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Inflationary Baryogenesis

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arxiv hep-ph/0103348 v3 pith:LMBGOIXH submitted 2001-03-30 hep-ph astro-phgr-qc

classification hep-phastro-phgr-qc
keywords fieldinflatoncomplexannihilationasymmetrycasecreationinflation
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In this letter we explore the possibility of creating the baryon asymmetry of the universe during inflation and reheating due to the decay of a field associated with the inflaton. CP violation is attained by assuming that this field is complex with a phase that varies as the inflaton evolves. We consider chaotic and natural inflation scenarios. In the former case, the complex decaying field is the inflaton itself and, in the latter case, the phase of the complex field is the inflaton. We calculate the asymmetry produced using the Bogolyubov formalism that relates annihilation and creation operators at late time to the annihilation and creation operators at early time.

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Cited by 1 Pith paper

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  1. Baryon asymmetry from higher-order matter contributions in gravity

    gr-qc 2025-04 conditional novelty 6.0 of 10

    A T^2-dependent coupling between the derivative of T_mu nu T^mu nu and the baryon current can generate the observed baryon asymmetry in GR and f(R,T^2) gravity, at the cost of fitted parameters.

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