Dark Matter in B-L Extended MSSM Models
Abstract
We analyze the dark matter problem in the context of supersymmetric U(1)B-L model. In this model, the lightest neutalino can be the B-L gaugino widetilde ZB-L or the extra Higgsinos widetildechi1,2 dominated. We compute the thermal relic abundance of these particles and show that, unlike the LSP in MSSM, they can account for the observed relic abundance with no conflict with other phenomenological constraints. The prospects for their direct detection, if they are part of our galactic halo, are also discussed.
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