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View from inside the filled SNO+ detector. A large transparent acrylic sphere filled with clear liquid, immersed in water. Surrounding the water, thousands of light-detecting photomultiplier tubes can be seen glinting with the reflective concentrators that surround them.

SNO+ detector. The inner vessel is filled with 780T of liquid scintillator and surrounded by a geodesic sphere of photomultiplier tubes immersed in ultra-pure water. The detector is located 2.1km underground at Canada's SNOLAB, outside of Sudbury, Western Ontario.

Credit: SNOLAB

Daniel Cookman

Graduate student

Research theme

  • Particle astrophysics & cosmology
  • Fundamental particles and interactions

Sub department

  • Particle Physics

Research groups

  • SNO+
daniel.cookman@physics.ox.ac.uk
Denys Wilkinson Building
  • About
  • Publications

The SNO+ Experiment

ArXiv 2104.11687 (2021)

Authors:

SNO Collaboration, V Albanese, R Alves, MR Anderson, S Andringa, L Anselmo, E Arushanova, S Asahi, M Askins, DJ Auty, AR Back, S Back, F Barão, Z Barnard, A Barr, N Barros, D Bartlett, R Bayes, C Beaudoin, EW Beier, G Berardi, A Bialek, SD Biller, E Blucher, R Bonventre, M Boulay, D Braid, E Caden, EJ Callaghan, J Caravaca, J Carvalho, L Cavalli, D Chauhan, M Chen, O Chkvorets, KJ Clark, B Cleveland, C Connors, D Cookman, IT Coulter, MA Cox, D Cressy, X Dai, C Darrach, B Davis-Purcell, C Deluce, MM Depatie, F Descamps, F Di Lodovico, J Dittmer, A Doxtator, N Duhaime, F Duncan, J Dunger, AD 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, OI González-Reina, D Gooding, P Gorel, K Graham, C Grant, J Grove, S Grullon, E Guillian, S Hall, AL Hallin, D Hallman, S Hans, J Hartnell, P Harvey, M Hedayatipour, WJ Heintzelman, J Heise, RL Helmer, B Hodak, M Hodak, M Hood, D Horne, B Hreljac, J Hu, SMA Hussain, T Iida, AS Inácio, CM Jackson, NA Jelley, CJ Jillings, C Jones, PG Jones, K Kamdin, T Kaptanoglu, J Kaspar, K Keeter, C Kefelian, P Khaghani, L Kippenbrock, JR Klein, R Knapik, J Kofron, LL Kormos, S Korte, B Krar, C Kraus, CB Krauss, T Kroupová, K Labe, F Lafleur, I Lam, C Lan, BJ Land, R Lane, S Langrock, P Larochelle, S Larose, A LaTorre, I Lawson, L Lebanowski, GM Lefeuvre, EJ Leming, A Li, O Li, J Lidgard, B Liggins, P Liimatainen, YH Lin, X Liu, Y Liu, V Lozza, M Luo, S Maguire, A Maio, K Majumdar, S Manecki, J Maneira, RD Martin, E Marzec, A Mastbaum, A Mathewson, N McCauley, AB McDonald, K McFarlane, P Mekarski, M Meyer, C Miller, C Mills, M Mlejnek, E Mony, B Morissette, I Morton-Blake, MJ Mottram, S Nae, M Nirkko, LJ Nolan, VM Novikov, HM O'Keeffe, E O'Sullivan, GD Orebi Gann, MJ Parnell, J Paton, SJM Peeters, T Pershing, Z Petriw, J Petzoldt, L Pickard, D Pracsovics, G Prior, JC Prouty, S Quirk, S Read, A Reichold, S Riccetto, R Richardson, M Rigan, I Ritchie, A Robertson, BC Robertson, J Rose, R Rosero, PM Rost, J Rumleskie, MA Schumaker, MH Schwendener, D Scislowski, J Secrest, M Seddighin, L Segui, S Seibert, I Semenec, F Shaker, T Shantz, MK Sharma, TM Shokair, L Sibley, JR Sinclair, K Singh, P Skensved, M Smiley, T Sonley, A Sörensen, M St-Amant, R Stainforth, S Stankiewicz, M Strait, MI Stringer, A Stripay, R Svoboda, S Tacchino, B Tam, C Tanguay, J Tatar, L Tian, N Tolich, J Tseng, HWC Tseung, E Turner, R Van Berg, E Vázquez-Jáuregui, JGC Veinot, CJ Virtue, B von Krosigk, JMG Walker, M Walker, J Wallig, SC Walton, J Wang, M Ward, O Wasalski, J Waterfield, JJ Weigand, RF White, JR Wilson, TJ Winchester, P Woosaree, A Wright, JP Yanez, M Yeh, T Zhang, Y Zhang, T Zhao, K Zuber, A Zummo

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.
More details from the publisher
Details from ORA
Details from ArXiV

Optical calibration of the SNO+ detector in the water phase with deployed sources

Journal of Instrumentation IOP Publishing 16 (2021) P10021

Authors:

Mr Anderson, S Andringa, M Askins, Dj Auty, F Barão, N Barros, R Bayes, Ew Beier, A Bialek, Sd Biller, E Blucher, M Boulay, E Caden, Ej Callaghan, J Caravaca, M Chen, O Chkvorets, B Cleveland, D Cookman, J Corning, Ma Cox, C Deluce, Mm Depatie, F Di Lodovico, J Dittmer, E Falk, N Fatemighomi, V Fischer, R Ford, K Frankiewicz, A Gaur, K Gilje, Oi González-Reina, D Gooding, C Grant, J Grove, Al Hallin, D Hallman, J Hartnell, Wj Heintzelman, Rl Helmer, J Hu, R Hunt-Stokes, Sma Hussain, As Inácio, Cj Jillings, T Kaptanoglu, P Khaghani, Armin Reichold

Abstract:

SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB, Sudbury, Canada. The detector acquired data for two years as a pure water Cherenkov detector, starting in May 2017. During this period, the optical properties of the detector were measured in situ using a deployed light diffusing sphere, with the goal of improving the detector model and the energy response systematic uncertainties. The measured parameters included the water attenuation coefficients, effective attenuation coefficients for the acrylic vessel, and the angular response of the photomultiplier tubes and their surrounding light concentrators, all across different wavelengths. The calibrated detector model was validated using a deployed tagged gamma source, which showed a 0.6% variation in energy scale across the primary target volume.
More details from the publisher
Details from ORA
More details
More details
Details from ArXiV

The SNO+ experiment

Journal of Instrumentation IOP Publishing 16:8 (2021) P08059

Authors:

V Albanese, R Alves, Mr Anderson, S Andringa, L Anselmo, E Arushanova, S Asahi, M Askins, Dj Auty, Ar Back, S Back, F Bar o, Z Barnard, A Barr, N Barros, D Bartlett, R Bayes, C Beaudoin, Ew Beier, G Berardi, A Bialek, Sd Biller, E Blucher, R Bonventre, M Boulay, D Braid, E Caden, Ej Callaghan, J Caravaca, J Carvalho, L Cavalli, D Chauhan, M Chen, O Chkvorets, Kj Clark, B Cleveland, C Connors, D Cookman, It Coulter, Ma Cox, D Cressy, X Dai, C Darrach, B Davis-Purcell, C Deluce, Mm Depatie, F Descamps, Armin Reichold

Abstract:

The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta (0νββ) decay will be conducted using 780 tonnes of liquid scintillator loaded with 3.9 tonnes of natural tellurium, corresponding to 1.3 tonnes of 130Te. 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 0νββ 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 0νββ decay is scalable: a future phase with high 130Te-loading is envisioned to probe an effective Majorana mass in the inverted mass ordering region.
More details from the publisher
Details from ORA
Details from ArXiV

Development, characterisation, and deployment of the SNO+ liquid scintillator

Journal of Instrumentation IOP Publishing 16 (2021) P05009

Authors:

Mr Anderson, S Andringa, L Anselmo, Sd Biller, Kj Clark, D Cookman, It Coulter, J Dunger, Jeffrey Lidgard, Krishanu Majumdar, I Morton-Blake, C Jones, J Paton, PG Jones, A Reichold, L Segui, Jeffrey Tseng, E Turner, J Wang

Abstract:

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-existing liquid scintillators while conferring other advantages including longer attenuation lengths, superior safety characteristics, chemical simplicity, ease of handling, and logistical availability. Its properties have been extensively characterized and are presented here. This liquid scintillator is now used in several neutrino physics experiments in addition to SNO+.
More details from the publisher
Details from ORA
More details
More details
Details from ArXiV

Development, characterisation, and deployment of the SNO+ liquid scintillator

JINST

Authors:

Sno Collaboration, Mr Anderson, S Andringa, L Anselmo, E Arushanova, S Asahi, M Askins, Dj Auty, Ar Back, Z Barnard, N Barros, D Bartlett, F Barão, R Bayes, Ew Beier, A Bialek, Sd Biller, E Blucher, R Bonventre, M Boulay, D Braid, E Caden, Ej Callaghan, J Caravaca, J Carvalho, L Cavalli, D Chauhan, M Chen, O Chkvorets, Kj Clark, B Cleveland, D Cookman, C Connors, It Coulter, Ma Cox, D Cressy, X Dai, C Darrach, B Davis-Purcell, C Deluce, Mm Depatie, F Descamps, J Dittmer, F Di Lodovico, N Duhaime, F Duncan, J Dunger, Ad Earle, D Fabris, E Falk

Abstract:

A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is compatible with acrylic and has a competitive light yield to pre-existing liquid scintillators while conferring other advantages including longer attenuation lengths, superior safety characteristics, chemical simplicity, ease of handling, and logistical availability. Its properties have been extensively characterized and are presented here. This liquid scintillator is now used in several neutrino physics experiments in addition to SNO+.

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