Antimatter in Different Baryogenesis Scenarios

Details Antimatter in Different Baryogenesis Scenarios Antimatter in Different Baryogenesis Scenarios

1996-05-11

arxiv.org/abs/hep-ph/9605280v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

Latex, 9 pages, presented at International Workshop on Baryon Instability, Oak Ridge, Tennessee, March 28-39, 1996. (to be pub

Scientific paper

Possible 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.

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