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Neutrino masses in astrophysics and cosmology

Abstract

Astrophysical and cosmological arguments and observations give us the most restrictive constraints on neutrino masses, electromagnetic couplings, and other properties. Conversely, massive neutrinos would contribute to the cosmic dark-matter density and would play an important role for the formation of structure in the universe. Neutrino oscillations may well solve the solar neutrino problem, and can have a significant impact on supernova physics. (author) 14 figs., tabs., 33 refs.
Authors:
Raffelt, G G [1] 
  1. Max-Planck-Institut fuer Physik, Muenchen (Germany)
Publication Date:
Nov 01, 1996
Product Type:
Miscellaneous
Report Number:
PSI-PROC-96-03; CONF-9608192-
Reference Number:
SCA: 662430; PA: AIX-28:026737; EDB-97:046099; SN: 97001753649
Resource Relation:
Conference: Physics with neutrinos, Zuoz (Switzerland), 4-10 Aug 1996; Other Information: PBD: Nov 1996; Related Information: Is Part Of Proceedings of the summer school on physics with neutrinos; Locher, M.P. [ed.]; PB: 266 p.; PSI-Proceedings--96-03
Subject:
66 PHYSICS; NEUTRINOS; ASTROPHYSICS; COSMOLOGY; MASS; EXPERIMENTAL DATA; NEUTRINO OSCILLATION; NONLUMINOUS MATTER; SOLAR NEUTRINOS; STANDARD MODEL; SUPERNOVAE; THEORETICAL DATA
OSTI ID:
444509
Country of Origin:
Switzerland
Language:
English
Other Identifying Numbers:
Journal ID: ISSN 1019-6447; Other: ON: DE97617666; TRN: CH9700119026737
Availability:
OSTI as DE97617666
Submitting Site:
CHN
Size:
pp. 69-78
Announcement Date:
Mar 28, 1997

Citation Formats

Raffelt, G G. Neutrino masses in astrophysics and cosmology. Switzerland: N. p., 1996. Web.
Raffelt, G G. Neutrino masses in astrophysics and cosmology. Switzerland.
Raffelt, G G. 1996. "Neutrino masses in astrophysics and cosmology." Switzerland.
@misc{etde_444509,
title = {Neutrino masses in astrophysics and cosmology}
author = {Raffelt, G G}
abstractNote = {Astrophysical and cosmological arguments and observations give us the most restrictive constraints on neutrino masses, electromagnetic couplings, and other properties. Conversely, massive neutrinos would contribute to the cosmic dark-matter density and would play an important role for the formation of structure in the universe. Neutrino oscillations may well solve the solar neutrino problem, and can have a significant impact on supernova physics. (author) 14 figs., tabs., 33 refs.}
place = {Switzerland}
year = {1996}
month = {Nov}
}