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Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </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/s10052-013-2365-2">10.1140/epjc/s10052-013-2365-2 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The MEG detector for $渭+\to e+纬$ decay search </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=Adam%2C+J">J. Adam</a>, <a href="/search/physics?searchtype=author&amp;query=Bai%2C+X">X. Bai</a>, <a href="/search/physics?searchtype=author&amp;query=Baldini%2C+A+M">A. M. Baldini</a>, <a href="/search/physics?searchtype=author&amp;query=Baracchini%2C+E">E. Baracchini</a>, <a href="/search/physics?searchtype=author&amp;query=Bemporad%2C+C">C. Bemporad</a>, <a href="/search/physics?searchtype=author&amp;query=Boca%2C+G">G. Boca</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=Cavoto%2C+G">G. Cavoto</a>, <a href="/search/physics?searchtype=author&amp;query=Cei%2C+F">F. Cei</a>, <a href="/search/physics?searchtype=author&amp;query=Cerri%2C+C">C. Cerri</a>, <a href="/search/physics?searchtype=author&amp;query=Corbo%2C+M">M. Corbo</a>, <a href="/search/physics?searchtype=author&amp;query=Curalli%2C+N">N. Curalli</a>, <a href="/search/physics?searchtype=author&amp;query=De+Bari%2C+A">A. De Bari</a>, <a href="/search/physics?searchtype=author&amp;query=De+Gerone%2C+M">M. De Gerone</a>, <a href="/search/physics?searchtype=author&amp;query=Del+Frate%2C+L">L. Del Frate</a>, <a href="/search/physics?searchtype=author&amp;query=Doke%2C+S">S. Doke</a>, <a href="/search/physics?searchtype=author&amp;query=Dussoni%2C+S">S. Dussoni</a>, <a href="/search/physics?searchtype=author&amp;query=Egger%2C+J">J. Egger</a>, <a href="/search/physics?searchtype=author&amp;query=Fratini%2C+K">K. Fratini</a>, <a href="/search/physics?searchtype=author&amp;query=Fujii%2C+Y">Y. Fujii</a>, <a href="/search/physics?searchtype=author&amp;query=Galli%2C+L">L. Galli</a>, <a href="/search/physics?searchtype=author&amp;query=Galeotti%2C+S">S. Galeotti</a>, <a href="/search/physics?searchtype=author&amp;query=Gallucci%2C+G">G. Gallucci</a>, <a href="/search/physics?searchtype=author&amp;query=Gatti%2C+F">F. Gatti</a>, <a href="/search/physics?searchtype=author&amp;query=Golden%2C+B">B. Golden</a> , et al. (51 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="1303.2348v4-abstract-short" style="display: inline;"> The MEG (Mu to Electron Gamma) experiment has been running at the Paul Scherrer Institut (PSI), Switzerland since 2008 to search for the decay \meg\ by using one of the most intense continuous $渭^+$ beams in the world. This paper presents the MEG components: the positron spectrometer, including a thin target, a superconducting magnet, a set of drift chambers for measuring the muon decay vertex and&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1303.2348v4-abstract-full').style.display = 'inline'; document.getElementById('1303.2348v4-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1303.2348v4-abstract-full" style="display: none;"> The MEG (Mu to Electron Gamma) experiment has been running at the Paul Scherrer Institut (PSI), Switzerland since 2008 to search for the decay \meg\ by using one of the most intense continuous $渭^+$ beams in the world. This paper presents the MEG components: the positron spectrometer, including a thin target, a superconducting magnet, a set of drift chambers for measuring the muon decay vertex and the positron momentum, a timing counter for measuring the positron time, and a liquid xenon detector for measuring the photon energy, position and time. The trigger system, the read-out electronics and the data acquisition system are also presented in detail. The paper is completed with a description of the equipment and techniques developed for the calibration in time and energy and the simulation of the whole apparatus. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1303.2348v4-abstract-full').style.display = 'none'; document.getElementById('1303.2348v4-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, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 10 March, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2013. </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">59 pages, 90 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Eur. Phys. J. C, 73 (2013) 2365 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1303.0754">arXiv:1303.0754</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1303.0754">pdf</a>, <a href="https://arxiv.org/ps/1303.0754">ps</a>, <a href="https://arxiv.org/format/1303.0754">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="Instrumentation and Detectors">physics.ins-det</span> </div> </div> <p class="title is-5 mathjax"> New constraint on the existence of the mu+-&gt; e+ gamma decay </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=MEG+Collaboration"> MEG Collaboration</a>, <a href="/search/physics?searchtype=author&amp;query=Adam%2C+J">J. Adam</a>, <a href="/search/physics?searchtype=author&amp;query=Bai%2C+X">X. Bai</a>, <a href="/search/physics?searchtype=author&amp;query=Baldini%2C+A+M">A. M. Baldini</a>, <a href="/search/physics?searchtype=author&amp;query=Baracchini%2C+E">E. Baracchini</a>, <a href="/search/physics?searchtype=author&amp;query=Bemporad%2C+C">C. Bemporad</a>, <a href="/search/physics?searchtype=author&amp;query=Boca%2C+G">G. Boca</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=Cavoto%2C+G">G. Cavoto</a>, <a href="/search/physics?searchtype=author&amp;query=Cei%2C+F">F. Cei</a>, <a href="/search/physics?searchtype=author&amp;query=Cerri%2C+C">C. Cerri</a>, <a href="/search/physics?searchtype=author&amp;query=de+Bari%2C+A">A. de Bari</a>, <a href="/search/physics?searchtype=author&amp;query=De+Gerone%2C+M">M. De Gerone</a>, <a href="/search/physics?searchtype=author&amp;query=Doke%2C+T">T. Doke</a>, <a href="/search/physics?searchtype=author&amp;query=Dussoni%2C+S">S. Dussoni</a>, <a href="/search/physics?searchtype=author&amp;query=Egger%2C+J">J. Egger</a>, <a href="/search/physics?searchtype=author&amp;query=Fratini%2C+K">K. Fratini</a>, <a href="/search/physics?searchtype=author&amp;query=Fujii%2C+Y">Y. Fujii</a>, <a href="/search/physics?searchtype=author&amp;query=Galli%2C+L">L. Galli</a>, <a href="/search/physics?searchtype=author&amp;query=Gallucci%2C+G">G. Gallucci</a>, <a href="/search/physics?searchtype=author&amp;query=Gatti%2C+F">F. Gatti</a>, <a href="/search/physics?searchtype=author&amp;query=Golden%2C+B">B. Golden</a>, <a href="/search/physics?searchtype=author&amp;query=Grassi%2C+M">M. Grassi</a>, <a href="/search/physics?searchtype=author&amp;query=Graziosi%2C+A">A. Graziosi</a>, <a href="/search/physics?searchtype=author&amp;query=Grigoriev%2C+D+N">D. N. Grigoriev</a> , et al. (49 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="1303.0754v2-abstract-short" style="display: inline;"> The analysis of a combined data set, totaling 3.6 \times 10^14 stopped muons on target, in the search for the lepton flavour violating decay mu^+ -&gt; e^+ gamma is presented. The data collected by the MEG experiment at the Paul Scherrer Institut show no excess of events compared to background expectations and yield a new upper limit on the branching ratio of this decay of 5.7 \times 10^-13 (90% conf&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1303.0754v2-abstract-full').style.display = 'inline'; document.getElementById('1303.0754v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1303.0754v2-abstract-full" style="display: none;"> The analysis of a combined data set, totaling 3.6 \times 10^14 stopped muons on target, in the search for the lepton flavour violating decay mu^+ -&gt; e^+ gamma is presented. The data collected by the MEG experiment at the Paul Scherrer Institut show no excess of events compared to background expectations and yield a new upper limit on the branching ratio of this decay of 5.7 \times 10^-13 (90% confidence level). This represents a four times more stringent limit than the previous world best limit set by MEG. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1303.0754v2-abstract-full').style.display = 'none'; document.getElementById('1303.0754v2-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 April, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 March, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">5 pages, 3 figures, a version accepted in Phys. Rev. Lett</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1112.0110">arXiv:1112.0110</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1112.0110">pdf</a>, <a href="https://arxiv.org/format/1112.0110">other</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> </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/10.1109/TNS.2012.2187311">10.1109/TNS.2012.2187311 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Development and commissioning of the Timing Counter for the MEG Experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=De+Gerone%2C+M">M. De Gerone</a>, <a href="/search/physics?searchtype=author&amp;query=Dussoni%2C+S">S. Dussoni</a>, <a href="/search/physics?searchtype=author&amp;query=Fratini%2C+K">K. Fratini</a>, <a href="/search/physics?searchtype=author&amp;query=Gatti%2C+F">F. Gatti</a>, <a href="/search/physics?searchtype=author&amp;query=Valle%2C+R">R. Valle</a>, <a href="/search/physics?searchtype=author&amp;query=Boca%2C+G">G. Boca</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=Nard%C3%B2%2C+R">R. Nard貌</a>, <a href="/search/physics?searchtype=author&amp;query=Rossella%2C+M">M. Rossella</a>, <a href="/search/physics?searchtype=author&amp;query=Galli%2C+L">L. Galli</a>, <a href="/search/physics?searchtype=author&amp;query=Grassi%2C+M">M. Grassi</a>, <a href="/search/physics?searchtype=author&amp;query=Nicol%C3%B2%2C+D">D. Nicol貌</a>, <a href="/search/physics?searchtype=author&amp;query=Uchiyama%2C+Y">Y. Uchiyama</a>, <a href="/search/physics?searchtype=author&amp;query=Zanello%2C+D">D. Zanello</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="1112.0110v2-abstract-short" style="display: inline;"> The Timing Counter of the MEG (Mu to Electron Gamma) experiment is designed to deliver trigger information and to accurately measure the timing of the $e^+$ in searching for the decay $渭^+ \rightarrow e^+纬$. It is part of a magnetic spectrometer with the $渭^+$ decay target in the center. It consists of two sectors upstream and downstream the target, each one with two layers: the inner one made wit&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1112.0110v2-abstract-full').style.display = 'inline'; document.getElementById('1112.0110v2-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1112.0110v2-abstract-full" style="display: none;"> The Timing Counter of the MEG (Mu to Electron Gamma) experiment is designed to deliver trigger information and to accurately measure the timing of the $e^+$ in searching for the decay $渭^+ \rightarrow e^+纬$. It is part of a magnetic spectrometer with the $渭^+$ decay target in the center. It consists of two sectors upstream and downstream the target, each one with two layers: the inner one made with scintillating fibers read out by APDs for trigger and track reconstruction, the outer one consisting in scintillating bars read out by PMTs for trigger and time measurement. The design criteria, the obtained performances and the commissioning of the detector are presented herein. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1112.0110v2-abstract-full').style.display = 'none'; document.getElementById('1112.0110v2-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 February, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 1 December, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2011. </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, 20 figures. Presented at the IEEE Nuclear Science Symposium 2010, Knoxville, TN, USA. Accepted by IEEE Transaction on Nuclear Science</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> IEEE Trans. on Nucl. Sci. Vol.59, No.2, (2012) 379-388 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1111.6482">arXiv:1111.6482</a> <span>&nbsp;[<a href="https://arxiv.org/pdf/1111.6482">pdf</a>]&nbsp;</span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Geophysics">physics.geo-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</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.dsr.2011.06.006">10.1016/j.dsr.2011.06.006 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&amp;query=van+Haren%2C+H">H. van Haren</a>, <a href="/search/physics?searchtype=author&amp;query=Taupier-Letage%2C+I">I. Taupier-Letage</a>, <a href="/search/physics?searchtype=author&amp;query=Aguilar%2C+J+A">J. A. Aguilar</a>, <a href="/search/physics?searchtype=author&amp;query=Albert%2C+A">A. Albert</a>, <a href="/search/physics?searchtype=author&amp;query=Anghinolfi%2C+M">M. Anghinolfi</a>, <a href="/search/physics?searchtype=author&amp;query=Anton%2C+G">G. Anton</a>, <a href="/search/physics?searchtype=author&amp;query=Anvar%2C+S">S. Anvar</a>, <a href="/search/physics?searchtype=author&amp;query=Ardid%2C+M">M. Ardid</a>, <a href="/search/physics?searchtype=author&amp;query=Jesus%2C+A+C+A">A. C. Assis Jesus</a>, <a href="/search/physics?searchtype=author&amp;query=Astraatmadja%2C+T">T. Astraatmadja</a>, <a href="/search/physics?searchtype=author&amp;query=Aubert%2C+J+-">J. -J. Aubert</a>, <a href="/search/physics?searchtype=author&amp;query=Auer%2C+R">R. Auer</a>, <a href="/search/physics?searchtype=author&amp;query=Baret%2C+B">B. Baret</a>, <a href="/search/physics?searchtype=author&amp;query=Basa%2C+S">S. Basa</a>, <a href="/search/physics?searchtype=author&amp;query=Bazzotti%2C+M">M. Bazzotti</a>, <a href="/search/physics?searchtype=author&amp;query=Bertin%2C+V">V. Bertin</a>, <a href="/search/physics?searchtype=author&amp;query=Biagi%2C+S">S. Biagi</a>, <a href="/search/physics?searchtype=author&amp;query=Bigongiari%2C+C">C. Bigongiari</a>, <a href="/search/physics?searchtype=author&amp;query=Bou-Cabof%2C+M">M. Bou-Cabof</a>, <a href="/search/physics?searchtype=author&amp;query=Bouwhuis%2C+M+C">M. C. Bouwhuis</a>, <a href="/search/physics?searchtype=author&amp;query=Brown%2C+A">A. Brown</a>, <a href="/search/physics?searchtype=author&amp;query=Brunner%2C+J">J. Brunner</a>, <a href="/search/physics?searchtype=author&amp;query=Busto%2C+J">J. Busto</a>, <a href="/search/physics?searchtype=author&amp;query=Camarena%2C+F">F. Camarena</a>, <a href="/search/physics?searchtype=author&amp;query=Capone%2C+A">A. Capone</a> , et al. (116 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="1111.6482v1-abstract-short" style="display: inline;"> An Acoustic Doppler Current Profiler (ADCP) was moored at the deep-sea site of the ANTARES neutrino telescope near Toulon, France, thus providing a unique opportunity to compare high-resolution acoustic and optical observations between 70 and 170 m above the sea bed at 2475 m. The ADCP measured downward vertical currents of magnitudes up to 0.03 m s-1 in late winter and early spring 2006. In the s&hellip; <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.6482v1-abstract-full').style.display = 'inline'; document.getElementById('1111.6482v1-abstract-short').style.display = 'none';">&#9661; More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1111.6482v1-abstract-full" style="display: none;"> An Acoustic Doppler Current Profiler (ADCP) was moored at the deep-sea site of the ANTARES neutrino telescope near Toulon, France, thus providing a unique opportunity to compare high-resolution acoustic and optical observations between 70 and 170 m above the sea bed at 2475 m. The ADCP measured downward vertical currents of magnitudes up to 0.03 m s-1 in late winter and early spring 2006. In the same period, observations were made of enhanced levels of acoustic reflection, interpreted as suspended particles including zooplankton, by a factor of about 10 and of horizontal currents reaching 0.35 m s-1. These observations coincided with high light levels detected by the telescope, interpreted as increased bioluminescence. During winter 2006 deep dense-water formation occurred in the Ligurian subbasin, thus providing a possible explanation for these observations. However, the 10-20 days quasi-periodic episodes of high levels of acoustic reflection, light and large vertical currents continuing into the summer are not direct evidence of this process. It is hypothesized that the main process allowing for suspended material to be moved vertically later in the year is local advection, linked with topographic boundary current instabilities along the rim of the &#39;Northern Current&#39;. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1111.6482v1-abstract-full').style.display = 'none'; document.getElementById('1111.6482v1-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, 2011; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2011. </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">30 pages, 7 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">MSC Class:</span> 86-02 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Deep-Sea Research I, 58 (2011), 875-884 </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 2020-02-24</a>&nbsp;&nbsp;</span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary"> <!-- MetaColumn 1 --> <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 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