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A Search for an N=2 Inflaton Potential

We consider N=2 supergravity theories that have the same spectrum as the R+R^2 supergravity, as predicted from the off-shell counting of degrees of freedom. These theories describe standard N=2 supergravity coupled to one or two long massive vector multiplets. The central charge is not gauged in the...

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Autores principales: Ceresole, Anna, Dall'Agata, Gianguido, Ferrara, Sergio, Trigiante, Mario, Van Proeyen, Antoine
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1002/prop.201400019
http://cds.cern.ch/record/1693953
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author Ceresole, Anna
Dall'Agata, Gianguido
Ferrara, Sergio
Trigiante, Mario
Van Proeyen, Antoine
author_facet Ceresole, Anna
Dall'Agata, Gianguido
Ferrara, Sergio
Trigiante, Mario
Van Proeyen, Antoine
author_sort Ceresole, Anna
collection CERN
description We consider N=2 supergravity theories that have the same spectrum as the R+R^2 supergravity, as predicted from the off-shell counting of degrees of freedom. These theories describe standard N=2 supergravity coupled to one or two long massive vector multiplets. The central charge is not gauged in these models and they have a Minkowski vacuum with N=2 unbroken supersymmetry. The gauge symmetry, being non-compact, is always broken. $\alpha$-deformed inflaton potentials are obtained, in the case of a single massive vector multiplet, with $\alpha=1/3$ and $2/3$. The $\alpha=1$ potential (i.e. the Starobinsky potential) is also obtained, but only at the prize of having a single massive vector and a residual unbroken gauge symmetry. The inflaton corresponds to one of the Cartan fields of the non-compact quaternionic-K{\"a}hler cosets.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
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spelling cern-16939532023-03-15T19:13:02Zdoi:10.1002/prop.201400019http://cds.cern.ch/record/1693953engCeresole, AnnaDall'Agata, GianguidoFerrara, SergioTrigiante, MarioVan Proeyen, AntoineA Search for an N=2 Inflaton PotentialParticle Physics - TheoryWe consider N=2 supergravity theories that have the same spectrum as the R+R^2 supergravity, as predicted from the off-shell counting of degrees of freedom. These theories describe standard N=2 supergravity coupled to one or two long massive vector multiplets. The central charge is not gauged in these models and they have a Minkowski vacuum with N=2 unbroken supersymmetry. The gauge symmetry, being non-compact, is always broken. $\alpha$-deformed inflaton potentials are obtained, in the case of a single massive vector multiplet, with $\alpha=1/3$ and $2/3$. The $\alpha=1$ potential (i.e. the Starobinsky potential) is also obtained, but only at the prize of having a single massive vector and a residual unbroken gauge symmetry. The inflaton corresponds to one of the Cartan fields of the non-compact quaternionic-K{\"a}hler cosets.We consider <span class="math"><img alt="equation image" src="http://onlinelibrary.wiley.com/store/10.1002/prop.201400019/asset/equation/tex2gif-ueqn-2.gif?v=1&t=hx4gtweq&s=1612f16a69829da7def2a2dd2839960f16f4bac0" class="inlineGraphic" /></span> supergravity theories that have the same spectrum as the R + R^2 supergravity, as predicted from the off-shell counting of degrees of freedom. These theories describe standard <span class="math"><img alt="equation image" src="http://onlinelibrary.wiley.com/store/10.1002/prop.201400019/asset/equation/tex2gif-ueqn-3.gif?v=1&t=hx4gtwer&s=30d00676293437387bd7e9574a4dda4997a9d3d6" class="inlineGraphic" /></span> supergravity coupled to one or two long massive vector multiplets. The central charge is not gauged in these models and they have a Minkowski vacuum with <span class="math"><img alt="equation image" src="http://onlinelibrary.wiley.com/store/10.1002/prop.201400019/asset/equation/tex2gif-ueqn-4.gif?v=1&t=hx4gtwes&s=91a12799ffe009474fb88fcb5bbaa8517901d56a" class="inlineGraphic" /></span> unbroken supersymmetry. The gauge symmetry, being non-compact, is always broken. alpha-deformed inflaton potentials are obtained, in the case of a single massive vector multiplet, with alpha = 1/3 and 2/3. The alpha = 1 potential (i.e. the Starobinsky potential) is also obtained, but only at the prize of having a single massive vector and a residual unbroken gauge symmetry. The inflaton corresponds to one of the Cartan fields of the non-compact quaternionic-Ka<hler cosets.We consider N=2 supergravity theories that have the same spectrum as the R+R^2 supergravity, as predicted from the off-shell counting of degrees of freedom. These theories describe standard N=2 supergravity coupled to one or two long massive vector multiplets. The central charge is not gauged in these models and they have a Minkowski vacuum with N=2 unbroken supersymmetry. The gauge symmetry, being non-compact, is always broken. $\alpha$-deformed inflaton potentials are obtained, in the case of a single massive vector multiplet, with $\alpha=1/3$ and $2/3$. The $\alpha=1$ potential (i.e. the Starobinsky potential) is also obtained, but only at the prize of having a single massive vector and a residual unbroken gauge symmetry. The inflaton corresponds to one of the Cartan fields of the non-compact quaternionic-K{\"a}hler cosets.arXiv:1404.1745CERN-PH-TH-2014-058DFPD-14-TH-05CERN-PH-TH-2014-058oai:cds.cern.ch:16939532014-04-07
spellingShingle Particle Physics - Theory
Ceresole, Anna
Dall'Agata, Gianguido
Ferrara, Sergio
Trigiante, Mario
Van Proeyen, Antoine
A Search for an N=2 Inflaton Potential
title A Search for an N=2 Inflaton Potential
title_full A Search for an N=2 Inflaton Potential
title_fullStr A Search for an N=2 Inflaton Potential
title_full_unstemmed A Search for an N=2 Inflaton Potential
title_short A Search for an N=2 Inflaton Potential
title_sort search for an n=2 inflaton potential
topic Particle Physics - Theory
url https://dx.doi.org/10.1002/prop.201400019
http://cds.cern.ch/record/1693953
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