Published 1986
| Version v1
Book
Lower limits on m/sub upsilon/ from the distribution of dark matter in galaxies
Description
If one flavour of neutrino and antineutrino of mass m/sub upsilon/ is responsible for the non-luminous matter in the outer parts of galaxies, one can obtain firm lower limits on the value of m/sub upsilon/ from the observed distribution of dark matter. Note that the method described here does not depend on the actual coarse-grained phase-space distribution of neutrinos in galaxies (except for assuming isotropy). Another approach to the problem with the same advantage is presented
Additional details
Publishing Information
- Publisher
- University of Chicago Press.
- Imprint Place
- Chicago, IL (USA)
- ISBN
- 0-226-45032-5
- Imprint Title
- Inner space/outer space. The interface between cosmology and particle physics
- Journal Page Range
- p. 510-511.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18044028
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC NEUTRINOS; COSMOLOGY; ELEMENT ABUNDANCE; FLAVOR MODEL; GALAXIES; MASS DISTRIBUTION; MASS SPECTRA; NONLUMINOUS MATTER; ORIGIN; PARTICLE PROPERTIES; PHASE SPACE; RELICT RADIATION; REST MASS; SPATIAL DISTRIBUTION; WEAK INTERACTIONS
- Descriptors DEC
- BASIC INTERACTIONS; COMPOSITE MODELS; COSMIC RADIATION; DISTRIBUTION; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; INTERACTIONS; IONIZING RADIATIONS; LEPTONS; MASS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATHEMATICAL SPACE; MATTER; MICROWAVE RADIATION; NEUTRINOS; PARTICLE MODELS; QUANTITY RATIO; QUARK MODEL; RADIATIONS; SPACE; SPECTRA