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F-term inflation in Superstring Theories

A supersymmetric inflationary stage dominated by an $F$-term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter $\eta$ gets contributions of order unity. We show that in $F$-term inflationary models based on strings there is nat...

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Detalles Bibliográficos
Autores principales: Casas, J.A., Gelmini, G.B., Riotto, A.
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(99)00683-8
http://cds.cern.ch/record/383052
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author Casas, J.A.
Gelmini, G.B.
Riotto, A.
author_facet Casas, J.A.
Gelmini, G.B.
Riotto, A.
author_sort Casas, J.A.
collection CERN
description A supersymmetric inflationary stage dominated by an $F$-term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter $\eta$ gets contributions of order unity. We show that in $F$-term inflationary models based on strings there is natural way of obtaining small values of $\eta$. This happens in models of hybrid inflation based on orbifold constructions, in which a modulus $T$ field is responsible for the large value of the potential during inflation, and a second field illustrate the mechanism with a model in which the inflaton potential is provided by gaugino condensation, leading to succesful inflation.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
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spelling cern-3830522023-10-04T08:18:00Zdoi:10.1016/S0370-2693(99)00683-8http://cds.cern.ch/record/383052engCasas, J.A.Gelmini, G.B.Riotto, A.F-term inflation in Superstring TheoriesParticle Physics - PhenomenologyA supersymmetric inflationary stage dominated by an $F$-term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter $\eta$ gets contributions of order unity. We show that in $F$-term inflationary models based on strings there is natural way of obtaining small values of $\eta$. This happens in models of hybrid inflation based on orbifold constructions, in which a modulus $T$ field is responsible for the large value of the potential during inflation, and a second field illustrate the mechanism with a model in which the inflaton potential is provided by gaugino condensation, leading to succesful inflation.A supersymmetric inflationary stage dominated by an $F$-term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter $\eta$ gets contributions of order unity. We show that in $F$-term inflationary models based on strings there is natural way of obtaining small values of $\eta$. This happens in models of hybrid inflation based on orbifold constructions, in which a modulus $T$ field is responsible for the large value of the potential during inflation, and a second field $\phi$ with appropriate modular weight is responsible for the roll-over. We illustrate the mechanism with a model in which the inflaton potential is provided by gaugino condensation, leading to succesful inflation.A supersymmetric inflationary stage dominated by an F -term has the problem that the flatness of the potential is spoiled by supergravity corrections, that is the slow-roll parameter η gets contributions of order unity. We show that in F -term inflationary models based on strings there is natural way of obtaining small values of η . This happens in models of hybrid inflation based on orbifold constructions, in which a modulus T field is responsible for the large value of the potential during inflation, and a second field φ with appropriate modular weight is responsible for the roll-over. We illustrate the mechanism with a model in which the inflaton potential is provided by gaugino condensation, leading to successful inflation.hep-ph/9903492CERN-TH-99-84IEM-FT-178-98IFT-UAM-CSIC-99-11CERN-TH-99-084IEM-FT-178IFT-UAM-CSIC-99-11oai:cds.cern.ch:3830521999-03-26
spellingShingle Particle Physics - Phenomenology
Casas, J.A.
Gelmini, G.B.
Riotto, A.
F-term inflation in Superstring Theories
title F-term inflation in Superstring Theories
title_full F-term inflation in Superstring Theories
title_fullStr F-term inflation in Superstring Theories
title_full_unstemmed F-term inflation in Superstring Theories
title_short F-term inflation in Superstring Theories
title_sort f-term inflation in superstring theories
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0370-2693(99)00683-8
http://cds.cern.ch/record/383052
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