Dark matter from Affleck-Dine baryogenesis

Journal Article · Thu Jul 15 00:00:00 EDT 1999 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.59410· OSTI ID:21208139

Kusenko, Alexander ^[1]

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

Fragmentation of the Affleck-Dine condensate into Q-balls could fill the Universe with dark matter either in the form of stable baryonic balls, or LSP produced from the decay of unstable Q-balls. The dark matter and the ordinary matter in the Universe may share the same origin.

• OSTI ID: 21208139
• Journal Information: AIP Conference Proceedings, Vol. 478, Issue 1; Conference: COSMO-98: 2. international workshop on particle physics and the early universe, Asilomar, CA (United States), 15-20 Nov 1998; Other Information: DOI: 10.1063/1.59410; (c) 1999 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
BARYONS
COSMOLOGY
NONLUMINOUS MATTER
PARTICLE DECAY
POSTULATED PARTICLES
SOLITONS
STABILITY
SUPERSYMMETRY
UNIVERSE