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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...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1998
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0550-3213(99)00177-7 http://cds.cern.ch/record/358286 |
_version_ | 1780892574387535872 |
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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. |
id | cern-358286 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1998 |
record_format | invenio |
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 |