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

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
JournalPhys.Rev.D
Volume102
Issue number062006
DOIs
Published29 Sep 2020

King's Authors

Abstract

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 2.47kton−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<30×10^3cm^2s^-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 ΦDSNB νe<19cm−2 s−1 (90% CI) in the energy range 22.9<Eν<36.9MeV.

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