/ Instrumentation


Direct Search for Dark Matter with DarkSide


Agnes, P. (APC, Paris) ; Alexander, T. (Massachusetts U., Amherst) ; Alton, A. (Augustana Coll., Sioux Falls) ; Arisaka, K. (Stanford U., Phys. Dept.) ; Back, H.O. (Princeton U.) ; Baldin, B. (Fermilab) ; Biery, K. (Fermilab) ; Bonfini, G. (Gran Sasso) ; Bossa, M. (Gran Sasso) ; Brigatti, A. (Milan U.) ; Brodsky, J. (Princeton U.) ; Budano, F. (Rome III U.) ; Cadonati, L. (Massachusetts U., Amherst) ; Calaprice, F. (Princeton U.) ; Canci, N. (Princeton U.) ; Candela, A. (Gran Sasso) ; Cao, H. (Princeton U.) ; Cariello, M. (INFN, Genoa) ; Cavalcante, P. (Gran Sasso) ; Chavarria, A. (Chicago U., KICP) ; Chepurnov, A. (SINP, Moscow) ; Cocco, A.G. (Naples U.) ; Crippa, L. (Milan U.) ; D'Angelo, D. (Milan U.) ; D'Incecco, M. (Gran Sasso) ; Davini, S. (Houston U.) ; De Deo, M. (Gran Sasso) ; Derbin, A. (St. Petersburg, INP) ; Devoto, A. (INFN, Cagliari) ; Eusanio, F.Di (Princeton U.) ; Pietro, G.Di (Milan U.) ; Edkins, E. (Hawaii U.) ; Empl, A. (Houston U.) ; Fan, A. (Naples U.) ; Fiorillo, G. (Naples U.) ; Fomenko, K. (Dubna, JINR) ; Forster, G. (Massachusetts U., Amherst) ; Franco, D. (APC, Paris) ; Gabriele, F. (Gran Sasso) ; Galbiati, C. (Princeton U.) ; Goretti, A. (Princeton U.) ; Grandi, L. (Chicago U., KICP) ; Gromov, M. (SINP, Moscow) ; Guan, M.Y. (Beijing, Inst. High Energy Phys.) ; Guardincerri, Y. (Fermilab) ; Hackett, B. (Hawaii U.) ; Herner, K. (Fermilab) ; Hungerford, E.V. (Houston U.) ; Ianni, Al (Gran Sasso) ; Ianni, An (Princeton U.) ; Jollet, C. (Strasbourg, IPHC) ; Keeter, K. (Black Hills State U.) ; Kendziora, C. (Fermilab) ; Kidner, S. (Virginia Tech.) ; Kobychev, V. (Kiev, INR) ; Koh, G. (Princeton U.) ; Korablev, D. (Dubna, JINR) ; Korga, G. (Houston U.) ; Kurlej, A. (Massachusetts U., Amherst) ; Li, P.X. (Beijing, Inst. High Energy Phys.) ; Loer, B. (Princeton U.) ; Lombardi, P. (Milan U.) ; Love, C. (Temple U.) ; Ludhova, L. (Milan U.) ; Luitz, S. (Temple U.) ; Ma, Y.Q. (Beijing, Inst. High Energy Phys.) ; Machulin, I. (Moscow Phys. Eng. Inst.) ; Mandarano, A. (Rome III U.) ; Mari, S. (Rome III U.) ; Maricic, J. (Hawaii U.) ; Marini, L. (Rome III U.) ; Martoff, C.J. (Temple U.) ; Meregaglia, A. (Strasbourg, IPHC) ; Meroni, E. (Milan U.) ; Meyers, P.D. (Princeton U.) ; Milincic, R. (Hawaii U.) ; Montanari, D. (Fermilab) ; Montuschi, M. (Gran Sasso) ; Monzani, M.E. (SLAC) ; Mosteiro, P. (Princeton U.) ; Mount, B. (Black Hills State U.) ; Muratova, V. (St. Petersburg, INP) ; Musico, P. (INFN, Genoa) ; Nelson, A. (Princeton U.) ; Odrowski, S. (Gran Sasso) ; Okounkova, M. (Princeton U.) ; Orsini, M. (Gran Sasso) ; Ortica, F. (Perugia U.) ; Pagani, L. (INFN, Genoa) ; Pallavicini, M. (INFN, Genoa) ; Pantic, E. (UC, Davis) ; Papp, L. (Virginia Tech.) ; Parmeggiano, S. (Milan U.) ; Parsells, R. (Princeton U.) ; Pelczar, K. (Jagiellonian U.) ; Pelliccia, N. (Perugia U.) ; Perasso, S. (APC, Paris) ; Pocar, A. (Massachusetts U., Amherst) ; Pordes, S. (Fermilab) ; Pugachev, D. (Kurchatov Inst., Moscow) ; Qian, H. (Princeton U.) ; Randle, K. (Massachusetts U., Amherst) ; Ranucci, G. (Milan U.) ; Razeto, A. (Gran Sasso) ; Reinhold, B. (Hawaii U.) ; Renshaw, A. (Stanford U., Phys. Dept.) ; Romani, A. (Perugia U.) ; Rossi, B. (Naples U.) ; Rossi, N. (Gran Sasso) ; Rountree, S.D. (Virginia Tech.) ; Sablone, D. (Houston U.) ; Saggese, P. (Gran Sasso) ; Saldanha, R. (Chicago U., KICP) ; Sands, W. (Princeton U.) ; Sangiorgio, S. (LLNL, Livermore) ; Segreto, E. (Gran Sasso) ; Semenov, D. (St. Petersburg, INP) ; Shields, E. (Princeton U.) ; Skorokhvatov, M. (Moscow Phys. Eng. Inst.) ; Smirnov, O. (Dubna, JINR) ; Sotnikov, A. (Dubna, JINR) ; Stanford, C. (Princeton U.) ; Suvorov, Y. (Stanford U., Phys. Dept.) ; Tartaglia, R. (Gran Sasso) ; Tatarowicz, J. (Temple U.) ; Testera, G. (INFN, Genoa) ; Tonazzo, A. (APC, Paris) ; Unzhakov, E. (St. Petersburg, INP) ; Vogelaar, R.B. (Virginia Tech.) ; Wada, M. (Princeton U.) ; Walker, S. (Naples U.) ; Wang, H. (Stanford U., Phys. Dept.) ; Wang, Y. (Beijing, Inst. High Energy Phys.) ; Watson, A. (Temple U.) ; Westerdale, S. (Princeton U.) ; Wojcik, M. (Jagiellonian U.) ; Wright, A. (Princeton U.) ; Xiang, X. (Princeton U.) ; Xu, J. (Princeton U.) ; Yang, C.G. (Beijing, Inst. High Energy Phys.) ; Yoo, J. (Fermilab) ; Zavatarelli, S. (INFN, Genoa) ; Zec, A. (Massachusetts U., Amherst) ; Zhu, C. (Princeton U.) ; Zuzel, G. (Jagiellonian U.)

Published in: J.Phys.Conf.Ser.
Year: 2015
Vol.: 650    Num./Issue: 1
Page No: 012006
Pages: 7
Year: 2015-11-16 published

Abstract: The DarkSide experiment is designed for the direct detection of Dark Matter with a double phase liquid Argon TPC operating underground at Laboratori Nazionali del Gran Sasso. The TPC is placed inside a 30 tons liquid organic scintillator sphere, acting as a neutron veto, which is in turn installed inside a 1 kt water Cherenkov detector. The current detector is running since November 2013 with a 50 kg atmospheric Argon fill and we report here the first null results of a Dark Matter search for a (1422 ± 67) kg.d exposure. This result correspond to a 90% CL upper limit on the WIMP-nucleon cross section of 6.1 × 10(-44) cm(2) (for a WIMP mass of 100 GeV/c(2)) and it's currently the most sensitive limit obtained with an Argon target.

Web-Page: http://inspirehep.net/record/1405580/files/1742-6596_650_1_012006.pdf


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DOI: 10.1088/1742-6596/650/1/012006
 Запись создана 2015-12-01, последняя модификация 2016-01-11


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