Abstract
The DarkSide-50 experiment, located at the “Laboratori Nazionali del Gran Sasso (INFN)”, is based on low-radioactivity argon double phase time projection chamber, surrounded by an active liquid scintillator veto, designed for the zero background achievement. The liquid argon features sufficient self shielding and easy scalability to multi-tons scale. The impressive reduction of the 39Ar isotope (compared to the atmospheric argon), along with the excellent pulse shape discrimination, make this technology a possible candidate for the forthcoming generation of multi-ton Dark Matter experiments.
| Original language | English (US) |
|---|---|
| Title of host publication | PARTICLE PHYSICS at the Year of Light |
| Editors | Alexander I. Studenikin, Alexander I. Studenikin |
| Publisher | World Scientific |
| Pages | 355-360 |
| Number of pages | 6 |
| ISBN (Print) | 9789813224551 |
| DOIs | |
| State | Published - 2017 |
| Event | 17th Lomonosov Conference on Elementary Particle Physics, 2015 - Moscow, Russian Federation Duration: Aug 20 2015 → Aug 26 2015 |
Publication series
| Name | Proceedings of the 17th Lomonosov Conference on Elementary Particle Physics - Particle Physics at the Year of Light, 2015 |
|---|---|
| Volume | 0 |
Other
| Other | 17th Lomonosov Conference on Elementary Particle Physics, 2015 |
|---|---|
| Country/Territory | Russian Federation |
| City | Moscow |
| Period | 8/20/15 → 8/26/15 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Nuclear and High Energy Physics
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PARTICLE PHYSICS at the Year of Light. ed. / Alexander I. Studenikin; Alexander I. Studenikin. World Scientific, 2017. p. 355-360 (Proceedings of the 17th Lomonosov Conference on Elementary Particle Physics - Particle Physics at the Year of Light, 2015; Vol. 0).
Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
TY - GEN
T1 - The darkside-50 experiment
T2 - 17th Lomonosov Conference on Elementary Particle Physics, 2015
AU - Agnes, P.
AU - Agostino, L.
AU - Albuquerque, I. F.M.
AU - Alexander, T.
AU - Alton, A. K.
AU - Arisaka, K.
AU - Back, H. O.
AU - Baldin, B.
AU - Biery, K.
AU - Bonfini, G.
AU - Bossa, M.
AU - Bottino, B.
AU - Brigatti, A.
AU - Brodsky, J.
AU - Budano, F.
AU - Bussino, S.
AU - Cadeddu, M.
AU - Cadonati, L.
AU - Cadoni, M.
AU - Calaprice, F.
AU - Canci, N.
AU - Candela, A.
AU - Cao, H.
AU - Cariello, M.
AU - Carlini, M.
AU - Catalanotti, S.
AU - Cavalcante, P.
AU - Chepurnov, A.
AU - Cocco, A. G.
AU - Covone, G.
AU - Crippa, L.
AU - D’Angelo, D.
AU - D’Incecco, M.
AU - Davini, S.
AU - de Cecco, S.
AU - de Deo, M.
AU - de Vincenzi, M.
AU - Derbin, A.
AU - Devoto, A.
AU - di Eusanio, F.
AU - di Pietro, G.
AU - Edkins, E.
AU - Empl, A.
AU - Fan, A.
AU - Fiorillo, G.
AU - Fomenko, K.
AU - Forster, G.
AU - Franco, D.
AU - Gabriele, F.
AU - Galbiati, C.
AU - Giganti, C.
AU - Goretti, A. M.
AU - Granato, F.
AU - Grandi, L.
AU - Gromov, M.
AU - Guan, M.
AU - Guardincerri, Y.
AU - Hackett, B. R.
AU - Herner, K.
AU - Hungerford, E. V.
AU - Ianni, Al
AU - Ianni, An
AU - James, I.
AU - Jollet, C.
AU - Keeter, K.
AU - Kendziora, C. L.
AU - Kobychev, V.
AU - Koh, G.
AU - Korablev, D.
AU - Korga, G.
AU - Kubankin, A.
AU - Li, X.
AU - Lissia, M.
AU - Lombardi, P.
AU - Luitz, S.
AU - Ma, Y.
AU - Machulin, I. N.
AU - Mandarano, A.
AU - Mari, S. M.
AU - Maricic, J.
AU - Marini, L.
AU - Martoff, C. J.
AU - Meregaglia, A.
AU - Meyers, P. D.
AU - Miletic, T.
AU - Milincic, R.
AU - Montanari, D.
AU - Monte, A.
AU - Montuschi, M.
AU - Monzani, M.
AU - Mosteiro, P.
AU - Mount, B. J.
AU - Muratova, V. N.
AU - Musico, P.
AU - Napolitano, J.
AU - Nelson, A.
AU - Odrowski, S.
AU - Orsini, M.
AU - Ortica, F.
AU - Pagani, L.
AU - Pallavicini, M.
AU - Pantic, E.
AU - Parmeggiano, S.
AU - Pelczar, K.
AU - Pelliccia, N.
AU - Perasso, S.
AU - Pocar, A.
AU - Pordes, S.
AU - Pugachev, D. A.
AU - Qian, H.
AU - Randle, K.
AU - Ranucci, G.
AU - Razeto, A.
AU - Reinhold, B.
AU - Renshaw, A. L.
AU - Romani, A.
AU - Rossi, B.
AU - Rossi, N.
AU - Rountree, D.
AU - Sablone, D.
AU - Saggese, P.
AU - Saldanha, R.
AU - Sands, W.
AU - Sangiorgio, S.
AU - Savarese, C.
AU - Segreto, E.
AU - Semenov, D. A.
AU - Shields, E.
AU - Singh, P. N.
AU - Skorokhvatov, M. D.
AU - Smirnov, O.
AU - Sotnikov, A.
AU - Stanford, C.
AU - Suvorov, Y.
AU - Tartaglia, R.
AU - Tatarowicz, J.
AU - Testera, G.
AU - Tonazzo, A.
AU - Trinchese, P.
AU - Unzhakov, E. V.
AU - Vishneva, A.
AU - Vogelaar, B.
AU - Wada, M.
AU - Walker, S.
AU - Wang, H.
AU - Wang, Y.
AU - Watson, A. W.
AU - Westerdale, S.
AU - Wilhelmi, J.
AU - Wojcik, M. M.
AU - Xiang, X.
AU - Xu, J.
AU - Yang, C.
AU - Yoo, J.
AU - Zavatarelli, S.
AU - Zec, A.
AU - Zhong, W.
AU - Zhu, C.
AU - Zuzel, G.
N1 - Funding Information: L’Aquila AQ 67100, Italy; 12Department of Physics, Università degli Studi, Genova 16146, Italy; 13Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Genova 16146, Italy; 14Istituto Nazionale di Fisica Nucleare, Sezione di Milano, Milano 20133, Italy; 15Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tre, Roma 00146, Italy; 16Department of Physics and Mathematics, Università degli Studi Roma Tre, Roma 00146, Italy; 17Department of Physics, Università degli Studi, Cagliari 09042, Italy; 18Istituto Nazionale di Fisica Nu-cleare, Sezione di Cagliari, Cagliari 09042, Italy; 19Department of Physics, University of Houston, Houston, TX 77204, USA; 20Department of Physics, Università degli Studi Federico II, Napoli 80126, Italy; 21Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli 80126, Italy; 22Department of Physics, Virginia Tech, Blacksburg, VA 24061, USA; 23Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119991, Russia; 24Department of Physics, Università degli Studi, Milano 20133, Italy; 25St. Petersburg Nuclear Physics Institute NRC Kurchatov Institute, Gatchina 188350, Russia; 26Department of Physics and Astronomy, University of Hawai’i, Honolulu, HI 96822, USA; 27Joint Institute for Nuclear Research, Dubna 14 1980, Russia; 28Department of Physics, Temple University, Philadelphia, PA 19122, USA; 29Kavli Institute, Enrico Fermi Institute, and Dept. of Physics, University of Chicago, Chicago, IL 60637, USA; 30Institute of High Energy Physics, Beijing 100049, China; 31Laboratorio Subterráneo de Canfranc, Can-franc Esta-ción 22880, Spain; 32IPHC, Universitéde Strasbourg, CNRS/IN2P3, Strasbourg 67037, France; 33School of Natural Sciences, Black Hills State University, Spearfish, SD 57799, USA; 34Institute for Nuclear Research, National Academy of Sciences of Ukraine, Kiev 03680, Ukraine; 35Radiation Physics Laboratory, Belgorod National Research University, Belgorod 308007, Russia ; 36SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA; 37National Research Centre Kurchatov Institute, Moscow 123182, Russia; 38National Research Nuclear University MEPhI, Moscow 115409, Russia; 39Department of Chemistry, Biology and Biotechnology, Università degli Studi, Perugia 06123, Italy; 40Istituto Nazionale di Fisica Nucleare, Sezione di Peru-gia, Perugia 06123, Italy; 41Department of Physics, University of California, Davis, CA 95616, USA; 42Smoluchowski Institute of Physics, Jagiellonian University, Krakow 30348, Poland; 43Lawrence Livermore National Laboratory, Livermore, CA 94550, USA; 44Institute of Physics Gleb Wataghin, Universi-dade Estadual de Campinas, São Paulo 13083-859, Brazil; 45School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China. Publisher Copyright: © 2017, World Scientific Publishing Co. Pte. Ltd. All rights reserved.
PY - 2017
Y1 - 2017
N2 - The DarkSide-50 experiment, located at the “Laboratori Nazionali del Gran Sasso (INFN)”, is based on low-radioactivity argon double phase time projection chamber, surrounded by an active liquid scintillator veto, designed for the zero background achievement. The liquid argon features sufficient self shielding and easy scalability to multi-tons scale. The impressive reduction of the 39Ar isotope (compared to the atmospheric argon), along with the excellent pulse shape discrimination, make this technology a possible candidate for the forthcoming generation of multi-ton Dark Matter experiments.
AB - The DarkSide-50 experiment, located at the “Laboratori Nazionali del Gran Sasso (INFN)”, is based on low-radioactivity argon double phase time projection chamber, surrounded by an active liquid scintillator veto, designed for the zero background achievement. The liquid argon features sufficient self shielding and easy scalability to multi-tons scale. The impressive reduction of the 39Ar isotope (compared to the atmospheric argon), along with the excellent pulse shape discrimination, make this technology a possible candidate for the forthcoming generation of multi-ton Dark Matter experiments.
UR - http://www.scopus.com/inward/record.url?scp=85048532064&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85048532064&partnerID=8YFLogxK
U2 - 10.1142/9789813224568_0057
DO - 10.1142/9789813224568_0057
M3 - Conference contribution
AN - SCOPUS:85048532064
SN - 9789813224551
T3 - Proceedings of the 17th Lomonosov Conference on Elementary Particle Physics - Particle Physics at the Year of Light, 2015
SP - 355
EP - 360
BT - PARTICLE PHYSICS at the Year of Light
A2 - Studenikin, Alexander I.
A2 - Studenikin, Alexander I.
PB - World Scientific
Y2 - 20 August 2015 through 26 August 2015
ER -