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Favoured Inflationary Models by SFC Baryogenesis

Published online by Cambridge University Press:  20 January 2023

Mariana Panayotova Open the ORCID record for Mariana Panayotova [Opens in a new window]  and
Daniela Kirilova
Mariana Panayotova
Affiliation:
Institute of Astronomy with National Astronomical Observatory, Bulgarian Academy of Sciences email: [email protected]
Daniela Kirilova
Affiliation:
Institute of Astronomy with National Astronomical Observatory, Bulgarian Academy of Sciences email: [email protected]
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Abstract

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We provide analysis of the baryon asymmetry generated in the Scalar Field Condensate (SFC) baryogenesis model obtained in new inflation, chaotic inflation, Starobinsky inflation, MSSM inflation, quintessential inflation, considering both cases of efficient thermalization after inflation and also delayed thermalization. We have found that baryon asymmetry generated in SFC baryogenesis model is considerably bigger than the observed one for the new inflation, new inflation model by Shafi and Vilenkin, MSSM inflation, chaotic inflation with high reheating temperature and the simplest Shafi-Vilenkin chaotic inflationary model. Therefore, strong diluting mechanisms are needed to reduce the baryon excess to its observational value today for these models. We have shown that for the SFC baryogenesis model a successful generation of the observed baryon asymmetry is possible in Modified Starobinsky inflation, chaotic inflation with low reheating temperature, chaotic inflation in SUGRA and quintessential inflationary model.

Keywords

early univese
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S362: The Predictive Power of Computational Astrophysics as a Discovery Tool , June 2020 , pp. 21 - 25
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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