The DarkSide project

P. Agnes 1 L. Agostino 2 I.F.M. Albuquerque T. Alexander A.K. Alton K. Arisaka H.O. Back B. Baldin K. Biery G. Bonfini M. Bossa B. Bottino A. Brigatti J. Brodsky F. Budano S. Bussino M. Cadeddu L. Cadonati M. Cadoni F. Calaprice N. Canci A. Candela H. Cao M. Cariello M. Carlini S. Catalanotti P. Cavalcante A. Chepurnov A.G. Cocco G. Covone L. Crippa D. D'Angelo M. D'Incecco S. Davini S. De Cecco 2 M. De Deo M. De Vincenzi A. Derbin A. Devoto F. Di Eusanio G. Di Pietro E. Edkins A. Empl A. Fan G. Fiorillo K. Fomenko G. Forster D. Franco 1 F. Gabriele C. Galbiati C. Giganti 2 A.M. Goretti F. Granato L. Grandi M. Gromov M. Guan Y. Guardincerri B.R. Hackett K. Herner E.V. Hungerford Al. Ianni An. Ianni I. James C. Jollet A.F.K. Keeter C.L. Kendziora V. Kobychev Ah G. Koh D. Korablev G. Korga A. Kubankin X. Li M. Lissia P. Lombardi S. Luitz Y. Ma I.N. Machulin Al A. Mandarano S.M. Mari J. Maricic L. Marini C.J. Martoff A. Meregaglia 3 P.D. Meyers T. Miletic R. Milincic D. Montanari A. Monte M. Montuschi M. Monzani P. Mosteiro B.J. Mount V.N. Muratova P. Musico J. Napolitano A. Nelson S. Odrowski M. Orsini F. Ortica L. Pagani M. Pallavicini E. Pantic S. Parmeggiano K. Pelczar N. Pelliccia S. Perasso 1 A. Pocar S. Pordes D.A. Pugachev H. Qian K. Randle G. Ranucci A. Razeto B. Reinhold A.L. Renshaw A. Romani B. Rossi N. Rossi D. Rountree D. Sablone P. Saggese R. Saldanha W. Sands S. Sangiorgio C. Savarese E. Segreto D.A. Semenov E. Shields P.N. Singh M.D. Skorokhvatov O. Smirnov A. Sotnikov C. Stanford Y. Suvorov R. Tartaglia J. Tatarowicz G. Testera A. Tonazzo 1 P. Trinchese E.V. Unzhakov A. Vishneva B. Vogelaar M. Wada S. Walker H. Wang Y. Wang A.W. Watson S. Westerdale J. Wilhelmi M.M. Wojcik X. Xiang J. Xu C. Yang J. Yoo S. Zavatarelli A. Zec W. Zhong C. Zhu G. Zuzel
Abstract : DarkSide is a graded experimental project based on radiopure argon, and is now, and will be, used in direct dark matter searches. The present DarkSide-50 detector, operating at the Gran Sasso National Laboratory, is a dual-phase, 50 kg, liquid argon time-projection-chamber surrounded by an active liquid scintillator veto. It is designed to be background free in 3 years of operation. DS-50 performances, when filled with atmospheric argon, are reported. However DS-50 filled with underground argon, shows impressive reduction of the (39)Ar isotope. The application of this powerful technology in a future generation of the DarkSide program is discussed.
Type de document :
Communication dans un congrès
LIght Detection in Noble Elements, Aug 2015, Albany, United States. JINST, 11 (02), pp.C02051, 2016, 〈10.1088/1748-0221/11/02/C02051〉
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https://hal.archives-ouvertes.fr/hal-02065890
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Soumis le : mercredi 13 mars 2019 - 09:04:15
Dernière modification le : vendredi 22 mars 2019 - 01:38:54

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P. Agnes, L. Agostino, I.F.M. Albuquerque, T. Alexander, A.K. Alton, et al.. The DarkSide project. LIght Detection in Noble Elements, Aug 2015, Albany, United States. JINST, 11 (02), pp.C02051, 2016, 〈10.1088/1748-0221/11/02/C02051〉. 〈hal-02065890〉

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