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The SNO+ experiment
Journal of Instrumentation ( IF 1.3 ) Pub Date : 2021-08-25 , DOI: 10.1088/1748-0221/16/08/p08059
V. Albanese 1 , R. Alves 2 , M.R. Anderson 3 , S. Andringa 4 , L. Anselmo 5 , E. Arushanova 6 , S. Asahi 3 , M. Askins 7, 8, 9 , D.J. Auty 10 , A.R. Back 6, 11 , S. Back 5 , F. Baro 4, 12 , Z. Barnard 1 , A. Barr 5 , N. Barros 4, 13, 14, 15 , D. Bartlett 3 , R. Bayes 1 , C. Beaudoin 1 , E.W. Beier 14 , G. Berardi 5 , A. Bialek 1, 5, 10 , S.D. Biller 16 , E. Blucher 17 , R. Bonventre 7, 8, 14 , M. Boulay 3 , D. Braid 1 , E. Caden 1, 3, 5 , E.J. Callaghan 7, 8, 14 , J. Caravaca 7, 8 , J. Carvalho 2, 18 , L. Cavalli 16 , D. Chauhan 1, 3, 4, 5 , M. Chen 3 , O. Chkvorets 1 , K.J. Clark 3, 11, 16 , B. Cleveland 1, 5 , C. Connors 1 , D. Cookman 16 , I.T. Coulter 14, 16 , M.A. Cox 4, 19 , D. Cressy 1 , X. Dai 3 , C. Darrach 1 , B. Davis-Purcell 20 , C. Deluce 5 , M.M. Depatie 1 , F. Descamps 7, 8 , F. DiLodovico 6, 21 , J. Dittmer 15 , A. Doxtator 5 , N. Duhaime 1 , F. Duncan 1, 5 , J. Dunger 6, 16 , A.D. Earle 11 , D. Fabris 5 , E. Falk 11 , A. Farrugia 1 , N. Fatemighomi 3, 5 , C. Felber 1 , V. Fischer 9 , E. Fletcher 3 , R. Ford 1, 5 , K. Frankiewicz 22 , N. Gagnon 5 , A. Gaur 10 , J. Gauthier 5 , A. Gibson-Foster 11 , K. Gilje 10 , O.I. Gonzlez-Reina 23 , D. Gooding 22 , P. Gorel 10 , K. Graham 3 , C. Grant 9, 22 , J. Grove 1 , S. Grullon 14 , E. Guillian 3 , S. Hall 5 , A.L. Hallin 10 , D. Hallman 1 , S. Hans 24 , J. Hartnell 11 , P. Harvey 3 , M. Hedayatipour 10 , W.J. Heintzelman 14 , J. Heise 3 , R.L. Helmer 20 , B. Hodak 3 , M. Hodak 5 , M. Hood 5 , D. Horne 3 , B. Hreljac 1, 3 , J. Hu 10 , S.M.A. Hussain 1 , T. Iida 3 , A.S. Incio 4, 13 , C.M. Jackson 7, 8 , N.A. Jelley 16 , C.J. Jillings 1, 5 , C. Jones 16 , P.G. Jones 6, 16 , K. Kamdin 7, 8 , T. Kaptanoglu 7, 8, 14 , J. Kaspar 25 , K. Keeter 26 , C. Kefelian 7, 8 , P. Khaghani 1 , L. Kippenbrock 25 , J.R. Klein 14 , R. Knapik 14, 27 , J. Kofron 25 , L.L. Kormos 28 , S. Korte 1 , B. Krar 3 , C. Kraus 1, 3 , C.B. Krauss 10 , T. Kroupov 16 , K. Labe 17 , F. Lafleur 5 , I. Lam 3 , C. Lan 3 , B.J. Land 7, 8, 14 , R. Lane 6 , S. Langrock 6 , P. Larochelle 5 , S. Larose 5 , A. LaTorre 17 , I. Lawson 1, 5 , L. Lebanowski 14 , G.M. Lefeuvre 11 , E.J. Leming 11, 16 , A. Li 22 , O. Li 5 , J. Lidgard 16 , B. Liggins 6 , P. Liimatainen 5 , Y.H. Lin 5 , X. Liu 3 , Y. Liu 3 , V. Lozza 4, 13, 15 , M. Luo 14 , S. Maguire 1, 5, 24 , A. Maio 4, 13 , K. Majumdar 16 , S. Manecki 3, 5 , J. Maneira 4, 13 , R.D. Martin 3 , E. Marzec 14 , A. Mastbaum 14, 17 , A. Mathewson 5 , N. McCauley 19 , A.B. McDonald 3 , K. McFarlane 5 , P. Mekarski 10 , M. Meyer 15 , C. Miller 3 , C. Mills 11 , M. Mlejnek 11 , E. Mony 3 , B. Morissette 5 , I. Morton-Blake 16 , M.J. Mottram 6, 11 , S. Nae 4, 13 , M. Nirkko 11 , L.J. Nolan 6 , V.M. Novikov 3 , H.M. O'Keeffe 3, 28 , E. O'Sullivan 3 , G.D. Orebi Gann 7, 8, 14 , M.J. Parnell 28 , J. Paton 16 , S.J.M. Peeters 11 , T. Pershing 9 , Z. Petriw 10 , J. Petzoldt 15 , L. Pickard 9 , D. Pracsovics 1 , G. Prior 4 , J.C. Prouty 7, 8 , S. Quirk 3 , S. Read 5 , A. Reichold 16 , S. Riccetto 3 , R. Richardson 1 , M. Rigan 11 , I. Ritchie 5 , A. Robertson 19 , B.C. Robertson 3 , J. Rose 19 , R. Rosero 24 , P.M. Rost 1 , J. Rumleskie 1 , M.A. Schumaker 1 , M.H. Schwendener 1 , D. Scislowski 25 , J. Secrest 14, 29 , M. Seddighin 3 , L. Segui 16 , S. Seibert 14 , I. Semenec 1, 3 , F. Shaker 10 , T. Shantz 1, 5 , M.K. Sharma 10 , T.M. Shokair 14 , L. Sibley 10 , J.R. Sinclair 11 , K. Singh 10 , P. Skensved 3 , M. Smiley 7, 8 , T. Sonley 3, 5 , A. Srensen 15 , M. St-Amant 5 , R. Stainforth 19 , S. Stankiewicz 5 , M. Strait 17 , M.I. Stringer 6, 11 , A. Stripay 1, 3, 5 , R. Svoboda 9 , S. Tacchino 5 , B. Tam 3 , C. Tanguay 1, 5 , J. Tatar 25 , L. Tian 3 , N. Tolich 25 , J. Tseng 16 , H.W.C. Tseung 25 , E. Turner 16 , R. VanBerg 14 , E. Vzquez-Juregui 1, 5, 23 , J.G.C. Veinot 10 , C.J. Virtue 1 , B. vonKrosigk 15 , J.M.G. Walker 19 , M. Walker 3 , J. Wallig 8 , S.C. Walton 1 , J. Wang 16 , M. Ward 3 , O. Wasalski 20 , J. Waterfield 11 , J.J. Weigand 15 , R.F. White 11 , J.R. Wilson 6, 21 , T.J. Winchester 25 , P. Woosaree 1 , A. Wright 3 , J.P. Yanez 10 , M. Yeh 24 , T. Zhang 9 , Y. Zhang 10 , T. Zhao 3 , K. Zuber 15, 30 , A. Zummo 14
Affiliation  

The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta (0νββ) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural tellurium, corresponding to 1.3 tonnes of 130Te. This paper provides a general overview of the SNO+ experiment, including detector design, construction of process plants, commissioning efforts, electronics upgrades, data acquisition systems, and calibration techniques. The SNO+ collaboration is reusing the acrylic vessel, PMT array, and electronics of the SNO detector, having made a number of experimental upgrades and essential adaptations for use with the liquid scintillator. With low backgrounds and a low energy threshold, the SNO+ collaboration will also pursue a rich physics program beyond the search for 0νββ decay, including studies of geo- and reactor antineutrinos, supernova and solar neutrinos, and exotic physics such as the search for invisible nucleon decay. The SNO+ approach to the search for 0νββ decay is scalable: a future phase with high 130Te-loading is envisioned to probe an effective Majorana mass in the inverted mass ordering region.



中文翻译:

SNO+ 实验

SNO+ 实验位于加拿大萨德伯里的 SNOLAB 地下 2 公里处。将使用 780 吨装有 3.9 吨天然碲的液体闪烁体,相当于 1.3 吨130特。本文概述了 SNO+ 实验,包括检测器设计、过程工厂的建设、调试工作、电子升级、数据采集系统和校准技术。SNO+ 合作正在重复使用 SNO 检测器的丙烯酸容器、PMT 阵列和电子设备,并进行了许多实验升级和必要的调整以与液体闪烁体配合使用。凭借低背景和低能量阈值,SNO+ 合作还将追求丰富的物理项目,超越寻找 0νββ 衰变,包括研究地球和反应堆反中微子、超新星和太阳中微子,以及寻找隐形核子等奇异物理学衰变。搜索 0νββ 衰变的 SNO+ 方法是可扩展的:具有高130的未来阶段Te-loading 被设想用于探测反向质量排序区域中的有效马约拉纳质量。

更新日期:2021-08-25
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