhysRevD.89.023524 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Billard%2C+J">J. Billard</a>, <a href="/search/hep-ph?searchtype=author&query=Strigari%2C+L">L. Strigari</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a> </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="1307.5458v3-abstract-short" style="display: inline;"> As direct dark matter experiments continue to increase in size, they will become sensitive to neutrinos from astrophysical sources. For experiments that do not have directional sensitivity, coherent neutrino scattering (CNS) from several sources represents an important background to understand, as it can almost perfectly mimic an authentic WIMP signal. Here we explore in detail the effect of neutr… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.5458v3-abstract-full').style.display = 'inline'; document.getElementById('1307.5458v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1307.5458v3-abstract-full" style="display: none;"> As direct dark matter experiments continue to increase in size, they will become sensitive to neutrinos from astrophysical sources. For experiments that do not have directional sensitivity, coherent neutrino scattering (CNS) from several sources represents an important background to understand, as it can almost perfectly mimic an authentic WIMP signal. Here we explore in detail the effect of neutrino backgrounds on the discovery potential of WIMPs over the entire mass range of 500 MeV to 10 TeV. We show that, given the theoretical and measured uncertainties on the neutrino backgrounds, direct detection experiments lose sensitivity to light (~10 GeV) and heavy (~100 GeV) WIMPs with a spin-independent cross section below 10^{-45} cm^2 and 10^{-49} cm^2, respectively. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.5458v3-abstract-full').style.display = 'none'; document.getElementById('1307.5458v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 January, 2014; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 20 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">15 pages, 12 figures, 7Be fluxes revised, conclusions unchanged</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. D 89, 023524 (2014) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1204.5379">arXiv:1204.5379</a> <span> [<a href="https://arxiv.org/pdf/1204.5379">pdf</a>, <a href="https://arxiv.org/format/1204.5379">other</a>] </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="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Light Sterile Neutrinos: A White Paper </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Abazajian%2C+K+N">K. N. Abazajian</a>, <a href="/search/hep-ph?searchtype=author&query=Acero%2C+M+A">M. A. Acero</a>, <a href="/search/hep-ph?searchtype=author&query=Agarwalla%2C+S+K">S. K. Agarwalla</a>, <a href="/search/hep-ph?searchtype=author&query=Aguilar-Arevalo%2C+A+A">A. A. Aguilar-Arevalo</a>, <a href="/search/hep-ph?searchtype=author&query=Albright%2C+C+H">C. H. Albright</a>, <a href="/search/hep-ph?searchtype=author&query=Antusch%2C+S">S. Antusch</a>, <a href="/search/hep-ph?searchtype=author&query=Arguelles%2C+C+A">C. A. Arguelles</a>, <a href="/search/hep-ph?searchtype=author&query=Balantekin%2C+A+B">A. B. Balantekin</a>, <a href="/search/hep-ph?searchtype=author&query=Barenboim%2C+G">G. Barenboim</a>, <a href="/search/hep-ph?searchtype=author&query=Barger%2C+V">V. Barger</a>, <a href="/search/hep-ph?searchtype=author&query=Bernardini%2C+P">P. Bernardini</a>, <a href="/search/hep-ph?searchtype=author&query=Bezrukov%2C+F">F. Bezrukov</a>, <a href="/search/hep-ph?searchtype=author&query=Bjaelde%2C+O+E">O. E. Bjaelde</a>, <a href="/search/hep-ph?searchtype=author&query=Bogacz%2C+S+A">S. A. Bogacz</a>, <a href="/search/hep-ph?searchtype=author&query=Bowden%2C+N+S">N. S. Bowden</a>, <a href="/search/hep-ph?searchtype=author&query=Boyarsky%2C+A">A. Boyarsky</a>, <a href="/search/hep-ph?searchtype=author&query=Bravar%2C+A">A. Bravar</a>, <a href="/search/hep-ph?searchtype=author&query=Berguno%2C+D+B">D. Bravo Berguno</a>, <a href="/search/hep-ph?searchtype=author&query=Brice%2C+S+J">S. J. Brice</a>, <a href="/search/hep-ph?searchtype=author&query=Bross%2C+A+D">A. D. Bross</a>, <a href="/search/hep-ph?searchtype=author&query=Caccianiga%2C+B">B. Caccianiga</a>, <a href="/search/hep-ph?searchtype=author&query=Cavanna%2C+F">F. Cavanna</a>, <a href="/search/hep-ph?searchtype=author&query=Chun%2C+E+J">E. J. Chun</a>, <a href="/search/hep-ph?searchtype=author&query=Cleveland%2C+B+T">B. T. Cleveland</a>, <a href="/search/hep-ph?searchtype=author&query=Collin%2C+A+P">A. P. Collin</a> , et al. (162 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="1204.5379v1-abstract-short" style="display: inline;"> This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1204.5379v1-abstract-full" style="display: none;"> This white paper addresses the hypothesis of light sterile neutrinos based on recent anomalies observed in neutrino experiments and the latest astrophysical data. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1204.5379v1-abstract-full').style.display = 'none'; document.getElementById('1204.5379v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 April, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2012. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1201.3805">arXiv:1201.3805</a> <span> [<a href="https://arxiv.org/pdf/1201.3805">pdf</a>, <a href="https://arxiv.org/format/1201.3805">other</a>] </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 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/10.1103/PhysRevD.86.013004">10.1103/PhysRevD.86.013004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measuring Active-to-Sterile Neutrino Oscillations with Neutral Current Coherent Neutrino-Nucleus Scattering </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Anderson%2C+A+J">A. J. Anderson</a>, <a href="/search/hep-ph?searchtype=author&query=Conrad%2C+J+M">J. M. Conrad</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a>, <a href="/search/hep-ph?searchtype=author&query=Ignarra%2C+C">C. Ignarra</a>, <a href="/search/hep-ph?searchtype=author&query=Karagiorgi%2C+G">G. Karagiorgi</a>, <a href="/search/hep-ph?searchtype=author&query=Scholberg%2C+K">K. Scholberg</a>, <a href="/search/hep-ph?searchtype=author&query=Shaevitz%2C+M+H">M. H. Shaevitz</a>, <a href="/search/hep-ph?searchtype=author&query=Spitz%2C+J">J. Spitz</a> </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="1201.3805v1-abstract-short" style="display: inline;"> Light sterile neutrinos have been introduced as an explanation for a number of oscillation signals at $螖m^2 \sim 1$ eV$^2$. Neutrino oscillations at relatively short baselines provide a probe of these possible new states. This paper describes an accelerator-based experiment using neutral current coherent neutrino-nucleus scattering to strictly search for active-to-sterile neutrino oscillations. Th… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1201.3805v1-abstract-full').style.display = 'inline'; document.getElementById('1201.3805v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1201.3805v1-abstract-full" style="display: none;"> Light sterile neutrinos have been introduced as an explanation for a number of oscillation signals at $螖m^2 \sim 1$ eV$^2$. Neutrino oscillations at relatively short baselines provide a probe of these possible new states. This paper describes an accelerator-based experiment using neutral current coherent neutrino-nucleus scattering to strictly search for active-to-sterile neutrino oscillations. This experiment could, thus, definitively establish the existence of sterile neutrinos and provide constraints on their mixing parameters. A cyclotron-based proton beam can be directed to multiple targets, producing a low energy pion and muon decay-at-rest neutrino source with variable distance to a single detector. Two types of detectors are considered: a germanium-based detector inspired by the CDMS design and a liquid argon detector inspired by the proposed CLEAR experiment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1201.3805v1-abstract-full').style.display = 'none'; document.getElementById('1201.3805v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 January, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">10 pages, 7 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/1107.3512">arXiv:1107.3512</a> <span> [<a href="https://arxiv.org/pdf/1107.3512">pdf</a>, <a href="https://arxiv.org/ps/1107.3512">ps</a>, <a href="https://arxiv.org/format/1107.3512">other</a>] </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 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/10.1103/PhysRevD.85.013009">10.1103/PhysRevD.85.013009 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Sterile Neutrinos, Coherent Scattering and Oscillometry Measurements with Low-temperature Bolometers </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Formaggio%2C+J+A">Joseph A. Formaggio</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a>, <a href="/search/hep-ph?searchtype=author&query=Anderson%2C+A+J">A. J. Anderson</a> </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="1107.3512v2-abstract-short" style="display: inline;"> Coherent neutrino-nucleon scattering offers a unique approach in the search for physics beyond the Standard Model. When used in conjunction with mono-energetic neutrino sources, the technique can be sensitive to the existence of light sterile neutrinos. The ability to utilize such reactions has been limited in the past due to the extremely low energy threshold (10-50 eV) needed for detection. In t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.3512v2-abstract-full').style.display = 'inline'; document.getElementById('1107.3512v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1107.3512v2-abstract-full" style="display: none;"> Coherent neutrino-nucleon scattering offers a unique approach in the search for physics beyond the Standard Model. When used in conjunction with mono-energetic neutrino sources, the technique can be sensitive to the existence of light sterile neutrinos. The ability to utilize such reactions has been limited in the past due to the extremely low energy threshold (10-50 eV) needed for detection. In this paper, we discuss an optimization of cryogenic solid state bolometers that enables reaching extremely low kinetic energy thresholds. We investigate the sensitivity of an array of such detectors to neutrino oscillations to sterile states. A recent analysis of available reactor data appears to favor the existence of such such a sterile neutrino with a mass splitting of $|螖m_{\rm sterile}|^2 \ge 1.5$ eV$^2$ and mixing strength of $\sin^2{2胃_{\rm sterile}} = 0.17\pm 0.08$ at 95% C.L. An array of such low-threshold detectors would be able to make a definitive statement as to the validity of the interpretation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1107.3512v2-abstract-full').style.display = 'none'; document.getElementById('1107.3512v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 21 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 18 July, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2011. </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">14 pages, 10 figures. Version 2: Temperature dependence on alpha fixed from earlier version</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1103.4894">arXiv:1103.4894</a> <span> [<a href="https://arxiv.org/pdf/1103.4894">pdf</a>, <a href="https://arxiv.org/format/1103.4894">other</a>] </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 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/10.1103/PhysRevD.84.013008">10.1103/PhysRevD.84.013008 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Coherent Neutrino Scattering in Dark Matter Detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Anderson%2C+A+J">A. J. Anderson</a>, <a href="/search/hep-ph?searchtype=author&query=Conrad%2C+J+M">J. M. Conrad</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa-Feliciano%2C+E">E. Figueroa-Feliciano</a>, <a href="/search/hep-ph?searchtype=author&query=Scholberg%2C+K">K. Scholberg</a>, <a href="/search/hep-ph?searchtype=author&query=Spitz%2C+J">J. Spitz</a> </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="1103.4894v2-abstract-short" style="display: inline;"> Coherent elastic neutrino- and WIMP-nucleus interaction signatures are expected to be quite similar. This paper discusses how a next generation ton-scale dark matter detector could discover neutrino-nucleus coherent scattering, a precisely-predicted Standard Model process. A high intensity pion- and muon- decay-at-rest neutrino source recently proposed for oscillation physics at underground labora… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1103.4894v2-abstract-full').style.display = 'inline'; document.getElementById('1103.4894v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1103.4894v2-abstract-full" style="display: none;"> Coherent elastic neutrino- and WIMP-nucleus interaction signatures are expected to be quite similar. This paper discusses how a next generation ton-scale dark matter detector could discover neutrino-nucleus coherent scattering, a precisely-predicted Standard Model process. A high intensity pion- and muon- decay-at-rest neutrino source recently proposed for oscillation physics at underground laboratories would provide the neutrinos for these measurements. In this paper, we calculate raw rates for various target materials commonly used in dark matter detectors and show that discovery of this interaction is possible with a 2 ton$\cdot$year GEODM exposure in an optimistic energy threshold and efficiency scenario. We also study the effects of the neutrino source on WIMP sensitivity and discuss the modulated neutrino signal as a sensitivity/consistency check between different dark matter experiments at DUSEL. Furthermore, we consider the possibility of coherent neutrino physics with a GEODM module placed within tens of meters of the neutrino source. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1103.4894v2-abstract-full').style.display = 'none'; document.getElementById('1103.4894v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 September, 2011; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 March, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2011. </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">8 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.D84:013008,2011 </p> </li> </ol> <div class="is-hidden-tablet">  <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>  </span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary">  <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 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