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F-term Hybrid Inflation in Effective Supergravity Theories

We show that the effective low energy supergravity theories which result from a generic string theory can provide a promising framework for models of hybrid inflation in which the potential energy which drives inflation originates from the F-term of the effective supergravity theory. In the class of...

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Detalles Bibliográficos
Autores principales: Bastero-Gil, M, King, S F
Lenguaje:eng
Publicado: 1998
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0550-3213(99)00177-7
http://cds.cern.ch/record/358286
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author Bastero-Gil, M
King, S F
author_facet Bastero-Gil, M
King, S F
author_sort Bastero-Gil, M
collection CERN
description We show that the effective low energy supergravity theories which result from a generic string theory can provide a promising framework for models of hybrid inflation in which the potential energy which drives inflation originates from the F-term of the effective supergravity theory. In the class of models considered the inflaton is protected from receiving mass during inflation by a Heisenberg symmetry and the potential during inflation takes the positive definite form $V \sim |F|^2$, which allows the possibility that $V\ll m_{3/2}^2 M_P^2$. We discuss a toy example where this is realised, then describe the application of this result to realistic models focusing on a particular example in which the $\mu$ problem and the strong CP-problem are addressed.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1998
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spelling cern-3582862019-09-30T06:29:59Zdoi:10.1016/S0550-3213(99)00177-7http://cds.cern.ch/record/358286engBastero-Gil, MKing, S FF-term Hybrid Inflation in Effective Supergravity TheoriesParticle Physics - PhenomenologyWe show that the effective low energy supergravity theories which result from a generic string theory can provide a promising framework for models of hybrid inflation in which the potential energy which drives inflation originates from the F-term of the effective supergravity theory. In the class of models considered the inflaton is protected from receiving mass during inflation by a Heisenberg symmetry and the potential during inflation takes the positive definite form $V \sim |F|^2$, which allows the possibility that $V\ll m_{3/2}^2 M_P^2$. We discuss a toy example where this is realised, then describe the application of this result to realistic models focusing on a particular example in which the $\mu$ problem and the strong CP-problem are addressed.hep-ph/9806477CERN-TH-98-190SHEP-98-10oai:cds.cern.ch:3582861998-06-26
spellingShingle Particle Physics - Phenomenology
Bastero-Gil, M
King, S F
F-term Hybrid Inflation in Effective Supergravity Theories
title F-term Hybrid Inflation in Effective Supergravity Theories
title_full F-term Hybrid Inflation in Effective Supergravity Theories
title_fullStr F-term Hybrid Inflation in Effective Supergravity Theories
title_full_unstemmed F-term Hybrid Inflation in Effective Supergravity Theories
title_short F-term Hybrid Inflation in Effective Supergravity Theories
title_sort f-term hybrid inflation in effective supergravity theories
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0550-3213(99)00177-7
http://cds.cern.ch/record/358286
work_keys_str_mv AT basterogilm ftermhybridinflationineffectivesupergravitytheories
AT kingsf ftermhybridinflationineffectivesupergravitytheories