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Results from the first use of low radioactivity argon in a dark matter search

Author(s): Agnes, P; Agostino, L; Albuquerque, IFM; Alexander, T; Alton, AK; et al

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dc.contributor.authorAgnes, P-
dc.contributor.authorAgostino, L-
dc.contributor.authorAlbuquerque, IFM-
dc.contributor.authorAlexander, T-
dc.contributor.authorAlton, AK-
dc.contributor.authorArisaka, K-
dc.contributor.authorBack, HO-
dc.contributor.authorBaldin, B-
dc.contributor.authorBiery, K-
dc.contributor.authorBonfini, G-
dc.contributor.authorBossa, M-
dc.contributor.authorBottino, B-
dc.contributor.authorBrigatti, A-
dc.contributor.authorBrodsky, J-
dc.contributor.authorBudano, F-
dc.contributor.authorBussino, S-
dc.contributor.authorCadeddu, M-
dc.contributor.authorCadonati, L-
dc.contributor.authorCadoni, M-
dc.contributor.authorCalaprice, Frank P-
dc.contributor.authorCanci, N-
dc.contributor.authorCandela, A-
dc.contributor.authorCao, H-
dc.contributor.authorCariello, M-
dc.contributor.authorCarlini, M-
dc.contributor.authorCatalanotti, S-
dc.contributor.authorCavalcante, P-
dc.contributor.authorChepurnov, A-
dc.contributor.authorCocco, AG-
dc.contributor.authorCovone, G-
dc.contributor.authorCrippa, L-
dc.contributor.authorD Angelo, D-
dc.contributor.authorD Incecco, M-
dc.contributor.authorDavini, S-
dc.contributor.authorDe Cecco, S-
dc.contributor.authorDe Deo, M-
dc.contributor.authorDe Vincenzi, M-
dc.contributor.authorDerbin, A-
dc.contributor.authorDevoto, A-
dc.contributor.authorDi Eusanio, F-
dc.contributor.authorDi Pietro, G-
dc.contributor.authorEdkins, E-
dc.contributor.authorEmpl, A-
dc.contributor.authorFan, A-
dc.contributor.authorFiorillo, G-
dc.contributor.authorFomenko, K-
dc.contributor.authorForster, G-
dc.contributor.authorFranco, D-
dc.contributor.authorGabriele, F-
dc.contributor.authorGalbiati, Cristiano-
dc.contributor.authorGiganti, C-
dc.contributor.authorGoretti, AM-
dc.contributor.authorGranato, F-
dc.contributor.authorGrandi, L-
dc.contributor.authorGromov, M-
dc.contributor.authorGuan, M-
dc.contributor.authorGuardincerri, Y-
dc.contributor.authorHackett, BR-
dc.contributor.authorHerner, K-
dc.contributor.authorHungerford, EV-
dc.contributor.authorIanni, Al-
dc.contributor.authorIanni, An-
dc.contributor.authorJames, I-
dc.contributor.authorJollet, C-
dc.contributor.authorKeeter, K-
dc.contributor.authorKendziora, CL-
dc.contributor.authorKobychev, V-
dc.contributor.authorKoh, G-
dc.contributor.authorKorablev, D-
dc.contributor.authorKorga, G-
dc.contributor.authorKubankin, A-
dc.contributor.authorLi, X-
dc.contributor.authorLissia, M-
dc.contributor.authorLombardi, P-
dc.contributor.authorLuitz, S-
dc.contributor.authorMa, Y-
dc.contributor.authorMachulin, IN-
dc.contributor.authorMandarano, A-
dc.contributor.authorMari, SM-
dc.contributor.authorMaricic, J-
dc.contributor.authorMarini, L-
dc.contributor.authorMartoff, CJ-
dc.contributor.authorMeregaglia, A-
dc.contributor.authorMeyers, Peter D-
dc.contributor.authorMiletic, T-
dc.contributor.authorMilincic, R-
dc.contributor.authorMontanari, D-
dc.contributor.authorMonte, A-
dc.contributor.authorMontuschi, M-
dc.contributor.authorMonzani, M-
dc.contributor.authorMosteiro, P-
dc.contributor.authorMount, BJ-
dc.contributor.authorMuratova, VN-
dc.contributor.authorMusico, P-
dc.contributor.authorNapolitano, J-
dc.contributor.authorNelson, A-
dc.contributor.authorOdrowski, S-
dc.contributor.authorOrsini, M-
dc.contributor.authorOrtica, F-
dc.contributor.authorPagani, L-
dc.contributor.authorPallavicini, M-
dc.contributor.authorPantic, E-
dc.contributor.authorParmeggiano, S-
dc.contributor.authorPelczar, K-
dc.contributor.authorPelliccia, N-
dc.contributor.authorPerasso, S-
dc.contributor.authorPocar, A-
dc.contributor.authorPordes, S-
dc.contributor.authorPugachev, DA-
dc.contributor.authorQian, H-
dc.contributor.authorRandle, K-
dc.contributor.authorRanucci, G-
dc.contributor.authorRazeto, A-
dc.contributor.authorReinhold, B-
dc.contributor.authorRenshaw, AL-
dc.contributor.authorRomani, A-
dc.contributor.authorRossi, B-
dc.contributor.authorRossi, N-
dc.contributor.authorRountree, D-
dc.contributor.authorSablone, D-
dc.contributor.authorSaggese, P-
dc.contributor.authorSaldanha, R-
dc.contributor.authorSands, W-
dc.contributor.authorSangiorgio, S-
dc.contributor.authorSavarese, C-
dc.contributor.authorSegreto, E-
dc.contributor.authorSemenov, DA-
dc.contributor.authorShields, E-
dc.contributor.authorSingh, PN-
dc.contributor.authorSkorokhvatov, MD-
dc.contributor.authorSmirnov, O-
dc.contributor.authorSotnikov, A-
dc.contributor.authorStanford, C-
dc.contributor.authorSuvorov, Y-
dc.contributor.authorTartaglia, R-
dc.contributor.authorTatarowicz, J-
dc.contributor.authorTestera, G-
dc.contributor.authorTonazzo, A-
dc.contributor.authorTrinchese, P-
dc.contributor.authorUnzhakov, EV-
dc.contributor.authorVishneva, A-
dc.contributor.authorVogelaar, B-
dc.contributor.authorWada, M-
dc.contributor.authorWalker, S-
dc.contributor.authorWang, H-
dc.contributor.authorWang, Y-
dc.contributor.authorWatson, AW-
dc.contributor.authorWesterdale, S-
dc.contributor.authorWilhelmi, J-
dc.contributor.authorWojcik, MM-
dc.contributor.authorXiang, X-
dc.contributor.authorXu, J-
dc.contributor.authorYang, C-
dc.contributor.authorYoo, J-
dc.contributor.authorZavatarelli, S-
dc.contributor.authorZec, A-
dc.contributor.authorZhong, W-
dc.contributor.authorZhu, C-
dc.contributor.authorZuzel, G-
dc.contributor.authorCollaboration, DarkSide-
dc.date.accessioned2017-11-21T19:36:05Z-
dc.date.available2017-11-21T19:36:05Z-
dc.date.issued2016-04-08en_US
dc.identifier.citationAgnes, P, Agostino, L, Albuquerque, IFM, Alexander, T, Alton, AK, Arisaka, K, Back, HO, Baldin, B, Biery, K, Bonfini, G, Bossa, M, Bottino, B, Brigatti, A, Brodsky, J, Budano, F, Bussino, S, Cadeddu, M, Cadonati, L, Cadoni, M, Calaprice, F, Canci, N, Candela, A, Cao, H, Cariello, M, Carlini, M, Catalanotti, S, Cavalcante, P, Chepurnov, A, Cocco, AG, Covone, G, Crippa, L, D Angelo, D, D Incecco, M, Davini, S, De Cecco, S, De Deo, M, De Vincenzi, M, Derbin, A, Devoto, A, Di Eusanio, F, Di Pietro, G, Edkins, E, Empl, A, Fan, A, Fiorillo, G, Fomenko, K, Forster, G, Franco, D, Gabriele, F, Galbiati, C, Giganti, C, Goretti, AM, Granato, F, Grandi, L, Gromov, M, Guan, M, Guardincerri, Y, Hackett, BR, Herner, K, Hungerford, EV, Ianni, Al, Ianni, An, James, I, Jollet, C, Keeter, K, Kendziora, CL, Kobychev, V, Koh, G, Korablev, D, Korga, G, Kubankin, A, Li, X, Lissia, M, Lombardi, P, Luitz, S, Ma, Y, Machulin, IN, Mandarano, A, Mari, SM, Maricic, J, Marini, L, Martoff, CJ, Meregaglia, A, Meyers, PD, Miletic, T, Milincic, R, Montanari, D, Monte, A, Montuschi, M, Monzani, M, Mosteiro, P, Mount, BJ, Muratova, VN, Musico, P, Napolitano, J, Nelson, A, Odrowski, S, Orsini, M, Ortica, F, Pagani, L, Pallavicini, M, Pantic, E, Parmeggiano, S, Pelczar, K, Pelliccia, N, Perasso, S, Pocar, A, Pordes, S, Pugachev, DA, Qian, H, Randle, K, Ranucci, G, Razeto, A, Reinhold, B, Renshaw, AL, Romani, A, Rossi, B, Rossi, N, Rountree, D, Sablone, D, Saggese, P, Saldanha, R, Sands, W, Sangiorgio, S, Savarese, C, Segreto, E, Semenov, DA, Shields, E, Singh, PN, Skorokhvatov, MD, Smirnov, O, Sotnikov, A, Stanford, C, Suvorov, Y, Tartaglia, R, Tatarowicz, J, Testera, G, Tonazzo, A, Trinchese, P, Unzhakov, EV, Vishneva, A, Vogelaar, B, Wada, M, Walker, S, Wang, H, Wang, Y, Watson, AW, Westerdale, S, Wilhelmi, J, Wojcik, MM, Xiang, X, Xu, J, Yang, C, Yoo, J, Zavatarelli, S, Zec, A, Zhong, W, Zhu, C, Zuzel, G, Collaboration, DarkSide. (2016). Results from the first use of low radioactivity argon in a dark matter search. PHYSICAL REVIEW D, 93 (10.1103/PhysRevD.93.081101en_US
dc.identifier.issn2470-0010-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1dd27-
dc.description.abstractLiquid argon is a bright scintillator with potent particle identification properties, making it an attractive target for direct-detection dark matter searches. The DarkSide-50 dark matter search here reports the first WIMP search results obtained using a target of low-radioactivity argon. DarkSide-50 is a dark matter detector, using a two-phase liquid argon time projection chamber, located at the Laboratori Nazionali del Gran Sasso. The underground argon is shown to contain Ar-39 at a level reduced by a factor (1.4 +/- 0.2) x 10(3) relative to atmospheric argon. We report a background-free null result from (2616 +/- 43) kg d of data, accumulated over 70.9 live days. When combined with our previous search using an atmospheric argon, the 90% C.L. upper limit on the WIMP-nucleon spin-independent cross section, based on zero events found in the WIMP search regions, is 2.0 x 10(-4)4 cm(2) (8.6 x 10(-44) cm(2), 8.0 x 10(-43) cm(2)) for a WIMP mass of 100 GeV/c(2) (1 TeV/c(2), 10 TeV/c(2)).en_US
dc.format.extent081101-1 - 081101-7en_US
dc.language.isoenen_US
dc.relation.ispartofPHYSICAL REVIEW Den_US
dc.rightsAuthor's manuscripten_US
dc.titleResults from the first use of low radioactivity argon in a dark matter searchen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1103/PhysRevD.93.081101-
dc.date.eissued2016-04-08en_US
dc.identifier.eissn2470-0029-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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