Published June 2000
| Version v1
Journal article
Baryonic dark matter
Creators
Description
Many searches for baryonic dark matter have been conducted but, so far, all have been unsuccessful. Indeed, no more than 1% of the dark matter can be in the form of hydrogen burning stars. It has recently been suggested that most of the baryons in the universe are still in the form of ionized gas so that it is possible that there is no baryonic dark matter. Although it is likely that a significant fraction of the dark matter in the Milky Way is in a halo of non-baryonic matter, the data do not exclude the possibility that a considerable amount, perhaps most of it, could be in a tenuous halo of diffuse ionized gas
Additional details
Identifiers
- PII
- S0920563200006277;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 87
- Journal Issue
- 1-3
- Journal Page Range
- p. 31-40
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 6. international workshop on topics in astroparticle and underground physics
- Dates
- 6-10 Sep 1999
- Place
- Paris (France)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 34062315
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BARYONS; HYDROGEN; HYDROGEN BURNING; IONIZED GASES; MILKY WAY; NONLUMINOUS MATTER; STARS; UNIVERSE
- Descriptors DEC
- ELEMENTARY PARTICLES; ELEMENTS; FERMIONS; FLUIDS; GALAXIES; GASES; HADRONS; MATTER; NONMETALS; STAR BURNING
Optional Information
- Copyright
- Copyright (c) 2000 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.