DarkSide uses a dual-phase Liquid Argon Time Projection Chamber to search for WIMP dark matter. The current detector, DarkSide-50, is running since mid 2015 with a target of 50 kg of Argon from an underground source. Here it is presented the latest results of searches of WIMP-nucleus interactions, with WIMP masses in the GeV-TeV range, and of WIMP-electron interactions, in the sub-GeV mass range. The future of DarkSide with a new generation experiment, involving a global collaboration from all the current Argon based experiments, is presented.

Sanfilippo, S., Agnes, P., M Albuquerque, I., Alexander, T., Alton, A., Asner, D., et al. (2019). DarkSide status and prospects. IL NUOVO CIMENTO C, 42(2-3) [10.1393/ncc/i2019-19079-8].

DarkSide status and prospects

Carpinelli M.;
2019

Abstract

DarkSide uses a dual-phase Liquid Argon Time Projection Chamber to search for WIMP dark matter. The current detector, DarkSide-50, is running since mid 2015 with a target of 50 kg of Argon from an underground source. Here it is presented the latest results of searches of WIMP-nucleus interactions, with WIMP masses in the GeV-TeV range, and of WIMP-electron interactions, in the sub-GeV mass range. The future of DarkSide with a new generation experiment, involving a global collaboration from all the current Argon based experiments, is presented.
Articolo in rivista - Articolo scientifico
Matter;
English
Sanfilippo, S., Agnes, P., M Albuquerque, I., Alexander, T., Alton, A., Asner, D., et al. (2019). DarkSide status and prospects. IL NUOVO CIMENTO C, 42(2-3) [10.1393/ncc/i2019-19079-8].
Sanfilippo, S; Agnes, P; M Albuquerque, I; Alexander, T; Alton, A; Asner, D; Ave, M; Back, H; Batignani, G; Biery, K; Bocci, V; Bonfini, G; Bonivento, W; Bottino, B; Budano, F; Bussino, S; Cadeddu, M; Cadoni, M; Calaprice, F; Caminata, A; Canci, N; Candela, A; Caravati, M; Cardenas, M; Cariello, M; Carlini, M; Carpinelli, M; Catalanotti, S; Cataudella, V; Cavalcante, P; Cavuoti, S; Chepurnov, A; Cicalo, C; Cifarelli, L; Cocco, A; Covone, G; D'Angelo, D; D'Incecco, M; D'Urso, D; Davini, S; De Candia, A; De Cecco, S; De Deo, M; De Filippis, G; De Rosa, G; De Vincenzi, M; Derbin, A; Devoto, A; Di Eusanio, F; Di Pietro, G; Dionisi, C; Edkins, E; Empl, A; Fiorillo, G; Fomenko, K; Franco, D; Gabriele, F; Galbiati, C; Garcia Abia, P; Ghiano, C; Giagu, S; Giganti, C; Giovanetti, G; Gorchakov, O; Goretti, A; Granato, F; Gromov, M; Guan, M; Guardincerri, Y; Gulino, M; Hackett, B; Herner, K; Horikawa, S; Hosseini, B; Hughes, D; Humble, P; Hungerford, E; Ianni, A; Ippolito, V; James, I; Keeter, K; Kendziora, C; Kochanek, I; Koh, G; Korablev, D; Korga, G; Kubankin, A; Kuss, M; La Commara, M; Lai, M; Li, X; Lissia, M; Longo, G; Machado, A; Machulin, I; Mandarano, A; Mapelli, L; Mari, S; Maricic, J; Jmartoff, C; Messina, A; Meyers, P; Milincic, R; Monte, A; Morrocchi, M; Muratova, V; Musico, P; Nania, R; Navrer Agasson, A; Nozdrina, A; Oleinik, A; Orsini, M; Ortica, F; Pagani, L; Pallavicini, M; Pandola, L; Pantic, E; Paoloni, E; Pelczar, K; Pelliccia, N; Pesudo, V; Picciau, E; Pocar, A; Pordes, S; Poudel, S; Pugachev, D; Qian, H; Ragusa, F; Razeti, M; Razeto, A; Renshaw, A; Rescigno, M; Riffard, Q; Romani, A; Rossi, B; Rossi, N; Sablone, D; Samoylov, O; Sands, W; Santorelli, R; Savarese, C; Scapparone, E; Schlitzer, B; Segreto, E; Semenov, D; Shchagin, A; Sheshukov, A; Simeone, M; Singh, P; Skorokhvatov, M; Smirnov, O; Sotnikov, A; Stanford, C; Stracka, S; Suvorov, Y; Tartaglia, R; Testera, G; Tonazzo, A; Trinchese, P; Unzhakov, E; Verducci, M; Vishneva, A; Vogelaar, B; Wada, M; Waldrop, T; Wang, H; Wang, Y; Watson, A; Westerdale, S; Wojcik, M; Xiang, X; Xiao, X; Yang, C; Ye, Z; Zhu, C; Zuzel, G
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/389113
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