Physics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..45.1059b&link_type=abstract
Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 45, Issue 4, 15 February 1992, pp.1059-1065
Physics
16
Supernovae
Scientific paper
The salient features of solar and supernova neutrino physics at the Sudbury Neutrino Observatory are examined. The possibility of detecting a solar-antineutrino flux, predicted as a result of resonant spin-flavor conversion, is emphasized. The antineutrino flux at Sudbury due to the commercial power reactors is calculated. Simplified, analytical expressions for the expected galactic supernova count rates are given.
Baha Balantekin A.
Loreti F.
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