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  • 2104.11687v1

    Rights statement: This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Instrumentation. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.1088/1748-0221/16/08/P08059

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The SNO+ Experiment

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The SNO+ Experiment. / SNO+ Collaboration ; Kormos, L. L.; O'Keeffe, H. M. et al.
In: Journal of Instrumentation, Vol. 16, P08059, 25.08.2021.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

SNO+ Collaboration, Kormos, LL, O'Keeffe, HM & Parnell, MJ 2021, 'The SNO+ Experiment', Journal of Instrumentation, vol. 16, P08059. https://doi.org/10.1088/1748-0221/16/08/P08059

APA

SNO+ Collaboration, Kormos, L. L., O'Keeffe, H. M., & Parnell, M. J. (2021). The SNO+ Experiment. Journal of Instrumentation, 16, Article P08059. https://doi.org/10.1088/1748-0221/16/08/P08059

Vancouver

SNO+ Collaboration, Kormos LL, O'Keeffe HM, Parnell MJ. The SNO+ Experiment. Journal of Instrumentation. 2021 Aug 25;16:P08059. doi: 10.1088/1748-0221/16/08/P08059

Author

SNO+ Collaboration ; Kormos, L. L. ; O'Keeffe, H. M. et al. / The SNO+ Experiment. In: Journal of Instrumentation. 2021 ; Vol. 16.

Bibtex

@article{e42cd7ac7dce426a9081900bcb75e076,
title = "The SNO+ Experiment",
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. ",
keywords = "physics.ins-det, hep-ex, nucl-ex",
author = "{SNO+ Collaboration} and R. Alves and S. Andringa and L. Anselmo and E. Arushanova and S. Asahi and Auty, {D. J.} and Back, {A. R.} and S. Back and F. Bar{\~a}o and Z. Barnard and A. Barr and N. Barros and D. Bartlett and R. Bayes and C. Beaudoin and Beier, {E. W.} and G. Berardi and A. Bialek and Biller, {S. D.} and E. Blucher and R. Bonventre and M. Boulay and D. Braid and E. Caden and Callaghan, {E. J.} and J. Caravaca and J. Carvalho and L. Cavalli and D. Chauhan and O. Chkvorets and Clark, {K. J.} and B. Cleveland and C. Connors and D. Cookman and Coulter, {I. T.} and D. Cressy and X. Dai and C. Darrach and B. Davis-Purcell and C. Deluce and Depatie, {M. M.} and F. Descamps and Lodovico, {F. Di} and Kormos, {L. L.} and O'Keeffe, {H. M.} and Parnell, {M. J.}",
note = "This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Instrumentation. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.1088/1748-0221/16/08/P08059",
year = "2021",
month = aug,
day = "25",
doi = "10.1088/1748-0221/16/08/P08059",
language = "English",
volume = "16",
journal = "Journal of Instrumentation",
issn = "1748-0221",
publisher = "Institute of Physics Publishing",

}

RIS

TY - JOUR

T1 - The SNO+ Experiment

AU - SNO+ Collaboration

AU - Alves, R.

AU - Andringa, S.

AU - Anselmo, L.

AU - Arushanova, E.

AU - Asahi, S.

AU - Auty, D. J.

AU - Back, A. R.

AU - Back, S.

AU - Barão, F.

AU - Barnard, Z.

AU - Barr, A.

AU - Barros, N.

AU - Bartlett, D.

AU - Bayes, R.

AU - Beaudoin, C.

AU - Beier, E. W.

AU - Berardi, G.

AU - Bialek, A.

AU - Biller, S. D.

AU - Blucher, E.

AU - Bonventre, R.

AU - Boulay, M.

AU - Braid, D.

AU - Caden, E.

AU - Callaghan, E. J.

AU - Caravaca, J.

AU - Carvalho, J.

AU - Cavalli, L.

AU - Chauhan, D.

AU - Chkvorets, O.

AU - Clark, K. J.

AU - Cleveland, B.

AU - Connors, C.

AU - Cookman, D.

AU - Coulter, I. T.

AU - Cressy, D.

AU - Dai, X.

AU - Darrach, C.

AU - Davis-Purcell, B.

AU - Deluce, C.

AU - Depatie, M. M.

AU - Descamps, F.

AU - Lodovico, F. Di

AU - Kormos, L. L.

AU - O'Keeffe, H. M.

AU - Parnell, M. J.

N1 - This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Instrumentation. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.1088/1748-0221/16/08/P08059

PY - 2021/8/25

Y1 - 2021/8/25

N2 - 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.

AB - 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.

KW - physics.ins-det

KW - hep-ex

KW - nucl-ex

U2 - 10.1088/1748-0221/16/08/P08059

DO - 10.1088/1748-0221/16/08/P08059

M3 - Journal article

VL - 16

JO - Journal of Instrumentation

JF - Journal of Instrumentation

SN - 1748-0221

M1 - P08059

ER -