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A Next-to-Minimal Supersymmetric Model of Hybrid Inflation

In this talk we discuss a model of inflation based on a simple variant of the NMSSM, called NMSSM [1], where the additional singlet plays the role of the inflaton in hybrid (or inverted hybrid) type models. As in the original NMSSM, the NMSSM solves the problem of the MSSM via the VEV of a gauge sin...

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Detalles Bibliográficos
Autores principales: Bastero-Gil, M., King, S.F.
Lenguaje:eng
Publicado: 1998
Materias:
Acceso en línea:https://dx.doi.org/10.1142/9789814447263_0040
http://cds.cern.ch/record/612306
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author Bastero-Gil, M.
King, S.F.
author_facet Bastero-Gil, M.
King, S.F.
author_sort Bastero-Gil, M.
collection CERN
description In this talk we discuss a model of inflation based on a simple variant of the NMSSM, called NMSSM [1], where the additional singlet plays the role of the inflaton in hybrid (or inverted hybrid) type models. As in the original NMSSM, the NMSSM solves the problem of the MSSM via the VEV of a gauge singlet N, but unlike the NMSSM does not suer from domain wall problems since the oending Z3 symmetry is replaced by an approximate Peccei-Quinn symmetry which also solves the strong CP problem, and leads to an invisible axion with interesting cosmological consequences. The model predicts a spectral index n = 1 to one part in 10$^{12}$.
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institution Organización Europea para la Investigación Nuclear
language eng
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spelling cern-6123062023-03-14T18:41:48Zdoi:10.1142/9789814447263_0040http://cds.cern.ch/record/612306engBastero-Gil, M.King, S.F.A Next-to-Minimal Supersymmetric Model of Hybrid InflationParticle Physics - PhenomenologyIn this talk we discuss a model of inflation based on a simple variant of the NMSSM, called NMSSM [1], where the additional singlet plays the role of the inflaton in hybrid (or inverted hybrid) type models. As in the original NMSSM, the NMSSM solves the problem of the MSSM via the VEV of a gauge singlet N, but unlike the NMSSM does not suer from domain wall problems since the oending Z3 symmetry is replaced by an approximate Peccei-Quinn symmetry which also solves the strong CP problem, and leads to an invisible axion with interesting cosmological consequences. The model predicts a spectral index n = 1 to one part in 10$^{12}$.In this talk we discuss a model of inflation based on a simple variant of the NMSSM, called $\phi$NMSSM \cite{phiNMSSM}, where the additional singlet $\phi$ plays the role of the inflaton in hybrid (or inverted hybrid) type models. As in the original NMSSM, the $\phi$NMSSM solves the $\mu$ problem of the MSSM via the VEV of a gauge singlet $N$, but unlike the NMSSM does not suffer from domain wall problems since the offending $Z_3$ symmetry is replaced by an approximate Peccei-Quinn symmetry which also solves the strong CP problem, and leads to an invisible axion with interesting cosmological consequences. The model predicts a spectral index $n=1$ to one part in $10^{12}$.hep-ph/9801451CERN-TH-98-25CERN-TH-98-025oai:cds.cern.ch:6123061998
spellingShingle Particle Physics - Phenomenology
Bastero-Gil, M.
King, S.F.
A Next-to-Minimal Supersymmetric Model of Hybrid Inflation
title A Next-to-Minimal Supersymmetric Model of Hybrid Inflation
title_full A Next-to-Minimal Supersymmetric Model of Hybrid Inflation
title_fullStr A Next-to-Minimal Supersymmetric Model of Hybrid Inflation
title_full_unstemmed A Next-to-Minimal Supersymmetric Model of Hybrid Inflation
title_short A Next-to-Minimal Supersymmetric Model of Hybrid Inflation
title_sort next-to-minimal supersymmetric model of hybrid inflation
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1142/9789814447263_0040
http://cds.cern.ch/record/612306
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