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No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets

We study the stability of vacua with spontaneously broken supersymmetry in N=2 supergravity theories with only hypermultiplets. Focusing on the projection of the scalar mass matrix along the sGoldstino directions, we are able to derive a universal upper bound on the lowest mass eigenvalue. This boun...

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Detalles Bibliográficos
Autores principales: Gómez-Reino, Marta, Louis, Jan, Scrucca, Claudio A
Lenguaje:eng
Publicado: 2008
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2009/02/003
http://cds.cern.ch/record/1143947
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author Gómez-Reino, Marta
Louis, Jan
Scrucca, Claudio A
author_facet Gómez-Reino, Marta
Louis, Jan
Scrucca, Claudio A
author_sort Gómez-Reino, Marta
collection CERN
description We study the stability of vacua with spontaneously broken supersymmetry in N=2 supergravity theories with only hypermultiplets. Focusing on the projection of the scalar mass matrix along the sGoldstino directions, we are able to derive a universal upper bound on the lowest mass eigenvalue. This bound only depends on the gravitino mass and the cosmological constant, but not on the details of the quaternionic manifold spanned by the scalar fields. Comparing with the Breitenlohner-Freedman bound shows that metastability requires the cosmological constant to be smaller than a certain negative critical value. Therefore, only AdS vacua with a sufficiently negative cosmological constant can be stable, while Minkowski and dS vacua necessarily have a tachyonic direction.
id cern-1143947
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2008
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spelling cern-11439472019-09-30T06:29:59Zdoi:10.1088/1126-6708/2009/02/003http://cds.cern.ch/record/1143947engGómez-Reino, MartaLouis, JanScrucca, Claudio ANo metastable de Sitter vacua in $N=2$ supergravity with only hypermultipletsParticle Physics - TheoryWe study the stability of vacua with spontaneously broken supersymmetry in N=2 supergravity theories with only hypermultiplets. Focusing on the projection of the scalar mass matrix along the sGoldstino directions, we are able to derive a universal upper bound on the lowest mass eigenvalue. This bound only depends on the gravitino mass and the cosmological constant, but not on the details of the quaternionic manifold spanned by the scalar fields. Comparing with the Breitenlohner-Freedman bound shows that metastability requires the cosmological constant to be smaller than a certain negative critical value. Therefore, only AdS vacua with a sufficiently negative cosmological constant can be stable, while Minkowski and dS vacua necessarily have a tachyonic direction.arXiv:0812.0884CERN-PH-TH-2008-215ZMP-HH-08-16oai:cds.cern.ch:11439472008-12-05
spellingShingle Particle Physics - Theory
Gómez-Reino, Marta
Louis, Jan
Scrucca, Claudio A
No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets
title No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets
title_full No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets
title_fullStr No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets
title_full_unstemmed No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets
title_short No metastable de Sitter vacua in $N=2$ supergravity with only hypermultiplets
title_sort no metastable de sitter vacua in $n=2$ supergravity with only hypermultiplets
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/1126-6708/2009/02/003
http://cds.cern.ch/record/1143947
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