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Baryonic dark matterBoth canonical primordial nucleosynthesis constraints and large-scale structure measurements, as well as observations of the fundamental cosmological parameters, appear to be consistent with the hypothesis that the universe predominantly consists of baryonic dark matter (BDM). The arguments for BDM to consist of compact objects that are either stellar relics or substellar objects are reviewed. Several techniques for searching for halo BDM are described.
Document ID
19930033657
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Silk, Joseph (Mount Stromlo and Siding Spring Observatories, Canberra, Australia; California Univ. Berkeley, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Publication Information
Publication: In: Primordial nucleosynthesis and evolution of early universe; Proceedings of the International Conference, Tokyo, Japan, Sept. 4-8, 1990 (A93-17626 05-90)
Publisher: Kluwer Academic Publishers
Subject Category
Astrophysics
Accession Number
93A17654
Distribution Limits
Public
Copyright
Other

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