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Record W3043655490 · doi:10.1103/physrevd.102.062006

Search for <i>hep</i> solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory

2020· article· en· W3043655490 on OpenAlexafffundabout
B. Aharmim, S. N. Ahmed, A. E. Anthony, N. Barros, A. Bellerive, B. Beltrán, M. Bergevin, S. D. Biller, R. Bonventre, K. Boudjemline, M. G. Boulay, B. Cai, J. Caravaca Rodríguez, Y. D. Chan, D. Chauhan, M. Chen, B. T. Cleveland, G. A. Cox, X. Dai, Huiqiu Deng, F. Descamps, J. A. Detwiler, P. J. Doe, G. Doucas, P.‐L. Drouin, M. Dunford, S. R. Elliott, H. C. Evans, G. T. Ewan, J. Farine, H. Fergani, F. Fleurot, R. Ford, J. A. Formaggio, N. Gagnon, K. Gilje, J. TM. Goon, K. Graham, E. Guillian, S. Habib, R. L. Hahn, A. L. Hallin, E. D. Hallman, P. J. Harvey, R. Hazama, W. J. Heintzelman, J. Heise, R. L. Helmer, A. Hime, C. Howard, M. Huang, P. Jagam, B. Jamieson, N.A. Jelley, M. Jerkins, K. Keeter, J. R. Klein, L. L. Kormos, M. Kos, C. Kraus, C. B. Krauss, A. Krüger, T. Kutter, Christopher C. M. Kyba, K. R. Labe, Benjamin Land, R. Lange, A. Latorre, J. Law, I. Lawson, K. T. Lesko, J. R. Leslie, I. Levine, J. C. Loach, R. MacLellan, Steve Majerus, H.‐B. Mak, J. Maneira, R. D. Martin, A. Mastbaum, N. McCauley, A. B. McDonald, S. McGee, M. L. Miller, B. Monreal, J. Monroe, B. G. Nickel, A. J. Noble, H. M. O’Keeffe, N. S. Oblath, C. Okada, R. W. Ollerhead, G. D. Orebi Gann, S. M. Oser, R. A. Ott, S. J. M. Peeters, A. W. P. Poon, G. Prior, S. D. Reitzner, K. Rielage, B.C. Robertson, R. G. H. Robertson, M. H. Schwendener, J. A. Secrest, S. R. Seibert, O. Simard, D. Sinclair, P. Skensved, T. Sonley, L. C. Stonehill, G. Tešić, N. Tolich, T. Tsui, R. Van Berg, B. A. VanDevender, C.J. Virtue, B. L. Wall, D. Waller, H. Wan Chan Tseung, D. L. Wark, J. Wendland, N. West, J. F. Wilkerson, J. R. Wilson, T. Winchester, A. Wright, M. Yeh, F. Zhang, Κ. Zuber

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsUniversity of British ColumbiaUniversity of GuelphLaurentian UniversityUniversity of AlbertaSnolabQueen's UniversityTRIUMFCarleton University
FundersFundação para a Ciência e a TecnologiaNuclear PhysicsAlfred P. Sloan FoundationNatural Sciences and Engineering Research Council of CanadaNational Nuclear Security AdministrationAtomic Energy of Canada LimitedQueen's UniversityCanada Research ChairsIndustry CanadaCanada Foundation for InnovationScience and Technology Facilities CouncilNational Research Council CanadaStrongU.S. Department of EnergyNational Science Foundation
KeywordsPhysicsSupernovaNeutrinoSolar neutrinoParticle physicsFlux (metallurgy)Type (biology)Energy (signal processing)AstrophysicsNuclear physicsNeutrino oscillationQuantum mechanics

Abstract

fetched live from OpenAlex

A search has been performed for neutrinos from two sources, the hep reaction in the solar $pp$ fusion chain and the ${\ensuremath{\nu}}_{e}$ component of the diffuse supernova neutrino background (DSNB), using the full dataset of the Sudbury Neutrino Observatory with a total exposure of $2.47\text{ }\text{ }\mathrm{kton}\text{\ensuremath{-}}\mathrm{years}$ after fiducialization. The hep search is performed using both a single-bin counting analysis and a likelihood fit. We find a best-fit flux that is compatible with solar model predictions while remaining consistent with zero flux, and set a one-sided upper limit of ${\mathrm{\ensuremath{\Phi}}}_{hep}&lt;30\ifmmode\times\else\texttimes\fi{}{10}^{3}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{s}}^{\ensuremath{-}1}$ [90% credible interval (CI)]. No events are observed in the DSNB search region, and we set an improved upper bound on the ${\ensuremath{\nu}}_{e}$ component of the DSNB flux of ${\mathrm{\ensuremath{\Phi}}}_{{\ensuremath{\nu}}_{e}}^{\mathrm{DSNB}}&lt;19\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{s}}^{\ensuremath{-}1}$ (90% CI) in the energy range $22.9&lt;{E}_{\ensuremath{\nu}}&lt;36.9\text{ }\text{ }\mathrm{MeV}$.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.622
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0030.002
Bibliometrics0.0000.001
Science and technology studies0.0000.001
Scholarly communication0.0000.001
Open science0.0020.001
Research integrity0.0000.002
Insufficient payload (model declined to judge)0.0000.000

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 head0.087
GPT teacher head0.427
Teacher spread0.340 · 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 teacher head, not a consensus.

Study designBench or experimental
Domainnot available
GenreEmpirical

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

Citations22
Published2020
Admission routes3
Has abstractyes

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