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<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/2402.19063">arXiv:2402.19063</a> <span> [<a href="https://arxiv.org/pdf/2402.19063">pdf</a>, <a href="https://arxiv.org/format/2402.19063">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> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.110.022008">10.1103/PhysRevD.110.022008 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for Axion dark matter with the QUAX-LNF tunable haloscope </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Rettaroli%2C+A">A. Rettaroli</a>, <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=Braggio%2C+C">C. Braggio</a>, <a href="/search/physics?searchtype=author&query=Carugno%2C+G">G. Carugno</a>, <a href="/search/physics?searchtype=author&query=D%27Agostino%2C+D">D. D'Agostino</a>, <a href="/search/physics?searchtype=author&query=D%27Elia%2C+A">A. D'Elia</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">D. Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Di+Vora%2C+R">R. Di Vora</a>, <a href="/search/physics?searchtype=author&query=Falferi%2C+P">P. Falferi</a>, <a href="/search/physics?searchtype=author&query=Gambardella%2C+U">U. Gambardella</a>, <a href="/search/physics?searchtype=author&query=Gardikiotis%2C+A">A. Gardikiotis</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">C. Gatti</a>, <a href="/search/physics?searchtype=author&query=Iannone%2C+G">G. Iannone</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">C. Ligi</a>, <a href="/search/physics?searchtype=author&query=Lombardi%2C+A">A. Lombardi</a>, <a href="/search/physics?searchtype=author&query=Maccarrone%2C+G">G. Maccarrone</a>, <a href="/search/physics?searchtype=author&query=Ortolan%2C+A">A. Ortolan</a>, <a href="/search/physics?searchtype=author&query=Ruoso%2C+G">G. Ruoso</a>, <a href="/search/physics?searchtype=author&query=Tocci%2C+S">S. Tocci</a>, <a href="/search/physics?searchtype=author&query=Vidali%2C+G">G. Vidali</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="2402.19063v3-abstract-short" style="display: inline;"> We report the first experimental results obtained with the new haloscope of the QUAX experiment located at Laboratori Nazionali di Frascati of INFN (LNF). The haloscope is composed of a OFHC Cu resonant cavity cooled down to about 30 mK and immersed in a magnetic field of 8 T. The cavity frequency was varied in a 6 MHz range between 8.831496 and 8.83803 GHz. This corresponds to a previously unprob… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2402.19063v3-abstract-full').style.display = 'inline'; document.getElementById('2402.19063v3-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2402.19063v3-abstract-full" style="display: none;"> We report the first experimental results obtained with the new haloscope of the QUAX experiment located at Laboratori Nazionali di Frascati of INFN (LNF). The haloscope is composed of a OFHC Cu resonant cavity cooled down to about 30 mK and immersed in a magnetic field of 8 T. The cavity frequency was varied in a 6 MHz range between 8.831496 and 8.83803 GHz. This corresponds to a previously unprobed mass range between 36.52413 and 36.5511 $渭$eV. We don't observe any excess in the power spectrum and set limits on the axion-photon coupling in this mass range down to $g_{a纬纬} < 0.861 \times 10^{-13}$ GeV$^{-1}$ with the confidence level set at $90\%$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2402.19063v3-abstract-full').style.display = 'none'; document.getElementById('2402.19063v3-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 May, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 29 February, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2024. </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 Physical Review D (https://journals.aps.org/prd/)</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2309.00351">arXiv:2309.00351</a> <span> [<a href="https://arxiv.org/pdf/2309.00351">pdf</a>, <a href="https://arxiv.org/format/2309.00351">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> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-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/10.1016/j.dark.2023.101370">10.1016/j.dark.2023.101370 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The future search for low-frequency axions and new physics with the FLASH resonant cavity experiment at Frascati National Laboratories </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alesini%2C+D">David Alesini</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">Danilo Babusci</a>, <a href="/search/physics?searchtype=author&query=Beltrame%2C+P">Paolo Beltrame</a>, <a href="/search/physics?searchtype=author&query=Bossi%2C+F">Fabio Bossi</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">Paolo Ciambrone</a>, <a href="/search/physics?searchtype=author&query=D%27Elia%2C+A">Alessandro D'Elia</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">Daniele Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Di+Pirro%2C+G">Giampiero Di Pirro</a>, <a href="/search/physics?searchtype=author&query=D%C3%B6brich%2C+B">Babette D枚brich</a>, <a href="/search/physics?searchtype=author&query=Falferi%2C+P">Paolo Falferi</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">Claudio Gatti</a>, <a href="/search/physics?searchtype=author&query=Giannotti%2C+M">Maurizio Giannotti</a>, <a href="/search/physics?searchtype=author&query=Gianotti%2C+P">Paola Gianotti</a>, <a href="/search/physics?searchtype=author&query=Lamanna%2C+G">Gianluca Lamanna</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">Carlo Ligi</a>, <a href="/search/physics?searchtype=author&query=Maccarrone%2C+G">Giovanni Maccarrone</a>, <a href="/search/physics?searchtype=author&query=Mazzitelli%2C+G">Giovanni Mazzitelli</a>, <a href="/search/physics?searchtype=author&query=Mirizzi%2C+A">Alessandro Mirizzi</a>, <a href="/search/physics?searchtype=author&query=Mueck%2C+M">Michael Mueck</a>, <a href="/search/physics?searchtype=author&query=Nardi%2C+E">Enrico Nardi</a>, <a href="/search/physics?searchtype=author&query=Nguyen%2C+F">Federico Nguyen</a>, <a href="/search/physics?searchtype=author&query=Rettaroli%2C+A">Alessio Rettaroli</a>, <a href="/search/physics?searchtype=author&query=Rezvani%2C+J">Javad Rezvani</a>, <a href="/search/physics?searchtype=author&query=Teofilo%2C+F+E">Francesco Enrico Teofilo</a>, <a href="/search/physics?searchtype=author&query=Tocci%2C+S">Simone Tocci</a> , et al. (3 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="2309.00351v1-abstract-short" style="display: inline;"> We present a proposal for a new experiment, the FINUDA magnet for Light Axion SearcH (FLASH), a large resonant-cavity haloscope in a high static magnetic field which is planned to probe new physics in the form of dark matter (DM) axions, scalar fields, chameleons, hidden photons, as well as high frequency gravitational waves (GWs). Concerning the QCD axion, FLASH will search for these particles as… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2309.00351v1-abstract-full').style.display = 'inline'; document.getElementById('2309.00351v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2309.00351v1-abstract-full" style="display: none;"> We present a proposal for a new experiment, the FINUDA magnet for Light Axion SearcH (FLASH), a large resonant-cavity haloscope in a high static magnetic field which is planned to probe new physics in the form of dark matter (DM) axions, scalar fields, chameleons, hidden photons, as well as high frequency gravitational waves (GWs). Concerning the QCD axion, FLASH will search for these particles as the DM in the mass range (0.49-1.49) ueV, thus filling the mass gap between the ranges covered by other planned searches. A dedicated Microstrip SQUID operating at ultra-cryogenic temperatures will amplify the signal. The frequency range accessible overlaps with the Very High Frequency (VHF) range of the radio wave spectrum and allows for a search in GWs in the frequency range (100-300) MHz. The experiment will make use of the cryogenic plant and magnet of the FINUDA experiment at INFN Frascati National Laboratories near Rome (Italy); the operations needed to restore the functionalities of the apparatus are currently underway. We present the setup of the experiment and the sensitivity forecasts for the detection of axions, scalar fields, chameleons, hidden photons, and GWs. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2309.00351v1-abstract-full').style.display = 'none'; document.getElementById('2309.00351v1-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 September, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> September 2023. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> CA21106; CA21136 </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Phys.Dark Univ. 42 (2023) 101370 </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2304.07505">arXiv:2304.07505</a> <span> [<a href="https://arxiv.org/pdf/2304.07505">pdf</a>, <a href="https://arxiv.org/format/2304.07505">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="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.108.062005">10.1103/PhysRevD.108.062005 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for galactic axions with a traveling wave parametric amplifier </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Di+Vora%2C+R">R. Di Vora</a>, <a href="/search/physics?searchtype=author&query=Lombardi%2C+A">A. Lombardi</a>, <a href="/search/physics?searchtype=author&query=Ortolan%2C+A">A. Ortolan</a>, <a href="/search/physics?searchtype=author&query=Pengo%2C+R">R. Pengo</a>, <a href="/search/physics?searchtype=author&query=Ruoso%2C+G">G. Ruoso</a>, <a href="/search/physics?searchtype=author&query=Braggio%2C+C">C. Braggio</a>, <a href="/search/physics?searchtype=author&query=Carugno%2C+G">G. Carugno</a>, <a href="/search/physics?searchtype=author&query=Taffarello%2C+L">L. Taffarello</a>, <a href="/search/physics?searchtype=author&query=Cappelli%2C+G">G. Cappelli</a>, <a href="/search/physics?searchtype=author&query=Crescini%2C+N">N. Crescini</a>, <a href="/search/physics?searchtype=author&query=Esposito%2C+M">M. Esposito</a>, <a href="/search/physics?searchtype=author&query=Planat%2C+L">L. Planat</a>, <a href="/search/physics?searchtype=author&query=Ranadive%2C+A">A. Ranadive</a>, <a href="/search/physics?searchtype=author&query=Roch%2C+N">N. Roch</a>, <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=D%27Elia%2C+A">A. D'Elia</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">D. Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">C. Gatti</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=Rettaroli%2C+A">A. Rettaroli</a>, <a href="/search/physics?searchtype=author&query=Tocci%2C+S">S. Tocci</a>, <a href="/search/physics?searchtype=author&query=D%27Agostino%2C+D">D. D'Agostino</a>, <a href="/search/physics?searchtype=author&query=Gambardella%2C+U">U. Gambardella</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="2304.07505v1-abstract-short" style="display: inline;"> A traveling wave parametric amplifier has been integrated in the haloscope of the QUAX experiment. A search for dark matter axions has been performed with a high Q dielectric cavity immersed in a 8 T magnetic field and read by a detection chain having a system noise temperature of about 2.1 K at the frequency of 10.353 GHz. Scanning has been conducted by varying the cavity frequency using sapphire… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.07505v1-abstract-full').style.display = 'inline'; document.getElementById('2304.07505v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2304.07505v1-abstract-full" style="display: none;"> A traveling wave parametric amplifier has been integrated in the haloscope of the QUAX experiment. A search for dark matter axions has been performed with a high Q dielectric cavity immersed in a 8 T magnetic field and read by a detection chain having a system noise temperature of about 2.1 K at the frequency of 10.353 GHz. Scanning has been conducted by varying the cavity frequency using sapphire rods immersed into the cavity. At multiple operating frequencies, the sensitivity of the instrument was at the level of viable axion models. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2304.07505v1-abstract-full').style.display = 'none'; document.getElementById('2304.07505v1-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 April, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2302.07556">arXiv:2302.07556</a> <span> [<a href="https://arxiv.org/pdf/2302.07556">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Quantum Physics">quant-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1109/TASC.2022.3218072">10.1109/TASC.2022.3218072 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Stepping closer to pulsed single microwave photon detectors for axions search </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=D%27Elia%2C+A">A. D'Elia</a>, <a href="/search/physics?searchtype=author&query=Rettaroli%2C+A">A. Rettaroli</a>, <a href="/search/physics?searchtype=author&query=Tocci%2C+S">S. Tocci</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Barone%2C+C">C. Barone</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M">M. Beretta</a>, <a href="/search/physics?searchtype=author&query=Buonomo%2C+B">B. Buonomo</a>, <a href="/search/physics?searchtype=author&query=Chiarello%2C+F">F. Chiarello</a>, <a href="/search/physics?searchtype=author&query=Chikhi%2C+N">N. Chikhi</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">D. Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Felici%2C+G">G. Felici</a>, <a href="/search/physics?searchtype=author&query=Filatrella%2C+G">G. Filatrella</a>, <a href="/search/physics?searchtype=author&query=Fistul%2C+M">M. Fistul</a>, <a href="/search/physics?searchtype=author&query=Foggetta%2C+L+G">L. G. Foggetta</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">C. Gatti</a>, <a href="/search/physics?searchtype=author&query=Il%27ichev%2C+E">E. Il'ichev</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">C. Ligi</a>, <a href="/search/physics?searchtype=author&query=Lisitskiy%2C+M">M. Lisitskiy</a>, <a href="/search/physics?searchtype=author&query=Maccarrone%2C+G">G. Maccarrone</a>, <a href="/search/physics?searchtype=author&query=Mattioli%2C+F">F. Mattioli</a>, <a href="/search/physics?searchtype=author&query=Oelsner%2C+G">G. Oelsner</a>, <a href="/search/physics?searchtype=author&query=Pagano%2C+S">S. Pagano</a>, <a href="/search/physics?searchtype=author&query=Piersanti%2C+L">L. Piersanti</a>, <a href="/search/physics?searchtype=author&query=Ruggiero%2C+B">B. Ruggiero</a>, <a href="/search/physics?searchtype=author&query=Torrioli%2C+G">G. Torrioli</a> , et al. (1 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="2302.07556v1-abstract-short" style="display: inline;"> Axions detection requires the ultimate sensitivity down to the single photon limit. In the microwave region this corresponds to energies in the yJ range. This extreme sensitivity has to be combined with an extremely low dark count rate, since the probability of axions conversion into microwave photons is supposed to be very low. To face this complicated task, we followed two promising approaches t… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.07556v1-abstract-full').style.display = 'inline'; document.getElementById('2302.07556v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2302.07556v1-abstract-full" style="display: none;"> Axions detection requires the ultimate sensitivity down to the single photon limit. In the microwave region this corresponds to energies in the yJ range. This extreme sensitivity has to be combined with an extremely low dark count rate, since the probability of axions conversion into microwave photons is supposed to be very low. To face this complicated task, we followed two promising approaches that both rely on the use of superconducting devices based on the Josephson effect. The first one is to use a single Josephson junction (JJ) as a switching detector (i.e. exploiting the superconducting to normal state transition in presence of microwave photons). We designed a device composed of a coplanar waveguide terminated on a current biased Josephson junction. We tested its efficiency to pulsed (pulse duration 10 ns) microwave signals, since this configuration is closer to an actual axions search experiment. We show how our device is able to reach detection capability of the order of 10 photons with frequency 8 GHz. The second approach is based on an intrinsically quantum device formed by two resonators coupled only via a superconducting qubit network (SQN). This approach relies on quantum nondemolition measurements of the resonator photons. We show that injecting RF power into the resonator, the frequency position of the resonant drop in the transmission coefficient (S21) can be modulated up to 4 MHz. We anticipate that, once optimized, both the devices have the potential to reach single photon sensitivity. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2302.07556v1-abstract-full').style.display = 'none'; document.getElementById('2302.07556v1-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, 2023; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> February 2023. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2208.12670">arXiv:2208.12670</a> <span> [<a href="https://arxiv.org/pdf/2208.12670">pdf</a>, <a href="https://arxiv.org/format/2208.12670">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="Instrumentation and Detectors">physics.ins-det</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1103/PhysRevD.106.052007">10.1103/PhysRevD.106.052007 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Search for galactic axions with a high-Q dielectric cavity </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=Braggio%2C+C">C. Braggio</a>, <a href="/search/physics?searchtype=author&query=Carugno%2C+G">G. Carugno</a>, <a href="/search/physics?searchtype=author&query=Crescini%2C+N">N. Crescini</a>, <a href="/search/physics?searchtype=author&query=DAgostino%2C+D">D. DAgostino</a>, <a href="/search/physics?searchtype=author&query=D%27Elia%2C+A">A. D'Elia</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">D. Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Di+Vora%2C+R">R. Di Vora</a>, <a href="/search/physics?searchtype=author&query=Falferi%2C+P">P. Falferi</a>, <a href="/search/physics?searchtype=author&query=Gambardella%2C+U">U. Gambardella</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">C. Gatti</a>, <a href="/search/physics?searchtype=author&query=Iannone%2C+G">G. Iannone</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">C. Ligi</a>, <a href="/search/physics?searchtype=author&query=Lombardi%2C+A">A. Lombardi</a>, <a href="/search/physics?searchtype=author&query=Maccarrone%2C+G">G. Maccarrone</a>, <a href="/search/physics?searchtype=author&query=Ortolan%2C+A">A. Ortolan</a>, <a href="/search/physics?searchtype=author&query=Pengo%2C+R">R. Pengo</a>, <a href="/search/physics?searchtype=author&query=Rettaroli%2C+A">A. Rettaroli</a>, <a href="/search/physics?searchtype=author&query=Ruoso%2C+G">G. Ruoso</a>, <a href="/search/physics?searchtype=author&query=Taffarello%2C+L">L. Taffarello</a>, <a href="/search/physics?searchtype=author&query=Tocci%2C+S">S. Tocci</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="2208.12670v1-abstract-short" style="display: inline;"> A haloscope of the QUAX--$a纬$ experiment, composed of an high-Q resonant cavity immersed in a 8 T magnet and cooled to $\sim 4.5$~K is operated to search for galactic axion with mass $m_a\simeq42.8~渭\text{eV}$. The design of the cavity with hollow dielectric cylinders concentrically inserted in a OFHC Cu cavity, allowed us to maintain a loaded quality-factor Q $\sim 300000$ during the measurements… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2208.12670v1-abstract-full').style.display = 'inline'; document.getElementById('2208.12670v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2208.12670v1-abstract-full" style="display: none;"> A haloscope of the QUAX--$a纬$ experiment, composed of an high-Q resonant cavity immersed in a 8 T magnet and cooled to $\sim 4.5$~K is operated to search for galactic axion with mass $m_a\simeq42.8~渭\text{eV}$. The design of the cavity with hollow dielectric cylinders concentrically inserted in a OFHC Cu cavity, allowed us to maintain a loaded quality-factor Q $\sim 300000$ during the measurements in presence of magnetic field. Through the cavity tuning mechanism it was possible to modulate the resonance frequency of the haloscope in the region $10.35337-10.35345$~GHz and thus acquire different dataset at different resonance frequencies. Acquiring each dataset for about 50 minutes, combining them and correcting for the axion's signal estimation-efficiency we set a limit on the axion-photon coupling $g_{a纬纬}< 0.731\times10^{-13}$ GeV$^{-1}$ with the confidence level set at $90\%$. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2208.12670v1-abstract-full').style.display = 'none'; document.getElementById('2208.12670v1-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> 26 August, 2022; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> August 2022. </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2107.01118">arXiv:2107.01118</a> <span> [<a href="https://arxiv.org/pdf/2107.01118">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="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1742-6596/1559/1/012020">10.1088/1742-6596/1559/1/012020 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1088/1742-6596/1559/1/012020">10.1088/1742-6596/1559/1/012020 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Development of a Josephson junction based single photon microwave detector for axion detection experiments </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=Barone%2C+C">C Barone</a>, <a href="/search/physics?searchtype=author&query=Buonomo%2C+B">B Buonomo</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M+M">M M Beretta</a>, <a href="/search/physics?searchtype=author&query=Bianchini%2C+L">L Bianchini</a>, <a href="/search/physics?searchtype=author&query=Castellano%2C+G">G Castellano</a>, <a href="/search/physics?searchtype=author&query=Chiarello%2C+F">F Chiarello</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=Felici%2C+G">G Felici</a>, <a href="/search/physics?searchtype=author&query=Filatrella%2C+G">G Filatrella</a>, <a href="/search/physics?searchtype=author&query=Foggetta%2C+L+G">L G Foggetta</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=Giazotto%2C+F">F Giazotto</a>, <a href="/search/physics?searchtype=author&query=Lamanna%2C+G">G Lamanna</a>, <a href="/search/physics?searchtype=author&query=Ligabue%2C+F">F Ligabue</a>, <a href="/search/physics?searchtype=author&query=Ligato%2C+N">N Ligato</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=Margesin%2C+B">B Margesin</a>, <a href="/search/physics?searchtype=author&query=Mattioli%2C+F">F Mattioli</a>, <a href="/search/physics?searchtype=author&query=Monticone%2C+E">E Monticone</a>, <a href="/search/physics?searchtype=author&query=Oberto%2C+L">L Oberto</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="2107.01118v1-abstract-short" style="display: inline;"> Josephson junctions, in appropriate configurations, can be excellent candidates for detection of single photons in the microwave frequency band. Such possibility has been recently addressed in the framework of galactic axion detection. Here are reported recent developments in the modelling and simulation of dynamic behaviour of a Josephson junction single microwave photon detector. For a Josephson… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.01118v1-abstract-full').style.display = 'inline'; document.getElementById('2107.01118v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2107.01118v1-abstract-full" style="display: none;"> Josephson junctions, in appropriate configurations, can be excellent candidates for detection of single photons in the microwave frequency band. Such possibility has been recently addressed in the framework of galactic axion detection. Here are reported recent developments in the modelling and simulation of dynamic behaviour of a Josephson junction single microwave photon detector. For a Josephson junction to be enough sensitive, small critical currents and operating temperatures of the order of ten of mK are necessary. Thermal and quantum tunnelling out of the zero-voltage state can also mask the detection process. Axion detection would require dark count rates in the order of 0.001 Hz. It is, therefore, is of paramount importance to identify proper device fabrication parameters and junction operation point. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.01118v1-abstract-full').style.display = 'none'; document.getElementById('2107.01118v1-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> 2 July, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 9 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> J. Phys.: Conf. Ser. 1559 012020 (2020) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2107.00558">arXiv:2107.00558</a> <span> [<a href="https://arxiv.org/pdf/2107.00558">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="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1007/s10909-020-02381-x">10.1007/s10909-020-02381-x <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Status of the SIMP Project: Toward the Single Microwave Photon Detection </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alesini%2C+D">David Alesini</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">Danilo Babusci</a>, <a href="/search/physics?searchtype=author&query=Barone%2C+C">Carlo Barone</a>, <a href="/search/physics?searchtype=author&query=Buonomo%2C+B">Bruno Buonomo</a>, <a href="/search/physics?searchtype=author&query=Beretta%2C+M+M">Matteo Mario Beretta</a>, <a href="/search/physics?searchtype=author&query=Bianchini%2C+L">Lorenzo Bianchini</a>, <a href="/search/physics?searchtype=author&query=Castellano%2C+G">Gabriella Castellano</a>, <a href="/search/physics?searchtype=author&query=Chiarello%2C+F">Fabio Chiarello</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">Daniele Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Falferi%2C+P">Paolo Falferi</a>, <a href="/search/physics?searchtype=author&query=Felici%2C+G">Giulietto Felici</a>, <a href="/search/physics?searchtype=author&query=Filatrella%2C+G">Giovanni Filatrella</a>, <a href="/search/physics?searchtype=author&query=Foggetta%2C+L+G">Luca Gennaro Foggetta</a>, <a href="/search/physics?searchtype=author&query=Gallo%2C+A">Alessandro Gallo</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">Claudio Gatti</a>, <a href="/search/physics?searchtype=author&query=Giazotto%2C+F">Francesco Giazotto</a>, <a href="/search/physics?searchtype=author&query=Lamanna%2C+G">Gianluca Lamanna</a>, <a href="/search/physics?searchtype=author&query=Ligabue%2C+F">Franco Ligabue</a>, <a href="/search/physics?searchtype=author&query=Ligato%2C+N">Nadia Ligato</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">Carlo Ligi</a>, <a href="/search/physics?searchtype=author&query=Maccarrone%2C+G">Giovanni Maccarrone</a>, <a href="/search/physics?searchtype=author&query=Margesin%2C+B">Benno Margesin</a>, <a href="/search/physics?searchtype=author&query=Mattioli%2C+F">Francesco Mattioli</a>, <a href="/search/physics?searchtype=author&query=Monticone%2C+E">Eugenio Monticone</a>, <a href="/search/physics?searchtype=author&query=Oberto%2C+L">Luca Oberto</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="2107.00558v1-abstract-short" style="display: inline;"> The Italian institute for nuclear physics (INFN) has financed the SIMP project (2019-2021) in order to strengthen its skills and technologies in the field of meV detectors with the ultimate aim of developing a single microwave photon detector. This goal will be pursued by improving the sensitivity and the dark count rate of two types of photodetectors: current biased Josephson Junction (JJ) for th… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.00558v1-abstract-full').style.display = 'inline'; document.getElementById('2107.00558v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2107.00558v1-abstract-full" style="display: none;"> The Italian institute for nuclear physics (INFN) has financed the SIMP project (2019-2021) in order to strengthen its skills and technologies in the field of meV detectors with the ultimate aim of developing a single microwave photon detector. This goal will be pursued by improving the sensitivity and the dark count rate of two types of photodetectors: current biased Josephson Junction (JJ) for the frequency range 10-50 GHz and Transition Edge Sensor (TES) for the frequency range 30-100 GHz. Preliminary results on materials and devices characterization are presented. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2107.00558v1-abstract-full').style.display = 'none'; document.getElementById('2107.00558v1-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 July, 2021; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2021. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">7 pages, 4 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Journal of Low Temperature Physics (2020) 199:348-354 </p> </li> <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/1811.06754">arXiv:1811.06754</a> <span> [<a href="https://arxiv.org/pdf/1811.06754">pdf</a>, <a href="https://arxiv.org/format/1811.06754">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> <p class="title is-5 mathjax"> The Klash Proposal: Status and Perspectives </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Gatti%2C+C">C. Gatti</a>, <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=Braggio%2C+C">C. Braggio</a>, <a href="/search/physics?searchtype=author&query=Carugno%2C+G">G. Carugno</a>, <a href="/search/physics?searchtype=author&query=Crescini%2C+N">N. Crescini</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=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=Ortolan%2C+A">A. Ortolan</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>, <a href="/search/physics?searchtype=author&query=Ruoso%2C+G">G. Ruoso</a>, <a href="/search/physics?searchtype=author&query=Tocci%2C+S">S. Tocci</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="1811.06754v1-abstract-short" style="display: inline;"> Recently some of the authors proposed a search for galactic axions with mass about 0.2~$渭$eV using a large volume resonant cavity, tens of cubic meters, cooled down to 4~K and immersed in a magnetic field of about 0.6~T generated inside the superconducting magnet of the KLOE experiment located at the National Laboratory of Frascati of INFN. This experiment, called KLASH (KLoe magnet for Axion Sear… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1811.06754v1-abstract-full').style.display = 'inline'; document.getElementById('1811.06754v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1811.06754v1-abstract-full" style="display: none;"> Recently some of the authors proposed a search for galactic axions with mass about 0.2~$渭$eV using a large volume resonant cavity, tens of cubic meters, cooled down to 4~K and immersed in a magnetic field of about 0.6~T generated inside the superconducting magnet of the KLOE experiment located at the National Laboratory of Frascati of INFN. This experiment, called KLASH (KLoe magnet for Axion SearcH), has a potential sensitivity on the axion-to-photon coupling, $g_{a纬纬}$, of about $6\times10^{-17}$ $\mbox{GeV}^{-1}$, reaching the region predicted by KSVZ\cite{KSVZ} and DFSZ\cite{DFSZ} models of QCD axions. We report here the status of the project. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1811.06754v1-abstract-full').style.display = 'none'; document.getElementById('1811.06754v1-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 November, 2018; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> November 2018. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">Contributed to the 14th Patras Workshop on Axions, WIMPs and WISPs, DESY in Hamburg, June 18 to 22, 2018</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1707.06010">arXiv:1707.06010</a> <span> [<a href="https://arxiv.org/pdf/1707.06010">pdf</a>, <a href="https://arxiv.org/format/1707.06010">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> <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"> The KLASH Proposal </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alesini%2C+D">David Alesini</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">Danilo Babusci</a>, <a href="/search/physics?searchtype=author&query=Di+Gioacchino%2C+D">Daniele Di Gioacchino</a>, <a href="/search/physics?searchtype=author&query=Gatti%2C+C">Claudio Gatti</a>, <a href="/search/physics?searchtype=author&query=Lamanna%2C+G">Gianluca Lamanna</a>, <a href="/search/physics?searchtype=author&query=Ligi%2C+C">Carlo Ligi</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="1707.06010v1-abstract-short" style="display: inline;"> We propose a search of galactic axions with mass about 0.2 microeV using a large volume resonant cavity, about 50 m^3, cooled down to 4 K and immersed in a moderate axial magnetic field of about 0.6 T generated inside the superconducting magnet of the KLOE experiment located at the National Laboratory of Frascati of INFN. This experiment, called KLASH (KLoe magnet for Axion SearcH) in the followin… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.06010v1-abstract-full').style.display = 'inline'; document.getElementById('1707.06010v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1707.06010v1-abstract-full" style="display: none;"> We propose a search of galactic axions with mass about 0.2 microeV using a large volume resonant cavity, about 50 m^3, cooled down to 4 K and immersed in a moderate axial magnetic field of about 0.6 T generated inside the superconducting magnet of the KLOE experiment located at the National Laboratory of Frascati of INFN. This experiment, called KLASH (KLoe magnet for Axion SearcH) in the following, has a potential sensitivity on the axion-to-photon coupling, g_agg, of about 6x10^-17 GeV-1, reaching the region predicted by KSVZ and DFSZ models of QCD axions. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1707.06010v1-abstract-full').style.display = 'none'; document.getElementById('1707.06010v1-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 July, 2017; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> July 2017. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Report number:</span> INFN-17-14/LNF </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/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/1210.6751">arXiv:1210.6751</a> <span> [<a href="https://arxiv.org/pdf/1210.6751">pdf</a>, <a href="https://arxiv.org/ps/1210.6751">ps</a>, <a href="https://arxiv.org/format/1210.6751">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> <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"> Exploring quantum vacuum with low-energy photons </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Milotti%2C+E">E. Milotti</a>, <a href="/search/physics?searchtype=author&query=Della+Valle%2C+F">F. Della Valle</a>, <a href="/search/physics?searchtype=author&query=Zavattini%2C+G">G. Zavattini</a>, <a href="/search/physics?searchtype=author&query=Messineo%2C+G">G. Messineo</a>, <a href="/search/physics?searchtype=author&query=Gastaldi%2C+U">U. Gastaldi</a>, <a href="/search/physics?searchtype=author&query=Pengo%2C+R">R. Pengo</a>, <a href="/search/physics?searchtype=author&query=Ruoso%2C+G">G. Ruoso</a>, <a href="/search/physics?searchtype=author&query=Babusci%2C+D">D. Babusci</a>, <a href="/search/physics?searchtype=author&query=Curceanu%2C+C">C. Curceanu</a>, <a href="/search/physics?searchtype=author&query=Iliescu%2C+M">M. Iliescu</a>, <a href="/search/physics?searchtype=author&query=Milardi%2C+C">C. Milardi</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="1210.6751v1-abstract-short" style="display: inline;"> Although quantum mechanics (QM) and quantum field theory (QFT) are highly successful, the seemingly simplest state -- vacuum -- remains mysterious. While the LHC experiments are expected to clarify basic questions on the structure of QFT vacuum, much can still be done at lower energies as well. For instance, experiments like PVLAS try to reach extremely high sensitivities, in their attempt to obse… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1210.6751v1-abstract-full').style.display = 'inline'; document.getElementById('1210.6751v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1210.6751v1-abstract-full" style="display: none;"> Although quantum mechanics (QM) and quantum field theory (QFT) are highly successful, the seemingly simplest state -- vacuum -- remains mysterious. While the LHC experiments are expected to clarify basic questions on the structure of QFT vacuum, much can still be done at lower energies as well. For instance, experiments like PVLAS try to reach extremely high sensitivities, in their attempt to observe the effects of the interaction of visible or near-visible photons with intense magnetic fields -- a process which becomes possible in quantum electrodynamics (QED) thanks to the vacuum fluctuations of the electronic field, and which is akin to photon-photon scattering. PVLAS is now close to data-taking and if it reaches the required sensitivity, it could provide important information on QED vacuum. PVLAS and other similar experiments face great challenges as they try to measure an extremely minute effect. However, raising the photon energy greatly increases the photon-photon cross-section, and gamma rays could help extract much more information from the observed light-light scattering. Here we discuss an experimental design to measure photon-photon scattering close to the peak of the photon-photon cross-section, that could fit in the proposed construction of an FEL facility at the Cabibbo Lab near Frascati (Rome, Italy). <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1210.6751v1-abstract-full').style.display = 'none'; document.getElementById('1210.6751v1-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> 25 October, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> October 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">19 pages, 5 figures. Extended version of a talk given by E. Milotti at the workshop "Quantum 2012", Turin, May 21-25 2012. Accepted for publication in the International Journal of Quantum Information</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1206.0680">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/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/0906.0875">arXiv:0906.0875</a> <span> [<a href="https://arxiv.org/pdf/0906.0875">pdf</a>, <a href="https://arxiv.org/ps/0906.0875">ps</a>, <a href="https://arxiv.org/format/0906.0875">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.2009.09.110">10.1016/j.nima.2009.09.110 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The Low Energy Tagger for 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=Bini%2C+C">C. Bini</a>, <a href="/search/physics?searchtype=author&query=Ciambrone%2C+P">P. Ciambrone</a>, <a href="/search/physics?searchtype=author&query=Corradi%2C+G">G. Corradi</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=Fiore%2C+S">S. Fiore</a>, <a href="/search/physics?searchtype=author&query=Gauzzi%2C+P">P. Gauzzi</a>, <a href="/search/physics?searchtype=author&query=Iannarelli%2C+M">M. Iannarelli</a>, <a href="/search/physics?searchtype=author&query=Miscetti%2C+S">S. Miscetti</a>, <a href="/search/physics?searchtype=author&query=Paglia%2C+C">C. Paglia</a>, <a href="/search/physics?searchtype=author&query=Tagnani%2C+D">D. Tagnani</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="0906.0875v1-abstract-short" style="display: inline;"> The KLOE experiment at the upgraded DAFNE e+e- collider in Frascati (KLOE-2) is going to start a new data taking at the beginning of 2010 with its detector upgraded with a tagging system for the identification of gamma-gamma interactions. The tagging stations for low-energy e+e- will consist in two calorimeters The calorimeter used to detect low-energy e+e- will be placed between the beam-pipe o… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0906.0875v1-abstract-full').style.display = 'inline'; document.getElementById('0906.0875v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0906.0875v1-abstract-full" style="display: none;"> The KLOE experiment at the upgraded DAFNE e+e- collider in Frascati (KLOE-2) is going to start a new data taking at the beginning of 2010 with its detector upgraded with a tagging system for the identification of gamma-gamma interactions. The tagging stations for low-energy e+e- will consist in two calorimeters The calorimeter used to detect low-energy e+e- will be placed between the beam-pipe outer support structure and the inner wall of the KLOE drift chamber. This calorimeter will be made of LYSO crystals readout by Silicon Photomultipliers, to achieve an energy resolution better than 8% at 200 MeV. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0906.0875v1-abstract-full').style.display = 'none'; document.getElementById('0906.0875v1-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, 2009; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> June 2009. </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, 5 figures, in the proceedings of "Frontier detectors for frontier physics", isola d'Elba, Italy, May 2009</span> </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" style="display: inline-block;"><a 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