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The DarkSide Multiton Detector for the Direct Dark Matter Search
Aalseth, CE; Agnes, P; Alton, A; Arisaka, K; Asner, DM; Back, HO; Baldin, B; Biery, K; Bonfini, G; Bossa, M; Brigatti, A; Brodsky, J; Budano, F; Cadonati, L; Cadoni, M; Calaprice, F; Canci, N; Candela, A; Cao, H; Cariello, M; Cavalcante, P; Chepurnov, A; Cocco, AG; Condon, C; Crippa, L; D'Angelo, D; D'Incecco, M; Davini, S; De Deo, M; Derbin, A; Devoto, A; Di Eusanio, F; Edkins, E; Empl, A; Fan, A; Fiorillo, G; Fomenko, K; Forster, G; Foxe, M; Franco, D; Gabriele, F; Galbiati, C; Goretti, A; Grandi, L; Gromov, M; Guan, MY; Guardincerri, Y; Hackett, B; Herner, K; Hime, A; Humble, P; Hungerford, E; Ianni, A; Ianni, A; Jaffe, DE; Jollet, C; Keeter, K; Kendziora, C; Kidner, S; Kobychev, V; Koh, G; Korablev, D; Korga, G; Kurlej, A; Li, PX; Lissia, M; Lombardi, P; Ludhova, L; Luitz, S; Lukyachenko, G; Ma, YQ; Machulin, I; Mandarano, A; Mari, SM; Maricic, J; Marini, L; Markov, D; Martoff, J; Meregaglia, A; Meroni, E; Meyers, PD; Miletic, T; Milincic, R; Montuschi, M; Monzani, ME; Mosteiro, P; Mount, B; Muratova, V; Musico, P; Montanari, D; Nelson, A; Odrowski, S; Odrzywolek, A; Orrell, JL; Orsini, M; Ortica, F; Pagani, L; Pallavicini, M; Pantic, E; Parmeggiano, S; Parsells, B; Pelczar, K; Pelliccia, N; Perasso, S; Perasso, L; Pocar, A; Pordes, S; Pugachev, D; Qian, H; Randle, K; Ranucci, G; Razeto, A; Recine, K; Reinhold, B; Renshaw, A; Romani, A; Rossi, N; Rossi, B; Rountree, SD; Sablone, D; Saggese, P; Saldanha, R; Sands, W; Sangiorgio, S; Segreto, E; Semenov, D; Shields, E; Skorokhvatov, M; Smallcomb, M; Smirnov, O; Sotnikov, A; Suvurov, Y; Tartaglia, R; Tatarowicz, J; Testera, G; Tonazzo, A; Unzhakov, E; Vogelaar, RB; Wada, M; Walker, SE; Wang, H; Wang, Y; Watson, AW; Westerdale, S; Williams, R; Wojcik, M; Xu, J; Yang, CG; Yoo, J; Yu, B; Zavatarelli, S; Zhong, WL; Zuzel, G; Guan MY(关梦云); Li PX(李佩弦); Ma YQ(马宇倩); Wang Y(王宇); Yang ZG(杨长根); Zhong WL(钟玮丽)
2015
发表期刊ADVANCES IN HIGH ENERGY PHYSICS
页码541362
文章类型Article
摘要Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (< 100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.
学科领域Physics
DOI10.1155/2015/541362
收录类别SCI
WOS类目Physics, Particles & Fields
WOS记录号WOS:000353133400001
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被引频次:8[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/228338
专题粒子天体物理中心
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Aalseth, CE,Agnes, P,Alton, A,et al. The DarkSide Multiton Detector for the Direct Dark Matter Search[J]. ADVANCES IN HIGH ENERGY PHYSICS,2015:541362.
APA Aalseth, CE.,Agnes, P.,Alton, A.,Arisaka, K.,Asner, DM.,...&钟玮丽.(2015).The DarkSide Multiton Detector for the Direct Dark Matter Search.ADVANCES IN HIGH ENERGY PHYSICS,541362.
MLA Aalseth, CE,et al."The DarkSide Multiton Detector for the Direct Dark Matter Search".ADVANCES IN HIGH ENERGY PHYSICS (2015):541362.
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