Current Status and Future Prospects of the SNO+ Experiment
Creators: name: Collaboration, SNO+
name: :
name: Andringa, S.
name: Arushanova, E.
name: Asahi, S.
name: Askins, M.
name: Auty, D. J.
name: Back, A. R.
name: Barnard, Z.
name: Barros, N.
name: Beier, E. W.
name: Bialek, A.
name: Biller, S. D.
name: Blucher, E.
name: Bonventre, R.
name: Braid, D.
name: Caden, E.
name: Callaghan, E.
name: Caravaca, J.
name: Carvalho, J.
name: Cavalli, L.
name: Chauhan, D.
name: Chen, M.
name: Chkvorets, O.
name: Clark, K.
name: Cleveland, B.
name: Coulter, I. T.
name: Cressy, D.
name: Dai, X.
name: Darrach, C.
name: Davis-Purcell, B.
name: Deen, R.
name: Depatie, M. M.
name: Descamps, F.
name: Di Lodovico, F.
name: Duhaime, N.
name: Duncan, F.
name: Dunger, J.
name: Falk, E.
name: Fatemighomi, N.
name: Ford, R.
name: Gorel, P.
name: Grant, C.
name: Grullon, S.
name: Guillian, E.
name: Hallin, A. L.
name: Hallman, D.
name: Hans, S.
name: Hartnell, J.
name: Harvey, P.
name: Hedayatipour, M.
name: Heintzelman, W. J.
name: Helmer, R. L.
name: Hreljac, B.
name: Hu, J.
name: Iida, T.
name: Jackson, C. M.
name: Jelley, N. A.
name: Jillings, C.
name: Jones, C.
name: Jones, P. G.
name: Kamdin, K.
name: Kaptanoglu, T.
name: Kaspar, J.
name: Keener, P.
name: Khaghani, P.
name: Kippenbrock, L.
name: Klein, J. R.
name: Knapik, R.
name: Kofron, J. N.
name: Kormos, L. L.
name: Korte, S.
name: Kraus, C.
name: Krauss, C. B.
name: Labe, K.
name: Lam, I.
name: Lan, C.
name: Land, B. J.
name: Langrock, S.
name: LaTorre, A.
name: Lawson, I.
name: Lefeuvre, G. M.
name: Leming, E. J.
name: Lidgard, J.
name: Liu, X.
name: Liu, Y.
name: Lozza, V.
name: Maguire, S.
name: Maio, A.
name: Majumdar, K.
name: Manecki, S.
name: Maneira, J.
name: Marzec, E.
name: Mastbaum, A.
name: McCauley, N.
name: McDonald, A. B.
name: McMillan, J. E.
name: Mekarski, P.
name: Miller, C.
name: Mohan, Y.
name: Mony, E.
name: Mottram, M. J.
name: Novikov, V.
name: O'Keeffe, H. M.
name: O'Sullivan, E.
name: Gann, G. D. Orebi
name: Parnell, M. J.
name: Peeters, S. J. M.
name: Pershing, T.
name: Petriw, Z.
name: Prior, G.
name: Prouty, J. C.
name: Quirk, S.
name: Reichold, A.
name: Robertson, A.
name: Rose, J.
name: Rosero, R.
name: Rost, P. M.
name: Rumleskie, J.
name: Schumaker, M. A.
name: Schwendener, M. H.
name: Scislowski, D.
name: Secrest, J.
name: Seddighin, M.
name: Segui, L.
name: Seibert, S.
name: Shantz, T.
name: Shokair, T. M.
name: Sibley, L.
name: Sinclair, J. R.
name: Singh, K.
name: Skensved, P.
name: Soerensen, A.
name: Sonley, T.
name: Stainforth, R.
name: Strait, M.
name: Stringer, M. I.
name: Svoboda, R.
name: Tatar, J.
name: Tian, L.
name: Tolich, N.
name: Tseng, J.
name: Tseung, H. W. C.
name: Van Berg, R.
name: Vázquez-Jáuregui, E.
name: Virtue, C.
name: von Krosigk, B.
name: Walker, J. M. G.
name: Walker, M.
name: Wasalski, O.
name: Waterfield, J.
name: White, R. F.
name: Wilson, J. R.
name: Winchester, T. J.
name: Wright, A.
name: Yeh, M.
name: Zhao, T.
name: Zuber, K.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: SNO+ is a large liquid scintillator-based experiment located 2km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m diameter acrylic vessel which will be filled with about 780 tonnes of ultra-pure liquid scintillator. Designed as a multipurpose neutrino experiment, the primary goal of SNO+ is a search for the neutrinoless double-beta decay (0$νββ$) of 130Te. In Phase I, the detector will be loaded with 0.3% natural tellurium, corresponding to nearly 800 kg of 130Te, with an expected effective Majorana neutrino mass sensitivity in the region of 55-133 meV, just above the inverted mass hierarchy. Recently, the possibility of deploying up to ten times more natural tellurium has been investigated, which would enable SNO+ to achieve sensitivity deep into the parameter space for the inverted neutrino mass hierarchy in the future. Additionally, SNO+ aims to measure reactor antineutrino oscillations, low-energy solar neutrinos, and geoneutrinos, to be sensitive to supernova neutrinos, and to search for exotic physics. A first phase with the detector filled with water will begin soon, with the scintillator phase expected to start after a few months of water data taking. The 0$νββ$ Phase I is foreseen for 2017.
description: Published in "Neutrino Masses and Oscillations" of Advances in High Energy Physics (Hindawi)