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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/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/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/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/2012.11749">arXiv:2012.11749</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/2012.11749">pdf</a>, <a href="https://arxiv.org/format/2012.11749">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.126.171801">10.1103/PhysRevLett.126.171801 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Measurement of the 2$谓尾尾$ Decay Half-life of $^{130}$Te with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Camilleri%2C+J">J. Camilleri</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a> , et al. (88 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2012.11749v2-abstract-short" style="display: inline;"> We measured two-neutrino double beta decay of $^{130}$Te using an exposure of 300.7 kg$\cdot$yr accumulated with the CUORE detector. Using a Bayesian analysis to fit simulated spectra to experimental data, it was possible to disentangle all the major background sources and precisely measure the two-neutrino contribution. The half-life is in agreement with past measurements with a strongly reduced&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.11749v2-abstract-full').style.display = 'inline'; document.getElementById('2012.11749v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2012.11749v2-abstract-full" style="display: none;"> We measured two-neutrino double beta decay of $^{130}$Te using an exposure of 300.7 kg$\cdot$yr accumulated with the CUORE detector. Using a Bayesian analysis to fit simulated spectra to experimental data, it was possible to disentangle all the major background sources and precisely measure the two-neutrino contribution. The half-life is in agreement with past measurements with a strongly reduced uncertainty: $T^{2谓}_{1/2} = 7.71^{+0.08}_{-0.06}\mathrm{(stat.)}^{+0.12}_{-0.15}\mathrm{(syst.)}\times10^{20}$ yr. This measurement is the most precise determination of the $^{130}$Te 2$谓尾尾$ decay half-life to date. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2012.11749v2-abstract-full').style.display = 'none'; document.getElementById('2012.11749v2-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 May, 2021; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 21 December, 2020; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2020. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Published in PRL</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">ACM Class:</span> J.2 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys. Rev. Lett. 126, 171801 (2021) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/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/1912.10966">arXiv:1912.10966</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1912.10966">pdf</a>, <a href="https://arxiv.org/format/1912.10966">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevLett.124.122501">10.1103/PhysRevLett.124.122501 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Improved Limit on Neutrinoless Double-Beta Decay in $^{130}$Te with CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chott%2C+N">N. Chott</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a> , et al. (86 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1912.10966v1-abstract-short" style="display: inline;"> We report new results from the search for neutrinoless double-beta decay in $^{130}$Te with the CUORE detector. This search benefits from a four-fold increase in exposure, lower trigger thresholds and analysis improvements relative to our previous results. We observe a background of $(1.38\pm0.07)\cdot10^{-2}$ counts$/($keV$\cdot$kg$\cdot$yr$)$ in the $0谓尾尾$ decay region of interest and, with a to&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1912.10966v1-abstract-full').style.display = 'inline'; document.getElementById('1912.10966v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1912.10966v1-abstract-full" style="display: none;"> We report new results from the search for neutrinoless double-beta decay in $^{130}$Te with the CUORE detector. This search benefits from a four-fold increase in exposure, lower trigger thresholds and analysis improvements relative to our previous results. We observe a background of $(1.38\pm0.07)\cdot10^{-2}$ counts$/($keV$\cdot$kg$\cdot$yr$)$ in the $0谓尾尾$ decay region of interest and, with a total exposure of 372.5 kg$\cdot$yr, we attain a median exclusion sensitivity of $1.7\cdot10^{25}$ yr. We find no evidence for $0谓尾尾$ decay and set a $90\%$ CI Bayesian lower limit of $3.2\cdot10^{25}$ yr on the $^{130}$Te half-life for this process. In the hypothesis that $0谓尾尾$ decay is mediated by light Majorana neutrinos, this results in an upper limit on the effective Majorana mass of 75-350 meV, depending on the nuclear matrix elements used. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1912.10966v1-abstract-full').style.display = 'none'; document.getElementById('1912.10966v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 23 December, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1905.07667">arXiv:1905.07667</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1905.07667">pdf</a>, <a href="https://arxiv.org/format/1905.07667">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> </div> <p class="title is-5 mathjax"> Results of CUORE </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=Dell%27Oro%2C+S">S. Dell&#39;Oro</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chott%2C+N">N. Chott</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Clemenza%2C+M">M. Clemenza</a> , et al. (87 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1905.07667v1-abstract-short" style="display: inline;"> The Cryogenic Underground Observatory for Rare Events (CUORE) at the Laboratori Nazionali del Gran Sasso, Italy, is the world&#39;s largest bolometric experiment. The detector consists of an array of 988 TeO2 crystals, for a total mass of 742 kg. CUORE is presently in data taking, searching for the neutrinoless double beta decay of 130 Te. CUORE is operational since the spring of 2017. The initial sci&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1905.07667v1-abstract-full').style.display = 'inline'; document.getElementById('1905.07667v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1905.07667v1-abstract-full" style="display: none;"> The Cryogenic Underground Observatory for Rare Events (CUORE) at the Laboratori Nazionali del Gran Sasso, Italy, is the world&#39;s largest bolometric experiment. The detector consists of an array of 988 TeO2 crystals, for a total mass of 742 kg. CUORE is presently in data taking, searching for the neutrinoless double beta decay of 130 Te. CUORE is operational since the spring of 2017. The initial science run already allowed to provide the most stringent limit on the neutrinoless double beta decay half-life of 130Te, and to perform the most precise measurement of the two-neutrino double beta decay half-life. Up to date, we have more than doubled the collected exposure. In this talk, we presenteded the most recent results and discuss the present status of the CUORE experiment. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1905.07667v1-abstract-full').style.display = 'none'; document.getElementById('1905.07667v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 May, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">contribution to the 2019 EW/QCD/Gravitation session of the 54th Rencontres de Moriond</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1808.10342">arXiv:1808.10342</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1808.10342">pdf</a>, <a href="https://arxiv.org/format/1808.10342">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> Update on the recent progress of the CUORE experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/nucl-ex?searchtype=author&amp;query=CUORE+Collaboration"> CUORE Collaboration</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Adams%2C+D+Q">D. Q. Adams</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alduino%2C+C">C. Alduino</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Alfonso%2C+K">K. Alfonso</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Avignone%2C+F+T">F. T. Avignone III</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Azzolini%2C+O">O. Azzolini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bari%2C+G">G. Bari</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bellini%2C+F">F. Bellini</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Benato%2C+G">G. Benato</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bersani%2C+A">A. Bersani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Biassoni%2C+M">M. Biassoni</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Branca%2C+A">A. Branca</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Brofferio%2C+C">C. Brofferio</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Bucci%2C+C">C. Bucci</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Caminata%2C+A">A. Caminata</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Campani%2C+A">A. Campani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Canonica%2C+L">L. Canonica</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cao%2C+X+G">X. G. Cao</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Capelli%2C+S">S. Capelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cappelli%2C+L">L. Cappelli</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cardani%2C+L">L. Cardani</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Carniti%2C+P">P. Carniti</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Casali%2C+N">N. Casali</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Cassina%2C+L">L. Cassina</a>, <a href="/search/nucl-ex?searchtype=author&amp;query=Chiesa%2C+D">D. Chiesa</a> , et al. (96 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1808.10342v1-abstract-short" style="display: inline;"> CUORE is a 741 kg array of 988 TeO$_2$ bolometeric crystals designed to search for the neutrinoless double beta decay of $^{130}$Te and other rare processes. CUORE has been taking data since summer 2017, and as of summer 2018 collected a total of 86.3 kg$\cdot$yr of TeO$_2$ exposure. Based on this exposure, we were able to set a limit on the $0谓尾尾$ half-life of $^{130}$Te of&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1808.10342v1-abstract-full').style.display = 'inline'; document.getElementById('1808.10342v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1808.10342v1-abstract-full" style="display: none;"> CUORE is a 741 kg array of 988 TeO$_2$ bolometeric crystals designed to search for the neutrinoless double beta decay of $^{130}$Te and other rare processes. CUORE has been taking data since summer 2017, and as of summer 2018 collected a total of 86.3 kg$\cdot$yr of TeO$_2$ exposure. Based on this exposure, we were able to set a limit on the $0谓尾尾$ half-life of $^{130}$Te of $T^{0谓}_{1/2}&gt;1.5\times10^{25}$ yr at 90% C.L. At this conference, we showed the decomposition of the CUORE background and were able to extract a $^{130}$Te $2谓尾尾$ half-life of $T_{1/2}^{2谓}=[7.9\pm0.1 \mathrm{(stat.)}\pm0.2 \mathrm{(syst.)}]\times10^{20}$ yr. This is the most precise measurement of this half-life and is consistent with previous measurements. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1808.10342v1-abstract-full').style.display = 'none'; document.getElementById('1808.10342v1-abstract-short').style.display = 'inline';">&#9651; Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 August, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Proceedings of the Neutrino 2018 Conference. 8 pages, 7 figures</span> </p> </li> </ol> <div class="is-hidden-tablet"> <!-- feedback for mobile only --> <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 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