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Record W1863641736 · doi:10.1155/2016/6194250

Current Status and Future Prospects of the SNO+ Experiment

2016· article· en· W1863641736 on OpenAlexafffundabout
S. Andringa, E. Arushanova, S. Asahi, M. Askins, D. J. Auty, H.O. Back, Z. Barnard, N. Barros, E. W. Beier, A. Białek, S. D. Biller, R. Bonventre, D. Braid, E. Caden, J. Caravaca Rodríguez, J. Carvalho, Luca Cavalli, D. Chauhan, M. Chen, O. Chkvorets, K. Clark, B. T. Cleveland, I. T. Coulter, David Cressy, X. Dai, C. Darrach, B. Davis-Purcell, Rehan Deen, M. M. Depatie, F. Descamps, F. Di Lodovico, N. Duhaime, F. A. Duncan, Jack 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. J. Harvey, M. Hedayatipour, W. J. Heintzelman, R. L. Helmer, B. Hreljac, Jun Hu, T. Iida, C. M. Jackson, N.A. Jelley, C. Jillings, C. L. Jones, P. Jones, K. Kamdin, T. Kaptanoglu, J. Kašpar, P. Keener, P. Khaghani, L. Kippenbrock, J. Klein, R. Knapik, J. Kofron, L. L. Kormos, Simon Korte, C. Kraus, C. B. Krauss, K. R. Labe, I. Lam, C. Lan, Benjamin Land, S. Langrock, A. Latorre, I. Lawson, G. Lefeuvre, E. J. Leming, J. Lidgard, X. Liu, Y. Liu, V. Lozza, Simon Maguire, K. Majumdar, S. Manecki, J. Maneira, E. Marzec, A. Mastbaum, N. McCauley, A. B. McDonald, J. E. McMillan, Pawel Mekarski, C. Miller, Y. Mohan, E. Mony, M. Mottram, V. Novikov, H. M. O’Keeffe, Erin O’Sullivan, G. D. Orebi Gann, M. J. Parnell, S. J. M. Peeters, T. Pershing, Z. Petriw, G. Prior, J. C. Prouty, Sarah Quirk, A. Reichold, A. Robertson, J. Rose, R. Rosero, P. M. Rost, J. Rumleskie, M. A. Schumaker, M. H. Schwendener, D. Ścisłowski, J. A. Secrest, M. Seddighin, L. Seguí, S. R. Seibert, T. Shantz, T. M. Shokair, L. Sibley, J. Sinclair, K. Singh, P. Skensved, A Sörensen, T. Sonley, R. Stainforth, M. Strait, M. Stringer, R. Svoboda, J. Tatar, Liyan Tian, N. Tolich, J. C-L. Tseng, H. Wan Chan Tseung, R. Van Berg, E. Vázquez-Jáuregui, C.J. Virtue, B. von Krosigk, J. M. G. Walker, M. Walker, O. Wasalski, J. Waterfield, Ryan White, J. R. Wilson, T. Winchester, A. Wright, M. Yeh, T. Zhao, Κ. Zuber

Bibliographic record

VenueAdvances in High Energy Physics · 2016
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsTRIUMFLaurentian UniversityUniversity of AlbertaQueen's University
FundersFundação para a Ciência e a TecnologiaOffice of ScienceDeutsche ForschungsgemeinschaftScience and Technology Facilities CouncilNuclear PhysicsNatural Sciences and Engineering Research Council of CanadaU.S. Department of EnergyEuropean CommissionCanadian Institute for Advanced ResearchNational Natural Science Foundation of ChinaUniversity of CaliforniaEuropean Research CouncilNational Science Foundation
KeywordsPhysicsNeutrinoScintillatorDouble beta decayNuclear physicsMAJORANASolar neutrinoNeutrino detectorSupernovaDetectorParticle physicsTelluriumBETA (programming language)Sensitivity (control systems)Neutrino oscillationAstrophysicsOpticsMaterials science

Abstract

fetched live from OpenAlex

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 (0<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="M1"><mml:mi>ν</mml:mi><mml:mi>β</mml:mi><mml:mi>β</mml:mi></mml:math>) of 130 Te. In Phase I, the detector will be loaded with 0.3% natural tellurium, corresponding to nearly 800 kg of 130 Te, 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<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" id="M2"><mml:mn mathvariant="normal">0</mml:mn><mml:mi>ν</mml:mi><mml:mi>β</mml:mi><mml:mi>β</mml:mi></mml:math>Phase I is foreseen for 2017.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.028
metaresearch head score (Gemma)0.008
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Review · Consensus signal: none
Teacher disagreement score0.028
Threshold uncertainty score0.149

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0280.008
Meta-epidemiology (narrow)0.0020.001
Meta-epidemiology (broad)0.0020.001
Bibliometrics0.0020.002
Science and technology studies0.0020.004
Scholarly communication0.0060.010
Open science0.0040.005
Research integrity0.0040.002
Insufficient payload (model declined to judge)0.0190.010

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.007
GPT teacher head0.281
Teacher spread0.274 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
Domainnot available
GenreReview

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations284
Published2016
Admission routes3
Has abstractyes

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