Status and perspective of the DarkSide experiment at LNGS

P. Agnes, L. Agostino, I. Albuquerque, T. Alexander, A. Alton, D. Asner, H. Back, B. Baldin, K. Biery, V. Bocci, G. Bonfini, W. Bonivento, M. Bossa, B. Bottino, A. Brigatti, J. Brodsky, F. Budano, S. Bussino, M. Cadeddu, M. Cadoni, F. Calaprice, N. Canci, A. Candela, M. Caravati, M. Cariello, M. Carlini, S. Catalanotti, P. Cavalcante, A. Chepurnov, C. Cicalò, A. Cocco, G. Covone, D. D’Angelo, M. D’Incecco, S. Davini, S. Cecco, M. Deo, M. Vincenzi, A. Derbin, A. Devoto, F. D. Eusanio, G. D. Pietro, C. Dionisi, E. Edkins, A. Empl, A. Fan, G. Fiorillo, K. Fomenko, D. Franco, F. Gabriele, C. Galbiati, S. Giagu, C. Giganti, G. Giovanetti, A. Goretti, F. Granato, M. Gromov, M. Guan, Y. Guardincerri, B. Hackett, K. Herner, D. Hughes, P. Humble, E. Hungerford, A. Ianni, A. Ianni, I. James, T. Johnson, C. Jollet, K. Keeter, C. Kendziora, G. Koh, D. Korablev, G. Korga, A. Kubankin, X. Li, M. Lissia, B. Loer, P. Lombardi, G. Longo, Y. Ma, A. Machado, I. Machulin, A. Mandarano, S. Mari, J. Maricic, L. Marini, C. Mart
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引用次数: 1

Abstract

The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-phase argon TPC. The current phase of the experiment, DarkSide-50, is acquiring data at Laboratori Nazionali del Gran Sasso and produced the most sensitive limit on the WIMP-nucleon cross section ever obtained with a liquid argon target (2.0 × 10−44 cm2 for a WIMP mass of 100 GeV/c2 ). The future phase of the experiment will be a 20 t fiducial mass detector, designed to reach a sensitivity of ∼ 1 × 10−47 cm2 (at 1 TeV/c2 WIMP mass) with a backgroundfree exposure of 100 ty. This work contains a discussion of the current status of the DarkSide-50 WIMP search and of the results which are more relevant for the construction of the future detector.
lng暗面实验现状与展望
DarkSide实验旨在用双相氩TPC对暗物质进行无背景直接搜索。实验的当前阶段,DarkSide-50,正在格兰萨索国家实验室获取数据,并产生了迄今为止用液态氩气靶获得的WIMP-核子截面最敏感的极限(对于100 GeV/c2的WIMP质量,为2.0 × 10−44 cm2)。实验的未来阶段将是一个20 t基准质量探测器,设计灵敏度为1 × 10−47 cm2(在1 TeV/c2 WIMP质量下),无背景曝光为100 ty。这项工作包括对darkday -50 WIMP搜索的当前状态的讨论,以及对未来探测器建设更相关的结果。
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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