Abstract

The appealing feature of inverse seesaw models is that the Standard Model (SM) neutrino mass emerges from the exchange of TeV scale singlets with sizable Yukawa couplings, which can be tested at colliders. However, the tiny Majorana mass splitting between TeV singlets, introduced to accommodate small neutrino masses, is left unexplained. Moreover, we argue that these models suffer from a structural limitation that prevents a successful leptogenesis if one insists on having unsuppressed Yukawa couplings and TeV scale singlets. In this work we propose a hybrid seesaw model, where we replace the mass splitting with a coupling to a high scale seesaw module including a TeV scalar. We show that this structure achieves the goal of filling both the above gaps with couplings of order unity. The necessary structure automatically arises embedding the seesaw mechanism in composite Higgs models, but may also be enforced by new gauge symmetries in a weakly-coupled theory. Our hybrid seesaw models have distinguishing features compared to the standard high scale type-I seesaw and inverse seesaw. Firstly, they have much richer phenomenology. Indeed, they generally predict new TeV scale physics (including scalars) potentially accessible at present and future colliders, whereas weakly-coupled versions may also have cosmological signature due to the presence of a light Nambu–Goldstone boson coupled to neutrinos. Secondly, our scenario features an interesting interplay between high scale and TeV scale physics in leptogenesis and enlarges the range of allowed high scale singlet masses beyond the usual ∼109–1015GeV, without large hierarchies in the Yukawa couplings nor small mass splitting among the singlets.

Highlights

  • The seesaw mechanism [1] elegantly explains the extreme smallness of the Standard Model (SM) neutrino masses

  • If for definiteness we focus on the strong washout region, in which KΨeff 1, the net lepton asymmetry can be obtained as3

  • The characteristic structure in eq (8) may be enforced introducing a U (1)B−L × U (1)X gauge symmetry [9]. In the simplest such realization, N appears in two generations, which coincides with the minimal number of generations necessary to obtain a realistic neutrino mass matrix

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Summary

Introduction

The seesaw mechanism [1] elegantly explains the extreme smallness of the SM neutrino masses. The Majorana nature of SM neutrino, i.e., the presence of leptonnumber violation, raises the highly attractive possibility of baryogenesis via leptogenesis [2, 3]. We consider a class of seesaw models called inverse seesaw [4]. We first emphasize two inadequacies of the standard inverse seesaw scenario and build an extended framework, which we will term hybrid seesaw, to overcome both issues

Inverse seesaw: μ-problem and leptogenesis
A hybrid seesaw model
Solution to the μ-problem
A two-step leptogenesis
Present-day asymmetry
Enlarging the MN window
Constraints and signatures
Constraints and signatures on fully-symmetric models
Outlook
Full Text
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