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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...

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Autores principales: Alexandre, Jean, Houston, Nick, Mavromatos, Nick E.
Lenguaje:eng
Publicado: 2013
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.89.027703
http://cds.cern.ch/record/1637842
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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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
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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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AT mavromatosnicke starobinskytypeinflationindynamicalsupergravitybreakingscenarios