Non-thermal baryogenesis from MSSM flat direction

Fuente: arXiv
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Autori principali: Haba, Naoyuki, Shimizu, Yasuhiro, Tanabe, Yoshihiro, Yamada, Toshifumi
Natura: Preprint
Pubblicazione: 2024
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author Haba, Naoyuki
Shimizu, Yasuhiro
Tanabe, Yoshihiro
Yamada, Toshifumi
author_facet Haba, Naoyuki
Shimizu, Yasuhiro
Tanabe, Yoshihiro
Yamada, Toshifumi
contents We study an inflection point inflation scenario where a flat direction of the minimal supersymmetric standard model (MSSM) is identified with the inflaton. We focus on the case where the flat direction (inflaton) has non-zero baryon number, and consider a non-thermal baryogenesis scenario where the decay of the inflaton at the reheating directly generates baryon asymmetry of the Universe. Specifically, we consider a udd flat direction that is lifted by a superpotential operator of dimension 6, and show that inflection point inflation with the udd flat direction can be compatible with cosmological observations and can account for the baryon asymmetry of the Universe.
format Preprint
id arxiv_https___arxiv_org_abs_2408_00228
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Non-thermal baryogenesis from MSSM flat direction
Haba, Naoyuki
Shimizu, Yasuhiro
Tanabe, Yoshihiro
Yamada, Toshifumi
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We study an inflection point inflation scenario where a flat direction of the minimal supersymmetric standard model (MSSM) is identified with the inflaton. We focus on the case where the flat direction (inflaton) has non-zero baryon number, and consider a non-thermal baryogenesis scenario where the decay of the inflaton at the reheating directly generates baryon asymmetry of the Universe. Specifically, we consider a udd flat direction that is lifted by a superpotential operator of dimension 6, and show that inflection point inflation with the udd flat direction can be compatible with cosmological observations and can account for the baryon asymmetry of the Universe.
title Non-thermal baryogenesis from MSSM flat direction
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2408.00228