A search has been made for neutrinos from the hep reaction in the Sun and from the diffuse supernova neutrino background (DSNB) using data collected during the first operational phase of the Sudbury Neutrino Observatory, with an exposure of 0.65 ktons yr. For the hep neutrino search, two events are observed in the effective electron energy range of 14:3 MeV… (More)
preprint (astro-ph/0511337v1). The GS98 elemental abundances are selected for reference model of solar neutrino fluxes
J. N. Bahcall, A. M. Serenelli, S. Basu
2005
Flux predictions from this paper have been increased by a factor of three, as recommended by the authors, to account for updated star formation rate data. Estimates for the νe DSNB