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</div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2402.01395">arXiv:2402.01395</a> <span> [<a href="https://arxiv.org/pdf/2402.01395">pdf</a>, <a href="https://arxiv.org/format/2402.01395">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"> Dark Matter-Electron Scattering Search Using Cryogenic Light Detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Zema%2C+V">V. Zema</a>, <a href="/search/hep-ph?searchtype=author&query=Figueroa%2C+P">P. Figueroa</a>, <a href="/search/hep-ph?searchtype=author&query=Angloher%2C+G">G. Angloher</a>, <a href="/search/hep-ph?searchtype=author&query=Bharadwaj%2C+M+R">M. R. Bharadwaj</a>, <a href="/search/hep-ph?searchtype=author&query=Frank%2C+T">T. Frank</a>, <a href="/search/hep-ph?searchtype=author&query=Hughes%2C+M+N">M. N. Hughes</a>, <a href="/search/hep-ph?searchtype=author&query=Kellermann%2C+M">M. Kellermann</a>, <a href="/search/hep-ph?searchtype=author&query=Pr%C3%B6bst%2C+F">F. Pr枚bst</a>, <a href="/search/hep-ph?searchtype=author&query=Sch%C3%A4ffner%2C+K">K. Sch盲ffner</a>, <a href="/search/hep-ph?searchtype=author&query=Shera%2C+K">K. Shera</a>, <a href="/search/hep-ph?searchtype=author&query=Stahlberg%2C+M">M. Stahlberg</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="2402.01395v2-abstract-short" style="display: inline;"> The CSC (cryogenic scintillating calorimeter) technology devoted to rare event searches is reaching the sensitivity level required for the hunt of dark matter-electron scatterings. Dark matter-electron interactions in scintillating targets are expected to stimulate the emission of single photons, each of energy equal to the target electronic band gap. The electronic band gap in scintillators like… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2402.01395v2-abstract-full').style.display = 'inline'; document.getElementById('2402.01395v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2402.01395v2-abstract-full" style="display: none;"> The CSC (cryogenic scintillating calorimeter) technology devoted to rare event searches is reaching the sensitivity level required for the hunt of dark matter-electron scatterings. Dark matter-electron interactions in scintillating targets are expected to stimulate the emission of single photons, each of energy equal to the target electronic band gap. The electronic band gap in scintillators like NaI/GaAs is of O(eV). The search for this signal can be done by an array of cryogenic light detectors with eV/sub-eV energy resolution. In this work, we describe the detection principle, the detector response and the envisioned detector design to search for dark matter interacting with electrons via the measurement of the scintillation light at millikelvin. First sensitivity projections are provided, which show the potential of this research. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2402.01395v2-abstract-full').style.display = 'none'; document.getElementById('2402.01395v2-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 October, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 2 February, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 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> [<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/1809.03753">arXiv:1809.03753</a> <span> [<a href="https://arxiv.org/pdf/1809.03753">pdf</a>, <a href="https://arxiv.org/format/1809.03753">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> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-018-6523-4">10.1140/epjc/s10052-018-6523-4 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Limits on Dark Matter Effective Field Theory Parameters with CRESST-II </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=Angloher%2C+G">G. Angloher</a>, <a href="/search/hep-ph?searchtype=author&query=Bauer%2C+P">P. Bauer</a>, <a href="/search/hep-ph?searchtype=author&query=Bento%2C+A">A. Bento</a>, <a href="/search/hep-ph?searchtype=author&query=Bertoldo%2C+E">E. Bertoldo</a>, <a href="/search/hep-ph?searchtype=author&query=Bucci%2C+C">C. Bucci</a>, <a href="/search/hep-ph?searchtype=author&query=Canonica%2C+L">L. Canonica</a>, <a href="/search/hep-ph?searchtype=author&query=D%27Addabbo%2C+A">A. D'Addabbo</a>, <a href="/search/hep-ph?searchtype=author&query=Defay%2C+X">X. Defay</a>, <a href="/search/hep-ph?searchtype=author&query=Di+Lorenzo%2C+S">S. Di Lorenzo</a>, <a href="/search/hep-ph?searchtype=author&query=Erb%2C+A">A. Erb</a>, <a href="/search/hep-ph?searchtype=author&query=Feilitzsch%2C+F+v">F. v. Feilitzsch</a>, <a href="/search/hep-ph?searchtype=author&query=Iachellini%2C+N+F">N. Ferreiro Iachellini</a>, <a href="/search/hep-ph?searchtype=author&query=Gorla%2C+P">P. Gorla</a>, <a href="/search/hep-ph?searchtype=author&query=Hauff%2C+D">D. Hauff</a>, <a href="/search/hep-ph?searchtype=author&query=Jochum%2C+J">J. Jochum</a>, <a href="/search/hep-ph?searchtype=author&query=Kiefer%2C+M">M. Kiefer</a>, <a href="/search/hep-ph?searchtype=author&query=Kluck%2C+H">H. Kluck</a>, <a href="/search/hep-ph?searchtype=author&query=Kraus%2C+H">H. Kraus</a>, <a href="/search/hep-ph?searchtype=author&query=Langenk%C3%A4mper%2C+A">A. Langenk盲mper</a>, <a href="/search/hep-ph?searchtype=author&query=Mancuso%2C+M">M. Mancuso</a>, <a href="/search/hep-ph?searchtype=author&query=Mokina%2C+V">V. Mokina</a>, <a href="/search/hep-ph?searchtype=author&query=Mondragon%2C+E">E. Mondragon</a>, <a href="/search/hep-ph?searchtype=author&query=Morgalyuk%2C+V">V. Morgalyuk</a>, <a href="/search/hep-ph?searchtype=author&query=M%C3%BCnster%2C+A">A. M眉nster</a>, <a href="/search/hep-ph?searchtype=author&query=Olmi%2C+M">M. Olmi</a> , et al. (20 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="1809.03753v1-abstract-short" style="display: inline;"> CRESST is a direct dark matter search experiment, aiming for an observation of nuclear recoils induced by the interaction of dark matter particles with cryogenic scintillating calcium tungstate crystals. Instead of confining ourselves to standard spin-independent and spin-dependent searches, we re-analyze data from CRESST-II using a more general effective field theory (EFT) framework. On many of t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1809.03753v1-abstract-full').style.display = 'inline'; document.getElementById('1809.03753v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1809.03753v1-abstract-full" style="display: none;"> CRESST is a direct dark matter search experiment, aiming for an observation of nuclear recoils induced by the interaction of dark matter particles with cryogenic scintillating calcium tungstate crystals. Instead of confining ourselves to standard spin-independent and spin-dependent searches, we re-analyze data from CRESST-II using a more general effective field theory (EFT) framework. On many of the EFT coupling constants, improved exclusion limits in the low-mass region (< 3-4 GeV) are presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1809.03753v1-abstract-full').style.display = 'none'; document.getElementById('1809.03753v1-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> 11 September, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 9 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/1408.2357">arXiv:1408.2357</a> <span> [<a href="https://arxiv.org/pdf/1408.2357">pdf</a>, <a href="https://arxiv.org/format/1408.2357">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="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/10.1016/j.astropartphys.2015.03.010">10.1016/j.astropartphys.2015.03.010 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Impact of Coherent Neutrino Nucleus Scattering on Direct Dark Matter Searches based on CaWO$_4$ Crystals </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/hep-ph?searchtype=author&query=G%C3%BCtlein%2C+A">A. G眉tlein</a>, <a href="/search/hep-ph?searchtype=author&query=Angloher%2C+G">G. Angloher</a>, <a href="/search/hep-ph?searchtype=author&query=Bento%2C+A">A. Bento</a>, <a href="/search/hep-ph?searchtype=author&query=Bucci%2C+C">C. Bucci</a>, <a href="/search/hep-ph?searchtype=author&query=Canonica%2C+L">L. Canonica</a>, <a href="/search/hep-ph?searchtype=author&query=Erb%2C+A">A. Erb</a>, <a href="/search/hep-ph?searchtype=author&query=Feilitzsch%2C+F+v">F. v. Feilitzsch</a>, <a href="/search/hep-ph?searchtype=author&query=Iachellini%2C+N+F">N. Ferreiro Iachellini</a>, <a href="/search/hep-ph?searchtype=author&query=Gorla%2C+P">P. Gorla</a>, <a href="/search/hep-ph?searchtype=author&query=Hauff%2C+D">D. Hauff</a>, <a href="/search/hep-ph?searchtype=author&query=Jochum%2C+J">J. Jochum</a>, <a href="/search/hep-ph?searchtype=author&query=Kiefer%2C+M">M. Kiefer</a>, <a href="/search/hep-ph?searchtype=author&query=Kluck%2C+H">H. Kluck</a>, <a href="/search/hep-ph?searchtype=author&query=Kraus%2C+H">H. Kraus</a>, <a href="/search/hep-ph?searchtype=author&query=Lanfranchi%2C+J+-">J. -C. Lanfranchi</a>, <a href="/search/hep-ph?searchtype=author&query=Loebell%2C+J">J. Loebell</a>, <a href="/search/hep-ph?searchtype=author&query=M%C3%BCnster%2C+A">A. M眉nster</a>, <a href="/search/hep-ph?searchtype=author&query=Petricca%2C+F">F. Petricca</a>, <a href="/search/hep-ph?searchtype=author&query=Potzel%2C+W">W. Potzel</a>, <a href="/search/hep-ph?searchtype=author&query=Pr%C3%B6bst%2C+F">F. Pr枚bst</a>, <a href="/search/hep-ph?searchtype=author&query=Reindl%2C+F">F. Reindl</a>, <a href="/search/hep-ph?searchtype=author&query=Roth%2C+S">S. Roth</a>, <a href="/search/hep-ph?searchtype=author&query=Rottler%2C+K">K. Rottler</a>, <a href="/search/hep-ph?searchtype=author&query=Sailer%2C+C">C. Sailer</a>, <a href="/search/hep-ph?searchtype=author&query=Sch%C3%A4ffner%2C+K">K. Sch盲ffner</a> , et al. (15 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="1408.2357v2-abstract-short" style="display: inline;"> Atmospheric and solar neutrinos scattering coherently off target nuclei will be an important background source for the next generation of direct dark matter searches. In this work we focus on calcium tungstate as target material. For comparison with existing works we calculate the neutrino floor indicating which sensitivities can be reached before the neutrino background appears. In addition, we i… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1408.2357v2-abstract-full').style.display = 'inline'; document.getElementById('1408.2357v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1408.2357v2-abstract-full" style="display: none;"> Atmospheric and solar neutrinos scattering coherently off target nuclei will be an important background source for the next generation of direct dark matter searches. In this work we focus on calcium tungstate as target material. For comparison with existing works we calculate the neutrino floor indicating which sensitivities can be reached before the neutrino background appears. In addition, we investigate the sensitivities of future direct dark matter searches using CRESST-II like detectors. Extending previous works we take into account achievable energy resolutions and thresholds as well as beta and gamma backgrounds for this investigation. We show that an exploration of WIMP-nucleon cross sections below the neutrino floor is possible for exposures of $\gtrsim10$ kg-years or higher. In the third part we show that a first detection of coherent neutrino nucleus scattering of atmospheric and solar neutrinos using the same detectors and the backgrounds is feasible for exposures of $\gtrsim50$ kg-years. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1408.2357v2-abstract-full').style.display = 'none'; document.getElementById('1408.2357v2-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 March, 2015; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 11 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">submitted to Astorparticle Physics</span> </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 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 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