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</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/1911.02427">arXiv:1911.02427</a> <span> [<a href="https://arxiv.org/pdf/1911.02427">pdf</a>, <a href="https://arxiv.org/format/1911.02427">other</a>] </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="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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="High Energy Physics - Phenomenology">hep-ph</span> </div> </div> <p class="title is-5 mathjax"> KLASH Conceptual Design Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alesini%2C+D">D. Alesini</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=J.%2C+P+B+S">P. Beltrame S. J.</a>, <a href="/search/physics?searchtype=author&query=Bj%C3%B6rkeroth%2C+F">F. Bj枚rkeroth</a>, <a href="/search/physics?searchtype=author&query=Bossi%2C+F">F. Bossi</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">P. Ciambrone</a>, <a href="/search/physics?searchtype=author&query=Monache%2C+G+D">G. Delle Monache</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">D. Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Falferi%2C+P">P. Falferi</a>, <a href="/search/physics?searchtype=author&query=Gallo%2C+A">A. Gallo</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">C. Gatti</a>, <a href="/search/physics?searchtype=author&query=Ghigo%2C+A">A. Ghigo</a>, <a href="/search/physics?searchtype=author&query=Giannotti%2C+M">M. Giannotti</a>, <a href="/search/physics?searchtype=author&query=Lamanna%2C+G">G. Lamanna</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">C. Ligi</a>, <a href="/search/physics?searchtype=author&query=Maccarrone%2C+G">G. Maccarrone</a>, <a href="/search/physics?searchtype=author&query=Mirizzi%2C+A">A. Mirizzi</a>, <a href="/search/physics?searchtype=author&query=Montanino%2C+D">D. Montanino</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Mostacci%2C+A">A. Mostacci</a>, <a href="/search/physics?searchtype=author&query=M%C3%BCck%2C+M">M. M眉ck</a>, <a href="/search/physics?searchtype=author&query=Nardi%2C+E">E. Nardi</a>, <a href="/search/physics?searchtype=author&query=Nguyen%2C+F">F. Nguyen</a>, <a href="/search/physics?searchtype=author&query=Pellegrino%2C+L">L. Pellegrino</a>, <a href="/search/physics?searchtype=author&query=Rettaroli%2C+A">A. Rettaroli</a> , et al. (4 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1911.02427v1-abstract-short" style="display: inline;"> The last decade witnessed an increasing interest in axions and axion-like particles with many theoretical works published and many new experimental proposals that started a real race towards their discovery. This paper is the Conceptual Design Report of the KLASH (KLoe magnet for Axion SearcH) experiment at the Laboratori Nazionali di Frascati (LNF). The idea of this experiment has been stimulated… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.02427v1-abstract-full').style.display = 'inline'; document.getElementById('1911.02427v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1911.02427v1-abstract-full" style="display: none;"> The last decade witnessed an increasing interest in axions and axion-like particles with many theoretical works published and many new experimental proposals that started a real race towards their discovery. This paper is the Conceptual Design Report of the KLASH (KLoe magnet for Axion SearcH) experiment at the Laboratori Nazionali di Frascati (LNF). The idea of this experiment has been stimulated by the availability of the large volume superconducting magnet, with a moderate magnetic field of 0.6 T, used in the KLOE detector at the DAFNE collider. The main conclusion we draw from this report is the possibility to build and put in operation at LNF in 2-3 years a large haloscope with the sensitivity to KSVZ axions in the low mass range between 0.2 and 1 $渭$eV, complementary to that of other experiments. Timeline and cost are competitive with respect to other proposals in the same mass region thanks to the availability of most of the infrastructure, in particular the superconducting magnet and the cryogenics plant. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1911.02427v1-abstract-full').style.display = 'none'; document.getElementById('1911.02427v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 6 November, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2019. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> INFN-19-18/LNF </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1910.11939">arXiv:1910.11939</a> <span> [<a href="https://arxiv.org/pdf/1910.11939">pdf</a>, <a href="https://arxiv.org/format/1910.11939">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1140/epja/s10050-020-00107-x">10.1140/epja/s10050-020-00107-x <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The BGOOD experimental setup at ELSA </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alef%2C+S">S. Alef</a>, <a href="/search/physics?searchtype=author&query=Bauer%2C+P">P. Bauer</a>, <a href="/search/physics?searchtype=author&query=Bayadilov%2C+D">D. Bayadilov</a>, <a href="/search/physics?searchtype=author&query=Beck%2C+R">R. Beck</a>, <a href="/search/physics?searchtype=author&query=Becker%2C+M">M. Becker</a>, <a href="/search/physics?searchtype=author&query=Bella%2C+A">A. Bella</a>, <a href="/search/physics?searchtype=author&query=Bieling%2C+J">J. Bieling</a>, <a href="/search/physics?searchtype=author&query=Boese%2C+S">S. Boese</a>, <a href="/search/physics?searchtype=author&query=Braghieri%2C+A">A. Braghieri</a>, <a href="/search/physics?searchtype=author&query=Brinkmann%2C+K+-">K. -Th. Brinkmann</a>, <a href="/search/physics?searchtype=author&query=Cole%2C+P">P. Cole</a>, <a href="/search/physics?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/physics?searchtype=author&query=Elsner%2C+D">D. Elsner</a>, <a href="/search/physics?searchtype=author&query=Fantini%2C+A">A. Fantini</a>, <a href="/search/physics?searchtype=author&query=Freyermuth%2C+O">O. Freyermuth</a>, <a href="/search/physics?searchtype=author&query=Frommberger%2C+F">F. Frommberger</a>, <a href="/search/physics?searchtype=author&query=Gervino%2C+G">G. Gervino</a>, <a href="/search/physics?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&query=Goertz%2C+S">S. Goertz</a>, <a href="/search/physics?searchtype=author&query=Gridnev%2C+A">A. Gridnev</a>, <a href="/search/physics?searchtype=author&query=Gutz%2C+E">E. Gutz</a>, <a href="/search/physics?searchtype=author&query=Hammann%2C+D">D. Hammann</a>, <a href="/search/physics?searchtype=author&query=Hannappel%2C+J">J. Hannappel</a>, <a href="/search/physics?searchtype=author&query=Hillert%2C+W">W. Hillert</a>, <a href="/search/physics?searchtype=author&query=Jahn%2C+O">O. Jahn</a> , et al. (36 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="1910.11939v3-abstract-short" style="display: inline;"> The BGOOD experiment at the ELSA facility in Bonn has been commissioned within the framework of an international collaboration. The experiment pursues a systematic investigation of non-strange and strange meson photoproduction, in particular $t$-channel processes at low momentum transfer. The setup uniquely combines a central almost $4蟺$ acceptance BGO crystal calorimeter with a large aperture for… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1910.11939v3-abstract-full').style.display = 'inline'; document.getElementById('1910.11939v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1910.11939v3-abstract-full" style="display: none;"> The BGOOD experiment at the ELSA facility in Bonn has been commissioned within the framework of an international collaboration. The experiment pursues a systematic investigation of non-strange and strange meson photoproduction, in particular $t$-channel processes at low momentum transfer. The setup uniquely combines a central almost $4蟺$ acceptance BGO crystal calorimeter with a large aperture forward magnetic spectrometer providing excellent detection of both neutral and charged particles, complementary to other setups such as Crystal Barrel, Crystal Ball, LEPS and CLAS. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1910.11939v3-abstract-full').style.display = 'none'; document.getElementById('1910.11939v3-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 18 February, 2020; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 24 October, 2019; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">26 pages, 37 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. A (2020) 56:104 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1610.03210">arXiv:1610.03210</a> <span> [<a href="https://arxiv.org/pdf/1610.03210">pdf</a>, <a href="https://arxiv.org/format/1610.03210">other</a>] </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/10.1016/j.nima.2016.10.047">10.1016/j.nima.2016.10.047 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Electron beam test of key elements of the laser-based calibration system for the muon $g$ $-$ $2$ experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Anastasi%2C+A">A. Anastasi</a>, <a href="/search/physics?searchtype=author&query=Basti%2C+A">A. Basti</a>, <a href="/search/physics?searchtype=author&query=Bedeschi%2C+F">F. Bedeschi</a>, <a href="/search/physics?searchtype=author&query=Bartolini%2C+M">M. Bartolini</a>, <a href="/search/physics?searchtype=author&query=Cantatore%2C+G">G. Cantatore</a>, <a href="/search/physics?searchtype=author&query=Cauz%2C+D">D. Cauz</a>, <a href="/search/physics?searchtype=author&query=Corradi%2C+G">G. Corradi</a>, <a href="/search/physics?searchtype=author&query=Dabagov%2C+S">S. Dabagov</a>, <a href="/search/physics?searchtype=author&query=DI+Sciascio%2C+G">G. DI Sciascio</a>, <a href="/search/physics?searchtype=author&query=Di+Stefano%2C+R">R. Di Stefano</a>, <a href="/search/physics?searchtype=author&query=Driutti%2C+A">A. Driutti</a>, <a href="/search/physics?searchtype=author&query=Escalante%2C+O">O. Escalante</a>, <a href="/search/physics?searchtype=author&query=Ferrari%2C+C">C. Ferrari</a>, <a href="/search/physics?searchtype=author&query=Fienberg%2C+A+T">A. T. Fienberg</a>, <a href="/search/physics?searchtype=author&query=Fioretti%2C+A">A. Fioretti</a>, <a href="/search/physics?searchtype=author&query=Gabbanini%2C+C">C. Gabbanini</a>, <a href="/search/physics?searchtype=author&query=Gioiosa%2C+A">A. Gioiosa</a>, <a href="/search/physics?searchtype=author&query=Hampai%2C+D">D. Hampai</a>, <a href="/search/physics?searchtype=author&query=Hertzog%2C+D+W">D. W. Hertzog</a>, <a href="/search/physics?searchtype=author&query=Iacovacci%2C+M">M. Iacovacci</a>, <a href="/search/physics?searchtype=author&query=Karuza%2C+M">M. Karuza</a>, <a href="/search/physics?searchtype=author&query=Kaspar%2C+J">J. Kaspar</a>, <a href="/search/physics?searchtype=author&query=Liedl%2C+A">A. Liedl</a>, <a href="/search/physics?searchtype=author&query=Lusiani%2C+A">A. Lusiani</a>, <a href="/search/physics?searchtype=author&query=Marignetti%2C+F">F. Marignetti</a> , et al. (8 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="1610.03210v1-abstract-short" style="display: inline;"> We report the test of many of the key elements of the laser-based calibration system for muon g - 2 experiment E989 at Fermilab. The test was performed at the Laboratori Nazionali di Frascati's Beam Test Facility using a 450 MeV electron beam impinging on a small subset of the final g - 2 lead-fluoride crystal calorimeter system. The calibration system was configured as planned for the E989 experi… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1610.03210v1-abstract-full').style.display = 'inline'; document.getElementById('1610.03210v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1610.03210v1-abstract-full" style="display: none;"> We report the test of many of the key elements of the laser-based calibration system for muon g - 2 experiment E989 at Fermilab. The test was performed at the Laboratori Nazionali di Frascati's Beam Test Facility using a 450 MeV electron beam impinging on a small subset of the final g - 2 lead-fluoride crystal calorimeter system. The calibration system was configured as planned for the E989 experiment and uses the same type of laser and most of the final optical elements. We show results regarding the calorimeter's response calibration, the maximum equivalent electron energy which can be provided by the laser and the stability of the calibration system components. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1610.03210v1-abstract-full').style.display = 'none'; document.getElementById('1610.03210v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 October, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2016. </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">Submitted to Nuclear Instrument and Methods A</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-PUB-16-441-E-PPD </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1504.00132">arXiv:1504.00132</a> <span> [<a href="https://arxiv.org/pdf/1504.00132">pdf</a>, <a href="https://arxiv.org/format/1504.00132">other</a>] </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/10.1016/j.nima.2015.03.071">10.1016/j.nima.2015.03.071 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Test of candidate light distributors for the muon (g$-$2) laser calibration system </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Anastasi%2C+A">A. Anastasi</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Baffigi%2C+F">F. Baffigi</a>, <a href="/search/physics?searchtype=author&query=Cantatore%2C+G">G. Cantatore</a>, <a href="/search/physics?searchtype=author&query=Cauz%2C+D">D. Cauz</a>, <a href="/search/physics?searchtype=author&query=Corradi%2C+G">G. Corradi</a>, <a href="/search/physics?searchtype=author&query=Dabagov%2C+S">S. Dabagov</a>, <a href="/search/physics?searchtype=author&query=Di+Sciascio%2C+G">G. Di Sciascio</a>, <a href="/search/physics?searchtype=author&query=Di+Stefano%2C+R">R. Di Stefano</a>, <a href="/search/physics?searchtype=author&query=Ferrari%2C+C">C. Ferrari</a>, <a href="/search/physics?searchtype=author&query=Fienberg%2C+A+T">A. T. Fienberg</a>, <a href="/search/physics?searchtype=author&query=Fioretti%2C+A">A. Fioretti</a>, <a href="/search/physics?searchtype=author&query=Fulgentini%2C+L">L. Fulgentini</a>, <a href="/search/physics?searchtype=author&query=Gabbanini%2C+C">C. Gabbanini</a>, <a href="/search/physics?searchtype=author&query=Gizzi%2C+L+A">L. A. Gizzi</a>, <a href="/search/physics?searchtype=author&query=Hampai%2C+D">D. Hampai</a>, <a href="/search/physics?searchtype=author&query=Hertzog%2C+D+W">D. W. Hertzog</a>, <a href="/search/physics?searchtype=author&query=Iacovacci%2C+M">M. Iacovacci</a>, <a href="/search/physics?searchtype=author&query=Karuza%2C+M">M. Karuza</a>, <a href="/search/physics?searchtype=author&query=Kaspar%2C+J">J. Kaspar</a>, <a href="/search/physics?searchtype=author&query=Koester%2C+P">P. Koester</a>, <a href="/search/physics?searchtype=author&query=Labate%2C+L">L. Labate</a>, <a href="/search/physics?searchtype=author&query=Mastroianni%2C+S">S. Mastroianni</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Pauletta%2C+G">G. Pauletta</a> , et al. (2 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="1504.00132v1-abstract-short" style="display: inline;"> The new muon (g-2) experiment E989 at Fermilab will be equipped with a laser calibration system for all the 1296 channels of the calorimeters. An integrating sphere and an alternative system based on an engineered diffuser have been considered as possible light distributors for the experiment. We present here a detailed comparison of the two based on temporal response, spatial uniformity, transmit… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1504.00132v1-abstract-full').style.display = 'inline'; document.getElementById('1504.00132v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1504.00132v1-abstract-full" style="display: none;"> The new muon (g-2) experiment E989 at Fermilab will be equipped with a laser calibration system for all the 1296 channels of the calorimeters. An integrating sphere and an alternative system based on an engineered diffuser have been considered as possible light distributors for the experiment. We present here a detailed comparison of the two based on temporal response, spatial uniformity, transmittance and time stability. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1504.00132v1-abstract-full').style.display = 'none'; document.getElementById('1504.00132v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 1 April, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2015. </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">accepted to Nucl.Instrum.Meth. A</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1502.04317">arXiv:1502.04317</a> <span> [<a href="https://arxiv.org/pdf/1502.04317">pdf</a>, <a href="https://arxiv.org/format/1502.04317">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</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/10.1063/1.4967465">10.1063/1.4967465 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A Storage Ring Experiment to Detect a Proton Electric Dipole Moment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Anastassopoulos%2C+V">V. Anastassopoulos</a>, <a href="/search/physics?searchtype=author&query=Andrianov%2C+S">S. Andrianov</a>, <a href="/search/physics?searchtype=author&query=Baartman%2C+R">R. Baartman</a>, <a href="/search/physics?searchtype=author&query=Bai%2C+M">M. Bai</a>, <a href="/search/physics?searchtype=author&query=Baessler%2C+S">S. Baessler</a>, <a href="/search/physics?searchtype=author&query=Benante%2C+J">J. Benante</a>, <a href="/search/physics?searchtype=author&query=Berz%2C+M">M. Berz</a>, <a href="/search/physics?searchtype=author&query=Blaskiewicz%2C+M">M. Blaskiewicz</a>, <a href="/search/physics?searchtype=author&query=Bowcock%2C+T">T. Bowcock</a>, <a href="/search/physics?searchtype=author&query=Brown%2C+K">K. Brown</a>, <a href="/search/physics?searchtype=author&query=Casey%2C+B">B. Casey</a>, <a href="/search/physics?searchtype=author&query=Conte%2C+M">M. Conte</a>, <a href="/search/physics?searchtype=author&query=Crnkovic%2C+J">J. Crnkovic</a>, <a href="/search/physics?searchtype=author&query=Fanourakis%2C+G">G. Fanourakis</a>, <a href="/search/physics?searchtype=author&query=Fedotov%2C+A">A. Fedotov</a>, <a href="/search/physics?searchtype=author&query=Fierlinger%2C+P">P. Fierlinger</a>, <a href="/search/physics?searchtype=author&query=Fischer%2C+W">W. Fischer</a>, <a href="/search/physics?searchtype=author&query=Gaisser%2C+M+O">M. O. Gaisser</a>, <a href="/search/physics?searchtype=author&query=Giomataris%2C+Y">Y. Giomataris</a>, <a href="/search/physics?searchtype=author&query=Grosse-Perdekamp%2C+M">M. Grosse-Perdekamp</a>, <a href="/search/physics?searchtype=author&query=Guidoboni%2C+G">G. Guidoboni</a>, <a href="/search/physics?searchtype=author&query=Haciomeroglu%2C+S">S. Haciomeroglu</a>, <a href="/search/physics?searchtype=author&query=Hoffstaetter%2C+G">G. Hoffstaetter</a>, <a href="/search/physics?searchtype=author&query=Huang%2C+H">H. Huang</a>, <a href="/search/physics?searchtype=author&query=Incagli%2C+M">M. Incagli</a> , et al. (66 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="1502.04317v1-abstract-short" style="display: inline;"> A new experiment is described to detect a permanent electric dipole moment of the proton with a sensitivity of $10^{-29}e\cdot$cm by using polarized "magic" momentum $0.7$~GeV/c protons in an all-electric storage ring. Systematic errors relevant to the experiment are discussed and techniques to address them are presented. The measurement is sensitive to new physics beyond the Standard Model at the… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1502.04317v1-abstract-full').style.display = 'inline'; document.getElementById('1502.04317v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1502.04317v1-abstract-full" style="display: none;"> A new experiment is described to detect a permanent electric dipole moment of the proton with a sensitivity of $10^{-29}e\cdot$cm by using polarized "magic" momentum $0.7$~GeV/c protons in an all-electric storage ring. Systematic errors relevant to the experiment are discussed and techniques to address them are presented. The measurement is sensitive to new physics beyond the Standard Model at the scale of 3000~TeV. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1502.04317v1-abstract-full').style.display = 'none'; document.getElementById('1502.04317v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 15 February, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">8 pages, 3 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/1501.06858">arXiv:1501.06858</a> <span> [<a href="https://arxiv.org/pdf/1501.06858">pdf</a>] </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> <p class="title is-5 mathjax"> Muon (g-2) Technical Design Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Grange%2C+J">J. Grange</a>, <a href="/search/physics?searchtype=author&query=Guarino%2C+V">V. Guarino</a>, <a href="/search/physics?searchtype=author&query=Winter%2C+P">P. Winter</a>, <a href="/search/physics?searchtype=author&query=Wood%2C+K">K. Wood</a>, <a href="/search/physics?searchtype=author&query=Zhao%2C+H">H. Zhao</a>, <a href="/search/physics?searchtype=author&query=Carey%2C+R+M">R. M. Carey</a>, <a href="/search/physics?searchtype=author&query=Gastler%2C+D">D. Gastler</a>, <a href="/search/physics?searchtype=author&query=Hazen%2C+E">E. Hazen</a>, <a href="/search/physics?searchtype=author&query=Kinnaird%2C+N">N. Kinnaird</a>, <a href="/search/physics?searchtype=author&query=Miller%2C+J+P">J. P. Miller</a>, <a href="/search/physics?searchtype=author&query=Mott%2C+J">J. Mott</a>, <a href="/search/physics?searchtype=author&query=Roberts%2C+B+L">B. L. Roberts</a>, <a href="/search/physics?searchtype=author&query=Benante%2C+J">J. Benante</a>, <a href="/search/physics?searchtype=author&query=Crnkovic%2C+J">J. Crnkovic</a>, <a href="/search/physics?searchtype=author&query=Morse%2C+W+M">W. M. Morse</a>, <a href="/search/physics?searchtype=author&query=Sayed%2C+H">H. Sayed</a>, <a href="/search/physics?searchtype=author&query=Tishchenko%2C+V">V. Tishchenko</a>, <a href="/search/physics?searchtype=author&query=Druzhinin%2C+V+P">V. P. Druzhinin</a>, <a href="/search/physics?searchtype=author&query=Khazin%2C+B+I">B. I. Khazin</a>, <a href="/search/physics?searchtype=author&query=Koop%2C+I+A">I. A. Koop</a>, <a href="/search/physics?searchtype=author&query=Logashenko%2C+I">I. Logashenko</a>, <a href="/search/physics?searchtype=author&query=Shatunov%2C+Y+M">Y. M. Shatunov</a>, <a href="/search/physics?searchtype=author&query=Solodov%2C+E">E. Solodov</a>, <a href="/search/physics?searchtype=author&query=Korostelev%2C+M">M. Korostelev</a>, <a href="/search/physics?searchtype=author&query=Newton%2C+D">D. Newton</a> , et al. (176 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="1501.06858v2-abstract-short" style="display: inline;"> The Muon (g-2) Experiment, E989 at Fermilab, will measure the muon anomalous magnetic moment a factor-of-four more precisely than was done in E821 at the Brookhaven National Laboratory AGS. The E821 result appears to be greater than the Standard-Model prediction by more than three standard deviations. When combined with expected improvement in the Standard-Model hadronic contributions, E989 should… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.06858v2-abstract-full').style.display = 'inline'; document.getElementById('1501.06858v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1501.06858v2-abstract-full" style="display: none;"> The Muon (g-2) Experiment, E989 at Fermilab, will measure the muon anomalous magnetic moment a factor-of-four more precisely than was done in E821 at the Brookhaven National Laboratory AGS. The E821 result appears to be greater than the Standard-Model prediction by more than three standard deviations. When combined with expected improvement in the Standard-Model hadronic contributions, E989 should be able to determine definitively whether or not the E821 result is evidence for physics beyond the Standard Model. After a review of the physics motivation and the basic technique, which will use the muon storage ring built at BNL and now relocated to Fermilab, the design of the new experiment is presented. This document was created in partial fulfillment of the requirements necessary to obtain DOE CD-2/3 approval. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.06858v2-abstract-full').style.display = 'none'; document.getElementById('1501.06858v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 11 May, 2018; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 27 January, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2015. </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">666 pages</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> FERMILAB-FN-0992-E </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1501.04779">arXiv:1501.04779</a> <span> [<a href="https://arxiv.org/pdf/1501.04779">pdf</a>, <a href="https://arxiv.org/format/1501.04779">other</a>] </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/10.5506/APhysPolB.46.81">10.5506/APhysPolB.46.81 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Commissioning of the new taggers of the KLOE-2 experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">P. Ciambrone</a>, <a href="/search/physics?searchtype=author&query=Mascolo%2C+M">M. Mascolo</a>, <a href="/search/physics?searchtype=author&query=Messi%2C+R">R. Messi</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Fiore%2C+S">S. Fiore</a>, <a href="/search/physics?searchtype=author&query=Gauzzi%2C+P">P. Gauzzi</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="1501.04779v1-abstract-short" style="display: inline;"> In order to fully reconstruct the gamma gamma processes (e+e- -> e+e- gamma gamma) in the energy region of the phi meson production, new detectors along the DAFNE beam line have been installed in order to detect the scattered e+e-. </span> <span class="abstract-full has-text-grey-dark mathjax" id="1501.04779v1-abstract-full" style="display: none;"> In order to fully reconstruct the gamma gamma processes (e+e- -> e+e- gamma gamma) in the energy region of the phi meson production, new detectors along the DAFNE beam line have been installed in order to detect the scattered e+e-. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1501.04779v1-abstract-full').style.display = 'none'; document.getElementById('1501.04779v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 January, 2015; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2015. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 5 figures, sumbitted to Acta Physica Polonica B</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1307.7967">arXiv:1307.7967</a> <span> [<a href="https://arxiv.org/pdf/1307.7967">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Experiment">hep-ex</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> </div> </div> <p class="title is-5 mathjax"> IRIDE White Book, An Interdisciplinary Research Infrastructure based on Dual Electron linacs&lasers </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alesini%2C+D">D. Alesini</a>, <a href="/search/physics?searchtype=author&query=Alessandroni%2C+M">M. Alessandroni</a>, <a href="/search/physics?searchtype=author&query=Anania%2C+M+P">M. P. Anania</a>, <a href="/search/physics?searchtype=author&query=Andreas%2C+S">S. Andreas</a>, <a href="/search/physics?searchtype=author&query=Angelone%2C+M">M. Angelone</a>, <a href="/search/physics?searchtype=author&query=Arcovito%2C+A">A. Arcovito</a>, <a href="/search/physics?searchtype=author&query=Arnesano%2C+F">F. Arnesano</a>, <a href="/search/physics?searchtype=author&query=Artioli%2C+M">M. Artioli</a>, <a href="/search/physics?searchtype=author&query=Avaldi%2C+L">L. Avaldi</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Bacci%2C+A">A. Bacci</a>, <a href="/search/physics?searchtype=author&query=Balerna%2C+A">A. Balerna</a>, <a href="/search/physics?searchtype=author&query=Bartalucci%2C+S">S. Bartalucci</a>, <a href="/search/physics?searchtype=author&query=Bedogni%2C+R">R. Bedogni</a>, <a href="/search/physics?searchtype=author&query=Bellaveglia%2C+M">M. Bellaveglia</a>, <a href="/search/physics?searchtype=author&query=Bencivenga%2C+F">F. Bencivenga</a>, <a href="/search/physics?searchtype=author&query=Benfatto%2C+M">M. Benfatto</a>, <a href="/search/physics?searchtype=author&query=Biedron%2C+S">S. Biedron</a>, <a href="/search/physics?searchtype=author&query=Bocci%2C+V">V. Bocci</a>, <a href="/search/physics?searchtype=author&query=Bolognesi%2C+M">M. Bolognesi</a>, <a href="/search/physics?searchtype=author&query=Bolognesi%2C+P">P. Bolognesi</a>, <a href="/search/physics?searchtype=author&query=Boni%2C+R">R. Boni</a>, <a href="/search/physics?searchtype=author&query=Bonifacio%2C+R">R. Bonifacio</a>, <a href="/search/physics?searchtype=author&query=Boscolo%2C+M">M. Boscolo</a>, <a href="/search/physics?searchtype=author&query=Boscherini%2C+F">F. Boscherini</a> , et al. (189 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="1307.7967v1-abstract-short" style="display: inline;"> This report describes the scientific aims and potentials as well as the preliminary technical design of IRIDE, an innovative tool for multi-disciplinary investigations in a wide field of scientific, technological and industrial applications. IRIDE will be a high intensity 'particle factory', based on a combination of a high duty cycle radio-frequency superconducting electron linac and of high ener… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.7967v1-abstract-full').style.display = 'inline'; document.getElementById('1307.7967v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1307.7967v1-abstract-full" style="display: none;"> This report describes the scientific aims and potentials as well as the preliminary technical design of IRIDE, an innovative tool for multi-disciplinary investigations in a wide field of scientific, technological and industrial applications. IRIDE will be a high intensity 'particle factory', based on a combination of a high duty cycle radio-frequency superconducting electron linac and of high energy lasers. Conceived to provide unique research possibilities for particle physics, for condensed matter physics, chemistry and material science, for structural biology and industrial applications, IRIDE will open completely new research possibilities and advance our knowledge in many branches of science and technology. IRIDE will contribute to open new avenues of discoveries and to address most important riddles: What does matter consist of? What is the structure of proteins that have a fundamental role in life processes? What can we learn from protein structure to improve the treatment of diseases and to design more efficient drugs? But also how does an electronic chip behave under the effect of radiations? How can the heat flow in a large heat exchanger be optimized? The scientific potential of IRIDE is far reaching and justifies the construction of such a large facility in Italy in synergy with the national research institutes and companies and in the framework of the European and international research. It will impact also on R&D work for ILC, FEL, and will be complementarity to other large scale accelerator projects. IRIDE is also intended to be realized in subsequent stages of development depending on the assigned priorities. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1307.7967v1-abstract-full').style.display = 'none'; document.getElementById('1307.7967v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 July, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 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">270 pages</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1306.5655">arXiv:1306.5655</a> <span> [<a href="https://arxiv.org/pdf/1306.5655">pdf</a>, <a href="https://arxiv.org/format/1306.5655">other</a>] </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> <p class="title is-5 mathjax"> SuperB Technical Design Report </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=SuperB+Collaboration"> SuperB Collaboration</a>, <a href="/search/physics?searchtype=author&query=Baszczyk%2C+M">M. Baszczyk</a>, <a href="/search/physics?searchtype=author&query=Dorosz%2C+P">P. Dorosz</a>, <a href="/search/physics?searchtype=author&query=Kolodziej%2C+J">J. Kolodziej</a>, <a href="/search/physics?searchtype=author&query=Kucewicz%2C+W">W. Kucewicz</a>, <a href="/search/physics?searchtype=author&query=Sapor%2C+M">M. Sapor</a>, <a href="/search/physics?searchtype=author&query=Jeremie%2C+A">A. Jeremie</a>, <a href="/search/physics?searchtype=author&query=Pous%2C+E+G">E. Grauges Pous</a>, <a href="/search/physics?searchtype=author&query=Bruno%2C+G+E">G. E. Bruno</a>, <a href="/search/physics?searchtype=author&query=De+Robertis%2C+G">G. De Robertis</a>, <a href="/search/physics?searchtype=author&query=Diacono%2C+D">D. Diacono</a>, <a href="/search/physics?searchtype=author&query=Donvito%2C+G">G. Donvito</a>, <a href="/search/physics?searchtype=author&query=Fusco%2C+P">P. Fusco</a>, <a href="/search/physics?searchtype=author&query=Gargano%2C+F">F. Gargano</a>, <a href="/search/physics?searchtype=author&query=Giordano%2C+F">F. Giordano</a>, <a href="/search/physics?searchtype=author&query=Loddo%2C+F">F. Loddo</a>, <a href="/search/physics?searchtype=author&query=Loparco%2C+F">F. Loparco</a>, <a href="/search/physics?searchtype=author&query=Maggi%2C+G+P">G. P. Maggi</a>, <a href="/search/physics?searchtype=author&query=Manzari%2C+V">V. Manzari</a>, <a href="/search/physics?searchtype=author&query=Mazziotta%2C+M+N">M. N. Mazziotta</a>, <a href="/search/physics?searchtype=author&query=Nappi%2C+E">E. Nappi</a>, <a href="/search/physics?searchtype=author&query=Palano%2C+A">A. Palano</a>, <a href="/search/physics?searchtype=author&query=Santeramo%2C+B">B. Santeramo</a>, <a href="/search/physics?searchtype=author&query=Sgura%2C+I">I. Sgura</a>, <a href="/search/physics?searchtype=author&query=Silvestris%2C+L">L. Silvestris</a> , et al. (384 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="1306.5655v1-abstract-short" style="display: inline;"> In this Technical Design Report (TDR) we describe the SuperB detector that was to be installed on the SuperB e+e- high luminosity collider. The SuperB asymmetric collider, which was to be constructed on the Tor Vergata campus near the INFN Frascati National Laboratory, was designed to operate both at the Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1} and at the tau/ch… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1306.5655v1-abstract-full').style.display = 'inline'; document.getElementById('1306.5655v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1306.5655v1-abstract-full" style="display: none;"> In this Technical Design Report (TDR) we describe the SuperB detector that was to be installed on the SuperB e+e- high luminosity collider. The SuperB asymmetric collider, which was to be constructed on the Tor Vergata campus near the INFN Frascati National Laboratory, was designed to operate both at the Upsilon(4S) center-of-mass energy with a luminosity of 10^{36} cm^{-2}s^{-1} and at the tau/charm production threshold with a luminosity of 10^{35} cm^{-2}s^{-1}. This high luminosity, producing a data sample about a factor 100 larger than present B Factories, would allow investigation of new physics effects in rare decays, CP Violation and Lepton Flavour Violation. This document details the detector design presented in the Conceptual Design Report (CDR) in 2007. The R&D and engineering studies performed to arrive at the full detector design are described, and an updated cost estimate is presented. A combination of a more realistic cost estimates and the unavailability of funds due of the global economic climate led to a formal cancelation of the project on Nov 27, 2012. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1306.5655v1-abstract-full').style.display = 'none'; document.getElementById('1306.5655v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 24 June, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 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">495 pages</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> INFN-13-01/PI, LAL 13-01, SLAC-R-1003 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1206.0680">arXiv:1206.0680</a> <span> [<a href="https://arxiv.org/pdf/1206.0680">pdf</a>, <a href="https://arxiv.org/format/1206.0680">other</a>] </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/10.1016/j.nima.2012.09.034">10.1016/j.nima.2012.09.034 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The KLOE-2 High Energy Tagger Detector </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Gonnella%2C+F">F. Gonnella</a>, <a href="/search/physics?searchtype=author&query=Iafolla%2C+L">L. Iafolla</a>, <a href="/search/physics?searchtype=author&query=Iannarelli%2C+M">M. Iannarelli</a>, <a href="/search/physics?searchtype=author&query=Mascolo%2C+M">M. Mascolo</a>, <a href="/search/physics?searchtype=author&query=Messi%2C+R">R. Messi</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Saputi%2C+A">A. Saputi</a>, <a href="/search/physics?searchtype=author&query=Turri%2C+E">E. Turri</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="1206.0680v1-abstract-short" style="display: inline;"> In order to fully reconstruct to the reaction e+e- to e+e- gamma-gamma in the energy region of the phi meson production, new detectors along the DAFNE beam line have to be installed in order to detect the scattered e+e-. The High Energy Tagger (HET) detector measures the deviation of leptons from their main orbit by determining their position and timing so to tag gamma-gamma physics events and dis… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0680v1-abstract-full').style.display = 'inline'; document.getElementById('1206.0680v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1206.0680v1-abstract-full" style="display: none;"> In order to fully reconstruct to the reaction e+e- to e+e- gamma-gamma in the energy region of the phi meson production, new detectors along the DAFNE beam line have to be installed in order to detect the scattered e+e-. The High Energy Tagger (HET) detector measures the deviation of leptons from their main orbit by determining their position and timing so to tag gamma-gamma physics events and disentangle them from background. The HET detectors are placed at the exit of the DAFNE dipole magnets, 11 m away from the IP, both on positron and electron lines. The HET sensitive area is made up of a set of 28 plastic scintillators. A dedicated DAQ electronics board based on a Xilinx Virtex-5 FPGA have been developed for this detector. It provides a MultiHit TDC with a time resolution of the order of 500 ps and the possibility to acquire data any 2.5 ns, thus allowing to clearly identify the correct bunch crossing. First results of the commissioning run are presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0680v1-abstract-full').style.display = 'none'; document.getElementById('1206.0680v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 June, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2012. </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">Submitted to proceedings of the 12th Pisa Meeting on Advanced Detectors 2012, La Biodola, Isola d'Elba, Italy</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1206.0679">arXiv:1206.0679</a> <span>  </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/10.1016/j.nima.2013.12.033">10.1016/j.nima.2013.12.033 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Low resource FPGA-based Time to Digital Converter </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Balla%2C+A">A. Balla</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M">M. Beretta</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">P. Ciambrone</a>, <a href="/search/physics?searchtype=author&query=Gatta%2C+M">M. Gatta</a>, <a href="/search/physics?searchtype=author&query=Gonnella%2C+F">F. Gonnella</a>, <a href="/search/physics?searchtype=author&query=Iafolla%2C+L">L. Iafolla</a>, <a href="/search/physics?searchtype=author&query=Mascolo%2C+M">M. Mascolo</a>, <a href="/search/physics?searchtype=author&query=Messi%2C+R">R. Messi</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Riondino%2C+D">D. Riondino</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="1206.0679v4-abstract-short" style="display: inline;"> Time to Digital Converters (TDCs) are very common devices in particles physics experiments. A lot of "off-the-shelf" TDCs can be employed but the necessity of a custom DAta acQuisition (DAQ) system makes the TDCs implemented on the Field-Programmable Gate Arrays (FPGAs) desirable. Most of the architectures developed so far are based on the tapped delay lines with precision down to 10 ps, obtained… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0679v4-abstract-full').style.display = 'inline'; document.getElementById('1206.0679v4-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1206.0679v4-abstract-full" style="display: none;"> Time to Digital Converters (TDCs) are very common devices in particles physics experiments. A lot of "off-the-shelf" TDCs can be employed but the necessity of a custom DAta acQuisition (DAQ) system makes the TDCs implemented on the Field-Programmable Gate Arrays (FPGAs) desirable. Most of the architectures developed so far are based on the tapped delay lines with precision down to 10 ps, obtained with high FPGA resources usage and non-linearity issues to be managed. Often such precision is not necessary; in this case TDC architectures with low resources occupancy are preferable allowing the implementation of data processing systems and of other utilities on the same device. In order to reconstruct gamma-gamma physics events tagged with High Energy Tagger (HET) in the KLOE-2 (K LOng Experiment 2), we need to measure the Time Of Flight (TOF) of the electrons and positrons from the KLOE-2 Interaction Point (IP) to our tagging stations (11 m apart). The required resolution must be better than the bunch spacing (2.7 ns). We have developed and implemented on a Xilinx Virtex-5 FPGA a 32 channel TDC with a precision of 255 ps and low non-linearity effects along with an embedded data acquisition systems and the interface to the online FARM of KLOE-2. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1206.0679v4-abstract-full').style.display = 'none'; document.getElementById('1206.0679v4-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 8 December, 2012; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 4 June, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2012. </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">I would like to withdraw this paper due to copyright problem</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1205.6663">arXiv:1205.6663</a> <span> [<a href="https://arxiv.org/pdf/1205.6663">pdf</a>] </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/10.1016/j.nima.2012.10.010">10.1016/j.nima.2012.10.010 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> FPGA-based Time to Digital Converter and Data Acquisition system for High Energy Tagger of KLOE-2 experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Iafolla%2C+L">L. Iafolla</a>, <a href="/search/physics?searchtype=author&query=Balla%2C+A">A. Balla</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M">M. Beretta</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">P. Ciambrone</a>, <a href="/search/physics?searchtype=author&query=Gatta%2C+M">M. Gatta</a>, <a href="/search/physics?searchtype=author&query=Gonnella%2C+F">F. Gonnella</a>, <a href="/search/physics?searchtype=author&query=Mascolo%2C+M">M. Mascolo</a>, <a href="/search/physics?searchtype=author&query=Messi%2C+R">R. Messi</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Riondino%2C+D">D. Riondino</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="1205.6663v1-abstract-short" style="display: inline;"> In order to reconstruct gamma-gamma physics events tagged with High Energy Tagger (HET) in the KLOE-2 (K LOng Experiment 2), we need to measure the Time Of Flight (TOF) of the electrons and positrons from the KLOE-2 Interaction Point (IP) to our tagging stations (11 m apart). The required resolution must be better than the bunch spacing (2.7 ns). We have developed and implemented on a Xilinx Virte… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1205.6663v1-abstract-full').style.display = 'inline'; document.getElementById('1205.6663v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1205.6663v1-abstract-full" style="display: none;"> In order to reconstruct gamma-gamma physics events tagged with High Energy Tagger (HET) in the KLOE-2 (K LOng Experiment 2), we need to measure the Time Of Flight (TOF) of the electrons and positrons from the KLOE-2 Interaction Point (IP) to our tagging stations (11 m apart). The required resolution must be better than the bunch spacing (2.7 ns). We have developed and implemented on a Xilinx Virtex-5 FPGA a Time to Digital Converter (TDC) with 625 ps resolution (LSB) along with an embedded data acquisition system and the interface to the online FARM of KLOE-2. We will describe briefly the architecture of the TDC and of the Data AcQuisition (DAQ) system. Some more details will be provided about the zero-suppression algorithm used to reduce the data throughput. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1205.6663v1-abstract-full').style.display = 'none'; document.getElementById('1205.6663v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 May, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2012. </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">Submitted to proceedings of the 12th Pisa Meeting on Advanced Detectors 2012, La Biodola, Isola d'Elba, Italy</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1005.5230">arXiv:1005.5230</a> <span> [<a href="https://arxiv.org/pdf/1005.5230">pdf</a>, <a href="https://arxiv.org/ps/1005.5230">ps</a>, <a href="https://arxiv.org/format/1005.5230">other</a>] </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="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Atomic Physics">physics.atom-ph</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.104.241601">10.1103/PhysRevLett.104.241601 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Limits on light-speed anisotropies from Compton scattering of high-energy electrons </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Bocquet%2C+J+-">J. -P. Bocquet</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Bellini%2C+V">V. Bellini</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M">M. Beretta</a>, <a href="/search/physics?searchtype=author&query=Casano%2C+L">L. Casano</a>, <a href="/search/physics?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/physics?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/physics?searchtype=author&query=Fantini%2C+A">A. Fantini</a>, <a href="/search/physics?searchtype=author&query=Franco%2C+D">D. Franco</a>, <a href="/search/physics?searchtype=author&query=Gervino%2C+G">G. Gervino</a>, <a href="/search/physics?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&query=Giardina%2C+G">G. Giardina</a>, <a href="/search/physics?searchtype=author&query=Girolami%2C+B">B. Girolami</a>, <a href="/search/physics?searchtype=author&query=Giusa%2C+A">A. Giusa</a>, <a href="/search/physics?searchtype=author&query=Gurzadyan%2C+V+G">V. G. Gurzadyan</a>, <a href="/search/physics?searchtype=author&query=Kashin%2C+A">A. Kashin</a>, <a href="/search/physics?searchtype=author&query=Knyazyan%2C+S">S. Knyazyan</a>, <a href="/search/physics?searchtype=author&query=Lapik%2C+A">A. Lapik</a>, <a href="/search/physics?searchtype=author&query=Lehnert%2C+R">R. Lehnert</a>, <a href="/search/physics?searchtype=author&query=Sandri%2C+P+L">P. Levi Sandri</a>, <a href="/search/physics?searchtype=author&query=Lleres%2C+A">A. Lleres</a>, <a href="/search/physics?searchtype=author&query=Mammoliti%2C+F">F. Mammoliti</a>, <a href="/search/physics?searchtype=author&query=Mandaglio%2C+G">G. Mandaglio</a>, <a href="/search/physics?searchtype=author&query=Manganaro%2C+M">M. Manganaro</a>, <a href="/search/physics?searchtype=author&query=Margarian%2C+A">A. Margarian</a> , et al. (13 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="1005.5230v2-abstract-short" style="display: inline;"> The possibility of anisotropies in the speed of light relative to the limiting speed of electrons is considered. The absence of sidereal variations in the energy of Compton-edge photons at the ESRF's GRAAL facility constrains such anisotropies representing the first non-threshold collision-kinematics study of Lorentz violation. When interpreted within the minimal Standard-Model Extension, this res… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1005.5230v2-abstract-full').style.display = 'inline'; document.getElementById('1005.5230v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1005.5230v2-abstract-full" style="display: none;"> The possibility of anisotropies in the speed of light relative to the limiting speed of electrons is considered. The absence of sidereal variations in the energy of Compton-edge photons at the ESRF's GRAAL facility constrains such anisotropies representing the first non-threshold collision-kinematics study of Lorentz violation. When interpreted within the minimal Standard-Model Extension, this result yields the two-sided limit of 1.6 x 10^{-14} at 95% confidence level on a combination of the parity-violating photon and electron coefficients kappa_{o+} and c. This new constraint provides an improvement over previous bounds by one order of magnitude. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1005.5230v2-abstract-full').style.display = 'none'; document.getElementById('1005.5230v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 9 June, 2010; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 28 May, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2010. </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">4 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Rev.Lett.104:241601,2010 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1004.2867">arXiv:1004.2867</a> <span> [<a href="https://arxiv.org/pdf/1004.2867">pdf</a>, <a href="https://arxiv.org/ps/1004.2867">ps</a>, <a href="https://arxiv.org/format/1004.2867">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</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/10.1142/9789814374552_0255">10.1142/9789814374552_0255 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> A new limit on the light speed isotropy from the GRAAL experiment at the ESRF </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Gurzadyan%2C+V+G">V. G. Gurzadyan</a>, <a href="/search/physics?searchtype=author&query=Bellini%2C+V">V. Bellini</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M">M. Beretta</a>, <a href="/search/physics?searchtype=author&query=Bocquet%2C+J+-">J. -P. Bocquet</a>, <a href="/search/physics?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/physics?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/physics?searchtype=author&query=Fantini%2C+A">A. Fantini</a>, <a href="/search/physics?searchtype=author&query=Franco%2C+D">D. Franco</a>, <a href="/search/physics?searchtype=author&query=Gervino%2C+G">G. Gervino</a>, <a href="/search/physics?searchtype=author&query=Giardina%2C+G">G. Giardina</a>, <a href="/search/physics?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&query=Girolami%2C+B">B. Girolami</a>, <a href="/search/physics?searchtype=author&query=Giusa%2C+A">A. Giusa</a>, <a href="/search/physics?searchtype=author&query=Kashin%2C+A">A. Kashin</a>, <a href="/search/physics?searchtype=author&query=Khachatryan%2C+H+G">H. G. Khachatryan</a>, <a href="/search/physics?searchtype=author&query=Knyazyan%2C+S">S. Knyazyan</a>, <a href="/search/physics?searchtype=author&query=Lapik%2C+A">A. Lapik</a>, <a href="/search/physics?searchtype=author&query=Sandri%2C+P+L">P. Levi Sandri</a>, <a href="/search/physics?searchtype=author&query=Lleres%2C+A">A. Lleres</a>, <a href="/search/physics?searchtype=author&query=Mammoliti%2C+F">F. Mammoliti</a>, <a href="/search/physics?searchtype=author&query=Mandaglio%2C+G">G. Mandaglio</a>, <a href="/search/physics?searchtype=author&query=Manganaro%2C+M">M. Manganaro</a>, <a href="/search/physics?searchtype=author&query=Margarian%2C+A">A. Margarian</a>, <a href="/search/physics?searchtype=author&query=Mehrabyan%2C+S">S. Mehrabyan</a>, <a href="/search/physics?searchtype=author&query=Messi%2C+R">R. Messi</a> , et al. (10 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="1004.2867v1-abstract-short" style="display: inline;"> When the electrons stored in the ring of the European Synchrotron Radiation Facility (ESRF, Grenoble) scatter on a laser beam (Compton scattering in flight) the lower energy of the scattered electron spectra, the Compton Edge (CE), is given by the two body photon-electron relativistic kinematics and depends on the velocity of light. A precision measurement of the position of this CE as a function… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.2867v1-abstract-full').style.display = 'inline'; document.getElementById('1004.2867v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1004.2867v1-abstract-full" style="display: none;"> When the electrons stored in the ring of the European Synchrotron Radiation Facility (ESRF, Grenoble) scatter on a laser beam (Compton scattering in flight) the lower energy of the scattered electron spectra, the Compton Edge (CE), is given by the two body photon-electron relativistic kinematics and depends on the velocity of light. A precision measurement of the position of this CE as a function of the daily variations of the direction of the electron beam in an absolute reference frame provides a one-way test of Relativistic Kinematics and the isotropy of the velocity of light. The results of GRAAL-ESRF measurements improve the previously existing one-way limits, thus showing the efficiency of this method and the interest of further studies in this direction. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1004.2867v1-abstract-full').style.display = 'none'; document.getElementById('1004.2867v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 16 April, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2010. </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">Proceed. MG12 meeting, Paris, July, 2009</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1002.2572">arXiv:1002.2572</a> <span> [<a href="https://arxiv.org/pdf/1002.2572">pdf</a>, <a href="https://arxiv.org/ps/1002.2572">ps</a>, <a href="https://arxiv.org/format/1002.2572">other</a>] </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> <p class="title is-5 mathjax"> Technical Design Report of the Inner Tracker for the KLOE-2 experiment </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Collaboration%2C+K">KLOE-2 Collaboration</a>, <a href="/search/physics?searchtype=author&query=%3A"> :</a>, <a href="/search/physics?searchtype=author&query=Archilli%2C+F">F. Archilli</a>, <a href="/search/physics?searchtype=author&query=Badoni%2C+D">D. Badoni</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Bencivenni%2C+G">G. Bencivenni</a>, <a href="/search/physics?searchtype=author&query=Bini%2C+C">C. Bini</a>, <a href="/search/physics?searchtype=author&query=Bloise%2C+C">C. Bloise</a>, <a href="/search/physics?searchtype=author&query=Bocci%2C+V">V. Bocci</a>, <a href="/search/physics?searchtype=author&query=Bossi%2C+F">F. Bossi</a>, <a href="/search/physics?searchtype=author&query=Branchini%2C+P">P. Branchini</a>, <a href="/search/physics?searchtype=author&query=Budano%2C+A">A. Budano</a>, <a href="/search/physics?searchtype=author&query=Bulychjev%2C+S+A">S. A. Bulychjev</a>, <a href="/search/physics?searchtype=author&query=Campana%2C+P">P. Campana</a>, <a href="/search/physics?searchtype=author&query=Capon%2C+G">G. Capon</a>, <a href="/search/physics?searchtype=author&query=Ceradini%2C+F">F. Ceradini</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">P. Ciambrone</a>, <a href="/search/physics?searchtype=author&query=Czerwinski%2C+E">E. Czerwinski</a>, <a href="/search/physics?searchtype=author&query=Dan%C3%A8%2C+E">E. Dan猫</a>, <a href="/search/physics?searchtype=author&query=De+Lucia%2C+E">E. De Lucia</a>, <a href="/search/physics?searchtype=author&query=De+Robertis%2C+G">G. De Robertis</a>, <a href="/search/physics?searchtype=author&query=De+Santis%2C+A">A. De Santis</a>, <a href="/search/physics?searchtype=author&query=De+Zorzi%2C+G">G. De Zorzi</a>, <a href="/search/physics?searchtype=author&query=Di+Domenico%2C+A">A. Di Domenico</a>, <a href="/search/physics?searchtype=author&query=Di+Donato%2C+C">C. Di Donato</a> , et al. (59 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1002.2572v1-abstract-short" style="display: inline;"> The technical design report of the Inner Tracker for the KLOE-2 experiment is presented </span> <span class="abstract-full has-text-grey-dark mathjax" id="1002.2572v1-abstract-full" style="display: none;"> The technical design report of the Inner Tracker for the KLOE-2 experiment is presented <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1002.2572v1-abstract-full').style.display = 'none'; document.getElementById('1002.2572v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 12 February, 2010; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2010. </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">77 pages</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> LNF-10/3(P) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/astro-ph/0701127">arXiv:astro-ph/0701127</a> <span> [<a href="https://arxiv.org/pdf/astro-ph/0701127">pdf</a>, <a href="https://arxiv.org/ps/astro-ph/0701127">ps</a>, <a href="https://arxiv.org/format/astro-ph/0701127">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics">astro-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</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/10.1393/ncb/i2007-10393-7">10.1393/ncb/i2007-10393-7 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Lowering the Light Speed Isotropy Limit: European Synchrotron Radiation Facility Measurements </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Gurzadyan%2C+V+G">V. G. Gurzadyan</a>, <a href="/search/physics?searchtype=author&query=Bocquet%2C+J+-">J. -P. Bocquet</a>, <a href="/search/physics?searchtype=author&query=Kashin%2C+A">A. Kashin</a>, <a href="/search/physics?searchtype=author&query=Margarian%2C+A">A. Margarian</a>, <a href="/search/physics?searchtype=author&query=Bartalini%2C+O">O. Bartalini</a>, <a href="/search/physics?searchtype=author&query=Bellini%2C+V">V. Bellini</a>, <a href="/search/physics?searchtype=author&query=Castoldi%2C+M">M. Castoldi</a>, <a href="/search/physics?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/physics?searchtype=author&query=Didelez%2C+J+-">J. -P. Didelez</a>, <a href="/search/physics?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/physics?searchtype=author&query=Fantini%2C+A">A. Fantini</a>, <a href="/search/physics?searchtype=author&query=Gervino%2C+G">G. Gervino</a>, <a href="/search/physics?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&query=Girolami%2C+B">B. Girolami</a>, <a href="/search/physics?searchtype=author&query=Giusa%2C+A">A. Giusa</a>, <a href="/search/physics?searchtype=author&query=Guidal%2C+M">M. Guidal</a>, <a href="/search/physics?searchtype=author&query=Hourany%2C+E">E. Hourany</a>, <a href="/search/physics?searchtype=author&query=Knyazyan%2C+S">S. Knyazyan</a>, <a href="/search/physics?searchtype=author&query=Kouznetsov%2C+V">V. Kouznetsov</a>, <a href="/search/physics?searchtype=author&query=Kunne%2C+R">R. Kunne</a>, <a href="/search/physics?searchtype=author&query=Lapik%2C+A">A. Lapik</a>, <a href="/search/physics?searchtype=author&query=Sandri%2C+P+L">P. Levi Sandri</a>, <a href="/search/physics?searchtype=author&query=Lleres%2C+A">A. Lleres</a>, <a href="/search/physics?searchtype=author&query=Mehrabyan%2C+S">S. Mehrabyan</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a> , et al. (9 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="astro-ph/0701127v2-abstract-short" style="display: inline;"> The measurement of the Compton edge of the scattered electrons in GRAAL facility in European Synchrotron Radiation Facility (ESRF) in Grenoble with respect to the Cosmic Microwave Background dipole reveals up to 10 sigma variations larger than the statistical errors. We now show that the variations are not due to the frequency variations of the accelerator. The nature of Compton edge variations… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/0701127v2-abstract-full').style.display = 'inline'; document.getElementById('astro-ph/0701127v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="astro-ph/0701127v2-abstract-full" style="display: none;"> The measurement of the Compton edge of the scattered electrons in GRAAL facility in European Synchrotron Radiation Facility (ESRF) in Grenoble with respect to the Cosmic Microwave Background dipole reveals up to 10 sigma variations larger than the statistical errors. We now show that the variations are not due to the frequency variations of the accelerator. The nature of Compton edge variations remains unclear, thus outlining the imperative of dedicated studies of light speed anisotropy. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/0701127v2-abstract-full').style.display = 'none'; document.getElementById('astro-ph/0701127v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 5 May, 2008; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 5 January, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Il Nuovo Cimento, B122 (2007) 515 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/astro-ph/0410742">arXiv:astro-ph/0410742</a> <span> [<a href="https://arxiv.org/pdf/astro-ph/0410742">pdf</a>, <a href="https://arxiv.org/ps/astro-ph/0410742">ps</a>, <a href="https://arxiv.org/format/astro-ph/0410742">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics">astro-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Accelerator Physics">physics.acc-ph</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/10.1142/S0217732305016294">10.1142/S0217732305016294 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Probing the Light Speed Anisotropy with respect to the Cosmic Microwave Background Radiation Dipole </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Gurzadyan%2C+V+G">V. G. Gurzadyan</a>, <a href="/search/physics?searchtype=author&query=Bocquet%2C+J+-">J. -P. Bocquet</a>, <a href="/search/physics?searchtype=author&query=Kashin%2C+A">A. Kashin</a>, <a href="/search/physics?searchtype=author&query=Margarian%2C+A">A. Margarian</a>, <a href="/search/physics?searchtype=author&query=Bartalini%2C+O">O. Bartalini</a>, <a href="/search/physics?searchtype=author&query=Bellini%2C+V">V. Bellini</a>, <a href="/search/physics?searchtype=author&query=Castoldi%2C+M">M. Castoldi</a>, <a href="/search/physics?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/physics?searchtype=author&query=Didelez%2C+J+-">J. -P. Didelez</a>, <a href="/search/physics?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/physics?searchtype=author&query=Fantini%2C+A">A. Fantini</a>, <a href="/search/physics?searchtype=author&query=Gervino%2C+G">G. Gervino</a>, <a href="/search/physics?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&query=Girolami%2C+B">B. Girolami</a>, <a href="/search/physics?searchtype=author&query=Giusa%2C+A">A. Giusa</a>, <a href="/search/physics?searchtype=author&query=Guidal%2C+M">M. Guidal</a>, <a href="/search/physics?searchtype=author&query=Hourany%2C+E">E. Hourany</a>, <a href="/search/physics?searchtype=author&query=Knyazyan%2C+S">S. Knyazyan</a>, <a href="/search/physics?searchtype=author&query=Kouznetsov%2C+V">V. Kouznetsov</a>, <a href="/search/physics?searchtype=author&query=Kunne%2C+R">R. Kunne</a>, <a href="/search/physics?searchtype=author&query=Lapik%2C+A">A. Lapik</a>, <a href="/search/physics?searchtype=author&query=Sandri%2C+P+L">P. Levi Sandri</a>, <a href="/search/physics?searchtype=author&query=Lleres%2C+A">A. Lleres</a>, <a href="/search/physics?searchtype=author&query=Mehrabyan%2C+S">S. Mehrabyan</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a> , et al. (9 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="astro-ph/0410742v2-abstract-short" style="display: inline;"> We have studied the angular fluctuations in the speed of light with respect to the apex of the dipole of Cosmic Microwave Background (CMB) radiation using the experimental data obtained with GRAAL facility, located at the European Synchrotron Radiation Facility (ESRF) in Grenoble. The measurements were based on the stability of the Compton edge of laser photons scattered on the 6 GeV monochromat… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/0410742v2-abstract-full').style.display = 'inline'; document.getElementById('astro-ph/0410742v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="astro-ph/0410742v2-abstract-full" style="display: none;"> We have studied the angular fluctuations in the speed of light with respect to the apex of the dipole of Cosmic Microwave Background (CMB) radiation using the experimental data obtained with GRAAL facility, located at the European Synchrotron Radiation Facility (ESRF) in Grenoble. The measurements were based on the stability of the Compton edge of laser photons scattered on the 6 GeV monochromatic electron beam. The results enable to obtain a conservative constraint on the anisotropy in the light speed variations 螖c(胃)/c < 3 10^{-12}, i.e. with higher precision than from previous experiments. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('astro-ph/0410742v2-abstract-full').style.display = 'none'; document.getElementById('astro-ph/0410742v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 10 January, 2005; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 October, 2004; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 2004. </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">The published version: reported at the workshop "Testing the Equivalence Principle in Space and on Ground" (STEP), Pescara, Italy, September, 2004</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Mod.Phys.Lett. A20 (2005) 19-28 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/physics/9709027">arXiv:physics/9709027</a> <span> [<a href="https://arxiv.org/pdf/physics/9709027">pdf</a>, <a href="https://arxiv.org/ps/physics/9709027">ps</a>, <a href="https://arxiv.org/format/physics/9709027">other</a>] </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/10.1016/S0168-9002(97)01124-8">10.1016/S0168-9002(97)01124-8 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The GRAAL high resolution BGO calorimeter and its energy calibration and monitoring system </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Ghio%2C+F">F. Ghio</a>, <a href="/search/physics?searchtype=author&query=Girolami%2C+B">B. Girolami</a>, <a href="/search/physics?searchtype=author&query=Capogni%2C+M">M. Capogni</a>, <a href="/search/physics?searchtype=author&query=Casano%2C+L">L. Casano</a>, <a href="/search/physics?searchtype=author&query=Ciciani%2C+L">L. Ciciani</a>, <a href="/search/physics?searchtype=author&query=D%27Angelo%2C+A">A. D'Angelo</a>, <a href="/search/physics?searchtype=author&query=Di+Salvo%2C+R">R. Di Salvo</a>, <a href="/search/physics?searchtype=author&query=Hu%2C+L">L. Hu</a>, <a href="/search/physics?searchtype=author&query=Moricciani%2C+D">D. Moricciani</a>, <a href="/search/physics?searchtype=author&query=Nicoletti%2C+L">L. Nicoletti</a>, <a href="/search/physics?searchtype=author&query=Nobili%2C+G">G. Nobili</a>, <a href="/search/physics?searchtype=author&query=Schaerf%2C+C">C. Schaerf</a>, <a href="/search/physics?searchtype=author&query=Sandri%2C+P+L">P. Levi Sandri</a>, <a href="/search/physics?searchtype=author&query=Castoldi%2C+M">M. Castoldi</a>, <a href="/search/physics?searchtype=author&query=Zucchiatti%2C+A">A. Zucchiatti</a>, <a href="/search/physics?searchtype=author&query=Bellini%2C+V">V. Bellini</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="physics/9709027v1-abstract-short" style="display: inline;"> We describe the electromagnetic calorimeter built for the GRAAL apparatus at the ESRF. Its monitoring system is presented in detail. Results from tests and the performance obtained during the first GRAAL experiments are given. The energy calibration accuracy and stability reached is a small fraction of the intrinsic detector resolution. </span> <span class="abstract-full has-text-grey-dark mathjax" id="physics/9709027v1-abstract-full" style="display: none;"> We describe the electromagnetic calorimeter built for the GRAAL apparatus at the ESRF. Its monitoring system is presented in detail. Results from tests and the performance obtained during the first GRAAL experiments are given. The energy calibration accuracy and stability reached is a small fraction of the intrinsic detector resolution. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('physics/9709027v1-abstract-full').style.display = 'none'; document.getElementById('physics/9709027v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 19 September, 1997; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 1997. </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">19 pages, 14 figures, submitted to Nuclear Instruments and Methods</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> LNF-97/030(P) </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nucl.Instrum.Meth. A404 (1998) 71-86 </p> </li> </ol> <div class="is-hidden-tablet">  <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>  </span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary">  <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 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg> <a href="https://info.arxiv.org/help/contact.html"> Contact</a> </li> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>subscribe to arXiv mailings</title><desc>Click here to subscribe</desc><path d="M476 3.2L12.5 270.6c-18.1 10.4-15.8 35.6 2.2 43.2L121 358.4l287.3-253.2c5.5-4.9 13.3 2.6 8.6 8.3L176 407v80.5c0 23.6 28.5 32.9 42.5 15.8L282 426l124.6 52.2c14.2 6 30.4-2.9 33-18.2l72-432C515 7.8 493.3-6.8 476 3.2z"/></svg> <a href="https://info.arxiv.org/help/subscribe"> Subscribe</a> </li> </ul> </div> </div> </div>   <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/license/index.html">Copyright</a></li> <li><a href="https://info.arxiv.org/help/policies/privacy_policy.html">Privacy Policy</a></li> </ul> </div> <div class="column sorry-app-links"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/help/web_accessibility.html">Web Accessibility Assistance</a></li> <li> <p class="help"> <a class="a11y-main-link" href="https://status.arxiv.org" target="_blank">arXiv Operational Status <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 256 512" class="icon filter-dark_grey" role="presentation"><path d="M224.3 273l-136 136c-9.4 9.4-24.6 9.4-33.9 0l-22.6-22.6c-9.4-9.4-9.4-24.6 0-33.9l96.4-96.4-96.4-96.4c-9.4-9.4-9.4-24.6 0-33.9L54.3 103c9.4-9.4 24.6-9.4 33.9 0l136 136c9.5 9.4 9.5 24.6.1 34z"/></svg></a><br> Get status notifications via <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/email/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 0-48-21.5-48-48V195.6c0-5 5.7-7.8 9.7-4.7 22.4 17.4 52.1 39.5 154.1 113.6 21.1 15.4 56.7 47.8 92.2 47.6 35.7.3 72-32.8 92.3-47.6 102-74.1 131.6-96.3 154-113.7zM256 320c23.2.4 56.6-29.2 73.4-41.4 132.7-96.3 142.8-104.7 173.4-128.7 5.8-4.5 9.2-11.5 9.2-18.9v-19c0-26.5-21.5-48-48-48H48C21.5 64 0 85.5 0 112v19c0 7.4 3.4 14.3 9.2 18.9 30.6 23.9 40.7 32.4 173.4 128.7 16.8 12.2 50.2 41.8 73.4 41.4z"/></svg>email</a> or <a class="is-link" href="https://subscribe.sorryapp.com/24846f03/slack/new" target="_blank"><svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 448 512" class="icon filter-black" role="presentation"><path d="M94.12 315.1c0 25.9-21.16 47.06-47.06 47.06S0 341 0 315.1c0-25.9 21.16-47.06 47.06-47.06h47.06v47.06zm23.72 0c0-25.9 21.16-47.06 47.06-47.06s47.06 21.16 47.06 47.06v117.84c0 25.9-21.16 47.06-47.06 47.06s-47.06-21.16-47.06-47.06V315.1zm47.06-188.98c-25.9 0-47.06-21.16-47.06-47.06S139 32 164.9 32s47.06 21.16 47.06 47.06v47.06H164.9zm0 23.72c25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06H47.06C21.16 243.96 0 222.8 0 196.9s21.16-47.06 47.06-47.06H164.9zm188.98 47.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06s-21.16 47.06-47.06 47.06h-47.06V196.9zm-23.72 0c0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06V79.06c0-25.9 21.16-47.06 47.06-47.06 25.9 0 47.06 21.16 47.06 47.06V196.9zM283.1 385.88c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06-25.9 0-47.06-21.16-47.06-47.06v-47.06h47.06zm0-23.72c-25.9 0-47.06-21.16-47.06-47.06 0-25.9 21.16-47.06 47.06-47.06h117.84c25.9 0 47.06 21.16 47.06 47.06 0 25.9-21.16 47.06-47.06 47.06H283.1z"/></svg>slack</a> </p> </li> </ul> </div> </div> </div>  </div> </footer> <script src="https://static.arxiv.org/static/base/1.0.0a5/js/member_acknowledgement.js"></script> </body> </html>

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