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Cosmic microwave background anisotropy in the decaying neutrino cosmology
Uppsala University.
Uppsala University.
Uppsala University.
1998 (English)In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, Vol. 301, no 1, 210-214 p.Article in journal (Other scientific) Published
Abstract [en]

It is attractive to suppose for several astrophysical reasons that the Universe has close to the critical density in light (similar to 30 eV) neutrinos which decay radiatively with a lifetime of similar to 10(23) s. In such a cosmology the Universe is re-

Place, publisher, year, edition, pages
BLACKWELL SCIENCE LTD , 1998. Vol. 301, no 1, 210-214 p.
Keyword [en]
cosmic microwave background; dark matter; HIGH DEUTERIUM ABUNDANCE; LARGE-SCALE STRUCTURE; DARK MATTER MODELS; LYMAN-ALPHA CLOUDS; GALAXY FORMATION; THERMAL HISTORY; PRIMEVAL PLASMA; UNIVERSE; REIONIZATION; RECOMBINATION
Identifiers
URN: urn:nbn:se:uu:diva-70149OAI: oai:DiVA.org:uu-70149DiVA: diva2:98060
Note
Addresses: Adams JA, Uppsala Univ, Dept Theoret Phys, Box 803, S-75108 Uppsala, Sweden. Uppsala Univ, Dept Theoret Phys, S-75108 Uppsala, Sweden. Univ Oxford, Oxford OX1 3NP, England. Int Ctr Theoret Phys, SISSA, I-34014 Trieste, Italy. Univ Oxford, NuclAvailable from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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