Review of solar neutrinos and the MSW effect
Conference
·
OSTI ID:6829204
I review the MSW solution to the solar neutrino problem in light of the existing data from the {sup 37}Cl and Kamiokande II experiments. Taken together, they disfavor the adiabatic solution and tend to support either the large angle solution or the nonadiabatic one. In both cases the {sup 71}Ga experiment will yield a much smaller signal than that predicted by the standard solar model; the suppression factor in the former case will be about the same as for {sup 37}Cl, and in the latter it could be as large as 10 or more. I await the outcome of this experiment with great anticipation. 10 refs.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- DOE/ER
- DOE Contract Number:
- W-7405-ENG-36
- OSTI ID:
- 6829204
- Report Number(s):
- LA-UR-90-1527; CONF-900183-5; ON: DE90011953; TRN: 90-027004
- Resource Relation:
- Conference: Recontres De Moriond '90: new and exotic phenomena, Les Arcs (France), 20-27 Jan 1990
- Country of Publication:
- United States
- Language:
- English
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72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
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645102* - High Energy Physics- Particle Interactions & Properties-Experimental- Weak Interactions & Properties
640104 - Astrophysics & Cosmology- Solar Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
SOLAR NEUTRINOS
NEUTRINO DETECTION
CHLORINE 37
GALLIUM 71
NEUTRINO OSCILLATION
CHLORINE ISOTOPES
DETECTION
ELEMENTARY PARTICLES
FERMIONS
GALLIUM ISOTOPES
INTERMEDIATE MASS NUCLEI
ISOTOPES
LEPTONS
LIGHT NUCLEI
MASSLESS PARTICLES
NEUTRINOS
NUCLEI
ODD-EVEN NUCLEI
RADIATION DETECTION
RADIATIONS
SOLAR PARTICLES
SOLAR RADIATION
STABLE ISOTOPES
STELLAR RADIATION
645102* - High Energy Physics- Particle Interactions & Properties-Experimental- Weak Interactions & Properties
640104 - Astrophysics & Cosmology- Solar Phenomena