Notice

This is not the latest version of this item. The latest version can be found at:https://dspace.mit.edu/handle/1721.1/135369.2

Show simple item record

dc.date.accessioned2021-10-27T20:23:10Z
dc.date.available2021-10-27T20:23:10Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/135369
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.
dc.language.isoen
dc.publisherAmerican Physical Society (APS)
dc.relation.isversionof10.1103/PHYSREVD.102.062006
dc.rightsCreative Commons Attribution 4.0 International license
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.sourceAPS
dc.titleSearch for hep solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory
dc.typeArticle
dc.relation.journalPhysical Review D
dc.eprint.versionFinal published version
dc.type.urihttp://purl.org/eprint/type/JournalArticle
eprint.statushttp://purl.org/eprint/status/PeerReviewed
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, K
dspace.date.submission2021-07-09T15:33:47Z
mit.journal.volume102
mit.journal.issue6
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Needed


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

VersionItemDateSummary

*Selected version