Published 1987
| Version v1
Book
Neutrino mass and the solar neutrino problem
Description
Theoretical ideas about neutrino mass based on grand-unified theories are reviewed. These give the see-saw formula in which neutrino mass is inversely proportional to a large mass scale M. For M between 10/sup 11/ and 10/sup 15/ Gev the study of solar neutrinos appears to be the best probe of neutrino masses and mixings
Additional details
Publishing Information
- Publisher
- Society of Photo-Optical Instrumentation Engineers.
- Imprint Place
- Bellingham, WA (USA)
- ISBN
- 9971-50-183-X
- Imprint Title
- Proceedings of the XXIII international conference on high energy physics
- Journal Page Range
- p. 893-896.
Conference
- Title
- 23. international conference on high-energy physics.
- Dates
- 16-23 Jul 1986.
- Place
- Berkeley, CA (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19007008
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC NEUTRINOS; GRAND UNIFIED THEORY; MASS; MASS FORMULAE; NEUTRINO DETECTION; NEUTRINO OSCILLATION; NEUTRINOS; REVIEWS; SOLAR NEUTRINOS; SUN; WEAK INTERACTIONS
- Descriptors DEC
- BASIC INTERACTIONS; COSMIC RADIATION; DETECTION; DOCUMENT TYPES; ELEMENTARY PARTICLES; FERMIONS; FIELD THEORIES; INTERACTIONS; IONIZING RADIATIONS; LEPTONS; MAIN SEQUENCE STARS; MASSLESS PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; QUANTUM FIELD THEORY; RADIATION DETECTION; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STARS; STELLAR RADIATION; UNIFIED GAUGE MODELS