Radiative Linear Seesaw model, Dark Matter and U(1)B−LU(1)_{B-L}

preprint2015arXivOpen access

Abstract

In this paper we propose a radiated linear seesaw model where the naturally small term μLμ_{L} are generated at one-loop level and its soft-breaking of lepton number symmetry attributes to the spontaneous breaking(SSB) of B-L gauge symmetry. The value of B−LB-L charges for new particles are assigned to satisfy the anomalies cancelation. It is founded that some new particles may have exotic values of B−LB-L charge such that there exists residual Z2×Z2′Z_{2}\times Z_{2}^{\prime} symmetry even after SSB of B−LB-L gauge symmetry. The Z2×Z2′Z_{2}\times Z_{2}^{\prime} discrete symmetry stabilizes the these particles as dark matter candidates. In the model, two classes of inert fermions and scalars with different B−LB-L charges are introduced, leading to two-component dark matter candidates. The lepton flavor violation processes, the relic density of dark matter, the direct detection of dark matter and the phenomenology at LHC are investigated.

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