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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="High Energy Physics - Experiment">hep-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1748-0221/16/10/P10024">10.1088/1748-0221/16/10/P10024 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The CaloCube calorimeter for high-energy cosmic-ray measurements in space: performance of a large-scale prototype </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adriani%2C+O">O. Adriani</a>, <a href="/search/physics?searchtype=author&amp;query=Agnesi%2C+A">A. Agnesi</a>, <a href="/search/physics?searchtype=author&amp;query=Albergo%2C+S">S. Albergo</a>, <a href="/search/physics?searchtype=author&amp;query=Antonelli%2C+M">M. Antonelli</a>, <a href="/search/physics?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/physics?searchtype=author&amp;query=Basti%2C+A">A. Basti</a>, <a href="/search/physics?searchtype=author&amp;query=Berti%2C+E">E. Berti</a>, <a href="/search/physics?searchtype=author&amp;query=Bigongiari%2C+G">G. Bigongiari</a>, <a href="/search/physics?searchtype=author&amp;query=Bonechi%2C+L">L. Bonechi</a>, <a href="/search/physics?searchtype=author&amp;query=Bongi%2C+M">M. Bongi</a>, <a href="/search/physics?searchtype=author&amp;query=Bonvicini%2C+V">V. Bonvicini</a>, <a href="/search/physics?searchtype=author&amp;query=Bottai%2C+S">S. Bottai</a>, <a href="/search/physics?searchtype=author&amp;query=Brogi%2C+P">P. Brogi</a>, <a href="/search/physics?searchtype=author&amp;query=Castellini%2C+G">G. Castellini</a>, <a href="/search/physics?searchtype=author&amp;query=Cattaneo%2C+P+W">P. W. Cattaneo</a>, <a href="/search/physics?searchtype=author&amp;query=Checchia%2C+C">C. Checchia</a>, <a href="/search/physics?searchtype=author&amp;query=Alessandro%2C+R+D">R. D Alessandro</a>, <a href="/search/physics?searchtype=author&amp;query=Detti%2C+S">S. Detti</a>, <a href="/search/physics?searchtype=author&amp;query=Fasoli%2C+M">M. Fasoli</a>, <a href="/search/physics?searchtype=author&amp;query=Finetti%2C+N">N. Finetti</a>, <a href="/search/physics?searchtype=author&amp;query=Italiano%2C+A">A. Italiano</a>, <a href="/search/physics?searchtype=author&amp;query=Maestro%2C+P">P. Maestro</a>, <a href="/search/physics?searchtype=author&amp;query=Marrocchesi%2C+P+S">P. S. Marrocchesi</a>, <a href="/search/physics?searchtype=author&amp;query=Mori%2C+N">N. Mori</a>, <a href="/search/physics?searchtype=author&amp;query=Orzan%2C+G">G. Orzan</a> , et al. (23 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2110.01561v1-abstract-short" style="display: inline;"> The direct observation of high-energy cosmic rays, up to the PeV energy region, will increasingly rely on highly performing calorimeters, and the physics performance will be primarily determined by their geometrical acceptance and energy resolution. Thus, it is extremely important to optimize their geometrical design, granularity and absorption depth, with respect to the totalmass of the apparatus&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2110.01561v1-abstract-full').style.display = 'inline'; document.getElementById('2110.01561v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2110.01561v1-abstract-full" style="display: none;"> The direct observation of high-energy cosmic rays, up to the PeV energy region, will increasingly rely on highly performing calorimeters, and the physics performance will be primarily determined by their geometrical acceptance and energy resolution. Thus, it is extremely important to optimize their geometrical design, granularity and absorption depth, with respect to the totalmass of the apparatus, which is amongst the most important constraints for a space mission. CaloCube is an homogeneous calorimeter whose basic geometry is cubic and isotropic, obtained by filling the cubic volume with small cubic scintillating crystals. In this way it is possible to detect particles arriving from every direction in space, thus maximizing the acceptance. This design summarizes a three-year R&amp;D activity, aiming to both optimize and study the full-scale performance of the calorimeter, in the perspective of a cosmic-ray space mission, and investigate a viable technical design by means of the construction of several sizable prototypes. A large scale prototype, made of a mesh of 5x5x18 CsI(Tl) crystals, has been constructed and tested on high-energy particle beams at CERN SPS accelerator. In this paper we describe the CaloCube design and present the results relative to the response of the large scale prototype to electrons. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2110.01561v1-abstract-full').style.display = 'none'; document.getElementById('2110.01561v1-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> 4 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">Comments:</span> <span class="has-text-grey-dark mathjax">24 pages, 19 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/1705.07027">arXiv:1705.07027</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1705.07027">pdf</a>, <a href="https://arxiv.org/format/1705.07027">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> </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/10.1088/1748-0221/12/06/C06004">10.1088/1748-0221/12/06/C06004 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> CaloCube: a novel calorimeter for high-energy cosmic rays in space </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Cattaneo%2C+P+W">P. W. Cattaneo</a>, <a href="/search/physics?searchtype=author&amp;query=Adriani%2C+O">O. Adriani</a>, <a href="/search/physics?searchtype=author&amp;query=Albergo%2C+S">S. Albergo</a>, <a href="/search/physics?searchtype=author&amp;query=Auditore%2C+L">L. Auditore</a>, <a href="/search/physics?searchtype=author&amp;query=Basti%2C+A">A. Basti</a>, <a href="/search/physics?searchtype=author&amp;query=Berti%2C+E">E. Berti</a>, <a href="/search/physics?searchtype=author&amp;query=Bigongiari%2C+G">G. Bigongiari</a>, <a href="/search/physics?searchtype=author&amp;query=Bonechi%2C+L">L. Bonechi</a>, <a href="/search/physics?searchtype=author&amp;query=Bonechi%2C+S">S. Bonechi</a>, <a href="/search/physics?searchtype=author&amp;query=Bongi%2C+M">M. Bongi</a>, <a href="/search/physics?searchtype=author&amp;query=Bonvicini%2C+V">V. Bonvicini</a>, <a href="/search/physics?searchtype=author&amp;query=Bottai%2C+S">S. Bottai</a>, <a href="/search/physics?searchtype=author&amp;query=Brogi%2C+P">P. Brogi</a>, <a href="/search/physics?searchtype=author&amp;query=Carotenuto%2C+G">G. Carotenuto</a>, <a href="/search/physics?searchtype=author&amp;query=Castellini%2C+G">G. Castellini</a>, <a href="/search/physics?searchtype=author&amp;query=%C4%8FAlessandro%2C+R">R. 膹Alessandro</a>, <a href="/search/physics?searchtype=author&amp;query=Detti%2C+S">S. Detti</a>, <a href="/search/physics?searchtype=author&amp;query=Fasoli%2C+M">M. Fasoli</a>, <a href="/search/physics?searchtype=author&amp;query=Finetti%2C+N">N. Finetti</a>, <a href="/search/physics?searchtype=author&amp;query=Italiano%2C+A">A. Italiano</a>, <a href="/search/physics?searchtype=author&amp;query=Lenzi%2C+P">P. Lenzi</a>, <a href="/search/physics?searchtype=author&amp;query=Maestro%2C+P">P. Maestro</a>, <a href="/search/physics?searchtype=author&amp;query=Marrocchesi%2C+P+S">P. S. Marrocchesi</a>, <a href="/search/physics?searchtype=author&amp;query=Mori%2C+N">N. Mori</a>, <a href="/search/physics?searchtype=author&amp;query=Olmi%2C+M">M. Olmi</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="1705.07027v2-abstract-short" style="display: inline;"> In order to extend the direct observation of high-energy cosmic rays up to the PeV region, highly performing calorimeters with large geometrical acceptance and high energy resolution are required. Within the constraint of the total mass of the apparatus, crucial for a space mission, the calorimeters must be optimized with respect to their geometrical acceptance, granularity and absorption depth. C&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1705.07027v2-abstract-full').style.display = 'inline'; document.getElementById('1705.07027v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1705.07027v2-abstract-full" style="display: none;"> In order to extend the direct observation of high-energy cosmic rays up to the PeV region, highly performing calorimeters with large geometrical acceptance and high energy resolution are required. Within the constraint of the total mass of the apparatus, crucial for a space mission, the calorimeters must be optimized with respect to their geometrical acceptance, granularity and absorption depth. CaloCube is a homogeneous calorimeter with cubic geometry, to maximise the acceptance being sensitive to particles from every direction in space; granularity is obtained by relying on small cubic scintillating crystals as active elements. Different scintillating materials have been studied. The crystal sizes and spacing among them have been optimized with respect to the energy resolution. A prototype, based on CsI(Tl) cubic crystals, has been constructed and tested with particle beams. Some results of tests with different beams at CERN are presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1705.07027v2-abstract-full').style.display = 'none'; document.getElementById('1705.07027v2-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 May, 2017; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 19 May, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2017. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Seven pages, seven pictures. 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