English

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

High Energy Physics - Phenomenology 2015-11-05 v2

Abstract

In this paper we propose a radiated linear seesaw model where the naturally small term μL\mu_{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 BLB-L charges for new particles are assigned to satisfy the anomalies cancelation. It is founded that some new particles may have exotic values of BLB-L charge such that there exists residual Z2×Z2Z_{2}\times Z_{2}^{\prime} symmetry even after SSB of BLB-L gauge symmetry. The Z2×Z2Z_{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 BLB-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.

Keywords

Cite

@article{arxiv.1508.00706,
  title  = {Radiative Linear Seesaw model, Dark Matter and $U(1)_{B-L}$},
  author = {Weijian Wang and Zhi-Long Han},
  journal= {arXiv preprint arXiv:1508.00706},
  year   = {2015}
}

Comments

23 pages, 13 figures, more discussions and references are added, published in PRD

R2 v1 2026-06-22T10:25:51.403Z