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Phenomenology of GUT-less Supersymmetry Breaking
We study models in which supersymmetry breaking appears at an intermediate scale, M_{in}, below the GUT scale. We assume that the soft supersymmetry-breaking parameters of the MSSM are universal at M_{in}, and analyze the morphology of the constraints from cosmology and collider experiments on the a...
Autores principales: | , , |
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Lenguaje: | eng |
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2007
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Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/2007/06/079 http://cds.cern.ch/record/1031823 |
_version_ | 1780912338773213184 |
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author | Ellis, Jonathan Richard Olive, Keith A Sandick, Pearl |
author_facet | Ellis, Jonathan Richard Olive, Keith A Sandick, Pearl |
author_sort | Ellis, Jonathan Richard |
collection | CERN |
description | We study models in which supersymmetry breaking appears at an intermediate scale, M_{in}, below the GUT scale. We assume that the soft supersymmetry-breaking parameters of the MSSM are universal at M_{in}, and analyze the morphology of the constraints from cosmology and collider experiments on the allowed regions of parameter space as M_{in} is reduced from the GUT scale. We present separate analyses of the (m_{1/2},m_0) planes for tan(beta)=10 and tan(beta)=50, as well as a discussion of non-zero trilinear couplings, A_0. Specific scenarios where the gaugino and scalar masses appear to be universal below the GUT scale have been found in mirage-mediation models, which we also address here. We demand that the lightest neutralino be the LSP, and that the relic neutralino density not conflict with measurements by WMAP and other observations. At moderate values of M_{in}, we find that the allowed regions of the (m_{1/2},m_0) plane are squeezed by the requirements of electroweak symmetry breaking and that the lightest neutralino be the LSP, whereas the constraint on the relic density is less severe. At very low M_{in}, the electroweak vacuum conditions become the dominant constraint, and a secondary source of astrophysical cold dark matter would be necessary to explain the measured relic density for nearly all values of the soft SUSY-breaking parameters and tan(beta). We calculate the neutralino-nucleon cross sections for viable sce narios and compare them with the present and projected limits from direct dark matter searches. |
id | cern-1031823 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2007 |
record_format | invenio |
spelling | cern-10318232019-09-30T06:29:59Zdoi:10.1088/1126-6708/2007/06/079http://cds.cern.ch/record/1031823engEllis, Jonathan RichardOlive, Keith ASandick, PearlPhenomenology of GUT-less Supersymmetry BreakingParticle Physics - PhenomenologyWe study models in which supersymmetry breaking appears at an intermediate scale, M_{in}, below the GUT scale. We assume that the soft supersymmetry-breaking parameters of the MSSM are universal at M_{in}, and analyze the morphology of the constraints from cosmology and collider experiments on the allowed regions of parameter space as M_{in} is reduced from the GUT scale. We present separate analyses of the (m_{1/2},m_0) planes for tan(beta)=10 and tan(beta)=50, as well as a discussion of non-zero trilinear couplings, A_0. Specific scenarios where the gaugino and scalar masses appear to be universal below the GUT scale have been found in mirage-mediation models, which we also address here. We demand that the lightest neutralino be the LSP, and that the relic neutralino density not conflict with measurements by WMAP and other observations. At moderate values of M_{in}, we find that the allowed regions of the (m_{1/2},m_0) plane are squeezed by the requirements of electroweak symmetry breaking and that the lightest neutralino be the LSP, whereas the constraint on the relic density is less severe. At very low M_{in}, the electroweak vacuum conditions become the dominant constraint, and a secondary source of astrophysical cold dark matter would be necessary to explain the measured relic density for nearly all values of the soft SUSY-breaking parameters and tan(beta). We calculate the neutralino-nucleon cross sections for viable sce narios and compare them with the present and projected limits from direct dark matter searches.arXiv:0704.3446CERN-PH-TH-2007-073FTPI-MINN-07-15UMN-TH-2602-07oai:cds.cern.ch:10318232007-04-27 |
spellingShingle | Particle Physics - Phenomenology Ellis, Jonathan Richard Olive, Keith A Sandick, Pearl Phenomenology of GUT-less Supersymmetry Breaking |
title | Phenomenology of GUT-less Supersymmetry Breaking |
title_full | Phenomenology of GUT-less Supersymmetry Breaking |
title_fullStr | Phenomenology of GUT-less Supersymmetry Breaking |
title_full_unstemmed | Phenomenology of GUT-less Supersymmetry Breaking |
title_short | Phenomenology of GUT-less Supersymmetry Breaking |
title_sort | phenomenology of gut-less supersymmetry breaking |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1088/1126-6708/2007/06/079 http://cds.cern.ch/record/1031823 |
work_keys_str_mv | AT ellisjonathanrichard phenomenologyofgutlesssupersymmetrybreaking AT olivekeitha phenomenologyofgutlesssupersymmetrybreaking AT sandickpearl phenomenologyofgutlesssupersymmetrybreaking |