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$\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$
We present a solution of the mu problem within a supersymmetric model based on the SU(2)_L x SU(2)_R x U(1)_{B-L} gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially cons...
Autores principales: | , , |
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Lenguaje: | eng |
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1997
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(98)00145-2 http://cds.cern.ch/record/335951 |
_version_ | 1780891299782590464 |
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author | Dvali, G.R. Lazarides, George Shafi, Q. |
author_facet | Dvali, G.R. Lazarides, George Shafi, Q. |
author_sort | Dvali, G.R. |
collection | CERN |
description | We present a solution of the mu problem within a supersymmetric model based on the SU(2)_L x SU(2)_R x U(1)_{B-L} gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially conserved as a result of an R-symmetry. Neutrinos with mass in the eV range can provide the `hot' dark matter component. |
id | cern-335951 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1997 |
record_format | invenio |
spelling | cern-3359512023-10-04T08:49:44Zdoi:10.1016/S0370-2693(98)00145-2http://cds.cern.ch/record/335951engDvali, G.R.Lazarides, GeorgeShafi, Q.$\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$Particle Physics - PhenomenologyWe present a solution of the mu problem within a supersymmetric model based on the SU(2)_L x SU(2)_R x U(1)_{B-L} gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially conserved as a result of an R-symmetry. Neutrinos with mass in the eV range can provide the `hot' dark matter component.We present a solution of the mu problem within a supersymmetric model based on the SU(2)_L x SU(2)_R x U(1)_{B-L} gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially conserved as a result of an R-symmetry. Neutrinos with mass in the eV range can provide the `hot' dark matter component.We present a solution of the mu problem within a supersymmetric model based on the SU(2)_L x SU(2)_R x U(1)_{B-L} gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially conserved as a result of an R-symmetry. Neutrinos with mass in the eV range can provide the `hot' dark matter component.We present a solution of the μ problem within a supersymmetric model based on the SU (2) L × SU (2) R × U (1) B − L gauge group. We show that this solution implies a built-in hybrid inflationary scenario, which may result in a successful baryogenesis via leptogenesis. Baryon number is essentially conserved as a result of an R-symmetry. Neutrinos with mass in the eV range can provide the `hot' dark matter component.hep-ph/9710314BA-97-25CERN-TH-97-275BA-97-25CERN-TH-97-275oai:cds.cern.ch:3359511997-10-13 |
spellingShingle | Particle Physics - Phenomenology Dvali, G.R. Lazarides, George Shafi, Q. $\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$ |
title | $\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$ |
title_full | $\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$ |
title_fullStr | $\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$ |
title_full_unstemmed | $\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$ |
title_short | $\mu$ Problem and Hybrid Inflation in Supersymmetric $SU(2)_L x SU(2)_R x U(1)_{B-L}$ |
title_sort | $\mu$ problem and hybrid inflation in supersymmetric $su(2)_l x su(2)_r x u(1)_{b-l}$ |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/S0370-2693(98)00145-2 http://cds.cern.ch/record/335951 |
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