Antimatter in Different Baryogenesis Scenarios

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dc.creatorDolgov, A. D.
dc.date1996-05-11
dc.date.accessioned2026-07-07T03:59:14Z
dc.date.available2026-07-07T03:59:14Z
dc.descriptionPossible mechanisms of abundant creation of antimatter in the universe are reviewed. The necessary conditions for that are: baryonic charge nonconservation, spontaneous breaking of charge symmetry or nonequilibrium initial state, and the formation of appropriate initial conditions during inflation. In this case the universe may be populated with domains, cells, or even stellar size objects consisting of antimatter.
dc.descriptionLatex, 9 pages, presented at International Workshop on Baryon Instability, Oak Ridge, Tennessee, March 28-39, 1996. (to be published in the Proceedings)
dc.identifierhttps://arxiv.org/abs/hep-ph/9605280
dc.identifierhttp://arxiv.org/abs/hep-ph/9605280
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46142
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleAntimatter in Different Baryogenesis Scenarios
dc.typetext

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