Flat direction inflation with running kinetic term and baryogenesis

We consider a possibility that one of the flat directions in the minimal supersymmetric standard model plays the role of the inflaton field and realizes large-field inflation. This is achieved by introducing a generalized shift symmetry on the flat direction, which enables us to control the inflaton...

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Main Authors: Shinta Kasuya, Fuminobu Takahashi
Format: Article
Language:English
Published: Elsevier 2014-09-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269314005577
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author Shinta Kasuya
Fuminobu Takahashi
author_facet Shinta Kasuya
Fuminobu Takahashi
author_sort Shinta Kasuya
collection DOAJ
description We consider a possibility that one of the flat directions in the minimal supersymmetric standard model plays the role of the inflaton field and realizes large-field inflation. This is achieved by introducing a generalized shift symmetry on the flat direction, which enables us to control the inflaton potential over large field values. After inflation, higher order terms allowed by the generalized shift symmetry automatically cause a helical motion of the field to create the baryon number of the universe, while baryonic isocurvature fluctuations are suppressed.
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spelling doaj.art-fff485242ca54c87b3241f77c73286b12022-12-22T00:32:33ZengElsevierPhysics Letters B0370-26931873-24452014-09-01736C52653210.1016/j.physletb.2014.07.055Flat direction inflation with running kinetic term and baryogenesisShinta Kasuya0Fuminobu Takahashi1Department of Mathematics and Physics, Kanagawa University, Kanagawa 259-1293, JapanDepartment of Physics, Tohoku University, Sendai 980-8578, JapanWe consider a possibility that one of the flat directions in the minimal supersymmetric standard model plays the role of the inflaton field and realizes large-field inflation. This is achieved by introducing a generalized shift symmetry on the flat direction, which enables us to control the inflaton potential over large field values. After inflation, higher order terms allowed by the generalized shift symmetry automatically cause a helical motion of the field to create the baryon number of the universe, while baryonic isocurvature fluctuations are suppressed.http://www.sciencedirect.com/science/article/pii/S0370269314005577
spellingShingle Shinta Kasuya
Fuminobu Takahashi
Flat direction inflation with running kinetic term and baryogenesis
Physics Letters B
title Flat direction inflation with running kinetic term and baryogenesis
title_full Flat direction inflation with running kinetic term and baryogenesis
title_fullStr Flat direction inflation with running kinetic term and baryogenesis
title_full_unstemmed Flat direction inflation with running kinetic term and baryogenesis
title_short Flat direction inflation with running kinetic term and baryogenesis
title_sort flat direction inflation with running kinetic term and baryogenesis
url http://www.sciencedirect.com/science/article/pii/S0370269314005577
work_keys_str_mv AT shintakasuya flatdirectioninflationwithrunningkinetictermandbaryogenesis
AT fuminobutakahashi flatdirectioninflationwithrunningkinetictermandbaryogenesis