Cargando…

Dark matter scenarios in a constrained model with Dirac gauginos

We perform the first analysis of Dark Matter scenarios in a constrained model with Dirac Gauginos. The model under investigation is the Constrained Minimal Dirac Gaugino Supersymmetric Standard model (CMDGSSM) where the Majorana mass terms of gauginos vanish. However, $R$-symmetry is broken in the H...

Descripción completa

Detalles Bibliográficos
Autores principales: Goodsell, Mark D., Krauss, Manuel E., Müller, Tobias, Porod, Werner, Staub, Florian
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP10(2015)132
http://cds.cern.ch/record/2031552
_version_ 1780947475988742144
author Goodsell, Mark D.
Krauss, Manuel E.
Müller, Tobias
Porod, Werner
Staub, Florian
author_facet Goodsell, Mark D.
Krauss, Manuel E.
Müller, Tobias
Porod, Werner
Staub, Florian
author_sort Goodsell, Mark D.
collection CERN
description We perform the first analysis of Dark Matter scenarios in a constrained model with Dirac Gauginos. The model under investigation is the Constrained Minimal Dirac Gaugino Supersymmetric Standard model (CMDGSSM) where the Majorana mass terms of gauginos vanish. However, $R$-symmetry is broken in the Higgs sector by an explicit and/or effective $B_\mu$-term. This causes a mass splitting between Dirac states in the fermion sector and the neutralinos, which provide the dark matter candidate, become pseudo-Dirac states. We discuss two scenarios: the universal case with all scalar masses unified at the GUT scale, and the case with non-universal Higgs soft-terms. We identify different regions in the parameter space which fullfil all constraints from the dark matter abundance, the limits from SUSY and direct dark matter searches and the Higgs mass. Most of these points can be tested with the next generation of direct dark matter detection experiments.
id cern-2031552
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
record_format invenio
spelling cern-20315522022-08-10T13:08:34Zdoi:10.1007/JHEP10(2015)132http://cds.cern.ch/record/2031552engGoodsell, Mark D.Krauss, Manuel E.Müller, TobiasPorod, WernerStaub, FlorianDark matter scenarios in a constrained model with Dirac gauginosParticle Physics - PhenomenologyWe perform the first analysis of Dark Matter scenarios in a constrained model with Dirac Gauginos. The model under investigation is the Constrained Minimal Dirac Gaugino Supersymmetric Standard model (CMDGSSM) where the Majorana mass terms of gauginos vanish. However, $R$-symmetry is broken in the Higgs sector by an explicit and/or effective $B_\mu$-term. This causes a mass splitting between Dirac states in the fermion sector and the neutralinos, which provide the dark matter candidate, become pseudo-Dirac states. We discuss two scenarios: the universal case with all scalar masses unified at the GUT scale, and the case with non-universal Higgs soft-terms. We identify different regions in the parameter space which fullfil all constraints from the dark matter abundance, the limits from SUSY and direct dark matter searches and the Higgs mass. Most of these points can be tested with the next generation of direct dark matter detection experiments.We perform the first analysis of Dark Matter scenarios in a constrained model with Dirac Gauginos. The model under investigation is the Constrained Minimal Dirac Gaugino Supersymmetric Standard model (CMDGSSM) where the Majorana mass terms of gauginos vanish. However, $R$-symmetry is broken in the Higgs sector by an explicit and/or effective $B_\mu$-term. This causes a mass splitting between Dirac states in the fermion sector and the neutralinos, which provide the dark matter candidate, become pseudo-Dirac states. We discuss two scenarios: the universal case with all scalar masses unified at the GUT scale, and the case with non-universal Higgs soft-terms. We identify different regions in the parameter space which fullfil all constraints from the dark matter abundance, the limits from SUSY and direct dark matter searches and the Higgs mass. Most of these points can be tested with the next generation of direct dark matter detection experiments.arXiv:1507.01010CERN-PH-TH-2015-152CERN-PH-TH-2015-152oai:cds.cern.ch:20315522015-07-03
spellingShingle Particle Physics - Phenomenology
Goodsell, Mark D.
Krauss, Manuel E.
Müller, Tobias
Porod, Werner
Staub, Florian
Dark matter scenarios in a constrained model with Dirac gauginos
title Dark matter scenarios in a constrained model with Dirac gauginos
title_full Dark matter scenarios in a constrained model with Dirac gauginos
title_fullStr Dark matter scenarios in a constrained model with Dirac gauginos
title_full_unstemmed Dark matter scenarios in a constrained model with Dirac gauginos
title_short Dark matter scenarios in a constrained model with Dirac gauginos
title_sort dark matter scenarios in a constrained model with dirac gauginos
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1007/JHEP10(2015)132
http://cds.cern.ch/record/2031552
work_keys_str_mv AT goodsellmarkd darkmatterscenariosinaconstrainedmodelwithdiracgauginos
AT kraussmanuele darkmatterscenariosinaconstrainedmodelwithdiracgauginos
AT mullertobias darkmatterscenariosinaconstrainedmodelwithdiracgauginos
AT porodwerner darkmatterscenariosinaconstrainedmodelwithdiracgauginos
AT staubflorian darkmatterscenariosinaconstrainedmodelwithdiracgauginos