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.