Baryonic Q-balls as dark matter

Simple item page
dc.creatorKusenko, Alexander
dc.date2000-09-07
dc.date.accessioned2026-07-07T03:42:32Z
dc.date.available2026-07-07T03:42:32Z
dc.descriptionSupersymmetric extensions of the Standard Model predict the existence of Q-balls, some of which can be entirely stable. Affleck-Dine baryogenesis can result in a copious production of stable baryonic Q-balls, which can presently exist as a form of dark matter.
dc.description10 pages, 4 figures; invited talk at 3rd International Conference on Dark Matter in Astro and Particle Physics (Dark 2000), Heidelberg, Germany, 10-16 Jul 2000
dc.identifierhttps://arxiv.org/abs/hep-ph/0009089
dc.identifierhttp://arxiv.org/abs/hep-ph/0009089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39930
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleBaryonic Q-balls as dark matter
dc.typetext

Files

Collections

arXiv