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dc.contributor.authorSNO Collaboration
dc.contributor.authorFormaggio, Joseph A
dc.contributor.authorMiller, M. L.
dc.contributor.authorMonreal, Benjamin
dc.contributor.authorMonroe, Jocelyn
dc.contributor.authorSolomon-Oblath, Noah
dc.contributor.authorOtt, Richard A.
dc.contributor.authorSonley, Thomas John
dc.date.accessioned2022-09-12T19:51:48Z
dc.date.available2021-10-27T20:23:10Z
dc.date.available2022-09-12T19:51:48Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/135369.2
dc.description.abstract© 2020 authors. Published by the American Physical Society. A search has been performed for neutrinos from two sources, the hep reaction in the solar pp fusion chain and the νe component of the diffuse supernova neutrino background (DSNB), using the full dataset of the Sudbury Neutrino Observatory with a total exposure of 2.47 kton-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 φhep<30×103 cm-2 s-1 [90% credible interval (CI)]. No events are observed in the DSNB search region, and we set an improved upper bound on the νe component of the DSNB flux of φνeDSNB<19 cm-2 s-1 (90% CI) in the energy range 22.9<Eν<36.9 MeV.en_US
dc.language.isoen
dc.publisherAmerican Physical Society (APS)en_US
dc.relation.isversionof10.1103/PHYSREVD.102.062006en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceAPSen_US
dc.titleSearch for hep solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatoryen_US
dc.typeArticleen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.relation.journalPhysical Review Den_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2021-07-09T15:33:46Z
dspace.orderedauthorsAharmim, B; Ahmed, SN; Anthony, AE; Barros, N; Beier, EW; Bellerive, A; Beltran, B; Bergevin, M; Biller, SD; Blucher, E; Bonventre, R; Boudjemline, K; Boulay, MG; Cai, B; Callaghan, EJ; Caravaca, J; Chan, YD; Chauhan, D; Chen, M; Cleveland, BT; Cox, GA; Dai, X; Deng, H; Descamps, FB; Detwiler, JA; Doe, PJ; Doucas, G; Drouin, P-L; Dunford, M; Elliott, SR; Evans, HC; Ewan, GT; Farine, J; Fergani, H; Fleurot, F; Ford, RJ; Formaggio, JA; Gagnon, N; Gilje, K; Goon, JT; Graham, K; Guillian, E; Habib, S; Hahn, RL; Hallin, AL; Hallman, ED; Harvey, PJ; Hazama, R; Heintzelman, WJ; Heise, J; Helmer, RL; Hime, A; Howard, C; Huang, M; Jagam, P; Jamieson, B; Jelley, NA; Jerkins, M; Keeter, KJ; Klein, JR; Kormos, LL; Kos, M; Kraus, C; Krauss, CB; Krüger, A; Kutter, T; Kyba, CCM; Labe, K; Land, BJ; Lange, R; LaTorre, A; Law, J; Lawson, IT; Lesko, KT; Leslie, JR; Levine, I; Loach, JC; MacLellan, R; Majerus, S; Mak, HB; Maneira, J; Martin, RD; Mastbaum, A; McCauley, N; McDonald, AB; McGee, SR; Miller, ML; Monreal, B; Monroe, J; Nickel, BG; Noble, AJ; O’Keeffe, HM; Oblath, NS; Okada, CE; Ollerhead, RW; Orebi Gann, GD; Oser, SM; Ott, RA; Peeters, SJM; Poon, AWP; Prior, G; Reitzner, SD; Rielage, K; Robertson, BC; Robertson, RGH; Schwendener, MH; Secrest, JA; Seibert, SR; Simard, O; Sinclair, D; Skensved, P; Sonley, TJ; Stonehill, LC; Tešić, G; Tolich, N; Tsui, T; Van Berg, R; VanDevender, BA; Virtue, CJ; Wall, BL; Waller, D; Wan Chan Tseung, H; Wark, DL; Wendland, J; West, N; Wilkerson, JF; Wilson, JR; Winchester, T; Wright, A; Yeh, M; Zhang, F; Zuber, Ken_US
dspace.date.submission2021-07-09T15:33:47Z
mit.journal.volume102en_US
mit.journal.issue6en_US
mit.licensePUBLISHER_CC
mit.metadata.statusPublication Information Neededen_US


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