/ Experiment-HEP


The DarkSide Experiment: Present Status and Future


Zuzel, G. (Jagiellonian U.) ; Agnes, P. (APC, Paris) ; Albuquerque, I.F.M. (Sao Paulo U.) ; Alexander, T. (PNL, Richland) ; Alton, A.K. (Augustana Coll., Sioux Falls) ; Asner, D.M. (PNL, Richland) ; Back, H.O. (PNL, Richland) ; Baldin, B. (Fermilab) ; Biery, K. (Fermilab) ; Bocci, V. (INFN, Rome) ; Bonfini, G. (Gran Sasso) ; Bonivento, W. (INFN, Cagliari) ; Bossa, M. (Gran Sasso) ; Bottino, B. (INFN, Genoa) ; Brigatti, A. (INFN, Milan) ; Brodsky, J. (Princeton U.) ; Budano, F. (Rome III U.) ; Bussino, S. (Rome III U.) ; Cadeddu, M. (INFN, Cagliari) ; Cadonati, L. (Massachusetts U., Amherst) ; Cadoni, M. (INFN, Cagliari) ; Calaprice, F. (Princeton U.) ; Canci, N. (Gran Sasso) ; Candela, A. (Gran Sasso) ; Caravati, M. (INFN, Cagliari) ; Cariello, M. (INFN, Genoa) ; Carlini, M. (Gran Sasso) ; Catalanotti, S. (INFN, Naples) ; Cavalcante, P. (Gran Sasso) ; Chepurnov, A. (SINP, Moscow) ; Cicalò, C. (INFN, Cagliari) ; Cocco, A.G. (INFN, Naples) ; Covone, G. (INFN, Naples) ; D'Angelo, D. (INFN, Milan) ; D'Incecco, M. (Gran Sasso) ; Davini, S. (INFN, Genoa) ; De Cecco, S. (Paris U., VI-VII) ; De Deo, M. (Gran Sasso) ; De Vincenzi, M. (Rome III U.) ; Derbin, A. (St. Petersburg, INP) ; Devoto, A. (INFN, Cagliari) ; Eusanio, F.Di (Princeton U.) ; Pietro, G.Di (INFN, Milan) ; Dionisi, C. (Rome U.) ; Edkins, E. (Hawaii U.) ; Empl, A. (Houston U.) ; Fan, A. (UCLA) ; Fiorillo, G. (INFN, Naples) ; Fomenko, K. (Dubna, JINR) ; Forster, G. (Fermilab) ; Franco, D. (APC, Paris) ; Gabriele, F. (Gran Sasso) ; Galbiati, C. (INFN, Milan) ; Giagu, S. (Rome U.) ; Giganti, C. (Paris U., VI-VII) ; Giovanetti, G.K. (Princeton U.) ; Goretti, A.M. (Gran Sasso) ; Granato, F. (Temple U.) ; Grandi, L. (Chicago U., KICP) ; Gromov, M. (SINP, Moscow) ; Guan, M. (Beijing, Inst. High Energy Phys.) ; Guardincerri, Y. (Fermilab) ; Hackett, B.R. (Hawaii U.) ; Herner, K. (Fermilab) ; Hughes, D. (Princeton U.) ; Humble, P. (PNL, Richland) ; Hungerford, E.V. (Houston U.) ; Ianni, Al. (Gran Sasso) ; Ianni, An. (Gran Sasso) ; James, I. (Rome III U.) ; Johnson, T.N. (UC, Davis) ; Jollet, C. (Strasbourg, IPHC) ; Keeter, K. (Black Hills State U.) ; Kendziora, C.L. (Fermilab) ; Koh, G. (Princeton U.) ; Korablev, D. (Dubna, JINR) ; Korga, G. (Gran Sasso) ; Kubankin, A. (Belgorod State U.) ; Li, X. (Princeton U.) ; Lissia, M. (INFN, Cagliari) ; Loer, B. (PNL, Richland) ; Lombardi, P. (INFN, Milan) ; Longo, G. (INFN, Naples) ; Ma, Y. (Beijing, Inst. High Energy Phys.) ; Machulin, I.N. (Moscow Phys. Eng. Inst.) ; Mandarano, A. (Gran Sasso) ; Mari, S.M. (Rome III U.) ; Maricic, J. (Hawaii U.) ; Marini, L. (INFN, Genoa) ; Martoff, C.J. (Temple U.) ; Meregaglia, A. (Strasbourg, IPHC) ; Meyers, P.D. (Princeton U.) ; Milincic, R. (Hawaii U.) ; Miller, J.D. (Houston U.) ; Montanari, D. (Fermilab) ; Monte, A. (Massachusetts U., Amherst) ; Mount, B.J. (Black Hills State U.) ; Muratova, V.N. (St. Petersburg, INP) ; Musico, P. (INFN, Genoa) ; Napolitano, J. (Temple U.) ; Navrer Agasson, A. (Paris U., VI-VII) ; Odrowski, S. (Gran Sasso) ; Orsini, M. (Gran Sasso) ; Ortica, F. (INFN, Perugia) ; Pagani, L. (INFN, Genoa) ; Pallavicini, M. (INFN, Genoa) ; Pantic, E. (UC, Davis) ; Parmeggiano, S. (INFN, Milan) ; Pelczar, K. (Jagiellonian U.) ; Pelliccia, N. (INFN, Perugia) ; Pocar, A. (Princeton U.) ; Pordes, S. (Fermilab) ; Pugachev, D.A. (Moscow Phys. Eng. Inst.) ; Qian, H. (Princeton U.) ; Randle, K. (Princeton U.) ; Ranucci, G. (INFN, Milan) ; Razeti, M. (INFN, Cagliari) ; Razeto, A. (Princeton U.) ; Reinhold, B. (Hawaii U.) ; Renshaw, A.L. (UCLA) ; Rescigno, M. (INFN, Rome) ; Riffard, Q. (APC, Paris) ; Romani, A. (INFN, Perugia) ; Rossi, B. (Princeton U.) ; Rossi, N. (Gran Sasso) ; Rountree, D. (Virginia Tech.) ; Sablone, D. (Gran Sasso) ; Saggese, P. (INFN, Milan) ; Saldanha, R. (Chicago U., KICP) ; Sands, W. (Princeton U.) ; Savarese, C. (Gran Sasso) ; Schlitzer, B. (UC, Davis) ; Segreto, E. (Campinas State U.) ; Semenov, D.A. (St. Petersburg, INP) ; Shields, E. (Princeton U.) ; Singh, P.N. (Houston U.) ; Skorokhvatov, M.D. (Moscow Phys. Eng. Inst.) ; Smirnov, O. (Dubna, JINR) ; Sotnikov, A. (Dubna, JINR) ; Stanford, C. (Princeton U.) ; Suvorov, Y. (Kurchatov Inst., Moscow) ; Tartaglia, R. (Gran Sasso) ; Tatarowicz, J. (Temple U.) ; Testera, G. (INFN, Genoa) ; Tonazzo, A. (APC, Paris) ; Trinchese, P. (Naples U.) ; Unzhakov, E.V. (St. Petersburg, INP) ; Verducci, M. (Rome U.) ; Vishneva, A. (Dubna, JINR) ; Vogelaar, B. (Virginia Tech.) ; Wada, M. (Princeton U.) ; Walker, S. (INFN, Naples) ; Wang, H. (UCLA) ; Wang, Y. (UCLA) ; Watson, A.W. (Temple U.) ; Westerdale, S. (Princeton U.) ; Wilhelmi, J. (Temple U.) ; Wojcik, M.M. (Jagiellonian U.) ; Xiang, Xi. (Princeton U.) ; Xiao, X. (UCLA) ; Xu, J. (Princeton U.) ; Yang, C. (Beijing, Inst. High Energy Phys.) ; Zec, A. (Massachusetts U., Amherst) ; Zhong, W. (Beijing, Inst. High Energy Phys.) ; Zhu, C. (Princeton U.)

Published in: J.Phys.Conf.Ser.
Year: 2017
Vol.: 798    Num./Issue: 1
Page No: 012109
Pages: 10
Year: 2017-03-15 published

Abstract: DarkSide is a multi-stage program devoted to direct searches of Dark Matter particles with detectors based on double phase liquid Argon Time Projection Chamber. The DarkSide-50 setup is running underground at the Laboratori Nazionali del Gran Sasso. First it was operated with Atmospheric Argon and during that run (1422 ± 67) kg×d of truly background-free exposure has been accumulated. Obtained data made it possible to set a 90% C.L. upper limit on the WIMP-nucleon cross section of 6.1 × 10(−)(44) cm(2) (for a WIMP mass of 100 GeV/c(2)). Presently the detector is filled with Underground Argon, which is depleted in (39)Ar by a factor of (1.4 ± 0.2)×10(3) with respect to Atmospheric Argon. Acquired so far (2616 ± 43) kg×d (71 live days) in combination with the data from the Atmospheric Argon run give us the 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section of 2.0×10(−)(44) cm(2) for a WIMP mass of 100 GeV/c(2). Up to date this is the best limit obtained with an argon target.

Total numbers of views: 268
Numbers of unique views: 129
DOI: 10.1088/1742-6596/798/1/012109
 Record created 2017-04-03, last modified 2017-04-03



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