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16 April 2024
 
  » arxiv » 1508.5759

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Current Status and Future Prospects of the SNO+ Experiment
SNO+ Collaboration ; 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 ; 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 ; M. Howe ; 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 ; 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 ; T. Sonley ; R. Stainforth ; M. Strait ; M. I. Stringer ; R. Svoboda ; A. Soerensen ; J. Tatar ; L. Tian ; N. Tolich ; J. Tseng ; H. W. C. Tseung ; R. Van Berg ; C. Virtue ; B. von Krosigk ; E. Vázquez-Jáuregui ; J. M. G. Walker ; M. Walker ; O. Wasalski ; J. Waterfield ; R. F. White ; J. F. Wilkerson ; J. R. Wilson ; T. J. Winchester ; A. Wright ; M. Yeh ; T. Zhao ; K. Zuber ;
Date 24 Aug 2015
AbstractSNO+ 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 multi-purpose neutrino experiment, the primary goal of SNO+ is a search for the neutrinoless double-beta decay (0$ uetaeta$) of 130Te. In Phase I, the detector will be loaded with 0.3% natural tellurium, corresponding to nearly 800 kg of 130Te, with an expected effective Majorana neutrino mass sensitivity in the region of 55-133 meV, just above the inverted mass hierarchy. Recently, the possibility to deploy up to ten times more natural tellurium has been investigated, which would enable SNO+ to achieve sensitivity deep into the parameter space for the inverted neutrino mass hierarchy in the future. Additionally, SNO+ aims to measure reactor antineutrino oscillations, low-energy solar neutrinos, geo-neutrinos, to be sensitive to supernova neutrinos, and to search for exotic physics. A first phase with the detector filled with water will begin soon, with the scintillator phase expected to start after a few months of water data taking. The 0$ uetaeta$ Phase I is foreseen for 2017.
Source arXiv, 1508.5759
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