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href="/search/?searchtype=author&amp;query=Casali%2C+N&amp;start=50" class="pagination-link " aria-label="Page 2" aria-current="page">2 </a> </li> </ul> </nav> <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/2405.17937">arXiv:2405.17937</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2405.17937">pdf</a>, <a href="https://arxiv.org/format/2405.17937">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</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.110.052003">10.1103/PhysRevD.110.052003 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Data-driven background model for the CUORE experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+J">J. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</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="2405.17937v1-abstract-short" style="display: inline;"> We present the model we developed to reconstruct the CUORE radioactive background based on the analysis of an experimental exposure of 1038.4 kg yr. The data reconstruction relies on a simultaneous Bayesian fit applied to energy spectra over a broad energy range. The high granularity of the CUORE detector, together with the large exposure and extended stable operations, allow for an in-depth explo&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.17937v1-abstract-full').style.display = 'inline'; document.getElementById('2405.17937v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2405.17937v1-abstract-full" style="display: none;"> We present the model we developed to reconstruct the CUORE radioactive background based on the analysis of an experimental exposure of 1038.4 kg yr. The data reconstruction relies on a simultaneous Bayesian fit applied to energy spectra over a broad energy range. The high granularity of the CUORE detector, together with the large exposure and extended stable operations, allow for an in-depth exploration of both spatial and time dependence of backgrounds. We achieve high sensitivity to both bulk and surface activities of the materials of the setup, detecting levels as low as 10 nBq kg$^{-1}$ and 0.1 nBq cm$^{-2}$, respectively. We compare the contamination levels we extract from the background model with prior radio-assay data, which informs future background risk mitigation strategies. The results of this background model play a crucial role in constructing the background budget for the CUPID experiment as it will exploit the same CUORE infrastructure. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.17937v1-abstract-full').style.display = 'none'; document.getElementById('2405.17937v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 May, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2405.10766">arXiv:2405.10766</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2405.10766">pdf</a>, <a href="https://arxiv.org/format/2405.10766">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Searching for Beyond the Standard Model physics using the improved description of $^{100}$Mo $2谓尾尾$ decay spectral shape with CUPID-Mo </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dixon%2C+T">T. Dixon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eitel%2C+K">K. Eitel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferri%2C+F">F. Ferri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fujikawa%2C+B+K">B. K. Fujikawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gascon%2C+J">J. Gascon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a> , et al. (58 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2405.10766v2-abstract-short" style="display: inline;"> The current experiments searching for neutrinoless double-$尾$ ($0谓尾尾$) decay also collect large statistics of Standard Model allowed two-neutrino double-$尾$ ($2谓尾尾$) decay events. These can be used to search for Beyond Standard Model (BSM) physics via $2谓尾尾$ decay spectral distortions. $^{100}$Mo has a natural advantage due to its relatively short half-life, allowing higher $2谓尾尾$ decay statistics&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.10766v2-abstract-full').style.display = 'inline'; document.getElementById('2405.10766v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2405.10766v2-abstract-full" style="display: none;"> The current experiments searching for neutrinoless double-$尾$ ($0谓尾尾$) decay also collect large statistics of Standard Model allowed two-neutrino double-$尾$ ($2谓尾尾$) decay events. These can be used to search for Beyond Standard Model (BSM) physics via $2谓尾尾$ decay spectral distortions. $^{100}$Mo has a natural advantage due to its relatively short half-life, allowing higher $2谓尾尾$ decay statistics at equal exposures compared to the other isotopes. We demonstrate the potential of the dual read-out bolometric technique exploiting a $^{100}$Mo exposure of 1.47 kg $\times$ y, acquired in the CUPID-Mo experiment at the Modane underground laboratory (France). We set limits on $0谓尾尾$ decays with the emission of one or more Majorons, on $2谓尾尾$ decay with Lorentz violation, and $2谓尾尾$ decay with a sterile neutrino emission. In this analysis, we investigate the systematic uncertainty induced by modeling the $2谓尾尾$ decay spectral shape parameterized through an improved model, an effect never considered before. This work motivates searches for BSM processes in the upcoming CUPID experiment, which will collect the largest amount of $2谓尾尾$ decay events among the next-generation experiments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.10766v2-abstract-full').style.display = 'none'; document.getElementById('2405.10766v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 August, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 May, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2404.04453">arXiv:2404.04453</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2404.04453">pdf</a>, <a href="https://arxiv.org/format/2404.04453">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> With or without $谓$? Hunting for the seed of the matter-antimatter asymmetry </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+J">J. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</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="2404.04453v1-abstract-short" style="display: inline;"> The matter-antimatter asymmetry underlines the incompleteness of the current understanding of particle physics. Neutrinoless double-beta ($0谓尾尾$) decay may help explain this asymmetry, while unveiling the Majorana nature of the neutrino. The CUORE experiment searches for $0谓尾尾$ decay of $^{130}$Te using a tonne-scale cryogenic calorimeter operated at milli-kelvin temperatures. We report no evidenc&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2404.04453v1-abstract-full').style.display = 'inline'; document.getElementById('2404.04453v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2404.04453v1-abstract-full" style="display: none;"> The matter-antimatter asymmetry underlines the incompleteness of the current understanding of particle physics. Neutrinoless double-beta ($0谓尾尾$) decay may help explain this asymmetry, while unveiling the Majorana nature of the neutrino. The CUORE experiment searches for $0谓尾尾$ decay of $^{130}$Te using a tonne-scale cryogenic calorimeter operated at milli-kelvin temperatures. We report no evidence for $0谓尾尾$ decay and place a lower limit on the half-life of T$_{1/2}$ $&gt;$ 3.8 $\times$ 10$^{25}$ years (90% C.I.) with over 2 tonne$\cdot$year TeO$_2$ exposure. The tools and techniques developed for this result and the 5 year stable operation of nearly 1000 detectors demonstrate the infrastructure for a next-generation experiment capable of searching for $0谓尾尾$ decay across multiple isotopes. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2404.04453v1-abstract-full').style.display = 'none'; document.getElementById('2404.04453v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 April, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2024. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2307.14086">arXiv:2307.14086</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2307.14086">pdf</a>, <a href="https://arxiv.org/format/2307.14086">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> </div> <p class="title is-5 mathjax"> Measurement of the $2谓尾尾$ decay rate and spectral shape of $^{100}$Mo from the CUPID-Mo experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+6+M">6 M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berge%2C+L">L. Berge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dixon%2C+T">T. Dixon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eitel%2C+K">K. Eitel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferri%2C+F">F. Ferri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fujikawa%2C+B+K">B. K. Fujikawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gascon%2C+J">J. Gascon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a> , et al. (59 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="2307.14086v1-abstract-short" style="display: inline;"> Neutrinoless double beta decay ($0谓尾尾$) is a yet unobserved nuclear process which would demonstrate Lepton Number violation, a clear evidence of beyond Standard Model physics. The process two neutrino double beta decay ($2谓尾尾)$ is allowed by the Standard Model and has been measured in numerous experiments. In this letter, we report a measurement of $2谓尾尾$ decay half-life of $^{100}$Mo to the groun&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2307.14086v1-abstract-full').style.display = 'inline'; document.getElementById('2307.14086v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2307.14086v1-abstract-full" style="display: none;"> Neutrinoless double beta decay ($0谓尾尾$) is a yet unobserved nuclear process which would demonstrate Lepton Number violation, a clear evidence of beyond Standard Model physics. The process two neutrino double beta decay ($2谓尾尾)$ is allowed by the Standard Model and has been measured in numerous experiments. In this letter, we report a measurement of $2谓尾尾$ decay half-life of $^{100}$Mo to the ground state of $^{100}$Ru of $(7.07~\pm~0.02~\text{(stat.)}~\pm~0.11~\text{(syst.)})~\times~10^{18}$~yr by the CUPID-Mo experiment. With a relative precision of $\pm~1.6$ \% this is the most precise measurement to date of a $2谓尾尾$ decay rate in $^{100}$Mo. In addition, we constrain higher-order corrections to the spectral shape which provides complementary nuclear structure information. We report a novel measurement of the shape factor $尉_{3,1}=0.45~\pm 0.03~\text{(stat.)} \ \pm 0.05 \ \text{(syst.)}$, which is compared to theoretical predictions for different nuclear models. We also extract the first value for the effective axial vector coupling constant obtained from a spectral shape study of $2谓尾尾$ decay. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2307.14086v1-abstract-full').style.display = 'none'; document.getElementById('2307.14086v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 26 July, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">8 pages, 5 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/2306.14654">arXiv:2306.14654</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2306.14654">pdf</a>, <a href="https://arxiv.org/format/2306.14654">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Measurement of the 2$谓尾尾$ Decay Half-Life of Se-82 with the Global CUPID-0 Background Model </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caracciolo%2C+V">V. Caracciolo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">I. Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Domp%C3%A8%2C+V">V. Domp猫</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fantini%2C+G">G. Fantini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a> , et al. (27 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="2306.14654v2-abstract-short" style="display: inline;"> We report on the results obtained with the global CUPID-0 background model, which combines the data collected in the two measurement campaigns for a total exposure of 8.82~kg$\times$yr of $^{82}$Se. We identify with improved precision the background sources within the 3 MeV energy region, where neutrinoless double $尾$-decay of $^{82}$Se and $^{100}$Mo is expected, making more solid the foundations&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2306.14654v2-abstract-full').style.display = 'inline'; document.getElementById('2306.14654v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2306.14654v2-abstract-full" style="display: none;"> We report on the results obtained with the global CUPID-0 background model, which combines the data collected in the two measurement campaigns for a total exposure of 8.82~kg$\times$yr of $^{82}$Se. We identify with improved precision the background sources within the 3 MeV energy region, where neutrinoless double $尾$-decay of $^{82}$Se and $^{100}$Mo is expected, making more solid the foundations for the background budget of the next-generation CUPID experiment. Relying on the excellent data reconstruction, we measure the two-neutrino double $尾$-decay half-life of $^{82}$Se with unprecedented accuracy: $T_{1/2}^{2谓} = [8.69 \pm 0.05 \textrm{(stat.)}~^{+0.09}_{-0.06} \textrm{(syst.)}] \times 10^{19}~\textrm{yr}$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2306.14654v2-abstract-full').style.display = 'none'; document.getElementById('2306.14654v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 November, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 June, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2304.04674">arXiv:2304.04674</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2304.04674">pdf</a>, <a href="https://arxiv.org/format/2304.04674">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/18/06/P06033">10.1088/1748-0221/18/06/P06033 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A first test of CUPID prototypal light detectors with NTD-Ge sensors in a pulse-tube cryostat </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUPID+collaboration"> CUPID collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armatol%2C+A">A. Armatol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balata%2C+M">M. Balata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barresi%2C+A">A. Barresi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baudin%2C+D">D. Baudin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berest%2C+V">V. Berest</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bettelli%2C+M">M. Bettelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boldrini%2C+V">V. Boldrini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a> , et al. (154 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="2304.04674v1-abstract-short" style="display: inline;"> CUPID is a next-generation bolometric experiment aiming at searching for neutrinoless double-beta decay with ~250 kg of isotopic mass of $^{100}$Mo. It will operate at $\sim$10 mK in a cryostat currently hosting a similar-scale bolometric array for the CUORE experiment at the Gran Sasso National Laboratory (Italy). CUPID will be based on large-volume scintillating bolometers consisting of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.04674v1-abstract-full').style.display = 'inline'; document.getElementById('2304.04674v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2304.04674v1-abstract-full" style="display: none;"> CUPID is a next-generation bolometric experiment aiming at searching for neutrinoless double-beta decay with ~250 kg of isotopic mass of $^{100}$Mo. It will operate at $\sim$10 mK in a cryostat currently hosting a similar-scale bolometric array for the CUORE experiment at the Gran Sasso National Laboratory (Italy). CUPID will be based on large-volume scintillating bolometers consisting of $^{100}$Mo-enriched Li$_2$MoO$_4$ crystals, facing thin Ge-wafer-based bolometric light detectors. In the CUPID design, the detector structure is novel and needs to be validated. In particular, the CUORE cryostat presents a high level of mechanical vibrations due to the use of pulse tubes and the effect of vibrations on the detector performance must be investigated. In this paper we report the first test of the CUPID-design bolometric light detectors with NTD-Ge sensors in a dilution refrigerator equipped with a pulse tube in an above-ground lab. Light detectors are characterized in terms of sensitivity, energy resolution, pulse time constants, and noise power spectrum. Despite the challenging noisy environment due to pulse-tube-induced vibrations, we demonstrate that all the four tested light detectors comply with the CUPID goal in terms of intrinsic energy resolution of 100 eV RMS baseline noise. Indeed, we have measured 70--90 eV RMS for the four devices, which show an excellent reproducibility. We have also obtained outstanding energy resolutions at the 356 keV line from a $^{133}$Ba source with one light detector achieving 0.71(5) keV FWHM, which is -- to our knowledge -- the best ever obtained when compared to $纬$ detectors of any technology in this energy range. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.04674v1-abstract-full').style.display = 'none'; document.getElementById('2304.04674v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 April, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 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">Prepared for submission to JINST; 16 pages, 7 figures, and 1 table</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2304.04611">arXiv:2304.04611</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2304.04611">pdf</a>, <a href="https://arxiv.org/format/2304.04611">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/18/06/P06018">10.1088/1748-0221/18/06/P06018 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Twelve-crystal prototype of Li$_2$MoO$_4$ scintillating bolometers for CUPID and CROSS experiments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUPID"> CUPID</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=collaborations%2C+C">CROSS collaborations</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%3A"> :</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armatol%2C+A">A. Armatol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balata%2C+M">M. Balata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bandac%2C+I+C">I. C. Bandac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barresi%2C+A">A. Barresi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baudin%2C+D">D. Baudin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berest%2C+V">V. Berest</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bettelli%2C+M">M. Bettelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boldrini%2C+V">V. Boldrini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a> , et al. (160 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="2304.04611v1-abstract-short" style="display: inline;"> An array of twelve 0.28 kg lithium molybdate (LMO) low-temperature bolometers equipped with 16 bolometric Ge light detectors, aiming at optimization of detector structure for CROSS and CUPID double-beta decay experiments, was constructed and tested in a low-background pulse-tube-based cryostat at the Canfranc underground laboratory in Spain. Performance of the scintillating bolometers was studied&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.04611v1-abstract-full').style.display = 'inline'; document.getElementById('2304.04611v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2304.04611v1-abstract-full" style="display: none;"> An array of twelve 0.28 kg lithium molybdate (LMO) low-temperature bolometers equipped with 16 bolometric Ge light detectors, aiming at optimization of detector structure for CROSS and CUPID double-beta decay experiments, was constructed and tested in a low-background pulse-tube-based cryostat at the Canfranc underground laboratory in Spain. Performance of the scintillating bolometers was studied depending on the size of phonon NTD-Ge sensors glued to both LMO and Ge absorbers, shape of the Ge light detectors (circular vs. square, from two suppliers), in different light collection conditions (with and without reflector, with aluminum coated LMO crystal surface). The scintillating bolometer array was operated over 8 months in the low-background conditions that allowed to probe a very low, $渭$Bq/kg, level of the LMO crystals radioactive contamination by $^{228}$Th and $^{226}$Ra. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.04611v1-abstract-full').style.display = 'none'; document.getElementById('2304.04611v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 April, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 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">Prepared for submission to JINST; 23 pages, 9 figures, and 4 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/2211.03631">arXiv:2211.03631</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2211.03631">pdf</a>, <a href="https://arxiv.org/format/2211.03631">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="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.130.211802">10.1103/PhysRevLett.130.211802 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Observation of a nuclear recoil peak at the 100 eV scale induced by neutron capture </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CRAB+Collaboration"> CRAB Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=NUCLEUS+Collaboration"> NUCLEUS Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Abele%2C+H">H. Abele</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Angloher%2C+G">G. Angloher</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bento%2C+A">A. Bento</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappella%2C+F">F. Cappella</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cerulli%2C+R">R. Cerulli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chalil%2C+A">A. Chalil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chebboubi%2C+A">A. Chebboubi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">I. Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Crocombette%2C+J+-">J. -P. Crocombette</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Del+Castello%2C+G">G. Del Castello</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Roccagiovine%2C+M+d+G">M. del Gallo Roccagiovine</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Desforge%2C+D">D. Desforge</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Doblhammer%2C+A">A. Doblhammer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumonteil%2C+E">E. Dumonteil</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dorer%2C+S">S. Dorer</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Erhart%2C+A">A. Erhart</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fuss%2C+A">A. Fuss</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Friedl%2C+M">M. Friedl</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Garai%2C+A">A. Garai</a> , et al. (53 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="2211.03631v2-abstract-short" style="display: inline;"> Coherent elastic neutrino-nucleus scattering and low-mass Dark Matter detectors rely crucially on the understanding of their response to nuclear recoils. We report the first observation of a nuclear recoil peak at around 112 eV induced by neutron capture. The measurement was performed with a CaWO$_4$ cryogenic detector from the NUCLEUS experiment exposed to a $^{252}$Cf source placed in a compact&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2211.03631v2-abstract-full').style.display = 'inline'; document.getElementById('2211.03631v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2211.03631v2-abstract-full" style="display: none;"> Coherent elastic neutrino-nucleus scattering and low-mass Dark Matter detectors rely crucially on the understanding of their response to nuclear recoils. We report the first observation of a nuclear recoil peak at around 112 eV induced by neutron capture. The measurement was performed with a CaWO$_4$ cryogenic detector from the NUCLEUS experiment exposed to a $^{252}$Cf source placed in a compact moderator. The measured spectrum is found in agreement with simulations and the expected peak structure from the single-$纬$ de-excitation of $^{183}$W is identified with 3 $蟽$ significance. This result demonstrates a new method for precise, in-situ, and non-intrusive calibration of low-threshold experiments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2211.03631v2-abstract-full').style.display = 'none'; document.getElementById('2211.03631v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 June, 2023; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 7 November, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 130, 211802 (2023) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2209.09490">arXiv:2209.09490</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2209.09490">pdf</a>, <a href="https://arxiv.org/format/2209.09490">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.107.032006">10.1103/PhysRevD.107.032006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Majoron-like particles with CUPID-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Collaboration%2C+C">CUPID-0 Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%3A"> :</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caracciolo%2C+V">V. Caracciolo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">I. Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Domp%C3%A8%2C+V">V. Domp猫</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fantini%2C+G">G. Fantini</a> , et al. (29 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="2209.09490v1-abstract-short" style="display: inline;"> We present the first search for the Majoron-emitting modes of the neutrinoless double $尾$ decay ($0谓尾尾蠂_0$) using scintillating cryogenic calorimeters. We analysed the CUPID-0 Phase I data using a Bayesian approach to reconstruct the background sources activities, and evaluate the potential contribution of the $^{82}$Se $0谓尾尾蠂_0$. We considered several possible theoretical models which predict the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2209.09490v1-abstract-full').style.display = 'inline'; document.getElementById('2209.09490v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2209.09490v1-abstract-full" style="display: none;"> We present the first search for the Majoron-emitting modes of the neutrinoless double $尾$ decay ($0谓尾尾蠂_0$) using scintillating cryogenic calorimeters. We analysed the CUPID-0 Phase I data using a Bayesian approach to reconstruct the background sources activities, and evaluate the potential contribution of the $^{82}$Se $0谓尾尾蠂_0$. We considered several possible theoretical models which predict the existence of a Majoron-like boson coupling to the neutrino. The energy spectra arising from the emission of such bosons in the neutrinoless double $尾$ decay have spectral indices $n=$ 1, 2, 3 or 7. We found no evidence of any of these decay modes, setting a lower limit (90% of credibility interval) on the half-life of 1.2 $\times$ 10$^{23}$ yr in the case of $n=$ 1, 3.8 $\times$ 10$^{22}$ yr for $n=$ 2, 1.4 $\times$ 10$^{22}$ yr for $n=$ 3 and 2.2 $\times$ 10$^{21}$ yr for $n=$ 7. These are the best limits on the $0谓尾尾蠂_0$ half-life of the $^{82}$Se, and demonstrate the potentiality of the CUPID-0 technology in this field. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2209.09490v1-abstract-full').style.display = 'none'; document.getElementById('2209.09490v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 September, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2207.09577">arXiv:2207.09577</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2207.09577">pdf</a>, <a href="https://arxiv.org/format/2207.09577">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> New measurement of double beta decays of $^{100}$Mo to excited states of $^{100}$Ru with the CUPID-Mo experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Collaboration%2C+C">CUPID-Mo Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%3A"> :</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dixon%2C+T">T. Dixon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eitel%2C+K">K. Eitel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferri%2C+F">F. Ferri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fujikawa%2C+B+K">B. K. Fujikawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gascon%2C+J">J. Gascon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a> , et al. (58 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="2207.09577v1-abstract-short" style="display: inline;"> The CUPID-Mo experiment, located at Laboratoire Souterrain de Modane (France), was a demonstrator experiment for CUPID. It consisted of an array of 20 Li$_2^{100}$MoO$_4$ (LMO) calorimeters each equipped with a Ge light detector (LD) for particle identification. In this work, we present the result of a search for two-neutrino and neutrinoless double beta decays of $^{100}$Mo to the first 0$^+$ and&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2207.09577v1-abstract-full').style.display = 'inline'; document.getElementById('2207.09577v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2207.09577v1-abstract-full" style="display: none;"> The CUPID-Mo experiment, located at Laboratoire Souterrain de Modane (France), was a demonstrator experiment for CUPID. It consisted of an array of 20 Li$_2^{100}$MoO$_4$ (LMO) calorimeters each equipped with a Ge light detector (LD) for particle identification. In this work, we present the result of a search for two-neutrino and neutrinoless double beta decays of $^{100}$Mo to the first 0$^+$ and $2^+$ excited states of $^{100}$Ru using the full CUPID-Mo exposure (2.71 kg$\times$yr of LMO). We measure the half-life of $2谓尾尾$ decay to the $0^{+}_1$ state as $T_{1/2}^{2谓\rightarrow 0_1^+}=7.5\pm 0.8 \ \text{(stat.)} \ ^{+ 0.4}_{-0.3} \ \text{(syst.)} )\times 10^{20} \ \mathrm{yr}$. The bolometric technique enables measurement of the electron energies as well as the gamma rays from nuclear de-excitation and this allows us to set new limits on the two-neutrino decay to the $2_1^+$ state of $T^{2谓\rightarrow 2_1^+}_{1/2}&gt;4.4\times 10^{21} \ \mathrm{yr} \ \text{(90 % c.i.)}$ and on the neutrinoless modes of $T_{1/2}^{0谓\rightarrow 2_1^+}&gt;2.1\times10^{23} \ \mathrm{yr}\ \text{(90 % c.i.)}$, $T_{1/2}^{0谓\rightarrow 0_1^+}&gt;1.2\times10^{23} \ \mathrm{yr}\ \text{(90 % c.i.)}$. Information on the electrons spectral shape is obtained which allows us to make the first comparison of the single state (SSD) and higher state (HSD) $2谓尾尾$ decay models for the $0_1^+$ excited state of $^{100}$Ru. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2207.09577v1-abstract-full').style.display = 'none'; document.getElementById('2207.09577v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 July, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">22 pages, 15 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/2206.05130">arXiv:2206.05130</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2206.05130">pdf</a>, <a href="https://arxiv.org/format/2206.05130">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.129.111801">10.1103/PhysRevLett.129.111801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Final Result on the Neutrinoless Double Beta Decay of $^{82}$Se with CUPID-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caracciolo%2C+V">V. Caracciolo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">I. Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Dominics%2C+F">F. De Dominics</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a> , et al. (23 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2206.05130v1-abstract-short" style="display: inline;"> CUPID-0, an array of Zn$^{82}$Se cryogenic calorimeters, was the first medium-scale demonstrator of the scintillating bolometers technology. The first project phase (March 2017 - December 2018) allowed the most stringent limit on the neutrinoless double beta decay half-life of the isotope of interest, $^{82}$Se, to be set. After a six months long detector upgrade, CUPID-0 began its second and last&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2206.05130v1-abstract-full').style.display = 'inline'; document.getElementById('2206.05130v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2206.05130v1-abstract-full" style="display: none;"> CUPID-0, an array of Zn$^{82}$Se cryogenic calorimeters, was the first medium-scale demonstrator of the scintillating bolometers technology. The first project phase (March 2017 - December 2018) allowed the most stringent limit on the neutrinoless double beta decay half-life of the isotope of interest, $^{82}$Se, to be set. After a six months long detector upgrade, CUPID-0 began its second and last phase (June 2019 - February 2020). In this letter, we describe the search for neutrinoless double beta decay of $^{82}$Se with a total exposure (phase I + II) of 8.82 kg$\times$yr of isotope. We set a limit on the half-life of $^{82}$Se to the ground state of $^{82}$Kr of T$^{0谓}_{1/2}$($^{82}$Se)$&gt;$ 4.6$\times \mathrm{10}^{24}$ yr (90\% credible interval), corresponding to an effective Majorana neutrino mass m$_{尾尾} &lt;$ (263 -- 545) meV. We also set the most stringent lower limits on the neutrinoless decays of $^{82}$Se to the 0$_1^+$, 2$_1^+$ and 2$_2^+$ excited states of $^{82}$Kr, finding 1.8$\times$10$^{23}$ yr, 3.0$\times$10$^{23}$ yr, 3.2$\times$10$^{23}$ yr (90$\%$ credible interval) respectively. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2206.05130v1-abstract-full').style.display = 'none'; document.getElementById('2206.05130v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 June, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2205.04549">arXiv:2205.04549</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2205.04549">pdf</a>, <a href="https://arxiv.org/format/2205.04549">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> An Energy-dependent Electro-thermal Response Model of CUORE Cryogenic Calorimeter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a> , et al. (96 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="2205.04549v2-abstract-short" style="display: inline;"> The Cryogenic Underground Observatory for Rare Events (CUORE) is the most sensitive experiment searching for neutrinoless double-beta decay ($0谓尾尾$) in $^{130}\text{Te}$. CUORE uses a cryogenic array of 988 TeO$_2$ calorimeters operated at $\sim$10 mK with a total mass of 741 kg. To further increase the sensitivity, the detector response must be well understood. Here, we present a non-linear therm&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2205.04549v2-abstract-full').style.display = 'inline'; document.getElementById('2205.04549v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2205.04549v2-abstract-full" style="display: none;"> The Cryogenic Underground Observatory for Rare Events (CUORE) is the most sensitive experiment searching for neutrinoless double-beta decay ($0谓尾尾$) in $^{130}\text{Te}$. CUORE uses a cryogenic array of 988 TeO$_2$ calorimeters operated at $\sim$10 mK with a total mass of 741 kg. To further increase the sensitivity, the detector response must be well understood. Here, we present a non-linear thermal model for the CUORE experiment on a detector-by-detector basis. We have examined both equilibrium and dynamic electro-thermal models of detectors by numerically fitting non-linear differential equations to the detector data of a subset of CUORE channels which are well characterized and representative of all channels. We demonstrate that the hot-electron effect and electric-field dependence of resistance in NTD-Ge thermistors alone are inadequate to describe our detectors&#39; energy dependent pulse shapes. We introduce an empirical second-order correction factor in the exponential temperature dependence of the thermistor, which produces excellent agreement with energy-dependent pulse shape data up to 6 MeV. We also present a noise analysis using the fitted thermal parameters and show that the intrinsic thermal noise is negligible compared to the observed noise for our detectors. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2205.04549v2-abstract-full').style.display = 'none'; document.getElementById('2205.04549v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 28 July, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 9 May, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 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">34 pages, 14 figures, 6 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/2205.03132">arXiv:2205.03132</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2205.03132">pdf</a>, <a href="https://arxiv.org/format/2205.03132">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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.129.222501">10.1103/PhysRevLett.129.222501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> New direct limit on neutrinoless double beta decay half-life of $^{128}$Te with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a> , et al. (95 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="2205.03132v1-abstract-short" style="display: inline;"> The Cryogenic Underground Observatory for Rare Events (CUORE) at Laboratori Nazionali del Gran Sasso of INFN in Italy is an experiment searching for neutrinoless double beta (0$谓尾尾$) decay. Its main goal is to investigate this decay in $^{130}$Te, but its ton-scale mass and low background make CUORE sensitive to other rare processes as well. In this work, we present our first results on the search&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2205.03132v1-abstract-full').style.display = 'inline'; document.getElementById('2205.03132v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2205.03132v1-abstract-full" style="display: none;"> The Cryogenic Underground Observatory for Rare Events (CUORE) at Laboratori Nazionali del Gran Sasso of INFN in Italy is an experiment searching for neutrinoless double beta (0$谓尾尾$) decay. Its main goal is to investigate this decay in $^{130}$Te, but its ton-scale mass and low background make CUORE sensitive to other rare processes as well. In this work, we present our first results on the search for \nbb decay of $^{128}$Te, the Te isotope with the second highest natural isotopic abundance. We find no evidence for this decay, and using a Bayesian analysis we set a lower limit on the $^{128}$Te \nbb decay half-life of T$_{1/2} &gt; 3.6 \times 10^{24}$ yr (90\% CI). This represents the most stringent limit on the half-life of this isotope, improving by over a factor 30 the previous direct search results, and exceeding those from geochemical experiments for the first time. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2205.03132v1-abstract-full').style.display = 'none'; document.getElementById('2205.03132v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 May, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2203.08684">arXiv:2203.08684</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2203.08684">pdf</a>, <a href="https://arxiv.org/format/2203.08684">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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/PhysRevC.105.065504">10.1103/PhysRevC.105.065504 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Neutrinoless $尾^+EC$ Decay of $^{120}$Te with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a> , et al. (96 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="2203.08684v2-abstract-short" style="display: inline;"> CUORE is a large scale cryogenic experiment searching for neutrinoless double beta decay ($0谓尾尾$) in $^{130}$Te. The CUORE detector is made of natural tellurium, providing the possibility of rare event searches on isotopes other than $^{130}$Te. In this work we describe a search for neutrinoless positron emitting electron capture ($0谓尾^+EC$) decay in $^{120}$Te with a total TeO$_2$ exposure of 355&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.08684v2-abstract-full').style.display = 'inline'; document.getElementById('2203.08684v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2203.08684v2-abstract-full" style="display: none;"> CUORE is a large scale cryogenic experiment searching for neutrinoless double beta decay ($0谓尾尾$) in $^{130}$Te. The CUORE detector is made of natural tellurium, providing the possibility of rare event searches on isotopes other than $^{130}$Te. In this work we describe a search for neutrinoless positron emitting electron capture ($0谓尾^+EC$) decay in $^{120}$Te with a total TeO$_2$ exposure of 355.7 kg $\cdot$ yr, corresponding to 0.2405 kg $\cdot$ yr of $^{120}$Te. Albeit $0 谓尾尾$ with two final state electrons represents the most promising channel, the emission of a positron and two 511-keV $纬$s make $0谓尾^+EC$ decay signature extremely clear. To fully exploit the potential offered by the detector modularity we include events with different topology and perform a simultaneous fit of five selected signal signatures. Using blinded data we extract a median exclusion sensitivity of $3.4 \cdot 10^{22}$ yr at 90% Credibility Interval (C.I.). After unblinding we find no evidence of $0谓尾^+EC$ signal and set a 90% C.I. Bayesian lower limit of $2.9 \cdot 10^{22}$ yr on $^{120}$Te half-life. This result improves by an order of magnitude the existing limit from the combined analysis of CUORE-0 and Cuoricino. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.08684v2-abstract-full').style.display = 'none'; document.getElementById('2203.08684v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 July, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 16 March, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2203.08386">arXiv:2203.08386</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2203.08386">pdf</a>, <a href="https://arxiv.org/format/2203.08386">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Toward CUPID-1T </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Armatol%2C+A">A. Armatol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balata%2C+M">M. Balata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ballen%2C+K">K. Ballen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barresi%2C+A">A. Barresi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baudin%2C+D">D. Baudin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bettelli%2C+M">M. Bettelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boldrini%2C+V">V. Boldrini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a> , et al. (150 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="2203.08386v2-abstract-short" style="display: inline;"> Current experiments to search for broken lepton-number symmetry through the observation of neutrinoless double-beta decay ($0\mathrm{谓尾尾}$) provide the most stringent limits on the Majorana nature of neutrinos and the effective Majorana neutrino mass ($m_{尾尾}$). The next-generation experiments will focus on the sensitivity to the $0\mathrm{谓尾尾}$ half-life of $\mathcal{O}(10^{27}$--$10^{28}$~years&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.08386v2-abstract-full').style.display = 'inline'; document.getElementById('2203.08386v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2203.08386v2-abstract-full" style="display: none;"> Current experiments to search for broken lepton-number symmetry through the observation of neutrinoless double-beta decay ($0\mathrm{谓尾尾}$) provide the most stringent limits on the Majorana nature of neutrinos and the effective Majorana neutrino mass ($m_{尾尾}$). The next-generation experiments will focus on the sensitivity to the $0\mathrm{谓尾尾}$ half-life of $\mathcal{O}(10^{27}$--$10^{28}$~years$)$ and $m_{尾尾}\lesssim15$~meV, which would provide complete coverage of the so-called Inverted Ordering region of the neutrino mass parameter space. By taking advantage of recent technological breakthroughs, new, future calorimetric experiments at the 1-ton scale can increase the sensitivity by at least another order of magnitude, exploring the large fraction of the parameter space that corresponds to the Normal neutrino mass ordering. In case of a discovery, such experiments could provide important insights toward a new understanding of the mechanism of $0\mathrm{谓尾尾}$. We present here a series of projects underway that will provide advancements in background reduction, cryogenic readout, and physics searches beyond $0\mathrm{谓尾尾}$, all moving toward the next-to-next generation CUPID-1T detector. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2203.08386v2-abstract-full').style.display = 'none'; document.getElementById('2203.08386v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 April, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 16 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 Snowmass 2021</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2202.08716">arXiv:2202.08716</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2202.08716">pdf</a>, <a href="https://arxiv.org/format/2202.08716">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-022-10942-5">10.1140/epjc/s10052-022-10942-5 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Final results on the $0谓尾尾$ decay half-life limit of $^{100}$Mo from the CUPID-Mo experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Marcillac%2C+P">P. de Marcillac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dixon%2C+T">T. Dixon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eitel%2C+K">K. Eitel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferri%2C+F">F. Ferri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Fujikawa%2C+B+K">B. K. Fujikawa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gascon%2C+J">J. Gascon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a> , et al. (54 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="2202.08716v2-abstract-short" style="display: inline;"> The CUPID-Mo experiment to search for 0$谓尾尾$ decay in $^{100}$Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0$谓尾尾$ decay experiment. CUPID-Mo was comprised of 20 enriched Li$_2$$^{100}$MoO$_4$ scintillating calorimeters, each with a mass of $\sim$ 0.2 kg, operated at $\sim$20&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.08716v2-abstract-full').style.display = 'inline'; document.getElementById('2202.08716v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2202.08716v2-abstract-full" style="display: none;"> The CUPID-Mo experiment to search for 0$谓尾尾$ decay in $^{100}$Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0$谓尾尾$ decay experiment. CUPID-Mo was comprised of 20 enriched Li$_2$$^{100}$MoO$_4$ scintillating calorimeters, each with a mass of $\sim$ 0.2 kg, operated at $\sim$20 mK. We present here the final analysis with the full exposure of CUPID-Mo ($^{100}$Mo exposure of 1.47 kg$\times$yr) used to search for lepton number violation via 0$谓尾尾$ decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the $^{100}$Mo 0$谓尾尾$ decay half-life of $T^{0谓}_{1/2} &gt; 1.8 \times 10^{24}$ year (stat.+syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of $\left&lt;m_{尾尾}\right&gt; &lt; (0.28$--$0.49)$ eV, dependent upon the nuclear matrix element utilized. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.08716v2-abstract-full').style.display = 'none'; document.getElementById('2202.08716v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 December, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 February, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2022. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C 82, 1033 (2022) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2202.06279">arXiv:2202.06279</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2202.06279">pdf</a>, <a href="https://arxiv.org/format/2202.06279">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Optimization of the first CUPID detector module </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUPID+collaboration"> CUPID collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armatol%2C+A">A. Armatol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balata%2C+M">M. Balata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ballen%2C+K">K. Ballen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barresi%2C+A">A. Barresi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baudin%2C+D">D. Baudin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bettelli%2C+M">M. Bettelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boldrini%2C+V">V. Boldrini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+C">C. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a> , et al. (153 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="2202.06279v1-abstract-short" style="display: inline;"> CUPID will be a next generation experiment searching for the neutrinoless double $尾$ decay, whose discovery would establish the Majorana nature of the neutrino. Based on the experience achieved with the CUORE experiment, presently taking data at LNGS, CUPID aims to reach a background free environment by means of scintillating Li$_{2}$$^{100}$MoO$_4$ crystals coupled to light detectors. Indeed, the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.06279v1-abstract-full').style.display = 'inline'; document.getElementById('2202.06279v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2202.06279v1-abstract-full" style="display: none;"> CUPID will be a next generation experiment searching for the neutrinoless double $尾$ decay, whose discovery would establish the Majorana nature of the neutrino. Based on the experience achieved with the CUORE experiment, presently taking data at LNGS, CUPID aims to reach a background free environment by means of scintillating Li$_{2}$$^{100}$MoO$_4$ crystals coupled to light detectors. Indeed, the simultaneous heat and light detection allows us to reject the dominant background of $伪$ particles, as proven by the CUPID-0 and CUPID-Mo demonstrators. In this work we present the results of the first test of the CUPID baseline module. In particular, we propose a new optimized detector structure and light sensors design to enhance the engineering and the light collection, respectively. We characterized the heat detectors, achieving an energy resolution of (5.9 $\pm$ 0.2) keV FWHM at the $Q$-value of $^{100}$Mo (about 3034 keV). We studied the light collection of the baseline CUPID design with respect to an alternative configuration which features gravity-assisted light detectors&#39; mounting. In both cases we obtained an improvement in the light collection with respect to past measures and we validated the particle identification capability of the detector, which ensures an $伪$ particle rejection higher than 99.9%, fully satisfying the requirements for CUPID. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2202.06279v1-abstract-full').style.display = 'none'; document.getElementById('2202.06279v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 February, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 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">10 pages, 5 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/2108.07883">arXiv:2108.07883</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2108.07883">pdf</a>, <a href="https://arxiv.org/format/2108.07883">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-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/10.1016/j.ppnp.2021.103902">10.1016/j.ppnp.2021.103902 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> CUORE Opens the Door to Tonne-scale Cryogenics Experiments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alessandria%2C+F">F. Alessandria</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andreotti%2C+E">E. Andreotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Balata%2C+M">M. Balata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bandac%2C+I">I. Bandac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Banks%2C+T+I">T. I. Banks</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barucci%2C+M">M. Barucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biare%2C+D">D. Biare</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bragazzi%2C+F">F. Bragazzi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bryant%2C+A">A. Bryant</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Buccheri%2C+A">A. Buccheri</a> , et al. (184 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="2108.07883v2-abstract-short" style="display: inline;"> The past few decades have seen major developments in the design and operation of cryogenic particle detectors. This technology offers an extremely good energy resolution - comparable to semiconductor detectors - and a wide choice of target materials, making low temperature calorimetric detectors ideal for a variety of particle physics applications. Rare event searches have continued to require eve&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2108.07883v2-abstract-full').style.display = 'inline'; document.getElementById('2108.07883v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2108.07883v2-abstract-full" style="display: none;"> The past few decades have seen major developments in the design and operation of cryogenic particle detectors. This technology offers an extremely good energy resolution - comparable to semiconductor detectors - and a wide choice of target materials, making low temperature calorimetric detectors ideal for a variety of particle physics applications. Rare event searches have continued to require ever greater exposures, which has driven them to ever larger cryogenic detectors, with the CUORE experiment being the first to reach a tonne-scale, mK-cooled, experimental mass. CUORE, designed to search for neutrinoless double beta decay, has been operational since 2017 at a temperature of about 10 mK. This result has been attained by the use of an unprecedentedly large cryogenic infrastructure called the CUORE cryostat: conceived, designed and commissioned for this purpose. In this article the main characteristics and features of the cryogenic facility developed for the CUORE experiment are highlighted. A brief introduction of the evolution of the field and of the past cryogenic facilities are given. The motivation behind the design and development of the CUORE cryogenic facility is detailed as are the steps taken toward realization, commissioning, and operation of the CUORE cryostat. The major challenges overcome by the collaboration and the solutions implemented throughout the building of the cryogenic facility will be discussed along with the potential improvements for future facilities. The success of CUORE has opened the door to a new generation of large-scale cryogenic facilities in numerous fields of science. Broader implications of the incredible feat achieved by the CUORE collaboration on the future cryogenic facilities in various fields ranging from neutrino and dark matter experiments to quantum computing will be examined. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2108.07883v2-abstract-full').style.display = 'none'; document.getElementById('2108.07883v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 December, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 17 August, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2021. </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">45 pages, 14 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Prog. Part. Nucl. Phys., 122 (2021), Article 103902 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2105.04409">arXiv:2105.04409</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2105.04409">pdf</a>, <a href="https://arxiv.org/format/2105.04409">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-021-09476-z">10.1140/epjc/s10052-021-09476-z <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Background identification in cryogenic calorimeters through $伪-伪$ delayed coincidences </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M. Martinez</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="2105.04409v2-abstract-short" style="display: inline;"> Localization and modeling of radioactive contaminations is a challenge that ultra-low background experiments are constantly facing. These are fundamental steps both to extract scientific results and to further reduce the background of the detectors. Here we present an innovative technique based on the analysis of $伪-伪$ delayed coincidences in $^{232}$Th and $^{238}$U decay chains, developed to inv&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.04409v2-abstract-full').style.display = 'inline'; document.getElementById('2105.04409v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2105.04409v2-abstract-full" style="display: none;"> Localization and modeling of radioactive contaminations is a challenge that ultra-low background experiments are constantly facing. These are fundamental steps both to extract scientific results and to further reduce the background of the detectors. Here we present an innovative technique based on the analysis of $伪-伪$ delayed coincidences in $^{232}$Th and $^{238}$U decay chains, developed to investigate the contaminations of the ZnSe crystals in the CUPID-0 experiment. This method allows to disentangle surface and bulk contaminations of the detectors relying on the different probability to tag delayed coincidences as function of the $伪$ decay position. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.04409v2-abstract-full').style.display = 'none'; document.getElementById('2105.04409v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 13 August, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 7 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C 81, 722 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2105.03329">arXiv:2105.03329</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2105.03329">pdf</a>, <a href="https://arxiv.org/format/2105.03329">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="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.physletb.2021.136642">10.1016/j.physletb.2021.136642 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of $^{216}$Po half-life with the CUPID-0 experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caracciolo%2C+V">V. Caracciolo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">I. Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a> , et al. (22 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="2105.03329v2-abstract-short" style="display: inline;"> Rare event physics demands very detailed background control, high-performance detectors, and custom analysis strategies. Cryogenic calorimeters combine all these ingredients very effectively, representing a promising tool for next-generation experiments. CUPID-0 is one of the most advanced examples of such a technique, having demonstrated its potential with several results obtained with limited ex&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.03329v2-abstract-full').style.display = 'inline'; document.getElementById('2105.03329v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2105.03329v2-abstract-full" style="display: none;"> Rare event physics demands very detailed background control, high-performance detectors, and custom analysis strategies. Cryogenic calorimeters combine all these ingredients very effectively, representing a promising tool for next-generation experiments. CUPID-0 is one of the most advanced examples of such a technique, having demonstrated its potential with several results obtained with limited exposure. In this paper, we present a further application. Exploiting the analysis of delayed coincidence, we can identify the signals caused by the $^{220}$Rn-$^{216}$Po decay sequence on an event-by-event basis. The analysis of these events allows us to extract the time differences between the two decays, leading to a new evaluation of $^{216}$ half-life, estimated as (143.3 $\pm$ 2.8) ms. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2105.03329v2-abstract-full').style.display = 'none'; document.getElementById('2105.03329v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 7 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2021. </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">5 pages, 2 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/2104.06906">arXiv:2104.06906</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2104.06906">pdf</a>, <a href="https://arxiv.org/format/2104.06906">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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/10.1038/s41586-022-04497-4">10.1038/s41586-022-04497-4 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Majorana neutrinos exploiting millikelvin cryogenics with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a> , et al. (89 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="2104.06906v2-abstract-short" style="display: inline;"> The possibility that neutrinos may be their own antiparticles, unique among the known fundamental particles, arises from the symmetric theory of fermions proposed by Ettore Majorana in 1937. Given the profound consequences of such Majorana neutrinos, among which is a potential explanation for the matter-antimatter asymmetry of the universe via leptogenesis, the Majorana nature of neutrinos command&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2104.06906v2-abstract-full').style.display = 'inline'; document.getElementById('2104.06906v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2104.06906v2-abstract-full" style="display: none;"> The possibility that neutrinos may be their own antiparticles, unique among the known fundamental particles, arises from the symmetric theory of fermions proposed by Ettore Majorana in 1937. Given the profound consequences of such Majorana neutrinos, among which is a potential explanation for the matter-antimatter asymmetry of the universe via leptogenesis, the Majorana nature of neutrinos commands intense experimental scrutiny globally; one of the primary experimental probes is neutrinoless double beta ($0 谓尾尾$) decay. Here we show results from the search for $0 谓尾尾$ decay of $^{130}$Te, using the latest advanced cryogenic calorimeters with the CUORE experiment. CUORE, operating just 10 millikelvin above absolute zero, has pushed the state of the art on three frontiers: the sheer mass held at such ultra-low temperatures, operational longevity, and the low levels of ionising radiation emanating from the cryogenic infrastructure. We find no evidence for $0 谓尾尾$ decay and set a lower bound of $T_{1/2}^{0 谓} &gt; 2.2 \times 10^{25}$ years at a 90% credibility interval. We discuss potential applications of the advances made with CUORE to other fields such as direct dark matter, neutrino and nuclear physics searches and large-scale quantum computing, which can benefit from sustained operation of large payloads in a low-radioactivity, ultra-low temperature cryogenic environment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2104.06906v2-abstract-full').style.display = 'none'; document.getElementById('2104.06906v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 April, 2022; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 14 April, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nature 604, 53 (2022) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2104.06850">arXiv:2104.06850</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2104.06850">pdf</a>, <a href="https://arxiv.org/format/2104.06850">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-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/10.1140/epjc/s10052-021-09454-5">10.1140/epjc/s10052-021-09454-5 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Final results of CALDER: Kinetic inductance light detectors to search for rare events </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">Laura Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">Nicola Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">Ivan Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">Angelo Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">Sergio Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">Maria Martinez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pettinacci%2C+V">Valerio Pettinacci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pettinari%2C+G">Giorgio Pettinari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vignati%2C+M">Marco Vignati</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="2104.06850v1-abstract-short" style="display: inline;"> The next generation of bolometric experiments searching for rave events, in particular for the neutrino-less double beta decay, needs fast, high-sensitivity and easy-to-scale cryogenic light detectors. The CALDER project (2014-2020) developed a new technology for light detection at cryogenic temperature. In this paper we describe the achievements and the final prototype of this project, consisting&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2104.06850v1-abstract-full').style.display = 'inline'; document.getElementById('2104.06850v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2104.06850v1-abstract-full" style="display: none;"> The next generation of bolometric experiments searching for rave events, in particular for the neutrino-less double beta decay, needs fast, high-sensitivity and easy-to-scale cryogenic light detectors. The CALDER project (2014-2020) developed a new technology for light detection at cryogenic temperature. In this paper we describe the achievements and the final prototype of this project, consisting of a $5\times5$ cm$^2$, 650 $渭$m thick silicon substrate coupled to a single kinetic inductance detector made of a three-layer aluminum-titanium-aluminum. The baseline energy resolution is 34$\pm$1(stat)$\pm$2(syst) eV RMS and the response time is 120 $渭$s. These features, along with the natural multiplexing capability of kinetic inductance detectors, meet the requirements of future large-scale experiments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2104.06850v1-abstract-full').style.display = 'none'; document.getElementById('2104.06850v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 April, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2021. </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, 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/2101.10702">arXiv:2101.10702</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2101.10702">pdf</a>, <a href="https://arxiv.org/format/2101.10702">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-021-09317-z">10.1140/epjc/s10052-021-09317-z <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Double-Beta Decay of $\mathrm{^{130}Te}$ to the $0^+$ States of $\mathrm{^{130}Xe}$ with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+M+B+A">M. Biassoni A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+P+C+N">P. Carniti N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Copello%2C+D+C+M+C+S">D. Chiesa M. Clemenza S. Copello</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cosmelli%2C+C">C. Cosmelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a> , et al. (83 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="2101.10702v2-abstract-short" style="display: inline;"> The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ($0谓尾尾$) in the isotope $\mathrm{^{130}Te}$. In this work we present the latest results on two searches for the double beta decay (DBD) of $\mathrm{^{130}Te}$ to the first $0^{+}_2$ excited state of $\mathrm{^{130}Xe}$: the $0谓尾尾$ decay and the Standard Model-allowed two-neutr&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.10702v2-abstract-full').style.display = 'inline'; document.getElementById('2101.10702v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2101.10702v2-abstract-full" style="display: none;"> The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ($0谓尾尾$) in the isotope $\mathrm{^{130}Te}$. In this work we present the latest results on two searches for the double beta decay (DBD) of $\mathrm{^{130}Te}$ to the first $0^{+}_2$ excited state of $\mathrm{^{130}Xe}$: the $0谓尾尾$ decay and the Standard Model-allowed two-neutrinos double beta decay ($2谓尾尾$). Both searches are based on a 372.5 kg$\times$yr TeO$_2$ exposure. The de-excitation gamma rays emitted by the excited Xe nucleus in the final state yield a unique signature, which can be searched for with low background by studying coincident events in two or more bolometers. The closely packed arrangement of the CUORE crystals constitutes a significant advantage in this regard. The median limit setting sensitivities at 90\% Credible Interval (C.I.) of the given searches were estimated as $\mathrm{S^{0谓}_{1/2} = 5.6 \times 10^{24} \: \mathrm{yr}}$ for the ${0谓尾尾}$ decay and $\mathrm{S^{2谓}_{1/2} = 2.1 \times 10^{24} \: \mathrm{yr}}$ for the ${2谓尾尾}$ decay. No significant evidence for either of the decay modes was observed and a Bayesian lower bound at $90\%$ C.I. on the decay half lives is obtained as: $\mathrm{(T_{1/2})^{0谓}_{0^+_2} &gt; 5.9 \times 10^{24} \: \mathrm{yr}}$ for the $0谓尾尾$ mode and $\mathrm{(T_{1/2})^{2谓}_{0^+_2} &gt; 1.3 \times 10^{24} \: \mathrm{yr}}$ for the $2谓尾尾$ mode. These represent the most stringent limits on the DBD of $^{130}$Te to excited states and improve by a factor $\sim5$ the previous results on this process. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2101.10702v2-abstract-full').style.display = 'none'; document.getElementById('2101.10702v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 July, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 January, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2021. </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, 6 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/2012.12648">arXiv:2012.12648</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2012.12648">pdf</a>, <a href="https://arxiv.org/format/2012.12648">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1742-6596/1643/1/012025">10.1088/1742-6596/1643/1/012025 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Results on $^{82}$Se $2谓尾尾$ with CUPID-0 Phase I </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Pagnanini%2C+L">L Pagnanini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J W Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G Keppel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M Martinez</a> , et al. (19 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="2012.12648v1-abstract-short" style="display: inline;"> The nucleus is an extraordinarily complex object where fundamental forces are at work. The solution of this many-body problem has challenged physicists for decades: several models with complementary virtues and flaws have been adopted, none of which has a universal predictive capability. Double beta decay is a second-order weak nuclear decay whose precise measurement might steer fundamental improv&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.12648v1-abstract-full').style.display = 'inline'; document.getElementById('2012.12648v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2012.12648v1-abstract-full" style="display: none;"> The nucleus is an extraordinarily complex object where fundamental forces are at work. The solution of this many-body problem has challenged physicists for decades: several models with complementary virtues and flaws have been adopted, none of which has a universal predictive capability. Double beta decay is a second-order weak nuclear decay whose precise measurement might steer fundamental improvements in nuclear theory. Its knowledge paves the way to a much better understanding of many-body nuclear dynamics and clarifies, in particular, the role of multiparticle states. This is a useful input to a complete understanding of the dynamics of neutrino-less double beta decay, the chief physical process whose discovery may shed light to the matter-antimatter asymmetry of the universe and unveil the true nature of neutrinos. Here, we report the study of $2谓尾尾$-decay in $^{82}$Se with the CUPID-0 detector, an array of ZnSe crystals maintained at a temperature close to &#39;absolute zero&#39; in an ultralow background environment. Thanks to the unprecedented accuracy in the measurement of the two electrons spectrum, we prove that the decay is dominated by a single intermediate state. We obtain also the most precise value for the $^{82}$Se $2谓尾尾$-decay half-life of $T^{2谓}_{1/2} = [8.6^{+0.2}_{-0.1}] \times 10^{19}$ yr. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.12648v1-abstract-full').style.display = 'none'; document.getElementById('2012.12648v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Journal of Physics: Conference Series 1643 (2020) 012025 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2012.11749">arXiv:2012.11749</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2012.11749">pdf</a>, <a href="https://arxiv.org/format/2012.11749">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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.126.171801">10.1103/PhysRevLett.126.171801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of the 2$谓尾尾$ Decay Half-life of $^{130}$Te with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a> , et al. (88 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="2012.11749v2-abstract-short" style="display: inline;"> We measured two-neutrino double beta decay of $^{130}$Te using an exposure of 300.7 kg$\cdot$yr accumulated with the CUORE detector. Using a Bayesian analysis to fit simulated spectra to experimental data, it was possible to disentangle all the major background sources and precisely measure the two-neutrino contribution. The half-life is in agreement with past measurements with a strongly reduced&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.11749v2-abstract-full').style.display = 'inline'; document.getElementById('2012.11749v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2012.11749v2-abstract-full" style="display: none;"> We measured two-neutrino double beta decay of $^{130}$Te using an exposure of 300.7 kg$\cdot$yr accumulated with the CUORE detector. Using a Bayesian analysis to fit simulated spectra to experimental data, it was possible to disentangle all the major background sources and precisely measure the two-neutrino contribution. The half-life is in agreement with past measurements with a strongly reduced uncertainty: $T^{2谓}_{1/2} = 7.71^{+0.08}_{-0.06}\mathrm{(stat.)}^{+0.12}_{-0.15}\mathrm{(syst.)}\times10^{20}$ yr. This measurement is the most precise determination of the $^{130}$Te 2$谓尾尾$ decay half-life to date. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.11749v2-abstract-full').style.display = 'none'; document.getElementById('2012.11749v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Published in PRL</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">ACM Class:</span> J.2 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 126, 171801 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2012.00644">arXiv:2012.00644</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2012.00644">pdf</a>, <a href="https://arxiv.org/format/2012.00644">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Double beta decay results from the CUPID-0 experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a> , et al. (21 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="2012.00644v1-abstract-short" style="display: inline;"> A convincing observation of neutrino-less double beta decay (0$谓$DBD) relies on the possibility of operating high energy-resolution detectors in background-free conditions. Scintillating cryogenic calorimeters are one of the most promising tools to fulfill the requirements for a next-generation experiment. Several steps have been taken to demonstrate the maturity of this technique, starting from t&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.00644v1-abstract-full').style.display = 'inline'; document.getElementById('2012.00644v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2012.00644v1-abstract-full" style="display: none;"> A convincing observation of neutrino-less double beta decay (0$谓$DBD) relies on the possibility of operating high energy-resolution detectors in background-free conditions. Scintillating cryogenic calorimeters are one of the most promising tools to fulfill the requirements for a next-generation experiment. Several steps have been taken to demonstrate the maturity of this technique, starting from the successful experience of CUPID-0. The CUPID-0 experiment demonstrated the complete rejection of the dominant alpha background measuring the lowest counting rate in the region of interest for this technique. Furthermore, the most stringent limit on the $^{82}$Se 0$谓$DBD was established running 26 ZnSe crystals during two years of continuous detector operation. In this contribution we present the final results of CUPID-0 Phase I including a detailed model of the background, the measurement of the $^{82}$Se 2$谓$DBD half-life and the evidence that this nuclear transition is single state dominated. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.00644v1-abstract-full').style.display = 'none'; document.getElementById('2012.00644v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">40th International Conference on High Energy physics - ICHEP2020 July 28 - August 6, 2020 Prague, Czech Republic (virtual meeting)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2011.13656">arXiv:2011.13656</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2011.13656">pdf</a>, <a href="https://arxiv.org/format/2011.13656">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Characterization of cubic Li$_{2}$$^{100}$MoO$_4$ crystals for the CUPID experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Armatol%2C+A">A. Armatol</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armengaud%2C+E">E. Armengaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armstrong%2C+W">W. Armstrong</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A">A. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barresi%2C+A">A. Barresi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Baudin%2C+D">D. Baudin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A8%2C+L">L. Berg猫</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Boldrini%2C+V">V. Boldrini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a> , et al. (147 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="2011.13656v1-abstract-short" style="display: inline;"> The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li$_{2}$$^{100}$MoO$_4$ crystals as suitable detectors for neutrinoless double beta&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.13656v1-abstract-full').style.display = 'inline'; document.getElementById('2011.13656v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2011.13656v1-abstract-full" style="display: none;"> The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li$_{2}$$^{100}$MoO$_4$ crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of (6.7$\pm$0.6) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of $伪$ particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this $伪$-induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.13656v1-abstract-full').style.display = 'none'; document.getElementById('2011.13656v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 27 November, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2020. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2011.13243">arXiv:2011.13243</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2011.13243">pdf</a>, <a href="https://arxiv.org/format/2011.13243">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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.126.181802">10.1103/PhysRevLett.126.181802 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> New Limit for Neutrinoless Double-Beta Decay of $^{100}$Mo from the CUPID-Mo Experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Armengaud%2C+E">E. Armengaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beno%C3%AEt%2C+A">A. Beno卯t</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bourgeois%2C+C">Ch. Bourgeois</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brudanin%2C+V+B">V. B. Brudanin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camus%2C+P">P. Camus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Charlieux%2C+F">F. Charlieux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Combarieu%2C+M">M. de Combarieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dixon%2C+T">T. Dixon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a> , et al. (69 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="2011.13243v2-abstract-short" style="display: inline;"> The CUPID-Mo experiment at the Laboratoire Souterrain de Modane (France) is a demonstrator for CUPID, the next-generation ton-scale cryogenic $0谓尾尾$ experiment. It consists of a 4.2 kg array of 20 enriched Li$_{2}$$^{100}$MoO$_4$ scintillating bolometers to search for the lepton number violating process of $0谓尾尾$ decay in $^{100}$Mo. With more than one year of operation (2.16 kg$\times$yr of physi&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.13243v2-abstract-full').style.display = 'inline'; document.getElementById('2011.13243v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2011.13243v2-abstract-full" style="display: none;"> The CUPID-Mo experiment at the Laboratoire Souterrain de Modane (France) is a demonstrator for CUPID, the next-generation ton-scale cryogenic $0谓尾尾$ experiment. It consists of a 4.2 kg array of 20 enriched Li$_{2}$$^{100}$MoO$_4$ scintillating bolometers to search for the lepton number violating process of $0谓尾尾$ decay in $^{100}$Mo. With more than one year of operation (2.16 kg$\times$yr of physics data), no event in the region of interest and hence no evidence for $0谓尾尾$ is observed. We report a new limit on the half-life of $0谓尾尾$ decay in $^{100}$Mo of $T_{1/2} &gt; 1.5 \times 10^{24}\,$yr at 90 % C.I. The limit corresponds to an effective Majorana neutrino mass $\langle m_{尾尾} \rangle$ $&lt;$ (0.31--0.54)$\,$eV, dependent on the nuclear matrix element in the light Majorana neutrino exchange interpretation. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.13243v2-abstract-full').style.display = 'none'; document.getElementById('2011.13243v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 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. 126, 181802 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2011.09295">arXiv:2011.09295</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2011.09295">pdf</a>, <a href="https://arxiv.org/format/2011.09295">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> New results from the CUORE experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Giachero%2C+A">A. Giachero</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a> , et al. (88 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="2011.09295v2-abstract-short" style="display: inline;"> The Cryogenic Underground Observatory for Rare Events (CUORE) is the first cryogenic experiment searching for neutrinoless double-beta ($0谓尾尾$) decay that has been able to reach the one-ton scale. The detector, located at the Laboratori Nazionali del Gran Sasso in Italy, consists of an array of 988 TeO$_2$ crystals arranged in a compact cylindrical structure of 19 towers. Following the completion&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.09295v2-abstract-full').style.display = 'inline'; document.getElementById('2011.09295v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2011.09295v2-abstract-full" style="display: none;"> The Cryogenic Underground Observatory for Rare Events (CUORE) is the first cryogenic experiment searching for neutrinoless double-beta ($0谓尾尾$) decay that has been able to reach the one-ton scale. The detector, located at the Laboratori Nazionali del Gran Sasso in Italy, consists of an array of 988 TeO$_2$ crystals arranged in a compact cylindrical structure of 19 towers. Following the completion of the detector construction in August 2016, CUORE began its first physics data run in 2017 at a base temperature of about 10 mK. Following multiple optimization campaigns in 2018, CUORE is currently in stable operating mode. In 2019, CUORE released its 2\textsuperscript{nd} result of the search for $0谓尾尾$ with a TeO$_2$ exposure of 372.5 kg$\cdot$yr and a median exclusion sensitivity to a $^{130}$Te $0谓尾尾$ decay half-life of $1.7\cdot 10^{25}$ yr. We find no evidence for $0谓尾尾$ decay and set a 90\% C.I. (credibility interval) Bayesian lower limit of $3.2\cdot 10^{25}$ yr on the $^{130}$Te $0谓尾尾$ decay half-life. In this work, we present the current status of CUORE&#39;s search for $0谓尾尾$, as well as review the detector performance. Finally, we give an update of the CUORE background model and the measurement of the $^{130}$Te two neutrino double-beta ($2谓尾尾$) decay half-life. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2011.09295v2-abstract-full').style.display = 'none'; document.getElementById('2011.09295v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 7 January, 2021; <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">Comments:</span> <span class="has-text-grey-dark mathjax">Proceeding of 40th International Conference on High Energy physics (ICHEP2020), July 28 - August 6, 2020, Prague, Czech Republic (virtual meeting). arXiv admin note: text overlap with arXiv:1905.07667</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2010.04033">arXiv:2010.04033</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2010.04033">pdf</a>, <a href="https://arxiv.org/format/2010.04033">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/16/03/P03032">10.1088/1748-0221/16/03/P03032 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Pulse Shape Discrimination in CUPID-Mo using Principal Component Analysis </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Huang%2C+R">R. Huang</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armengaud%2C+E">E. Armengaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beno%C3%AEt%2C+A">A. Beno卯t</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bourgeois%2C+C">Ch. Bourgeois</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brudanin%2C+V+B">V. B. Brudanin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camus%2C+P">P. Camus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Charlieux%2C+F">F. Charlieux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Combarieu%2C+M">M. de Combarieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dixon%2C+T">T. Dixon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a> , et al. (64 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="2010.04033v2-abstract-short" style="display: inline;"> CUPID-Mo is a cryogenic detector array designed to search for neutrinoless double-beta decay ($0谓尾尾$) of $^{100}$Mo. It uses 20 scintillating $^{100}$Mo-enriched Li$_2$MoO$_4$ bolometers instrumented with Ge light detectors to perform active suppression of $伪$ backgrounds, drastically reducing the expected background in the $0谓尾尾$ signal region. As a result, pileup events and small detector instab&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2010.04033v2-abstract-full').style.display = 'inline'; document.getElementById('2010.04033v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2010.04033v2-abstract-full" style="display: none;"> CUPID-Mo is a cryogenic detector array designed to search for neutrinoless double-beta decay ($0谓尾尾$) of $^{100}$Mo. It uses 20 scintillating $^{100}$Mo-enriched Li$_2$MoO$_4$ bolometers instrumented with Ge light detectors to perform active suppression of $伪$ backgrounds, drastically reducing the expected background in the $0谓尾尾$ signal region. As a result, pileup events and small detector instabilities that mimic normal signals become non-negligible potential backgrounds. These types of events can in principle be eliminated based on their signal shapes, which are different from those of regular bolometric pulses. We show that a purely data-driven principal component analysis based approach is able to filter out these anomalous events, without the aid of detector response simulations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2010.04033v2-abstract-full').style.display = 'none'; document.getElementById('2010.04033v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 March, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 October, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> JINST 16 (2021) P03032 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2003.10840">arXiv:2003.10840</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2003.10840">pdf</a>, <a href="https://arxiv.org/format/2003.10840">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-020-8280-4">10.1140/epjc/s10052-020-8280-4 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Neutrino-less Double Beta Decay of $^{64}$Zn and $^{70}$Zn with CUPID-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremomesi%2C+O">O. Cremomesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a> , et al. (21 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="2003.10840v2-abstract-short" style="display: inline;"> CUPID-0 is the first pilot experiment of CUPID, a next-generation project searching for neutrino-less double beta decay. In its first scientific run, CUPID-0 operated 26 ZnSe cryogenic calorimeters coupled to light detectors in the underground Laboratori Nazionali del Gran Sasso. In this work, we analyzed a ZnSe exposure of 11.34 kg$\times$yr to search for the neutrino-less double beta decay of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2003.10840v2-abstract-full').style.display = 'inline'; document.getElementById('2003.10840v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2003.10840v2-abstract-full" style="display: none;"> CUPID-0 is the first pilot experiment of CUPID, a next-generation project searching for neutrino-less double beta decay. In its first scientific run, CUPID-0 operated 26 ZnSe cryogenic calorimeters coupled to light detectors in the underground Laboratori Nazionali del Gran Sasso. In this work, we analyzed a ZnSe exposure of 11.34 kg$\times$yr to search for the neutrino-less double beta decay of $^{70}$Zn and for the neutrino-less positron-emitting electron capture of $^{64}$Zn. We found no evidence for these decays and set 90$\%$ credible interval limits of ${\rm T}_{1/2}^{0谓尾尾}(^{70}{\rm Zn}) &gt; 1.6 \times 10^{21}$ yr and ${\rm T}_{1/2}^{0谓EC 尾+}(^{64}{\rm Zn}) &gt; 1.2 \times 10^{22}$ yr, surpassing by almost two orders of magnitude the previous experimental results <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2003.10840v2-abstract-full').style.display = 'none'; document.getElementById('2003.10840v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 September, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 March, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2020. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1912.10966">arXiv:1912.10966</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1912.10966">pdf</a>, <a href="https://arxiv.org/format/1912.10966">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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.124.122501">10.1103/PhysRevLett.124.122501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Improved Limit on Neutrinoless Double-Beta Decay in $^{130}$Te with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chott%2C+N">N. Chott</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a> , et al. (86 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="1912.10966v1-abstract-short" style="display: inline;"> We report new results from the search for neutrinoless double-beta decay in $^{130}$Te with the CUORE detector. This search benefits from a four-fold increase in exposure, lower trigger thresholds and analysis improvements relative to our previous results. We observe a background of $(1.38\pm0.07)\cdot10^{-2}$ counts$/($keV$\cdot$kg$\cdot$yr$)$ in the $0谓尾尾$ decay region of interest and, with a to&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1912.10966v1-abstract-full').style.display = 'inline'; document.getElementById('1912.10966v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1912.10966v1-abstract-full" style="display: none;"> We report new results from the search for neutrinoless double-beta decay in $^{130}$Te with the CUORE detector. This search benefits from a four-fold increase in exposure, lower trigger thresholds and analysis improvements relative to our previous results. We observe a background of $(1.38\pm0.07)\cdot10^{-2}$ counts$/($keV$\cdot$kg$\cdot$yr$)$ in the $0谓尾尾$ decay region of interest and, with a total exposure of 372.5 kg$\cdot$yr, we attain a median exclusion sensitivity of $1.7\cdot10^{25}$ yr. We find no evidence for $0谓尾尾$ decay and set a $90\%$ CI Bayesian lower limit of $3.2\cdot10^{25}$ yr on the $^{130}$Te half-life for this process. In the hypothesis that $0谓尾尾$ decay is mediated by light Majorana neutrinos, this results in an upper limit on the effective Majorana mass of 75-350 meV, depending on the nuclear matrix elements used. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1912.10966v1-abstract-full').style.display = 'none'; document.getElementById('1912.10966v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 December, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2019. </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, 5 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/1912.07272">arXiv:1912.07272</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1912.07272">pdf</a>, <a href="https://arxiv.org/ps/1912.07272">ps</a>, <a href="https://arxiv.org/format/1912.07272">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-020-8203-4">10.1140/epjc/s10052-020-8203-4 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Precise measurement of $2谓尾尾$ decay of $^{100}$Mo with the CUPID-Mo detection technology </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Armengaud%2C+E">E. Armengaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beno%C3%AEt%2C+A">A. Beno卯t</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bourgeois%2C+C">Ch. Bourgeois</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Briere%2C+M">M. Briere</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brudanin%2C+V">V. Brudanin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camus%2C+P">P. Camus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Charlieux%2C+F">F. Charlieux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Combarieu%2C+M">M. de Combarieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eitel%2C+K">K. Eitel</a> , et al. (65 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1912.07272v1-abstract-short" style="display: inline;"> We report the measurement of the two-neutrino double-beta ($2谓尾尾$) decay of $^{100}$Mo to the ground state of $^{100}$Ru using lithium molybdate (\crystal) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory. From a total exposure of $42.235$ kg$\times$d, the half-life of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1912.07272v1-abstract-full').style.display = 'inline'; document.getElementById('1912.07272v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1912.07272v1-abstract-full" style="display: none;"> We report the measurement of the two-neutrino double-beta ($2谓尾尾$) decay of $^{100}$Mo to the ground state of $^{100}$Ru using lithium molybdate (\crystal) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory. From a total exposure of $42.235$ kg$\times$d, the half-life of $^{100}$Mo is determined to be $T_{1/2}^{2谓}=[7.12^{+0.18}_{-0.14}\,\mathrm{(stat.)}\pm0.10\,\mathrm{(syst.)}]\times10^{18}$ years. This is the most accurate determination of the $2谓尾尾$ half-life of $^{100}$Mo to date. We also confirm, with the statistical significance of $&gt;3蟽$, that the single-state dominance model of the $2谓尾尾$ decay of $^{100}$Mo is favored over the high-state dominance model. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1912.07272v1-abstract-full').style.display = 'none'; document.getElementById('1912.07272v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 December, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2019. </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">11 pages, 6 figures, 4 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/1911.10426">arXiv:1911.10426</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1911.10426">pdf</a>, <a href="https://arxiv.org/format/1911.10426">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1742-6596/1468/1/012129">10.1088/1742-6596/1468/1/012129 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First data from the CUPID-Mo neutrinoless double beta decay experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Schmidt%2C+B">B. Schmidt</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Armengaud%2C+E">E. Armengaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beno%C3%AEt%2C+A">A. Beno卯t</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bourgeois%2C+C">Ch. Bourgeois</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Briere%2C+M">M. Briere</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brudanin%2C+V+B">V. B. Brudanin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camus%2C+P">P. Camus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Charlieux%2C+F">F. Charlieux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Combarieu%2C+M">M. de Combarieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a> , et al. (65 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1911.10426v1-abstract-short" style="display: inline;"> The CUPID-Mo experiment is searching for neutrinoless double beta decay in $^{100}$Mo, evaluating the technology of cryogenic scintillating Li$_{2}^{100}$MoO$_4$ detectors for CUPID (CUORE Upgrade with Particle ID). CUPID-Mo detectors feature background suppression using a dual-readout scheme with Li$_{2}$MoO$_4$ crystals complemented by Ge bolometers for light detection. The detection of both hea&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.10426v1-abstract-full').style.display = 'inline'; document.getElementById('1911.10426v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1911.10426v1-abstract-full" style="display: none;"> The CUPID-Mo experiment is searching for neutrinoless double beta decay in $^{100}$Mo, evaluating the technology of cryogenic scintillating Li$_{2}^{100}$MoO$_4$ detectors for CUPID (CUORE Upgrade with Particle ID). CUPID-Mo detectors feature background suppression using a dual-readout scheme with Li$_{2}$MoO$_4$ crystals complemented by Ge bolometers for light detection. The detection of both heat and scintillation light signals allows the efficient discrimination of $伪$ from $纬$&amp;$尾$ events. In this proceedings, we discuss results from the first 2 months of data taking in spring 2019. In addition to an excellent bolometric performance of 6.7$\,$keV (FWHM) at 2615$\,$keV and an $伪$ separation of better than 99.9\% for all detectors, we report on bulk radiopurity for Th and U. Finally, we interpret the accumulated physics data in terms of a limit of $T_{1/2}^{0谓}\,&gt; 3\times10^{23}\,$yr for $^{100}$Mo and discuss the sensitivity of CUPID-Mo until the expected end of physics data taking in early 2020. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.10426v1-abstract-full').style.display = 'none'; document.getElementById('1911.10426v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 November, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2019. </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">Proceedings for TAUP 2019, submitted to IOP Journal of Physics: Conference Series</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Journal of Physics: Conference Series 1468 (2020) 012129 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1911.02446">arXiv:1911.02446</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1911.02446">pdf</a>, <a href="https://arxiv.org/format/1911.02446">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="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.100.092002">10.1103/PhysRevD.100.092002 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First search for Lorentz violation in double beta decay with scintillating calorimeters </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M. Martinez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nagorny%2C+S">S. Nagorny</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="1911.02446v1-abstract-short" style="display: inline;"> We present the search for Lorentz violation in the double beta decay of ^{82}Se~with CUPID-0, using an exposure of 9.95 kg x y. We found no evidence for the searched signal and set a limit on the isotropic components of the Lorentz violating coefficient of $\mathring{a}_{\text{of}}^{(3)} &lt; 4.1\cdot10^{-6}$ GeV (90\% Credible Interval). This results is obtained with a Bayesian analysis of the exper&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.02446v1-abstract-full').style.display = 'inline'; document.getElementById('1911.02446v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1911.02446v1-abstract-full" style="display: none;"> We present the search for Lorentz violation in the double beta decay of ^{82}Se~with CUPID-0, using an exposure of 9.95 kg x y. We found no evidence for the searched signal and set a limit on the isotropic components of the Lorentz violating coefficient of $\mathring{a}_{\text{of}}^{(3)} &lt; 4.1\cdot10^{-6}$ GeV (90\% Credible Interval). This results is obtained with a Bayesian analysis of the experimental data and fully includes the systematic uncertainties of the model. This is the first limit on $\mathring{a}_{\text{of}}^{(3)}$ obtained with a scintillating bolometer, showing the potentiality of this technique. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.02446v1-abstract-full').style.display = 'none'; document.getElementById('1911.02446v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 November, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> O. Azzolini et al., Phys. Rev. D 100, 092002 - Published 6 November 2019 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1909.03397">arXiv:1909.03397</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1909.03397">pdf</a>, <a href="https://arxiv.org/format/1909.03397">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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.123.262501">10.1103/PhysRevLett.123.262501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Evidence of Single State Dominance in the Two-Neutrino Double-$尾$ Decay of Se-82 with CUPID-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kotila%2C+J">J. Kotila</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M. Martinez</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="1909.03397v2-abstract-short" style="display: inline;"> We report on the measurement of the two-neutrino double-$尾$ decay of $^{82}$Se performed for the first time with cryogenic calorimeters, in the framework of the CUPID-0~experiment. With an exposure of 9.95 kg$\times$yr of Zn$^{82}$Se, we determine the two-neutrino double-$尾$ decay half-life of $^{82}$Se with an unprecedented precision level,&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1909.03397v2-abstract-full').style.display = 'inline'; document.getElementById('1909.03397v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1909.03397v2-abstract-full" style="display: none;"> We report on the measurement of the two-neutrino double-$尾$ decay of $^{82}$Se performed for the first time with cryogenic calorimeters, in the framework of the CUPID-0~experiment. With an exposure of 9.95 kg$\times$yr of Zn$^{82}$Se, we determine the two-neutrino double-$尾$ decay half-life of $^{82}$Se with an unprecedented precision level, $T_{1/2}^{2谓} = [8.60 \pm 0.03 \textrm{(stat.)}~^{+0.17}_{-0.10} \textrm{(syst.)}] \times 10^{19}~\textrm{yr}$. The very high signal-to-background ratio, along with the detailed reconstruction of the background sources allowed us to identify the single state dominance as the underlying mechanism of such process, demonstrating that the higher state dominance hypothesis is disfavored at the level of 5.5 $蟽$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1909.03397v2-abstract-full').style.display = 'none'; document.getElementById('1909.03397v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 November, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 September, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 123, 262501 (2019) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1909.02994">arXiv:1909.02994</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1909.02994">pdf</a>, <a href="https://arxiv.org/format/1909.02994">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-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/10.1140/epjc/s10052-019-7578-6">10.1140/epjc/s10052-019-7578-6 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The CUPID-Mo experiment for neutrinoless double-beta decay: performance and prospects </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Armengaud%2C+E">E. Armengaud</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Augier%2C+C">C. Augier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barabash%2C+A+S">A. S. Barabash</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beno%C3%AEt%2C+A">A. Beno卯t</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Berg%C3%A9%2C+L">L. Berg茅</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Billard%2C+J">J. Billard</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Borovlev%2C+Y+A">Yu. A. Borovlev</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bourgeois%2C+C">Ch. Bourgeois</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Briere%2C+M">M. Briere</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brudanin%2C+V+B">V. B. Brudanin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camus%2C+P">P. Camus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cazes%2C+A">A. Cazes</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chapellier%2C+M">M. Chapellier</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Charlieux%2C+F">F. Charlieux</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=de+Combarieu%2C+M">M. de Combarieu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Danevich%2C+F+A">F. A. Danevich</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=De+Jesus%2C+M">M. De Jesus</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dumoulin%2C+L">L. Dumoulin</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Eitel%2C+K">K. Eitel</a> , et al. (64 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="1909.02994v1-abstract-short" style="display: inline;"> CUPID-Mo is a bolometric experiment to search for neutrinoless double-beta decay ($0谓尾尾$) of $^{100}$Mo. In this article, we detail the CUPID-Mo detector concept, assembly, installation in the underground laboratory in Modane in 2018, and provide results from the first datasets. The demonstrator consists of an array of 20 scintillating bolometers comprised of $^{100}$Mo-enriched 0.2 kg Li$_2$MoO&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1909.02994v1-abstract-full').style.display = 'inline'; document.getElementById('1909.02994v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1909.02994v1-abstract-full" style="display: none;"> CUPID-Mo is a bolometric experiment to search for neutrinoless double-beta decay ($0谓尾尾$) of $^{100}$Mo. In this article, we detail the CUPID-Mo detector concept, assembly, installation in the underground laboratory in Modane in 2018, and provide results from the first datasets. The demonstrator consists of an array of 20 scintillating bolometers comprised of $^{100}$Mo-enriched 0.2 kg Li$_2$MoO$_4$ crystals. The detectors are complemented by 20 thin cryogenic Ge bolometers acting as light detectors to distinguish $伪$ from $纬$/$尾$ events by the detection of both heat and scintillation light signals. We observe good detector uniformity, facilitating the operation of a large detector array as well as excellent energy resolution of 5.3 keV (6.5 keV) FWHM at 2615 keV, in calibration (physics) data. Based on the observed energy resolutions and light yields a separation of $伪$ particles at much better than 99.9\% with equally high acceptance for $纬$/$尾$ events is expected for events in the region of interest for $^{100}$Mo $0谓尾尾$. We present limits on the crystals&#39; radiopurity ($\leq$3 $渭$Bq/kg of $^{226}$Ra and $\leq$2 $渭$Bq/kg of $^{232}$Th). Based on these initial results we also discuss a sensitivity study for the science reach of the CUPID-Mo experiment, in particular, the ability to set the most stringent half-life limit on the $^{100}$Mo $0谓尾尾$ decay after half a year of livetime. The achieved results show that CUPID-Mo is a successful demonstrator of the technology - developed in the framework of the LUMINEU project - selected for the CUPID experiment, a proposed follow-up of CUORE, the currently running first tonne-scale cryogenic $0谓尾尾$ experiment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1909.02994v1-abstract-full').style.display = 'none'; document.getElementById('1909.02994v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 September, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2019. </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, 18 figures, 3 tables; to be submitted to EPJC</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1907.03647">arXiv:1907.03647</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1907.03647">pdf</a>, <a href="https://arxiv.org/format/1907.03647">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-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/10.1140/epjc/s10052-019-7242-1">10.1140/epjc/s10052-019-7242-1 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Phonon and light read out of a Li$_2$MoO$_4$ crystal with multiplexed kinetic inductance detectors </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Colantoni%2C+I">I. Colantoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M. Martinez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pettinari%2C+G">G. Pettinari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vignati%2C+M">M. Vignati</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="1907.03647v2-abstract-short" style="display: inline;"> Molybdenum based crystals such as Li$_2$MoO$_4$ and CaMoO$_4$ are emerging as leading candidates for next generation experiments searching for neutrino-less double beta decay with cryogenic calorimeters (CUPID, AMoRE). The exquisite energy resolution and high radio-purity of these crystals come at the cost of a potentially detrimental background source: the two neutrinos double beta decay of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1907.03647v2-abstract-full').style.display = 'inline'; document.getElementById('1907.03647v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1907.03647v2-abstract-full" style="display: none;"> Molybdenum based crystals such as Li$_2$MoO$_4$ and CaMoO$_4$ are emerging as leading candidates for next generation experiments searching for neutrino-less double beta decay with cryogenic calorimeters (CUPID, AMoRE). The exquisite energy resolution and high radio-purity of these crystals come at the cost of a potentially detrimental background source: the two neutrinos double beta decay of $^{100}$Mo. Indeed, the fast half-life of this decay mode, combined with the slow response of cryogenic calorimeters, would result in pile-up events in the energy region of interest for neutrino-less double beta decay, reducing the experimental sensitivity. This background can be suppressed using fast and high sensitivity cryogenic light detectors, provided that the scintillation time constant itself does not limit the time resolution. We developed a new detection technique exploiting the high sensitivity, the fast time response and the multiplexing capability of Kinetic Inductance Detectors. We applied the proposed technique to a $2\times2\times2$ cm$^3$ Li$_2$MoO$_4$ crystal, which was chosen as baseline option for CUPID. We measured simultaneously both the phonon and scintillation signals with KIDs. We derived the scintillation time constant of this compound at millikelvin temperatures obtaining $蟿_{scint} = 84.5\pm4.5\rm{(syst)}\pm1.0\rm{(stat)}$ $渭$s, constant between 10 and 190 mK. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1907.03647v2-abstract-full').style.display = 'none'; document.getElementById('1907.03647v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 22 August, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 8 July, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2019. </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/1906.05001">arXiv:1906.05001</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1906.05001">pdf</a>, <a href="https://arxiv.org/format/1906.05001">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-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.123.032501">10.1103/PhysRevLett.123.032501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Final result of CUPID-0 phase-I in the search for the $^{82}$Se Neutrinoless Double Beta Decay </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M. Martinez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nagorny%2C+S">S. Nagorny</a> , et al. (19 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="1906.05001v1-abstract-short" style="display: inline;"> CUPID-0 is the first pilot experiment of CUPID, a next-generation project for the measurement of neutrinoless double beta decay (0$谓$DBD) with scintillating bolometers. The detector, consisting of 24 enriched and 2 natural ZnSe crystals, has been taking data at Laboratori Nazionali del Gran Sasso from June 2017 to December 2018, collecting a $^{82}$Se exposure of 5.29 kg$\times$yr. In this paper w&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1906.05001v1-abstract-full').style.display = 'inline'; document.getElementById('1906.05001v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1906.05001v1-abstract-full" style="display: none;"> CUPID-0 is the first pilot experiment of CUPID, a next-generation project for the measurement of neutrinoless double beta decay (0$谓$DBD) with scintillating bolometers. The detector, consisting of 24 enriched and 2 natural ZnSe crystals, has been taking data at Laboratori Nazionali del Gran Sasso from June 2017 to December 2018, collecting a $^{82}$Se exposure of 5.29 kg$\times$yr. In this paper we present the phase-I results in the search for 0$谓$DBD. We demonstrate that the technology implemented by CUPID-0 allows us to reach the lowest background for calorimetric experiments: $(3.5^{+1.0}_{-0.9})\times10^{-3}$ counts/(keV kg yr). Monitoring 3.88$\times$10$^{25}$ $^{82}$Se nuclei$\times$yr we reach a 90% credible interval median sensitivity of $\rm{T}^{0谓}_{1/2}&gt;5.0\times10^{24} \rm{yr}$ and set the most stringent limit on the half-life of $^{82}$Se 0$谓$DBD : $\rm{T}^{0谓}_{1/2}&gt;3.5\times10^{24} \rm{yr}$ (90% credible interval), corresponding to m$_{尾尾} &lt;$ (311-638) meV depending on the nuclear matrix element calculations. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1906.05001v1-abstract-full').style.display = 'none'; document.getElementById('1906.05001v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 June, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 3 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 123, 032501 (2019) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1905.07667">arXiv:1905.07667</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1905.07667">pdf</a>, <a href="https://arxiv.org/format/1905.07667">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Results of CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Oro%2C+S">S. Dell&#39;Oro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chott%2C+N">N. Chott</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a> , et al. (87 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="1905.07667v1-abstract-short" style="display: inline;"> The Cryogenic Underground Observatory for Rare Events (CUORE) at the Laboratori Nazionali del Gran Sasso, Italy, is the world&#39;s largest bolometric experiment. The detector consists of an array of 988 TeO2 crystals, for a total mass of 742 kg. CUORE is presently in data taking, searching for the neutrinoless double beta decay of 130 Te. CUORE is operational since the spring of 2017. The initial sci&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1905.07667v1-abstract-full').style.display = 'inline'; document.getElementById('1905.07667v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1905.07667v1-abstract-full" style="display: none;"> The Cryogenic Underground Observatory for Rare Events (CUORE) at the Laboratori Nazionali del Gran Sasso, Italy, is the world&#39;s largest bolometric experiment. The detector consists of an array of 988 TeO2 crystals, for a total mass of 742 kg. CUORE is presently in data taking, searching for the neutrinoless double beta decay of 130 Te. CUORE is operational since the spring of 2017. The initial science run already allowed to provide the most stringent limit on the neutrinoless double beta decay half-life of 130Te, and to perform the most precise measurement of the two-neutrino double beta decay half-life. Up to date, we have more than doubled the collected exposure. In this talk, we presenteded the most recent results and discuss the present status of the CUORE experiment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1905.07667v1-abstract-full').style.display = 'none'; document.getElementById('1905.07667v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 May, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">contribution to the 2019 EW/QCD/Gravitation session of the 54th Rencontres de Moriond</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1904.10397">arXiv:1904.10397</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1904.10397">pdf</a>, <a href="https://arxiv.org/format/1904.10397">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-019-7078-8">10.1140/epjc/s10052-019-7078-8 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Background Model of the CUPID-0 Experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gotti%2C+C">C. Gotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Keppel%2C+G">G. Keppel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Martinez%2C+M">M. Martinez</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nagorny%2C+S">S. Nagorny</a> , et al. (19 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="1904.10397v2-abstract-short" style="display: inline;"> CUPID-0 is the first large mass array of enriched Zn$^{82}$Se scintillating low temperature calorimeters, operated at LNGS since 2017. During its first scientific runs, CUPID-0 collected an exposure of 9.95 kg yr. Thanks to the excellent rejection of $伪$ particles, we attained the lowest background ever measured with thermal detectors in the energy region where we search for the signature of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1904.10397v2-abstract-full').style.display = 'inline'; document.getElementById('1904.10397v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1904.10397v2-abstract-full" style="display: none;"> CUPID-0 is the first large mass array of enriched Zn$^{82}$Se scintillating low temperature calorimeters, operated at LNGS since 2017. During its first scientific runs, CUPID-0 collected an exposure of 9.95 kg yr. Thanks to the excellent rejection of $伪$ particles, we attained the lowest background ever measured with thermal detectors in the energy region where we search for the signature of $^{82}$Se neutrinoless double beta decay. In this work we develop a model to reconstruct the CUPID-0 background over the whole energy range of experimental data. We identify the background sources exploiting their distinctive signatures and we assess their extremely low contribution (down to $\sim10^{-4}$ counts/(keV kg yr)) in the region of interest for $^{82}$Se neutrinoless double beta decay search. This result represents a crucial step towards the comprehension of the background in experiments based on scintillating calorimeters and in next generation projects such as CUPID. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1904.10397v2-abstract-full').style.display = 'none'; document.getElementById('1904.10397v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 July, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 23 April, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2019. </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">This is a post-peer-review, pre-copyedit version of an article published in Eur. Phys. J. C. The final authenticated version is available online at: https://doi.org/10.1140/epjc/s10052-019-7078-8</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> O. Azzolini et al., Eur. Phys. J. C (2019) 79: 583 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1901.10434">arXiv:1901.10434</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1901.10434">pdf</a>, <a href="https://arxiv.org/format/1901.10434">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/14/08/P08017">10.1088/1748-0221/14/08/P08017 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Resolution enhancement with light/heat decorrelation in CUPID-0 bolometric detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pagnanini%2C+L">L. Pagnanini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pattavina%2C+L">L. Pattavina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pavan%2C+M">M. Pavan</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pirro%2C+S">S. Pirro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pozzi%2C+S">S. Pozzi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Previtali%2C+E">E. Previtali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Rusconi%2C+C">C. Rusconi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Tomei%2C+C">C. Tomei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Vignati%2C+M">M. Vignati</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="1901.10434v3-abstract-short" style="display: inline;"> The CUPID-0 experiment searches for neutrinoless double beta decay ($0谓尾尾$) using the first array of enriched Zn$^{82}$Se scintillating bolometers with double (heat and light) read-out. To further enhance the CUPID-0 detector performances, the heat-light correlation has been exploited to improve the energy resolution. Different decorrelation algorithms have been studied and the best result is the&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.10434v3-abstract-full').style.display = 'inline'; document.getElementById('1901.10434v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1901.10434v3-abstract-full" style="display: none;"> The CUPID-0 experiment searches for neutrinoless double beta decay ($0谓尾尾$) using the first array of enriched Zn$^{82}$Se scintillating bolometers with double (heat and light) read-out. To further enhance the CUPID-0 detector performances, the heat-light correlation has been exploited to improve the energy resolution. Different decorrelation algorithms have been studied and the best result is the average reduction of the full width at half maximum (FWHM) energy resolution to $(90.5\pm0.6)~\%$ of its original value , corresponding to a change from $\text{FWHM}=(20.7\pm0.5)~\text{keV}$ to $\text{FWHM}=(18.7\pm0.5)~\text{keV}$ at the 2615 keV $纬$ line. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1901.10434v3-abstract-full').style.display = 'none'; document.getElementById('1901.10434v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 9 May, 2019; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 January, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2019. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1811.10363">arXiv:1811.10363</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1811.10363">pdf</a>, <a href="https://arxiv.org/format/1811.10363">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-019-7275-5">10.1140/epjc/s10052-019-7275-5 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Double-beta decay of ${}^{130}$Te to the first $0^+$ excited state of ${}^{130}$Xe with CUORE-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Artusa%2C+D+R">D. R. Artusa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Banks%2C+T+I">T. I. Banks</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carbone%2C+L">L. Carbone</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a> , et al. (96 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="1811.10363v3-abstract-short" style="display: inline;"> We report on a search for double beta decay of $^{130}$Te to the first $0^{+}$ excited state of $^{130}$Xe using a 9.8 kg$\cdot$yr exposure of $^{130}$Te collected with the CUORE-0 experiment. In this work we exploit different topologies of coincident events to search for both the neutrinoless and two-neutrino double-decay modes. We find no evidence for either mode and place lower bounds on the ha&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1811.10363v3-abstract-full').style.display = 'inline'; document.getElementById('1811.10363v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1811.10363v3-abstract-full" style="display: none;"> We report on a search for double beta decay of $^{130}$Te to the first $0^{+}$ excited state of $^{130}$Xe using a 9.8 kg$\cdot$yr exposure of $^{130}$Te collected with the CUORE-0 experiment. In this work we exploit different topologies of coincident events to search for both the neutrinoless and two-neutrino double-decay modes. We find no evidence for either mode and place lower bounds on the half-lives: $蟿^{0谓}_{0^+}&gt;7.9\cdot 10^{23}$ yr and $蟿^{2谓}_{0^+}&gt;2.4\cdot 10^{23}$ yr. Combining our results with those obtained by the CUORICINO experiment, we achieve the most stringent constraints available for these processes: $蟿^{0谓}_{0^+}&gt;1.4\cdot 10^{24}$ yr and $蟿^{2谓}_{0^+}&gt;2.5\cdot 10^{23}$ yr. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1811.10363v3-abstract-full').style.display = 'none'; document.getElementById('1811.10363v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 29 November, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 26 November, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 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">9 pages, 5 figures, 5 tables</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C 79, 795 (2019) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1808.10342">arXiv:1808.10342</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1808.10342">pdf</a>, <a href="https://arxiv.org/format/1808.10342">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <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"> Update on the recent progress of the CUORE experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a> , et al. (96 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="1808.10342v1-abstract-short" style="display: inline;"> CUORE is a 741 kg array of 988 TeO$_2$ bolometeric crystals designed to search for the neutrinoless double beta decay of $^{130}$Te and other rare processes. CUORE has been taking data since summer 2017, and as of summer 2018 collected a total of 86.3 kg$\cdot$yr of TeO$_2$ exposure. Based on this exposure, we were able to set a limit on the $0谓尾尾$ half-life of $^{130}$Te of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1808.10342v1-abstract-full').style.display = 'inline'; document.getElementById('1808.10342v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1808.10342v1-abstract-full" style="display: none;"> CUORE is a 741 kg array of 988 TeO$_2$ bolometeric crystals designed to search for the neutrinoless double beta decay of $^{130}$Te and other rare processes. CUORE has been taking data since summer 2017, and as of summer 2018 collected a total of 86.3 kg$\cdot$yr of TeO$_2$ exposure. Based on this exposure, we were able to set a limit on the $0谓尾尾$ half-life of $^{130}$Te of $T^{0谓}_{1/2}&gt;1.5\times10^{25}$ yr at 90% C.L. At this conference, we showed the decomposition of the CUORE background and were able to extract a $^{130}$Te $2谓尾尾$ half-life of $T_{1/2}^{2谓}=[7.9\pm0.1 \mathrm{(stat.)}\pm0.2 \mathrm{(syst.)}]\times10^{20}$ yr. This is the most precise measurement of this half-life and is consistent with previous measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1808.10342v1-abstract-full').style.display = 'none'; document.getElementById('1808.10342v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 August, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 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">Proceedings of the Neutrino 2018 Conference. 8 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/1807.00665">arXiv:1807.00665</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1807.00665">pdf</a>, <a href="https://arxiv.org/format/1807.00665">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epjc/s10052-018-6340-9">10.1140/epjc/s10052-018-6340-9 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search of the neutrino-less double beta decay of $^{82}$Se into the excited states of $^{82}$Kr with CUPID-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barrera%2C+M+T">M. T. Barrera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bossio%2C+E">E. Bossio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gorla%2C+P">P. Gorla</a> , et al. (25 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1807.00665v3-abstract-short" style="display: inline;"> The CUPID0 experiment searches for double beta decay using cryogenic calorimeters with double (heat and light) read-out. The detector, consisting of 24 ZnSe crystals 95$\%$ enriched in $^{82}$Se and 2 natural ZnSe crystals, started data-taking in 2017 at Laboratori Nazionali del Gran Sasso. We present the search for the neutrino-less double beta decay of $^{82}$Se into the 0$_1^+$, 2$_1^+$ and 2&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.00665v3-abstract-full').style.display = 'inline'; document.getElementById('1807.00665v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1807.00665v3-abstract-full" style="display: none;"> The CUPID0 experiment searches for double beta decay using cryogenic calorimeters with double (heat and light) read-out. The detector, consisting of 24 ZnSe crystals 95$\%$ enriched in $^{82}$Se and 2 natural ZnSe crystals, started data-taking in 2017 at Laboratori Nazionali del Gran Sasso. We present the search for the neutrino-less double beta decay of $^{82}$Se into the 0$_1^+$, 2$_1^+$ and 2$_2^+$ excited states of $^{82}$Kr with an exposure of 5.74 kg$\cdot$yr (2.24$\times$10$^{25}$ emitters$\cdot$yr). We found no evidence of the decays and set the most stringent limits on the widths of these processes: $螕$($^{82}$Se $\rightarrow ^{82}$Kr$_{0_1^+}$)$&lt;$8.55$\times$10$^{-24}$ yr$^{-1}$, $螕$($^{82}$Se $\rightarrow ^{82}$Kr$_{2_1^+}$)$&lt;6.25 \times10^{-24}$ yr$^{-1}$, $螕$($^{82}$Se $\rightarrow ^{82}$Kr$_{2_2^+}$)$&lt;$8.25$\times$10$^{-24}$ yr$^{-1}$ (90$\%$ credible interval <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1807.00665v3-abstract-full').style.display = 'none'; document.getElementById('1807.00665v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 October, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 2 July, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2018. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1802.07791">arXiv:1802.07791</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1802.07791">pdf</a>, <a href="https://arxiv.org/format/1802.07791">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="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.120.232502">10.1103/PhysRevLett.120.232502 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First Result on the Neutrinoless Double Beta Decay of $^{82}$Se with CUPID-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=collaboration%2C+C">CUPID-0 collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=%3A"> :</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barrera%2C+M+T">M. T. Barrera</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beretta%2C+M">M. Beretta</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cremonesi%2C+O">O. Cremonesi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cruciani%2C+A">A. Cruciani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=D%27Addabbo%2C+A">A. D&#39;Addabbo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Dafinei%2C+I">I. Dafinei</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Di+Domizio%2C+S">S. Di Domizio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ferroni%2C+F">F. Ferroni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Gironi%2C+L">L. Gironi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Giuliani%2C+A">A. Giuliani</a> , et al. (28 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="1802.07791v3-abstract-short" style="display: inline;"> We report the result of the search for neutrinoless double beta decay of $^{82}$Se obtained with CUPID-0, the first large array of scintillating Zn$^{82}$Se cryogenic calorimeters implementing particle identification. We observe no signal in a 1.83 kg yr $^{82}$Se exposure and we set the most stringent lower limit on the \onu $^{82}$Se half-life T$^{0谓}_{1/2}&gt;$ 2.4$\times \mathrm{10}^{24}$ yr (90\&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1802.07791v3-abstract-full').style.display = 'inline'; document.getElementById('1802.07791v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1802.07791v3-abstract-full" style="display: none;"> We report the result of the search for neutrinoless double beta decay of $^{82}$Se obtained with CUPID-0, the first large array of scintillating Zn$^{82}$Se cryogenic calorimeters implementing particle identification. We observe no signal in a 1.83 kg yr $^{82}$Se exposure and we set the most stringent lower limit on the \onu $^{82}$Se half-life T$^{0谓}_{1/2}&gt;$ 2.4$\times \mathrm{10}^{24}$ yr (90\% credible interval), which corresponds to an effective Majorana neutrino mass m$_{尾尾} &lt;$ (376-770) meV depending on the nuclear matrix element calculations. The heat-light readout provides a powerful tool for the rejection of \al\ particles and allows to suppress the background in the region of interest down to (3.6$^{+1.9}_{-1.4}$)$\times$10$^{-3}$\ckky, an unprecedented level for this technique. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1802.07791v3-abstract-full').style.display = 'none'; document.getElementById('1802.07791v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 June, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 February, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 120, 232502 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1801.05403">arXiv:1801.05403</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1801.05403">pdf</a>, <a href="https://arxiv.org/format/1801.05403">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> Study of Rare Nuclear Processes with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chott%2C+N">N. Chott</a> , et al. (94 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="1801.05403v2-abstract-short" style="display: inline;"> TeO2 bolometers have been used for many years to search for neutrinoless double beta decay in 130-Te. CUORE, a tonne-scale TeO2 detector array, recently published the most sensitive limit on the half-life, $T_{1/2}^{0谓} &gt; 1.5 \times 10^{25}\,$yr, which corresponds to an upper bound of $140-400$~meV on the effective Majorana mass of the neutrino. While it makes CUORE a world-leading experiment look&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1801.05403v2-abstract-full').style.display = 'inline'; document.getElementById('1801.05403v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1801.05403v2-abstract-full" style="display: none;"> TeO2 bolometers have been used for many years to search for neutrinoless double beta decay in 130-Te. CUORE, a tonne-scale TeO2 detector array, recently published the most sensitive limit on the half-life, $T_{1/2}^{0谓} &gt; 1.5 \times 10^{25}\,$yr, which corresponds to an upper bound of $140-400$~meV on the effective Majorana mass of the neutrino. While it makes CUORE a world-leading experiment looking for neutrinoless double beta decay, it is not the only study that CUORE will contribute to in the field of nuclear and particle physics. As already done over the years with many small-scale experiments, CUORE will investigate both rare decays (such as the two-neutrino double beta decay of 130-Te and the hypothesized electron capture in 123-Te), and rare processes (e.g., dark matter and axion interactions). This paper describes some of the achievements of past experiments that used TeO2 bolometers, and perspectives for CUORE. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1801.05403v2-abstract-full').style.display = 'none'; document.getElementById('1801.05403v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 17 January, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 16 January, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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">36 pages, 13 figures, sumbitted to IJMPA Special Issue &#34;Results and Developments in the investigation of rare nuclear decays and processes&#34;</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1710.07988">arXiv:1710.07988</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1710.07988">pdf</a>, <a href="https://arxiv.org/format/1710.07988">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <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.120.132501">10.1103/PhysRevLett.120.132501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> First Results from CUORE: A Search for Lepton Number Violation via $0谓尾尾$ Decay of $^{130}$Te </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Andreotti%2C+E">E. Andreotti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Arnaboldi%2C+C">C. Arnaboldi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bandac%2C+I">I. Bandac</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Banks%2C+T+I">T. I. Banks</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Barucci%2C+M">M. Barucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biare%2C+D">D. Biare</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bryant%2C+A">A. Bryant</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Buccheri%2C+A">A. Buccheri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bulfon%2C+C">C. Bulfon</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camacho%2C+A">A. Camacho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a> , et al. (140 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="1710.07988v3-abstract-short" style="display: inline;"> The CUORE experiment, a ton-scale cryogenic bolometer array, recently began operation at the Laboratori Nazionali del Gran Sasso in Italy. The array represents a significant advancement in this technology, and in this work we apply it for the first time to a high-sensitivity search for a lepton-number--violating process: $^{130}$Te neutrinoless double-beta decay. Examining a total TeO$_2$ exposure&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1710.07988v3-abstract-full').style.display = 'inline'; document.getElementById('1710.07988v3-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1710.07988v3-abstract-full" style="display: none;"> The CUORE experiment, a ton-scale cryogenic bolometer array, recently began operation at the Laboratori Nazionali del Gran Sasso in Italy. The array represents a significant advancement in this technology, and in this work we apply it for the first time to a high-sensitivity search for a lepton-number--violating process: $^{130}$Te neutrinoless double-beta decay. Examining a total TeO$_2$ exposure of 86.3 kg$\cdot$yr, characterized by an effective energy resolution of (7.7 $\pm$ 0.5) keV FWHM and a background in the region of interest of (0.014 $\pm$ 0.002) counts/(keV$\cdot$kg$\cdot$yr), we find no evidence for neutrinoless double-beta decay. The median statistical sensitivity of this search is $7.0\times10^{24}$ yr. Including systematic uncertainties, we place a lower limit on the decay half-life of $T^{0谓}_{1/2}$($^{130}$Te) &gt; $1.3\times 10^{25}$ yr (90% C.L.). Combining this result with those of two earlier experiments, Cuoricino and CUORE-0, we find $T^{0谓}_{1/2}$($^{130}$Te) &gt; $1.5\times 10^{25}$ yr (90% C.L.), which is the most stringent limit to date on this decay. Interpreting this result as a limit on the effective Majorana neutrino mass, we find $m_{尾尾}&lt;(110 - 520)$ meV, where the range reflects the nuclear matrix element estimates employed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1710.07988v3-abstract-full').style.display = 'none'; document.getElementById('1710.07988v3-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 April, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 22 October, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">Published in PRL, reference and DOI added</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 120, 132501 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1710.07459">arXiv:1710.07459</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1710.07459">pdf</a>, <a href="https://arxiv.org/ps/1710.07459">ps</a>, <a href="https://arxiv.org/format/1710.07459">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </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/PhysRevC.97.055502">10.1103/PhysRevC.97.055502 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Neutrinoless $尾^{+}\hspace{-0.2em}EC$ Decay of $^{120}$Te with CUORE-0 </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Artusa%2C+D+R">D. R. Artusa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camacho%2C+A">A. Camacho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</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="1710.07459v1-abstract-short" style="display: inline;"> We have performed a search for neutrinoless $尾^{+}\hspace{-0.2em}EC$ decay of $^{120}$Te using the final CUORE-0 data release. We describe a new analysis method for the simultaneous fit of signatures with different event topology, and of data subsets with different signal efficiency, obtaining a limit on the half-life of the decay of $T_{1/2}&gt;1.6\cdot10^{21}$ yr at $90\%$ CI. Combining this with r&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1710.07459v1-abstract-full').style.display = 'inline'; document.getElementById('1710.07459v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1710.07459v1-abstract-full" style="display: none;"> We have performed a search for neutrinoless $尾^{+}\hspace{-0.2em}EC$ decay of $^{120}$Te using the final CUORE-0 data release. We describe a new analysis method for the simultaneous fit of signatures with different event topology, and of data subsets with different signal efficiency, obtaining a limit on the half-life of the decay of $T_{1/2}&gt;1.6\cdot10^{21}$ yr at $90\%$ CI. Combining this with results from Cuoricino, a predecessor experiment, we obtain the strongest limit to date, corresponding to $T_{1/2}&gt;2.7\cdot10^{21}$ yr at $90\%$ CI. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1710.07459v1-abstract-full').style.display = 'none'; document.getElementById('1710.07459v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 October, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">10 pages, 6 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. C 97, 055502 (2018) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1708.07809">arXiv:1708.07809</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1708.07809">pdf</a>, <a href="https://arxiv.org/format/1708.07809">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Low Energy Analysis Techniques for CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Artusa%2C+D+R">D. R. Artusa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Beeman%2C+J+W">J. W. Beeman</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camacho%2C+A">A. Camacho</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a> , et al. (99 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="1708.07809v2-abstract-short" style="display: inline;"> CUORE is a tonne-scale cryogenic detector operating at the Laboratori Nazionali del Gran Sasso (LNGS) that uses tellurium dioxide bolometers to search for neutrinoless double-beta decay of $^{130}$Te. CUORE is also suitable to search for low energy rare events such as solar axions or WIMP scattering, thanks to its ultra-low background and large target mass. However, to conduct such sensitive searc&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1708.07809v2-abstract-full').style.display = 'inline'; document.getElementById('1708.07809v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1708.07809v2-abstract-full" style="display: none;"> CUORE is a tonne-scale cryogenic detector operating at the Laboratori Nazionali del Gran Sasso (LNGS) that uses tellurium dioxide bolometers to search for neutrinoless double-beta decay of $^{130}$Te. CUORE is also suitable to search for low energy rare events such as solar axions or WIMP scattering, thanks to its ultra-low background and large target mass. However, to conduct such sensitive searches requires improving the energy threshold to 10 keV. In this paper, we describe the analysis techniques developed for the low energy analysis of CUORE-like detectors, using the data acquired from November 2013 to March 2015 by CUORE-0, a single-tower prototype designed to validate the assembly procedure and new cleaning techniques of CUORE. We explain the energy threshold optimization, continuous monitoring of the trigger efficiency, data and event selection, and energy calibration at low energies in detail. We also present the low energy background spectrum of CUORE-0 below 60keV. Finally, we report the sensitivity of CUORE to WIMP annual modulation using the CUORE-0 energy threshold and background, as well as an estimate of the uncertainty on the nuclear quenching factor from nuclear recoils in CUORE-0. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1708.07809v2-abstract-full').style.display = 'none'; document.getElementById('1708.07809v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 December, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 25 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">Comments:</span> <span class="has-text-grey-dark mathjax">11 pages, 6 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C (2017) 77: 857 </p> </li> </ol> <nav class="pagination is-small is-centered breathe-horizontal" role="navigation" aria-label="pagination"> <a href="" class="pagination-previous is-invisible">Previous </a> <a href="/search/?searchtype=author&amp;query=Casali%2C+N&amp;start=50" class="pagination-next" >Next </a> <ul class="pagination-list"> <li> <a href="/search/?searchtype=author&amp;query=Casali%2C+N&amp;start=0" class="pagination-link is-current" aria-label="Goto page 1">1 </a> </li> <li> <a href="/search/?searchtype=author&amp;query=Casali%2C+N&amp;start=50" class="pagination-link " aria-label="Page 2" aria-current="page">2 </a> </li> </ul> </nav> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- 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