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

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arxiv 1609.01018 v2 pith:32JIXUL2 submitted 2016-09-05 hep-ph

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

classification hep-ph
keywords higgsregionsignaturesbenchmarkconstraintsdarkdetectiondirect
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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 $M_{s_1}$ that can survive the present and even the future experiments: (1) the Higgs resonance region with $M_{s_1}\sim M_h/2$, (2) the Higgs region with $M_{s_1}\sim M_h$, and (3) the coannihilation region with $M_{s_2}\sim M_{s_1}$. Here $s_{1,2}$ are two scalar singlets with the lighter $s_1$ 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 $5\sigma$ significance with an integrated luminosity of 100/fb.

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