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Physics > Instrumentation and Detectors

arXiv:2104.11687 (physics)
[Submitted on 23 Apr 2021 (v1), last revised 25 Aug 2021 (this version, v3)]

Title:The SNO+ Experiment

Authors:SNO+ Collaboration: V. Albanese, R. Alves, M. R. Anderson, S. Andringa, L. Anselmo, E. Arushanova, S. Asahi, M. Askins, D. J. Auty, A. R. Back, S. Back, F. Barão, Z. Barnard, A. Barr, N. Barros, D. Bartlett, R. Bayes, C. Beaudoin, E. W. Beier, G. Berardi, A. Bialek, S. D. Biller, E. Blucher, R. Bonventre, M. Boulay, D. Braid, E. Caden, E. J. Callaghan, J. Caravaca, J. Carvalho, L. Cavalli, D. Chauhan, M. Chen, O. Chkvorets, K. J. Clark, B. Cleveland, C. Connors, D. Cookman, I. T. Coulter, M. A. Cox, D. Cressy, X. Dai, C. Darrach, B. Davis-Purcell, C. Deluce, M. M. Depatie, F. Descamps, F. Di Lodovico, J. Dittmer, A. Doxtator, N. Duhaime, F. Duncan, J. Dunger, A. D. Earle, D. Fabris, E. Falk, A. Farrugia, N. Fatemighomi, C. Felber, V. Fischer, E. Fletcher, R. Ford, K. Frankiewicz, N. Gagnon, A. Gaur, J. Gauthier, A. Gibson-Foster, K. Gilje, O. I. González-Reina, D. Gooding, P. Gorel, K. Graham, C. Grant, J. Grove, S. Grullon, E. Guillian, S. Hall, A. L. Hallin, D. Hallman, S. Hans, J. Hartnell, P. Harvey, M. Hedayatipour, W. J. Heintzelman, J. Heise, R. L. Helmer, B. Hodak, M. Hodak, M. Hood, D. Horne, B. Hreljac, J. Hu, S. M. A. Hussain, T. Iida, A. S. Inácio, C. M. Jackson, N. A. Jelley, C. J. Jillings, C. Jones
, P. G. Jones, K. Kamdin, T. Kaptanoglu, J. Kaspar, K. Keeter, C. Kefelian, P. Khaghani, L. Kippenbrock, J. R. Klein, R. Knapik, J. Kofron, L. L. Kormos, S. Korte, B. Krar, C. Kraus, C. B. Krauss, T. Kroupová, K. Labe, F. Lafleur, I. Lam, C. Lan, B. J. Land, R. Lane, S. Langrock, P. Larochelle, S. Larose, A. LaTorre, I. Lawson, L. Lebanowski, G. M. Lefeuvre, E. J. Leming, A. Li, O. Li, J. Lidgard, B. Liggins, P. Liimatainen, Y. H. Lin, X. Liu, Y. Liu, V. Lozza, M. Luo, S. Maguire, A. Maio, K. Majumdar, S. Manecki, J. Maneira, R. D. Martin, E. Marzec, A. Mastbaum, A. Mathewson, N. McCauley, A. B. McDonald, K. McFarlane, P. Mekarski, M. Meyer, C. Miller, C. Mills, M. Mlejnek, E. Mony, B. Morissette, I. Morton-Blake, M. J. Mottram, S. Nae, M. Nirkko, L. J. Nolan, V. M. Novikov, H. M. O'Keeffe, E. O'Sullivan, G. D. Orebi Gann, M. J. Parnell, J. Paton, S. J. M. Peeters, T. Pershing, Z. Petriw, J. Petzoldt, L. Pickard, D. Pracsovics, G. Prior, J. C. Prouty, S. Quirk, S. Read, A. Reichold, S. Riccetto, R. Richardson, M. Rigan, I. Ritchie, A. Robertson, B. C. Robertson, J. Rose, R. Rosero, P. M. Rost, J. Rumleskie, M. A. Schumaker, M. H. Schwendener, D. Scislowski, J. Secrest, M. Seddighin, L. Segui, S. Seibert, I. Semenec, F. Shaker, T. Shantz, M. K. Sharma, T. M. Shokair, L. Sibley, J. R. Sinclair, K. Singh, P. Skensved, M. Smiley, T. Sonley, A. Sörensen, M. St-Amant, R. Stainforth, S. Stankiewicz, M. Strait, M. I. Stringer, A. Stripay, R. Svoboda, S. Tacchino, B. Tam, C. Tanguay, J. Tatar, L. Tian, N. Tolich, J. Tseng, H. W. C. Tseung, E. Turner, R. Van Berg, E. Vázquez-Jáuregui, J. G. C. Veinot, C. J. Virtue, B. von Krosigk, J. M. G. Walker, M. Walker, J. Wallig, S. C. Walton, J. Wang, M. Ward, O. Wasalski, J. Waterfield, J. J. Weigand, R. F. White, J. R. Wilson, T. J. Winchester, P. Woosaree, A. Wright, J. P. Yanez, M. Yeh, T. Zhang, Y. Zhang, T. Zhao, K. Zuber, A. Zummo
et al. (153 additional authors not shown)  You must enable JavaScript to view entire author list.
View a PDF of the paper titled The SNO+ Experiment, by SNO+ Collaboration: V. Albanese and 251 other authors
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Abstract:The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta ($0\nu\beta\beta$) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural tellurium, corresponding to 1.3 tonnes of $^{130}$Te. 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 $0\nu\beta\beta$ 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 $0\nu\beta\beta$ decay is scalable: a future phase with high $^{130}$Te-loading is envisioned to probe an effective Majorana mass in the inverted mass ordering region.
Comments: 61 pages, 23 figures, 4 tables
Subjects: Instrumentation and Detectors (physics.ins-det); High Energy Physics - Experiment (hep-ex); Nuclear Experiment (nucl-ex)
Cite as: arXiv:2104.11687 [physics.ins-det]
  (or arXiv:2104.11687v3 [physics.ins-det] for this version)
  https://doi.org/10.48550/arXiv.2104.11687
arXiv-issued DOI via DataCite
Journal reference: The SNO+ collaboration, 2021 JINST 16 P08059
Related DOI: https://doi.org/10.1088/1748-0221/16/08/P08059
DOI(s) linking to related resources

Submission history

From: Martti Nirkko [view email]
[v1] Fri, 23 Apr 2021 16:27:17 UTC (8,482 KB)
[v2] Fri, 23 Jul 2021 14:41:15 UTC (8,486 KB)
[v3] Wed, 25 Aug 2021 18:44:38 UTC (8,391 KB)
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