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)
刊名ADVANCES IN HIGH ENERGY PHYSICS
2015
页码541362
学科分类Physics
DOI10.1155/2015/541362
文章类型Article
英文摘要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.
类目[WOS]Physics, Particles & Fields
收录类别SCI
WOS记录号WOS:000353133400001
引用统计
被引频次:7[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
专题中国科学院高能物理研究所_粒子天体物理中心_期刊论文
中国科学院高能物理研究所_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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