Implications of combined solar-neutrino observations and their theoretical uncertainties
Journal Article
·
· Physical Review, D (Particles Fields); (United States)
- Department of Physics, University of Pennsylvania, Philadelphia, Pennsylvania 19104 (United States)
Constraints on the core temperature ([ital T][sub [ital c]]) of the Sun and on neutrino-oscillation parameters are obtained from the existing solar neutrino data, including the recent GALLEX, SAGE, and Kamiokande III results. (1) A purely astrophysical solution to the solar-neutrino problem is strongly disfavored by the data: the Homestake and Kamiokande data together are incompatible with any temperature in the Sun; the central values of both the SAGE and GALLEX results require a large reduction of [ital T][sub [ital c]] when they are fit to a cooler Sun. (2) Assuming the standard solar model (SSM) and matter-enhanced neutrino oscillations, the Mikheyev-Smirnov-Wolfenstein (MSW) parameters are constrained to two small regions: nonadiabatic oscillations with [Delta][ital m][sup 2]=(0.3--1.2)[times]10[sup [minus]5] eV[sup 2], sin[sup 2]2[theta]=(0.4--1.5)[times]10[sup [minus]2], or large mixing-angle oscillations with [Delta][ital m][sup 2]=(0.3--3)[times]10[sup [minus]5] eV[sup 2], sin[sup 2]2[theta]=0.6--0.9. The nonadiabatic solution gives a considerably better fit. For [nu][sub [ital e]] oscillations into sterile neutrinos, the allowed region (90% C.L.) is constrained to nonadiabatic oscillations. As long as the SSM is assumed, the neutrino mixing angles are at least four times larger, or considerably smaller, than the corresponding quark mixing angles.
- DOE Contract Number:
- AC02-76ER03071; FG02-88ER40479
- OSTI ID:
- 7060206
- Journal Information:
- Physical Review, D (Particles Fields); (United States), Journal Name: Physical Review, D (Particles Fields); (United States) Vol. 47:6; ISSN PRVDAQ; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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662430* -- Properties of Leptons-- (1992-)
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ALPHA REACTIONS
BARYON REACTIONS
BERYLLIUM 7 TARGET
CHARGED-PARTICLE REACTIONS
CROSS SECTIONS
ELEMENTARY PARTICLES
FERMIONS
HADRON REACTIONS
HELIUM 3 TARGET
LEPTONS
LIMITING VALUES
MASSLESS PARTICLES
MIXING
NEUTRINO OSCILLATION
NEUTRINOS
NUCLEAR REACTIONS
NUCLEON REACTIONS
PARAMETRIC ANALYSIS
PROTON REACTIONS
RADIATIONS
SOLAR NEUTRINOS
SOLAR PARTICLES
SOLAR RADIATION
STELLAR RADIATION
TARGETS
TEMPERATURE DEPENDENCE
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ALPHA REACTIONS
BARYON REACTIONS
BERYLLIUM 7 TARGET
CHARGED-PARTICLE REACTIONS
CROSS SECTIONS
ELEMENTARY PARTICLES
FERMIONS
HADRON REACTIONS
HELIUM 3 TARGET
LEPTONS
LIMITING VALUES
MASSLESS PARTICLES
MIXING
NEUTRINO OSCILLATION
NEUTRINOS
NUCLEAR REACTIONS
NUCLEON REACTIONS
PARAMETRIC ANALYSIS
PROTON REACTIONS
RADIATIONS
SOLAR NEUTRINOS
SOLAR PARTICLES
SOLAR RADIATION
STELLAR RADIATION
TARGETS
TEMPERATURE DEPENDENCE