Dark matter from Affleck-Dine baryogenesis
High Energy Physics - Phenomenology
2009-10-31 v1 Astrophysics
Abstract
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.
Keywords
Cite
@article{arxiv.hep-ph/9901353,
title = {Dark matter from Affleck-Dine baryogenesis},
author = {Alexander Kusenko},
journal= {arXiv preprint arXiv:hep-ph/9901353},
year = {2009}
}
Comments
4 pages, aipproc macro included; to appear in "Particle Physics and the Early Universe (COSMO-98)", ed. by David O. Caldwell, American Institute of Physics