Supersymmetric baryogenesis in a hybrid inflation model

Abstract We study baryogenesis in a hybrid inflation model which is embedded to the minimal supersymmetric model with right-handed neutrinos. Inflation is induced by a linear combination of the right-handed sneutrinos and its decay reheats the universe. The decay products are stored in conserved num...

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Main Authors: Yoshihiro Gunji, Koji Ishiwata, Takahiro Yoshida
Format: Article
Language:English
Published: SpringerOpen 2023-08-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP08(2023)201
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author Yoshihiro Gunji
Koji Ishiwata
Takahiro Yoshida
author_facet Yoshihiro Gunji
Koji Ishiwata
Takahiro Yoshida
author_sort Yoshihiro Gunji
collection DOAJ
description Abstract We study baryogenesis in a hybrid inflation model which is embedded to the minimal supersymmetric model with right-handed neutrinos. Inflation is induced by a linear combination of the right-handed sneutrinos and its decay reheats the universe. The decay products are stored in conserved numbers, which are transported under the interactions in equilibrium as the temperature drops down. We find that at least a few percent of the initial lepton asymmetry is left under the strong wash-out due to the lighter right-handed (s)neutrinos. To account for the observed baryon number and the active neutrino masses after a successful inflation, the inflaton mass and the Majorana mass scale should be 1013 GeV and O $$ \mathcal{O} $$ (109–1010) GeV, respectively.
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spelling doaj.art-0cf38224e86f4770a6ba1569d12c58d22023-10-29T12:10:38ZengSpringerOpenJournal of High Energy Physics1029-84792023-08-012023811810.1007/JHEP08(2023)201Supersymmetric baryogenesis in a hybrid inflation modelYoshihiro Gunji0Koji Ishiwata1Takahiro Yoshida2Institute for Theoretical Physics, Kanazawa UniversityInstitute for Theoretical Physics, Kanazawa UniversityDepartment of Information, Kaishi Professional UniversityAbstract We study baryogenesis in a hybrid inflation model which is embedded to the minimal supersymmetric model with right-handed neutrinos. Inflation is induced by a linear combination of the right-handed sneutrinos and its decay reheats the universe. The decay products are stored in conserved numbers, which are transported under the interactions in equilibrium as the temperature drops down. We find that at least a few percent of the initial lepton asymmetry is left under the strong wash-out due to the lighter right-handed (s)neutrinos. To account for the observed baryon number and the active neutrino masses after a successful inflation, the inflaton mass and the Majorana mass scale should be 1013 GeV and O $$ \mathcal{O} $$ (109–1010) GeV, respectively.https://doi.org/10.1007/JHEP08(2023)201Baryo-and LeptogenesisCosmology of Theories BSMEarly Universe Particle PhysicsSupersymmetry
spellingShingle Yoshihiro Gunji
Koji Ishiwata
Takahiro Yoshida
Supersymmetric baryogenesis in a hybrid inflation model
Journal of High Energy Physics
Baryo-and Leptogenesis
Cosmology of Theories BSM
Early Universe Particle Physics
Supersymmetry
title Supersymmetric baryogenesis in a hybrid inflation model
title_full Supersymmetric baryogenesis in a hybrid inflation model
title_fullStr Supersymmetric baryogenesis in a hybrid inflation model
title_full_unstemmed Supersymmetric baryogenesis in a hybrid inflation model
title_short Supersymmetric baryogenesis in a hybrid inflation model
title_sort supersymmetric baryogenesis in a hybrid inflation model
topic Baryo-and Leptogenesis
Cosmology of Theories BSM
Early Universe Particle Physics
Supersymmetry
url https://doi.org/10.1007/JHEP08(2023)201
work_keys_str_mv AT yoshihirogunji supersymmetricbaryogenesisinahybridinflationmodel
AT kojiishiwata supersymmetricbaryogenesisinahybridinflationmodel
AT takahiroyoshida supersymmetricbaryogenesisinahybridinflationmodel