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Thermal right-handed sneutrino dark matter in the NMSSM

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3264550· OSTI ID:21322951
 [1]
  1. Departamento de Fisica Teorica C-XI, and Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, Cantoblanco, E-28049 Madrid (Spain)
The right-handed sneutrino is a viable WIMP dark matter candidate within the context of the Next-to-MSSM. This is possible through the inclusion of a new singlet superfield with direct coupling to the singlet Higgs. I will review here the main details of this construction, together with the properties of the right-handed sneutrino, including its annihilation channels and direct detection prospects. Sneutrinos within a mass-range of 5-200 GeV can reproduce the correct dark matter relic abundance while not being excluded by current direct searches, and for natural values of the input parameters. Some interesting features regarding collider phenomenology are also pointed out.
OSTI ID:
21322951
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1178; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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