DarkSide-20k:用于 LNGS 直接暗物质探测的 20 吨级两相液氩时间投影室
仪器与探测器
2018-08-09 v1
摘要
基于 DarkSide-50 探测器成功运行的经验,DarkSide 合作组将建造 DarkSide-20k,这是一个直接 WIMP 搜寻探测器,采用两相液氩时间投影室 (LArTPC),有效(基准)质量为 23 吨(20 吨)。DarkSide-20k 的 LArTPC 将部署在一个屏蔽/反符合系统内,该系统由一个球形液体闪烁体反符合探测器 (LSV) 置于一个圆柱形水切伦科夫反符合探测器 (WCV) 内部构成。DarkSide-50 的运行表明,在使用从地下源提取的氩气时,在应用脉冲形状分析之前,主要的 Ar 本底已大幅降低。来自 DarkSide-50 的数据,结合蒙特卡洛模拟和解析模型,表明电子反冲与核反冲的鉴别抑制因子可达 。这一点,连同反符合系统的使用,是解锁通往大型 LArTPC 探测器质量路径的关键,同时保持一个“无仪器本底”实验,即在计划的曝光期间,预计在 WIMP 搜寻区域内发生少于 0.1 个(由 引起的核反冲除外)事例。DarkSide-20k 将具有可原位测量的超低本底。这将使其对质量为 TeV ( TeV) 的 WIMP 的 WIMP-核子散射截面灵敏度达到 cm ( cm),该灵敏度将在产生 100 吨·年无任何仪器本底曝光的 5 年运行期内实现。随后,DarkSide-20k 可将运行时间延长至十年,将曝光量增加到 200 吨·年,从而对质量为 TeV ( TeV) 的 WIMP 达到 cm ( cm) 的灵敏度。
引用
@article{arxiv.1707.08145,
title = {DarkSide-20k: A 20 Tonne Two-Phase LAr TPC for Direct Dark Matter Detection at LNGS},
author = {C. E. Aalseth and F. Acerbi and P. Agnes and I. F. M. Albuquerque and T. Alexander and A. Alici and A. K. Alton and P. Antonioli and S. Arcelli and R. Ardito and I. J. Arnquist and D. M. Asner and M. Ave and H. O. Back and A. I. Barrado Olmedo and G. Batignani and E. Bertoldo and S. Bettarini and M. G. Bisogni and V. Bocci and A. Bondar and G. Bonfini and W. Bonivento and M. Bossa and B. Bottino and M. Boulay and R. Bunker and S. Bussino and A. Buzulutskov and M. Cadeddu and M. Cadoni and A. Caminata and N. Canci and A. Candela and C. Cantini and M. Caravati and M. Cariello and M. Carlini and M. Carpinelli and A. Castellani and S. Catalanotti and V. Cataudella and P. Cavalcante and S. Cavuoti and R. Cereseto and A. Chepurnov and C. Cicalò and L. Cifarelli and M. Citterio and A. G. Cocco and M. Colocci and S. Corgiolu and G. Covone and P. Crivelli and I. D'Antone and M. D'Incecco and D. D'Urso and M. D. Da Rocha Rolo and M. Daniel and S. Davini and A. de Candia and S. De Cecco and M. De Deo and G. De Filippis and G. De Guido and G. De Rosa and G. Dellacasa and M. Della Valle and P. Demontis and A. Derbin and A. Devoto and F. Di Eusanio and G. Di Pietro and C. Dionisi and A. Dolgov and I. Dormia and S. Dussoni and A. Empl and M. Fernandez Diaz and A. Ferri and C. Filip and G. Fiorillo and K. Fomenko and D. Franco and G. E. Froudakis and F. Gabriele and A. Gabrieli and C. Galbiati and P. Garcia Abia and A. Gendotti and A. Ghisi and S. Giagu and P. Giampa and G. Gibertoni and C. Giganti and M. A. Giorgi and G. K. Giovanetti and M. L. Gligan and A. Gola and O. Gorchakov and A. M. Goretti and F. Granato and M. Grassi and J. W. Grate and G. Y. Grigoriev and M. Gromov and M. Guan and M. B. B. Guerra and M. Guerzoni and M. Gulino and R. K. Haaland and A. Hallin and B. Harrop and E. W. Hoppe and S. Horikawa and B. Hosseini and D. Hughes and P. Humble and E. V. Hungerford and An. Ianni and C. Jillings and T. N. Johnson and K. Keeter and C. L. Kendziora and S. Kim and G. Koh and D. Korablev and G. Korga and A. Kubankin and M. Kuss and M. Kuźniak and B. Lehnert and X. Li and M. Lissia and G. U. Lodi and B. Loer and G. Longo and P. Loverre and R. Lussana and L. Luzzi and Y. Ma and A. A. Machado and I. N. Machulin and A. Mandarano and L. Mapelli and M. Marcante and A. Margotti and S. M. Mari and M. Mariani and J. Maricic and C. J. Martoff and M. Mascia and M. Mayer and A. B. McDonald and A. Messina and P. D. Meyers and R. Milincic and A. Moggi and S. Moioli and J. Monroe and A. Monte and M. Morrocchi and B. J. Mount and W. Mu and V. N. Muratova and S. Murphy and P. Musico and R. Nania and A. Navrer Agasson and I. Nikulin and V. Nosov and A. O. Nozdrina and N. N. Nurakhov and A. Oleinik and V. Oleynikov and M. Orsini and F. Ortica and L. Pagani and M. Pallavicini and S. Palmas and L. Pandola and E. Pantic and E. Paoloni and G. Paternoster and V. Pavletcov and F. Pazzona and S. Peeters and K. Pelczar and L. A. Pellegrini and N. Pelliccia and F. Perotti and R. Perruzza and V. Pesudo Fortes and C. Piemonte and F. Pilo and A. Pocar and T. Pollmann and D. Portaluppi and D. A. Pugachev and H. Qian and B. Radics and F. Raffaelli and F. Ragusa and M. Razeti and A. Razeto and V. Regazzoni and C. Regenfus and B. Reinhold and A. L. Renshaw and M. Rescigno and F. Retière and Q. Riffard and A. Rivetti and S. Rizzardini and A. Romani and L. Romero and B. Rossi and N. Rossi and A. Rubbia and D. Sablone and P. Salatino and O. Samoylov and E. Sánchez García and W. Sands and M. Sant and R. Santorelli and C. Savarese and E. Scapparone and B. Schlitzer and G. Scioli and E. Segreto and A. Seifert and D. A. Semenov and A. Shchagin and L. Shekhtman and E. Shemyakina and A. Sheshukov and M. Simeone and P. N. Singh and P. Skensved and M. D. Skorokhvatov and O. Smirnov and G. Sobrero and A. Sokolov and A. Sotnikov and F. Speziale and R. Stainforth and C. Stanford and G. B. Suffritti and Y. Suvorov and R. Tartaglia and G. Testera and A. Tonazzo and A. Tosi and P. Trinchese and E. V. Unzhakov and A. Vacca and E. Vázquez-Jáuregui and M. Verducci and T. Viant and F. Villa and A. Vishneva and B. Vogelaar and M. Wada and J. Wahl and J. Walding and S. Walker and H. Wang and Y. Wang and A. W. Watson and S. Westerdale and R. Williams and M. M. Wojcik and S. Wu and X. Xiang and X. Xiao and C. Yang and Z. Ye and A. Yllera de Llano and F. Zappa and G. Zappalà and C. Zhu and A. Zichichi and M. Zullo and A. Zullo},
journal= {arXiv preprint arXiv:1707.08145},
year = {2018}
}