Implications of new GALLEX results for the Mikheyev-Smirnov-Wolfenstein solution of the solar neutrino problem
Journal Article
·
· Physical Review Letters; (United States)
- NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510 (United States)
- Department of Physics, The University of Texas at Arlington, Arlington, Texas 76019 (United States)
We compare the implications for {sup 7}Be and {ital pp} neutrinos of the two Mikheyev-Smirnov-Wolfenstein fits to the new GALLEX solar neutrino measurements. Small-mixing-angle solutions tend to suppress the former as electron neutrinos, but not the latter, and large-angle solutions tend to reduce both by about a factor of 2. The consequences for BOREXINO and similar solar neutrino-electron scattering experiments are discussed.
- DOE Contract Number:
- FG05-92ER40691
- OSTI ID:
- 7199607
- Journal Information:
- Physical Review Letters; (United States), Journal Name: Physical Review Letters; (United States) Vol. 69:13; ISSN PRLTA; ISSN 0031-9007
- Country of Publication:
- United States
- Language:
- English
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662340 -- Hadron Interactions-- (1992-)
662430* -- Properties of Leptons-- (1992-)
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ALKALINE EARTH ISOTOPES
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BERYLLIUM 7
BERYLLIUM ISOTOPES
BETA DECAY RADIOISOTOPES
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662430* -- Properties of Leptons-- (1992-)
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ALKALINE EARTH ISOTOPES
BARYON-BARYON INTERACTIONS
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DAYS LIVING RADIOISOTOPES
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ELEMENTARY PARTICLES
ENERGY RANGE
EVEN-ODD NUCLEI
FERMIONS
HADRON-HADRON INTERACTIONS
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LEPTONS
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MASS
MASSLESS PARTICLES
NEUTRINO DETECTION
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NUCLEI
NUCLEON-NUCLEON INTERACTIONS
PARTICLE INTERACTIONS
PROBABILITY
PROTON-NUCLEON INTERACTIONS
PROTON-PROTON INTERACTIONS
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SOLAR PARTICLES
SOLAR RADIATION
STELLAR RADIATION