Supersymmetric Q-balls: theory and cosmology

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dc.creatorKusenko, Alexander
dc.date1998-06-30
dc.date.accessioned2026-07-07T04:04:11Z
dc.date.available2026-07-07T04:04:11Z
dc.descriptionMSSM predicts the existence of Q-balls, some of which can be entirely stable. Both stable and unstable Q-balls can play an important role in cosmology. In particular, 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.descriptiontalk presented at PASCOS-98; transparencies available at http://wwwinfo.cern.ch/~kusenko/PASCOS98.ps; 4 pages, latex, sprocl, psfig
dc.identifierhttps://arxiv.org/abs/hep-ph/9806529
dc.identifierhttp://arxiv.org/abs/hep-ph/9806529
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/47987
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSupersymmetric Q-balls: theory and cosmology
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