| Texto completo | |
| Autor(es): Mostrar menos - |
Agnes, P.
[1]
;
Albuquerque, I. F. M.
[2]
;
Alexander, T.
[3]
;
Alton, A. K.
[4]
;
Asner, D. M.
[3]
;
Back, H. O.
[3]
;
Biery, K.
[5]
;
Bocci, V.
[6]
;
Bonfini, G.
[7]
;
Bonivento, W.
[8]
;
Bossa, M.
[9, 7]
;
Bottino, B.
[10, 11]
;
Budano, F.
[12, 13]
;
Bussino, S.
[12, 13]
;
Cadeddu, M.
[8, 14]
;
Cadoni, M.
[8, 14]
;
Calaprice, F.
[15]
;
Canci, N.
[1, 7]
;
Candela, A.
[7]
;
Caravati, M.
[8, 14]
;
Cariello, M.
[10]
;
Carlini, M.
[7]
;
Catalanotti, S.
[16, 17]
;
Cataudella, V.
[16, 17]
;
Cavalcante, P.
[18, 7]
;
Chepurnov, A.
[19]
;
Cicalo, C.
[8]
;
Cocco, A. G.
[17]
;
Covone, G.
[16, 17]
;
D'Angelo, D.
[20, 21]
;
D'Incecco, M.
[7]
;
Davini, S.
[9, 10]
;
de Candia, A.
[16, 17]
;
De Cecco, S.
[22]
;
De Deo, M.
[7]
;
De Filippis, G.
[16, 17]
;
De Vincenzi, M.
[12, 13]
;
Derbin, A. V.
[23]
;
De Rosa, G.
[16, 17]
;
Devoto, A.
[8, 14]
;
Di Eusanio, F.
[15]
;
Di Pietro, G.
[7, 21]
;
Dionisi, C.
[6, 22]
;
Edkins, E.
[24]
;
Empl, A.
[1]
;
Fan, A.
[25]
;
Fiorillo, G.
[16, 17]
;
Fomenko, K.
[26]
;
Franco, D.
[27]
;
Gabriele, F.
[7]
;
Galbiati, C.
[15, 21]
;
Giagu, S.
[6, 22]
;
Giganti, C.
[28]
;
Giovanetti, G. K.
[15]
;
Goretti, A. M.
[7]
;
Granato, F.
[29]
;
Gromov, M.
[19]
;
Guan, M.
[4]
;
Guardincerri, Y.
[5]
;
Hackett, B. R.
[24]
;
Herner, K.
[5]
;
Hughes, D.
[15]
;
Humble, P.
[3]
;
Hungerford, E. V.
[1]
;
Ianni, An.
[15, 7]
;
James, I.
[12, 13]
;
Johnson, T. N.
[30]
;
Keeter, K.
[31]
;
Kendziora, C. L.
[5]
;
Koh, G.
[15]
;
Korablev, D.
[26]
;
Korga, G.
[1, 7]
;
Kubankin, A.
[32]
;
Li, X.
[15]
;
Lissia, M.
[8]
;
Loer, B.
[3]
;
Longo, G.
[16, 17]
;
Ma, Y.
[4]
;
Machado, A. A.
;
Machulin, I. N.
[33, 34]
;
Mandarano, A.
[9, 7]
;
Mari, S. M.
[12, 13]
;
Maricic, J.
[24]
;
Martoff, C. J.
[29]
;
Meyers, P. D.
[15]
;
Milincic, R.
[24]
;
Monte, A.
[35, 36]
;
Mount, B. J.
[31]
;
Muratova, V. N.
[23]
;
Musico, P.
[10]
;
Napolitano, J.
[29]
;
Agasson, A. Navrer
[28]
;
Oleinik, A.
[32]
;
Orsini, M.
[7]
;
Ortica, F.
[37, 38]
;
Pagani, L.
[30]
;
Pallavicini, M.
[10, 11]
;
Pantic, E.
[30]
;
Pelczar, K.
[7]
;
Pelliccia, N.
[37, 38]
;
Pocar, A.
[35, 36]
;
Pordes, S.
[5]
;
Pugachev, D. A.
[34]
;
Qian, H.
[15]
;
Randle, K.
[15]
;
Razeti, M.
[8]
;
Razeto, A.
[15, 7]
;
Reinhold, B.
[24]
;
Renshaw, A. L.
[1]
;
Rescigno, M.
[6]
;
Riffard, Q.
[27]
;
Romani, A.
[37, 38]
;
Rossi, B.
[17]
;
Rossi, N.
[7]
;
Sablone, D.
[15, 7]
;
Sands, W.
[15]
;
Sanfilippo, S.
[12, 13]
;
Savarese, C.
[9, 7]
;
Schlitzer, B.
[30]
;
Segreto, E.
[39]
;
Semenov, D. A.
[23]
;
Singh, P. N.
[1]
;
Skorokhvatov, M. D.
[33, 34]
;
Smirnov, O.
[26]
;
Sotnikov, A.
[26]
;
Stanford, C.
[25, 34, 7]
;
Suvorov, Y.
[25, 34, 7]
;
Tartaglia, R.
[7]
;
Testera, G.
[10]
;
Tonazzo, A.
[27]
;
Trinchese, P.
[16, 17]
;
Unzhakov, E. V.
[23]
;
Verducci, M.
[6, 22]
;
Vishneva, A.
[26]
;
Vogelaar, B.
[18]
;
Wada, M.
[15]
;
Walker, S.
[16, 17]
;
Wang, H.
[25]
;
Wang, Y.
[25, 40]
;
Watson, A. W.
[29]
;
Westerdale, S.
[15]
;
Wilhelmi, J.
[29]
;
Wojcik, M. M.
[41]
;
Xiang, X.
[15]
;
Xiao, X.
[25]
;
Yang, C.
[40]
;
Ye, Z.
[1]
;
Zhu, C.
[15]
;
Zuzel, G.
[41]
;
Collaboration, DarkSide
Número total de Autores: 150
|
| Afiliação do(s) autor(es): Mostrar menos - | [1] Univ Houston, Dept Phys, Houston, TX 77204 - USA
[2] Univ Sao Paulo, Inst Fis, BR-05508090 Sao Paulo - Brazil
[3] Pacific Northwest Natl Lab, Richland, WA 99352 - USA
[4] Augustana Univ, Dept Phys, Sioux Falls, SD 57197 - USA
[5] Fermilab Natl Accelerator Lab, Batavia, IL 60510 - USA
[6] INFN, Sez Roma, I-00185 Rome - Italy
[7] INFN, Lab Nazl Gran Sasso, I-67100 Assergi AQ - Italy
[8] INFN Cagliari, I-09042 Cagliari - Italy
[9] Gran Sasso Sci Inst, I-67100 Laquila - Italy
[10] INFN Genova, I-16146 Genoa - Italy
[11] Univ Genoa, Phys Dept, I-16146 Genoa - Italy
[12] INFN Roma Tre, I-00146 Rome - Italy
[13] Univ Rome Tre, Math & Phys Dept, I-00146 Rome - Italy
[14] Univ Cagliari, Phys Dept, I-09042 Cagliari - Italy
[15] Princeton Univ, Dept Phys, Princeton, NJ 08544 - USA
[16] Univ Federico II Naples, Phys Dept, I-80126 Naples - Italy
[17] INFN Napoli, I-80126 Naples - Italy
[18] Virginia Tech, Blacksburg, VA 24061 - USA
[19] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991 - Russia
[20] Univ Milan, Phys Dept, I-20133 Milan - Italy
[21] INFN Milano, I-20133 Milan - Italy
[22] Sapienza Univ Roma, Phys Dept, I-00185 Rome - Italy
[23] St Petersburg Nucl Phys Inst, Gatchina 188350 - Russia
[24] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 - USA
[25] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 - USA
[26] Joint Inst Nucl Res, Dubna 141980 - Russia
[27] USPC, Univ Paris Diderot, APC, CNRS IN2P3, CEA Irfu, Obs Paris, F-75205 Paris - France
[28] Univ Paris 06, Sorbonne Univ, LPNHE, CNRS IN2P3, F-75252 Paris - France
[29] Temple Univ, Dept Phys, Philadelphia, PA 19122 - USA
[30] Univ Calif Davis, Dept Phys, Davis, CA 95616 - USA
[31] Black Hills State Univ, Sch Nat Sci, Spearfish, SD 57799 - USA
[32] Belgorod Natl Res Univ, Radiat Phys Lab, Belgorod 308007 - Russia
[33] Natl Res Nucl Univ MEPhI, Moscow 115409 - Russia
[34] Natl Res Ctr Kurchatov Inst, Moscow 123182 - Russia
[35] Univ Massachusetts, Dept Phys, Amherst, MA 01003 - USA
[36] Univ Massachusetts, Amherst Ctr Fundamental Interact, Amherst, MA 01003 - USA
[37] Univ Perugia, Chem Biol & Biotechnol Dept, I-06123 Perugia - Italy
[38] INFN Perugia, I-06123 Perugia - Italy
[39] Univ Estadual Campinas, Phys Inst, BR-13083 Campinas, SP - Brazil
[40] Inst High Energy Phys, Beijing 100049 - Peoples R China
[41] Jagiellonian Univ, M Smoluchowski Inst Phys, PL-30348 Krakow - Poland
Número total de Afiliações: 41
|
| Tipo de documento: | Artigo Científico |
| Fonte: | Journal of Instrumentation; v. 12, OCT 2017. |
| Citações Web of Science: | 11 |
| Resumo | |
A Geant4-based Monte Carlo package named G4DS has been developed to simulate the response of DarkSide-50, an experiment operating since 2013 at LNGS, designed to detect WIMP interactions in liquid argon. In the process of WIMP searches, DarkSide-50 has achieved two fundamental milestones: the rejection of electron recoil background with a power of similar to 10(7), using the pulse shape discrimination technique, and the measurement of the residual Ar-39 contamination in underground argon, similar to 3 orders of magnitude lower with respect to atmospheric argon. These results rely on the accurate simulation of the detector response to the liquid argon scintillation, its ionization, and electron-ion recombination processes. This work provides a complete overview of the DarkSide Monte Carlo and of its performance, with a particular focus on PARIS, the custommade liquid argon response model. (AU) | |
| Processo FAPESP: | 16/09084-0 - Deteção direta de matéria escura e o experimento "DarkSide" |
| Beneficiário: | Ivone Freire da Mota e Albuquerque |
| Modalidade de apoio: | Auxílio à Pesquisa - Regular |