Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter

Journal Article · Fri Oct 01 00:00:00 EDT 1993 · Physical Review, D (Particles Fields); (United States)

DOI:https://doi.org/10.1103/PhysRevD.48.3259· OSTI ID:6216247

Caldwell, D O ^[1]; Mohapatra, R N ^[2]

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1. Department of Physics, University of California, Santa Barbara, California 93106-9530 (United States)
2. Department of Physics, University of Maryland, College Park, Maryland 20742 (United States)

If the solar and atmospheric neutrino deficits and the apparent need for a hot dark matter component all result from neutrino mass, one of three neutrino mass patterns is required. Of these, two appear quite unlikely, leading to a unique solution which points to further experimental tests. We briefly outline possible theoretical models which could generate these three neutrino mass matrices without adjustment of parameters.

• OSTI ID: 6216247
• Journal Information: Physical Review, D (Particles Fields); (United States), Vol. 48:7; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Pa
NEUTRINOS
MASS
ENERGY DENSITY
MASS DIFFERENCE
NEUTRINO OSCILLATION
NUCLEOSYNTHESIS
SOLAR NEUTRINOS
ELEMENTARY PARTICLES
FERMIONS
LEPTONS
MASSLESS PARTICLES
PARTICLE PROPERTIES
RADIATIONS
SOLAR PARTICLES
SOLAR RADIATION
STELLAR RADIATION
SYNTHESIS
662430* - Properties of Leptons- (1992-)
662210 - Specific Theories & Interaction Models
Particle Systematics- Unified Theories & Models- (1992-)