Current status of the dark matter experiment DarkSide-50

L. Marini, L. Pagani, P. Agnes, T. Alexander, A. Alton, K. Arisaka, H. Back, B. Baldin, K. Biery, G. Bonfini, M. Bossa, A. Brigatti, J. Brodsky, F. Budano, L. Cadonati, F. Calaprice, N. Canci, A. Candela, H. Cao, M. Cariello, P. Cavalcante, A. Chavarria, A. Chepurnov, A. Cocco, D. D’Angelo, M. D’Incecco, S. Davini, M. Deo, A. Derbin, A. Devoto, F. D. Eusanio, G. D. Pietro, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, G. Forster, D. Franco, F. Gabriele, C. Galbiati, A. Goretti, L. Grandi, M. Gromov, M. Guan, Y. Guardincerri, B. Hackett, K. Herner, P. Humble, E. Hungerford, A. Ianni, A. Ianni, C. Jollet, K. Keeter, C. Kendziora, S. Kidner, V. Kobychev, G. Koh, D. Korablev, G. Korga, A. Kurlej, P. Li, P. Lombardi, C. Love, L. Ludhova, S. Luitz, Yanhui Ma, I. Machulin, A. Mandarano, S. Mari, J. Maricic, C. Martoff, A. Meregaglia, E. Meroni, P. Meyers, R. Milincic, D. Montanari, M. Montuschi, M. Monzani, P. Mosteiro, B. Mount, V. Muratova, P. Musico, A. Nelson, S. Odrowski, M. Okounkova, M. Orsini, F.
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引用次数: 1

Abstract

DarkSide-50 is a dark matter direct search experiment at LNGS, searching for rare nuclear recoils possibly induced by WIMPs. It has two nested vetoes and a dual phase liquid argon TPC as dark matter detector. Key features of this experiment are the use of underground argon as radio-pure target and of muon and neutron active vetoes to suppress the background. The first data-taking campaign was running from November 2013 to April 2015 with an atmospheric argon target and a reduced efficiency neutron veto due to internal contamination. However, an upper limit on the WIMP-nucleon cross section of 6.1×10−44 cm2 at 90% CL was obtained for a WIMP mass of 100 GeV/c2 and an exposure of (1422 ± 67) kg·d. At present DarkSide-50 started a 3 years run, intended to be background-free because the neutron veto was successfully recovered and underground argon replaced the atmospheric one. Additionally calibration campaigns for both the TPC and the neutron veto were completed. Thanks to the good performance of the background rejection, the results obtained so far suggest the scalability of DarkSide-50 to a ton-scale detector, which will play a key role into the dark matter search scenario.
暗物质实验DarkSide-50的现状
DarkSide-50是LNGS的暗物质直接搜索实验,寻找可能由wimp引起的罕见核反冲。它有两个嵌套的探针和一个双相液态氩TPC作为暗物质探测器。该实验的主要特点是利用地下氩气作为放射性纯靶,利用介子和中子的活性抑制来抑制背景辐射。第一次数据采集活动于2013年11月至2015年4月进行,以大气氩气为目标,由于内部污染导致效率降低的中子否决。然而,当WIMP质量为100 GeV/c2,暴露量为(1422±67)kg·d时,90% CL下WIMP-核子截面的上限为6.1×10−44 cm2。目前,DarkSide-50开始了为期3年的运行,由于中子否决权被成功回收,地下氩气取代了大气氩气,因此打算无背景。此外,完成了TPC和中子否决的校准活动。由于具有良好的背景抑制性能,到目前为止获得的结果表明,DarkSide-50探测器的可扩展性将达到吨级,这将在暗物质搜索场景中发挥关键作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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