Right-handed Sneutrino Dark Matter in Supersymmetric B-L Model

Details Right-handed Sneutrino Dark Matter in Supersymmetric B-L Model Right-handed Sneutrino Dark Matter in Supersymmetric B-L Model

2011-02-21

arxiv.org/abs/1102.4249v2

JHEP 1107:026,2011

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages, 7 figures; version accepted for publication in Journal of High Energy Physics

Scientific paper

10.1007/JHEP07(2011)026

We show that the lightest right-handed sneutrino in TeV scale supersymmetric B-L model with inverse seesaw mechanism is a viable candidate for cold dark matter. We find that it accounts for the observed dark matter relic abundance in a wide range of parameter space. The spin-independent cross section of B-L right-handed sneutrino is consistent with the recent results CDMS II and XENON experiments and it is detectable in future direct detection experiments. Although the B-L right-handed sneutrinos annihilate into leptons, the PAMELA results can not be explained in this model unless a huge boost factor is considered. Also the muon flux generated by B-L right-handed sneutrino in the galactic center is smaller than Super-Kamiokande's upper bound.

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