Published October 1981
| Version v1
Book
Neutrino mass and galaxy formation
Description
By studying the formation process of galaxies and clusters of galaxies in the neutrino dominated universe, we show that neutrino mass of 20 -- 25 eV predicts the correct mass scales of galaxies and clusters as --1012 M sub(solar mass) and --1016 M sub(solar mass), respectively and that it also resolves the missing mass problem of those objects. (author)
Additional details
Publishing Information
- Publisher
- Tokyo Univ., Inst. for Nuclear Study.
- Imprint Place
- Tokyo (Japan)
- Imprint Title
- Proceedings of 1981 INS symposium on quark and lepton physics
- Imprint Pagination
- 371 p.
- Journal Page Range
- p. 271-275.
Conference
- Title
- 1981 INS symposium on quark and lepton physics.
- Dates
- 25-27 Jun 1981.
- Place
- Tokyo (Japan).
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 15004535
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMOLOGY; EV RANGE 10-100; GALACTIC EVOLUTION; GALAXY CLUSTERS; HUBBLE EFFECT; MASS; MISSING MASS; NEUTRINOS; ORIGIN; UNIVERSE
- Descriptors DEC
- ELEMENTARY PARTICLES; ENERGY RANGE; EV RANGE; FERMIONS; LEPTONS; MASSLESS PARTICLES