Superball dark matter

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dc.creatorKusenko, Alexander
dc.date1998-08-10
dc.date.accessioned2026-07-07T04:04:30Z
dc.date.available2026-07-07T04:04:30Z
dc.descriptionSupersymmetric models predict a natural dark-matter candidate, stable baryonic Q-balls. They could be copiously produced in the early Universe as a by-product of the Affleck-Dine baryogenesis. I review the cosmological and astrophysical implications, methods of detection, and the present limits on this form of dark matter.
dc.description15 pages, 5 figures; Invited talk at Second International Conference on Dark Matter in Astrophysics and Particle Physics (DARK-98), Heidelberg, Germany, July 20-25, 1998. (latex, psfig, epsf)
dc.identifierhttps://arxiv.org/abs/hep-ph/9808276
dc.identifierhttp://arxiv.org/abs/hep-ph/9808276
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/48118
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Theory
dc.titleSuperball dark matter
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