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name="order"><option selected value="-announced_date_first">Announcement date (newest first)</option><option value="announced_date_first">Announcement date (oldest first)</option><option value="-submitted_date">Submission date (newest first)</option><option value="submitted_date">Submission date (oldest first)</option><option value="">Relevance</option></select> </span> </div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/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/2401.16059">arXiv:2401.16059</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2401.16059">pdf</a>, <a href="https://arxiv.org/format/2401.16059">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="Nuclear Theory">nucl-th</span> </div> </div> <p class="title is-5 mathjax"> Simultaneous Measurement of Half-Life and Spectral Shape of $^{115}$In $尾$-decay with an Indium Iodide Cryogenic Calorimeter </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=Benato%2C+G">G. Benato</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=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=Corbett%2C+J">J. Corbett</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=Di+Stefano%2C+P">P. Di Stefano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ghislandi%2C+S">S. Ghislandi</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=Helis%2C+D+L">D. L. Helis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Knobel%2C+R">R. Knobel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kostensalo%2C+J">J. Kostensalo</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=Nagorny%2C+S">S. Nagorny</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pessina%2C+G">G. Pessina</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=Puiu%2C+A">A. Puiu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Quitadamo%2C+S">S. Quitadamo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sisti%2C+M">M. Sisti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suhonen%2C+J">J. Suhonen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kuznetsov%2C+S">S. Kuznetsov</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="2401.16059v1-abstract-short" style="display: inline;"> Current bounds on neutrino Majorana mass are affected by significant uncertainties in the nuclear calculations for neutrinoless double-beta decay. A key issue for a data-driven improvement of the nuclear theory is the actual value of the axial coupling constant $g_A$, which can be investigated through forbidden $尾$-decays. We present the first measurement of 4$^{th}$-forbidden $尾$-decay of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2401.16059v1-abstract-full').style.display = 'inline'; document.getElementById('2401.16059v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2401.16059v1-abstract-full" style="display: none;"> Current bounds on neutrino Majorana mass are affected by significant uncertainties in the nuclear calculations for neutrinoless double-beta decay. A key issue for a data-driven improvement of the nuclear theory is the actual value of the axial coupling constant $g_A$, which can be investigated through forbidden $尾$-decays. We present the first measurement of 4$^{th}$-forbidden $尾$-decay of $^{115}$In with a cryogenic calorimeter based on Indium Iodide. Exploiting the enhanced spectral shape method for the first time to this isotope, our study accurately determines simultaneously spectral shape, $g_A$, and half-life. The Interacting Shell Model, which best fits our data, indicates a half-life for this decay at $T_{1/2}=(5.26\pm0.06) \times 10^{14}$,yr. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2401.16059v1-abstract-full').style.display = 'none'; document.getElementById('2401.16059v1-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 January, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 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/2305.01949">arXiv:2305.01949</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2305.01949">pdf</a>, <a href="https://arxiv.org/format/2305.01949">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/10.1140/epjp/s13360-023-03946-x">10.1140/epjp/s13360-023-03946-x <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Array of Cryogenic Calorimeters to Evaluate the Spectral Shape of forbidden $尾$-decays: the ACCESS project </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=Benato%2C+G">G. Benato</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=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=Corbett%2C+J">J. Corbett</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=Di+Stefano%2C+P">P. Di Stefano</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Ghislandi%2C+S">S. Ghislandi</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=Helis%2C+D+L">D. L. Helis</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Knobel%2C+R">R. Knobel</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kostensalo%2C+J">J. Kostensalo</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=Nagorny%2C+S">S. Nagorny</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Pessina%2C+G">G. Pessina</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=Puiu%2C+A">A. Puiu</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Quitadamo%2C+S">S. Quitadamo</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Sisti%2C+M">M. Sisti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Suhonen%2C+J">J. Suhonen</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Kuznetsov%2C+S">S. Kuznetsov</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="2305.01949v1-abstract-short" style="display: inline;"> The ACCESS (Array of Cryogenic Calorimeters to Evaluate Spectral Shapes) project aims to establish a novel technique to perform precision measurements of forbidden \b{eta}-decays, which can serve as an important benchmark for nuclear physics calculations and represent a significant background in astroparticle physics experiments. ACCESS will operate a pilot array of cryogenic calorimeters based on&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2305.01949v1-abstract-full').style.display = 'inline'; document.getElementById('2305.01949v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2305.01949v1-abstract-full" style="display: none;"> The ACCESS (Array of Cryogenic Calorimeters to Evaluate Spectral Shapes) project aims to establish a novel technique to perform precision measurements of forbidden \b{eta}-decays, which can serve as an important benchmark for nuclear physics calculations and represent a significant background in astroparticle physics experiments. ACCESS will operate a pilot array of cryogenic calorimeters based on natural and doped crystals containing \b{eta}-emitting radionuclides. In this way, natural (e.g. 113 Cd and 115In) and synthetic isotopes (e.g. 99Tc) will be simultaneously measured with a common experimental technique. The array will also include further crystals optimised to disentangle the different background sources, thus reducing the systematic uncertainty. In this paper, we give an overview of the ACCESS research program, discussing a detector design study and promising results of 115In. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2305.01949v1-abstract-full').style.display = 'none'; document.getElementById('2305.01949v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 3 May, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 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">12 pages, 12 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. Plus 138, 445 (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/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/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/2202.06279">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/2110.03934">arXiv:2110.03934</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2110.03934">pdf</a>, <a href="https://arxiv.org/format/2110.03934">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/10.1016/j.nima.2022.166682">10.1016/j.nima.2022.166682 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Development of cryogenic calorimeters to measure the spectral shape of In-115 beta decay </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Celi%2C+E">E. Celi</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Galazka%2C+Z">Z. Galazka</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Laubenstein%2C+M">M. Laubenstein</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Nagorny%2C+S">S. Nagorny</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=Pirro%2C+S">S. Pirro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Puiu%2C+A">A. Puiu</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="2110.03934v1-abstract-short" style="display: inline;"> The spectral shape of forbidden beta-decays is a crucial benchmark for nuclear physics calculations and has important implications also for astroparticle physics experiments. Among the interesting isotopes in this field, $^{115}$In is an excellent candidate, being a primordial nuclide featuring a good compromise among Q-value (497.954 keV) and half-life (4.41$\times$10$^{14}$ yr). In this paper, w&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2110.03934v1-abstract-full').style.display = 'inline'; document.getElementById('2110.03934v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2110.03934v1-abstract-full" style="display: none;"> The spectral shape of forbidden beta-decays is a crucial benchmark for nuclear physics calculations and has important implications also for astroparticle physics experiments. Among the interesting isotopes in this field, $^{115}$In is an excellent candidate, being a primordial nuclide featuring a good compromise among Q-value (497.954 keV) and half-life (4.41$\times$10$^{14}$ yr). In this paper, we propose to exploit a cryogenic calorimeter based on In$_2$O$_3$ crystal to perform a high-precision measurement of the $尾$-decay energy spectrum, discussing also the results obtained within a preliminary test of this crystal and the next steps to improve the detector performance. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2110.03934v1-abstract-full').style.display = 'none'; document.getElementById('2110.03934v1-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 October, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> 166682 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl.Instrum.Meth.A 1033 (2022) 166682 </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/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/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/2012.00644">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/2011.09295">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/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> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a 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