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Current Status and Future Prospects of the SNO+ Experiment

  • S. Andringa
  • , E. Arushanova
  • , S. Asahi
  • , M. Askins
  • , D. J. Auty
  • , A. R. Back
  • , Z. Barnard
  • , N. Barros
  • , E. W. Beier
  • , A. Bialek
  • , S. D. Biller
  • , E. Blucher
  • , R. Bonventre
  • , D. Braid
  • , E. Caden
  • , E. Callaghan
  • , J. Caravaca
  • , J. Carvalho
  • , L. Cavalli
  • , D. Chauhan
  • M. Chen, O. Chkvorets, K. Clark, B. Cleveland, I. T. Coulter, D. Cressy, X. Dai, C. Darrach, B. Davis-Purcell, R. Deen, M. M. Depatie, F. Descamps, F. Di Lodovico, N. Duhaime, F. Duncan, J. Dunger, E. Falk, N. Fatemighomi, R. Ford, P. Gorel, C. Grant, S. Grullon, E. Guillian, A. L. Hallin, D. Hallman, S. Hans, J. Hartnell, P. Harvey, M. Hedayatipour, W. J. Heintzelman, R. L. Helmer, B. Hreljac, J. Hu, T. Iida, C. M. Jackson, N. A. Jelley, C. Jillings, C. Jones, P. G. Jones, K. Kamdin, T. Kaptanoglu, J. Kaspar, P. Keener, P. Khaghani, L. Kippenbrock, J. R. Klein, R. Knapik, J. N. Kofron, L. L. Kormos, S. Korte, C. Kraus, C. B. Krauss, K. Labe, I. Lam, C. Lan, B. J. Land, S. Langrock, A. Latorre, I. Lawson, G. M. Lefeuvre, E. J. Leming, J. Lidgard, X. Liu, Y. Liu, V. Lozza, S. Maguire, A. Maio, K. Majumdar, S. Manecki, J. Maneira, E. Marzec, A. Mastbaum, N. Mccauley, A. B. Mcdonald, J. E. Mcmillan, P. Mekarski, C. Miller, Y. Mohan, E. Mony, M. J. Mottram, V. Novikov, H. M. O'Keeffe, E. O'Sullivan, G. D. Orebi Gann, M. J. Parnell, S. J.M. Peeters, T. Pershing, Z. Petriw, G. Prior, J. C. Prouty, S. Quirk, A. Reichold, A. 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, T. Shantz, T. M. Shokair, L. Sibley, J. R. Sinclair, K. Singh, P. Skensved, A. Sörensen, T. Sonley, R. Stainforth, M. Strait, M. I. Stringer, R. Svoboda, J. Tatar, L. Tian, N. Tolich, J. Tseng, H. W.C. Tseung, R. Van Berg, E. Vázquez-Jáuregui, C. Virtue, B. Von Krosigk, J. M.G. Walker, M. Walker, O. Wasalski, J. Waterfield, R. F. White, J. R. Wilson, T. J. Winchester, A. Wright, M. Yeh, T. Zhao, K. Zuber
  • Laboratório de Instrumentação e Física Experimental de Partículas
  • Queen Mary University of London
  • Queen's University Kingston
  • University of California, Davis
  • University of Alberta
  • University of Sussex
  • Laurentian University
  • University of Pennsylvania
  • University of Oxford
  • The University of Chicago
  • University of California, Berkeley
  • Berkeley National Laboratory
  • University of Coimbra
  • Creighton Mine No. 9
  • TRIUMF
  • United States Department of Energy
  • University of Washington
  • Norwich University
  • Lancaster University
  • Technische Universität Dresden
  • University of Lisbon
  • University of Liverpool
  • University of Sheffield
  • Armstrong Atlantic State University
  • National Autonomous University of Mexico

Research output: Contribution to journalSystematic reviewpeer-review

257 Scopus citations

Abstract

SNO+ is a large liquid scintillator-based experiment located 2 km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12 m 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 (0ββ) 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 0νββ Phase I is foreseen for 2017.

Original languageEnglish
Article number6194250
JournalAdvances in High Energy Physics
Volume2016
DOIs
StatePublished - 2016

Scopus Subject Areas

  • Nuclear and High Energy Physics

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