Abstract

The radiative neutrino mass model can relate neutrino masses and dark matter at a TeV scale. If we apply this model to thermal leptogenesis, we need to consider resonant leptogenesis at that scale. It requires both finely degenerate masses for the right-handed neutrinos and a tiny neutrino Yukawa coupling. We propose an extension of the model with a U(1) gauge symmetry, in which these conditions are shown to be simultaneously realized through a TeV scale symmetry breaking. Moreover, this extension can bring about a small quartic scalar coupling between the Higgs doublet scalar and an inert doublet scalar which characterizes the radiative neutrino mass generation. It also is the origin of the $Z_2$ symmetry which guarantees the stability of dark matter. Several assumptions which are independently supposed in the original model are closely connected through this extension.

Highlights

  • ATLAS and CMS groups in the LHC experiment have reported the discovery of the Higgs-like particle [1,2]

  • We show that (i) both the almost degenerate right-handed neutrino masses and a tiny neutrino Yukawa coupling, which are indispensable for TeV scale resonant leptogenesis [37–40], are brought about after the breaking of this symmetry

  • We have considered an extension of the radiative neutrino mass model proposed by Ma with a low energy U (1) gauge symmetry

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Summary

Introduction

ATLAS and CMS groups in the LHC experiment have reported the discovery of the Higgs-like particle [1,2]. The existence of neutrino masses and dark matter has been confirmed through various experiments and observations [3–14], it cannot be explained in the standard model. The standard model cannot give a framework for the generation of baryon number asymmetry in the Universe, either [15–17]. A Yukawa coupling of the lightest right-handed neutrino becomes much smaller than that of the heavier one To realize this scenario, we introduce a low energy U (1) gauge symmetry to the model. We find that this extension can explain important key features required in the original Ma model, that is, (ii) a small quartic coupling between the Higgs doublet scalar and an inert doublet scalar which plays a crucial role in the neutrino mass generation, and (iii) the origin of the Z2 symmetry which guarantees the stability of dark matter.

An extended model
Scalar sector
Degenerate right-handed neutrinos
Resonant leptogenesis
Relic abundance and detection of dark matter
Cosmological signal
Findings
Conclusion
Full Text
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