Published November 2007 | Version v1
Journal article

Sterile dark matter and reionization

  • 1. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547 (United States)

Description

Sterile neutrinos with masses in the keV range can be the dark matter, and their emission from a supernova can explain the observed velocities of pulsars. The sterile neutrino decays could produce the x-ray radiation in the early universe, which could have an important effect on the formation of the first stars. X-rays could ionize gas and could catalyze the production of molecular hydrogen during the 'dark ages'. The increased fraction of molecular hydrogen could facilitate the cooling and collapse of the primordial gas clouds in which the first stars are formed

Availability note (English)

Available from http://dx.doi.org/10.1016/j.nuclphysbps.2007.08.141

Additional details

Identifiers

DOI
10.1016/j.nuclphysbps.2007.08.141;
arXiv
arXiv:astro-ph/0609375v1;
PII
S0920-5632(07)00638-X;

Publishing Information

Journal Title
Nuclear Physics. B, Proceedings Supplements
Journal Volume
173
Journal Page Range
p. 24-27
ISSN
0920-5632
CODEN
NPBSE7

Conference

Title
7. UCLA symposium on sources and detection of dark matter and dark energy in the Universe
Dates
22-24 Feb 2006
Place
Marina del Rey, CA (United States)

Optional Information

Copyright
Copyright (c) 2007 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.