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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...
Autores principales: | , , , , |
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Lenguaje: | eng |
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2014
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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. |
id | cern-1693953 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2014 |
record_format | invenio |
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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