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Charge and colour breaking in the constrained MSSM
We show that the physical minimum of the Constrained MSSM is only free from dangerous charge and colour breaking minima in the region of parameter space bounded by 110< m_1/2< 400 GeV and 80< m_0< 170 GeV. In the remaining regions, the cosmology is severely constrained.
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1998
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(98)01401-4 http://cds.cern.ch/record/367598 |
_version_ | 1780892976309862400 |
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author | Abel, Steven Falk, Toby |
author_facet | Abel, Steven Falk, Toby |
author_sort | Abel, Steven |
collection | CERN |
description | We show that the physical minimum of the Constrained MSSM is only free from dangerous charge and colour breaking minima in the region of parameter space bounded by 110< m_1/2< 400 GeV and 80< m_0< 170 GeV. In the remaining regions, the cosmology is severely constrained. |
id | cern-367598 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1998 |
record_format | invenio |
spelling | cern-3675982023-03-14T18:44:13Zdoi:10.1016/S0370-2693(98)01401-4http://cds.cern.ch/record/367598engAbel, StevenFalk, TobyCharge and colour breaking in the constrained MSSMParticle Physics - PhenomenologyWe show that the physical minimum of the Constrained MSSM is only free from dangerous charge and colour breaking minima in the region of parameter space bounded by 110< m_1/2< 400 GeV and 80< m_0< 170 GeV. In the remaining regions, the cosmology is severely constrained.We show that the physical minimum of the Constrained MSSM is only free from dangerous charge and colour breaking minima in the region of parameter space bounded by 110< m_1/2< 400 GeV and 80< m_0< 170 GeV. In the remaining regions, the cosmology is severely constrained.We show that the physical minimum of the Constrained MSSM is only free from dangerous charge and colour breaking minima in the region of parameter space bounded by 110≲m 1/2 ≲400 GeV and 80≲m 0 ≲170 GeV . In the remaining regions the cosmology is severely constrained.hep-ph/9810297CERN-TH-98-322MADPH-98-1083CERN-TH-98-322MAD-PH-1083oai:cds.cern.ch:3675981998-10-09 |
spellingShingle | Particle Physics - Phenomenology Abel, Steven Falk, Toby Charge and colour breaking in the constrained MSSM |
title | Charge and colour breaking in the constrained MSSM |
title_full | Charge and colour breaking in the constrained MSSM |
title_fullStr | Charge and colour breaking in the constrained MSSM |
title_full_unstemmed | Charge and colour breaking in the constrained MSSM |
title_short | Charge and colour breaking in the constrained MSSM |
title_sort | charge and colour breaking in the constrained mssm |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1016/S0370-2693(98)01401-4 http://cds.cern.ch/record/367598 |
work_keys_str_mv | AT abelsteven chargeandcolourbreakingintheconstrainedmssm AT falktoby chargeandcolourbreakingintheconstrainedmssm |