Solar and supernova neutrino physics with Sudbury Neutrino Observatory
- 15 February 1992
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 45 (4) , 1059-1065
- https://doi.org/10.1103/physrevd.45.1059
Abstract
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 spinflavor 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.Keywords
This publication has 61 references indexed in Scilit:
- Search for day-night and semiannual variations in the solar neutrino flux observed in the Kamiokande-II detectorPhysical Review Letters, 1991
- Results from one thousand days of real-time, directional solar-neutrino dataPhysical Review Letters, 1990
- Constraints on neutrino-oscillation parameters from the Kamiokande-II solar-neutrino dataPhysical Review Letters, 1990
- Observation ofsolar neutrinos in the Kamiokande-II detectorPhysical Review Letters, 1989
- Neutrino-electron scattering and the choice between different Mikheyev-Smirnov-Wolfenstein solutions of the solar neutrino problemPhysical Review D, 1989
- Resonant amplification of ν oscillations in matter and solar-neutrino spectroscopyIl Nuovo Cimento C, 1986
- Standard solar models and the uncertainties in predicted capture rates of solar neutrinosReviews of Modern Physics, 1982
- Neutrino oscillations and stellar collapsePhysical Review D, 1979
- Neutrino oscillations in matterPhysical Review D, 1978
- Search for Neutrinos from the SunPhysical Review Letters, 1968