Light neutralino dark matter in MSSM

Three dark matter direct detection experiments, DAMA, COGENT and CRESST, have reported a possible signal of WIMP interaction corresponding to very light particles, close to the edge of the XENON 100 and CDMS sensitivity. Imposing the latest constraints from colliders, flavour physics, electroweak pr...

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Detalles Bibliográficos
Autores principales: Mahmoudi, Farvah, Arbey, Alexandre, Battaglia, Marco
Lenguaje:eng
Publicado: 2012
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.22323/1.174.0447
http://cds.cern.ch/record/1493858
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author Mahmoudi, Farvah
Arbey, Alexandre
Battaglia, Marco
author_facet Mahmoudi, Farvah
Arbey, Alexandre
Battaglia, Marco
author_sort Mahmoudi, Farvah
collection CERN
description Three dark matter direct detection experiments, DAMA, COGENT and CRESST, have reported a possible signal of WIMP interaction corresponding to very light particles, close to the edge of the XENON 100 and CDMS sensitivity. Imposing the latest constraints from colliders, flavour physics, electroweak precision tests and direct and indirect dark matter searches, we show that viable MSSM scenarios with a light neutralino, in agreement with all the present data, are feasible. An analysis of the characteristics of the resulting scenarios will be presented.
id cern-1493858
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
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spelling cern-14938582023-03-14T19:37:51Zdoi:10.22323/1.174.0447http://cds.cern.ch/record/1493858engMahmoudi, FarvahArbey, AlexandreBattaglia, MarcoLight neutralino dark matter in MSSMParticle Physics - PhenomenologyThree dark matter direct detection experiments, DAMA, COGENT and CRESST, have reported a possible signal of WIMP interaction corresponding to very light particles, close to the edge of the XENON 100 and CDMS sensitivity. Imposing the latest constraints from colliders, flavour physics, electroweak precision tests and direct and indirect dark matter searches, we show that viable MSSM scenarios with a light neutralino, in agreement with all the present data, are feasible. An analysis of the characteristics of the resulting scenarios will be presented.Three dark matter direct detection experiments, DAMA, COGENT and CRESST, have reported a possible signal of WIMP interaction corresponding to very light particles, close to the edge of the XENON 100 and CDMS sensitivity. Imposing the latest constraints from colliders, flavour physics, electroweak precision tests and direct and indirect dark matter searches, we show that viable MSSM scenarios with a light neutralino, in agreement with all the present data, are feasible. An analysis of the characteristics of the resulting scenarios will be presented.arXiv:1211.2795CERN-PH-TH-2012-308CERN-PH-TH-2012-308oai:cds.cern.ch:14938582012-11-13
spellingShingle Particle Physics - Phenomenology
Mahmoudi, Farvah
Arbey, Alexandre
Battaglia, Marco
Light neutralino dark matter in MSSM
title Light neutralino dark matter in MSSM
title_full Light neutralino dark matter in MSSM
title_fullStr Light neutralino dark matter in MSSM
title_full_unstemmed Light neutralino dark matter in MSSM
title_short Light neutralino dark matter in MSSM
title_sort light neutralino dark matter in mssm
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.22323/1.174.0447
http://cds.cern.ch/record/1493858
work_keys_str_mv AT mahmoudifarvah lightneutralinodarkmatterinmssm
AT arbeyalexandre lightneutralinodarkmatterinmssm
AT battagliamarco lightneutralinodarkmatterinmssm

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