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Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios
In the context of dynamical breaking of local supersymmetry (supergravity), including the Deser-Zumino super-Higgs effect, for the simple but quite representative cases of N=1, D=4 supergravity, we discuss the emergence of Starobinsky-type inflation, due to quantum corrections in the effective actio...
Autores principales: | , , |
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Lenguaje: | eng |
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2013
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Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.89.027703 http://cds.cern.ch/record/1637842 |
_version_ | 1780934659605004288 |
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author | Alexandre, Jean Houston, Nick Mavromatos, Nick E. |
author_facet | Alexandre, Jean Houston, Nick Mavromatos, Nick E. |
author_sort | Alexandre, Jean |
collection | CERN |
description | In the context of dynamical breaking of local supersymmetry (supergravity), including the Deser-Zumino super-Higgs effect, for the simple but quite representative cases of N=1, D=4 supergravity, we discuss the emergence of Starobinsky-type inflation, due to quantum corrections in the effective action arising from integrating out gravitino fields in their massive phase. This type of inflation may occur after a first-stage small-field inflation that characterises models near the origin of the one-loop effective potential, and it may occur at the non-trivial minima of the latter. Phenomenologically realistic scenarios, compatible with the Planck data, may be expected for the conformal supergravity variants of the basic model. |
id | cern-1637842 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2013 |
record_format | invenio |
spelling | cern-16378422023-03-14T17:48:56Zdoi:10.1103/PhysRevD.89.027703http://cds.cern.ch/record/1637842engAlexandre, JeanHouston, NickMavromatos, Nick E.Starobinsky-type Inflation in Dynamical Supergravity Breaking ScenariosGeneral Relativity and Cosmologyhep-thParticle Physics - Theoryastro-ph.COAstrophysics and Astronomygr-qcGeneral Relativity and CosmologyIn the context of dynamical breaking of local supersymmetry (supergravity), including the Deser-Zumino super-Higgs effect, for the simple but quite representative cases of N=1, D=4 supergravity, we discuss the emergence of Starobinsky-type inflation, due to quantum corrections in the effective action arising from integrating out gravitino fields in their massive phase. This type of inflation may occur after a first-stage small-field inflation that characterises models near the origin of the one-loop effective potential, and it may occur at the non-trivial minima of the latter. Phenomenologically realistic scenarios, compatible with the Planck data, may be expected for the conformal supergravity variants of the basic model.In the context of dynamical breaking of local supersymmetry (supergravity), including the Deser-Zumino super-Higgs effect, for the simple but quite representative cases of <math display="inline"><mi mathvariant="script">N</mi><mo>=</mo><mn>1</mn></math> , <math display="inline"><mi>D</mi><mo>=</mo><mn>4</mn></math> supergravity, we discuss the emergence of Starobinsky-type inflation, due to quantum corrections in the effective action arising from integrating out gravitino fields in their massive phase. This type of inflation may occur after a first-stage small-field inflation that characterizes models near the origin of the one-loop effective potential, and it may occur at the nontrivial minima of the latter. Phenomenologically realistic scenarios, compatible with the Planck data, may be expected for the conformal supergravity variants of the basic model.In the context of dynamical breaking of local supersymmetry (supergravity), including the Deser-Zumino super-Higgs effect, for the simple but quite representative cases of N=1, D=4 supergravity, we discuss the emergence of Starobinsky-type inflation, due to quantum corrections in the effective action arising from integrating out gravitino fields in their massive phase. This type of inflation may occur after a first-stage small-field inflation that characterises models near the origin of the one-loop effective potential, and it may occur at the non-trivial minima of the latter. Phenomenologically realistic scenarios, compatible with the Planck data, may be expected for the conformal supergravity variants of the basic model.arXiv:1312.5197KCL-PH-TH-2013-39LCTS-2013-26KCL-PH-TH-2013-39LCTS-2013-26oai:cds.cern.ch:16378422013-12-18 |
spellingShingle | General Relativity and Cosmology hep-th Particle Physics - Theory astro-ph.CO Astrophysics and Astronomy gr-qc General Relativity and Cosmology Alexandre, Jean Houston, Nick Mavromatos, Nick E. Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios |
title | Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios |
title_full | Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios |
title_fullStr | Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios |
title_full_unstemmed | Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios |
title_short | Starobinsky-type Inflation in Dynamical Supergravity Breaking Scenarios |
title_sort | starobinsky-type inflation in dynamical supergravity breaking scenarios |
topic | General Relativity and Cosmology hep-th Particle Physics - Theory astro-ph.CO Astrophysics and Astronomy gr-qc General Relativity and Cosmology |
url | https://dx.doi.org/10.1103/PhysRevD.89.027703 http://cds.cern.ch/record/1637842 |
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