000131829 001__ 131829
000131829 005__ 20241125101156.0
000131829 0247_ $$2doi$$a10.1016/j.dark.2023.101370
000131829 0248_ $$2sideral$$a137129
000131829 037__ $$aART-2023-137129
000131829 041__ $$aeng
000131829 100__ $$aAlesini, David
000131829 245__ $$aThe future search for low-frequency axions and new physics with the FLASH resonant cavity experiment at Frascati National Laboratories
000131829 260__ $$c2023
000131829 5060_ $$aAccess copy available to the general public$$fUnrestricted
000131829 5203_ $$aWe 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
, 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
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.
000131829 540__ $$9info:eu-repo/semantics/openAccess$$aby-nc-nd$$uhttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
000131829 590__ $$a5.0$$b2023
000131829 592__ $$a1.377$$b2023
000131829 591__ $$aASTRONOMY & ASTROPHYSICS$$b14 / 84 = 0.167$$c2023$$dQ1$$eT1
000131829 593__ $$aSpace and Planetary Science$$c2023$$dQ1
000131829 593__ $$aAstronomy and Astrophysics$$c2023$$dQ1
000131829 594__ $$a9.6$$b2023
000131829 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/submittedVersion
000131829 700__ $$aBabusci, Danilo
000131829 700__ $$aBeltrame, Paolo
000131829 700__ $$aBossi, Fabio
000131829 700__ $$aCiambrone, Paolo
000131829 700__ $$aD’Elia, Alessandro
000131829 700__ $$aDi Gioacchino, Daniele
000131829 700__ $$aDi Pirro, Giampiero
000131829 700__ $$aDöbrich, Babette
000131829 700__ $$aFalferi, Paolo
000131829 700__ $$aGatti, Claudio
000131829 700__ $$aGiannotti, Maurizio$$uUniversidad de Zaragoza
000131829 700__ $$aGianotti, Paola
000131829 700__ $$aLamanna, Gianluca
000131829 700__ $$aLigi, Carlo
000131829 700__ $$aMaccarrone, Giovanni
000131829 700__ $$aMazzitelli, Giovanni
000131829 700__ $$aMirizzi, Alessandro
000131829 700__ $$aMueck, Michael
000131829 700__ $$aNardi, Enrico
000131829 700__ $$aNguyen, Federico
000131829 700__ $$aRettaroli, Alessio
000131829 700__ $$aRezvani, Javad
000131829 700__ $$aTeofilo, Francesco Enrico
000131829 700__ $$aTocci, Simone
000131829 700__ $$aTomassini, Sandro
000131829 700__ $$aVisinelli, Luca
000131829 700__ $$aZantedeschi, Michael
000131829 7102_ $$12004$$2038$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Astronomía y Astrofísica
000131829 773__ $$g42 (2023), 101370 [26 pp.]$$pPhys. dark universe$$tPhysics of the Dark Universe$$x2212-6864
000131829 8564_ $$s6945733$$uhttps://zaguan.unizar.es/record/131829/files/texto_completo.pdf$$yPreprint$$zinfo:eu-repo/date/embargoEnd/2024-10-31
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000131829 909CO $$ooai:zaguan.unizar.es:131829$$particulos$$pdriver
000131829 951__ $$a2024-11-22-12:09:39
000131829 980__ $$aARTICLE