Testing Type II Radiative Seesaw Model: from Dark Matter Detection to LHC Signatures

preprint2016arXivOpen access

Abstract

We analyse the testability of the type II radiative seesaw in which neutrino mass and dark matter (DM) are related at one-loop level. Under the constraints from DM relic density, direct and indirect detection, and invisible Higgs decays, we find three possible regions of DM mass Ms1M_{s_1} that can survive the present and even the future experiments: (1) the Higgs resonance region with Ms1∼Mh/2M_{s_1}\sim M_h/2, (2) the Higgs region with Ms1∼MhM_{s_1}\sim M_h, and (3) the coannihilation region with Ms2∼Ms1M_{s_2}\sim M_{s_1}. Here s1,2s_{1,2} are two scalar singlets with the lighter s1s_1 being the DM candidate. Based on DM properties and direct collider constraints, we choose three benchmark points to illustrate the testability of this model at LHC. We perform a detailed simulation of the four-lepton and tri-lepton signatures at 13 (14) TeV LHC. While both signatures are found to be promising at all benchmark points, the tri-lepton one is even better: it is possible to reach the 5σ5σ significance with an integrated luminosity of 100/fb.

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