Dark Matter in Supersymmetric U(1)B-L Model

Details Dark Matter in Supersymmetric U(1)B-L Model Dark Matter in Supersymmetric U(1)B-L Model

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1115..266k&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP Conference Proceedings, Volume

Physics

Neutrino Mass And Mixing, Dark Matter, Standard-Model Higgs Bosons

Scientific paper

We analyze the dark matter problem in the context of supersymmetric, U(1)B-L model. In this model, the lightest neutalino can be B-L gaugino Z~B-L or Higgsinos χ~1,2 dominated. We examine the thermal relic abundance of these particles and discuss the prospects for their direct detection if they form part of our galactic halo.

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