Solar and supernova neutrino physics with Sudbury Neutrino Observatory

Journal Article · Sat Feb 15 00:00:00 EST 1992 · Physical Review, D (Particles Fields); (United States)

DOI:https://doi.org/10.1103/PhysRevD.45.1059· OSTI ID:7277515

Balantekin, A B; Loreti, F ^[1]

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1. Physics Department, University of Wisconsin, Madison, Wisconsin 53706 (United States)

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.

• OSTI ID: 7277515
• Journal Information: Physical Review, D (Particles Fields); (United States), Vol. 45:4; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
SOLAR NEUTRINOS
DETECTION
SUPERNOVAE
NEUTRINO DETECTION
ANGULAR DISTRIBUTION
ANTINEUTRINOS
CHARGED-CURRENT INTERACTIONS
CROSS SECTIONS
ENERGY DEPENDENCE
FLAVOR MODEL
GALAXIES
MAGNETIC MOMENTS
NEUTRAL-CURRENT INTERACTIONS
SPIN
ANGULAR MOMENTUM
ANTILEPTONS
ANTIMATTER
ANTIPARTICLES
COMPOSITE MODELS
DISTRIBUTION
ELEMENTARY PARTICLES
ERUPTIVE VARIABLE STARS
FERMIONS
INTERACTIONS
LEPTONS
MASSLESS PARTICLES
MATHEMATICAL MODELS
MATTER
NEUTRINOS
PARTICLE INTERACTIONS
PARTICLE MODELS
PARTICLE PROPERTIES
QUARK MODEL
RADIATION DETECTION
RADIATIONS
SOLAR PARTICLES
SOLAR RADIATION
STARS
STELLAR RADIATION
VARIABLE STARS
662430* - Properties of Leptons- (1992-)
662320 - Neutrino Interactions- (1992-)