Abstract

We consider the Peccei-Quinn (PQ) mechanism as the one behind the Dirac neutrino masses when these are generated through the $d=5$ effective operator $\bar{L}\tilde{H}N_R\phi$ at one loop level, with $\phi$ being a Standard Model singlet scalar. In this setup, the PQ symmetry guarantees that the one-loop realization of such an effective operator gives the leading contribution to the Dirac neutrino masses by forbidding the contributions arising from its tree level realizations. All the mediators in the one-loop neutrino mass diagrams can be stabilized by a remnant $Z_N$ symmetry from the PQ symmetry breaking, thus forming a dark sector besides the axion sector and leading to mixed axion/WIMP dark matter scenarios.

Highlights

  • In the last decades the neutrino oscillations have been firmly established thanks to a great dedicated experimental program [1], leading to a concise and a clear understanding of the neutrino oscillation pattern [2]

  • It worth noting here that the main motivation for considering weakly interacting massive particle (WIMP) is that they lie at the scale at which the physics beyond the Standard Model (SM) is expected to appear, leading to signals in dedicated experiments looking for dark matter (DM)

  • In this work we have studied the one-loop realizations of the d 1⁄4 5 operator L H NRS that leads to Dirac neutrino masses, with S being a singlet scalar field that hosts the QCD axion

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Summary

INTRODUCTION

In the last decades the neutrino oscillations have been firmly established thanks to a great dedicated experimental program [1], leading to a concise and a clear understanding of the neutrino oscillation pattern [2]. Mechanism [38] to scotogenic models with one-loop Dirac neutrino masses through identification of φ in O5 as the scalar field hosting the QCD axion and the PQ symmetry as responsible for the absence of O4 and the stability of the possible WIMP candidates. It follows that after the spontaneous electroweak and PQ symmetry breaking Dirac neutrino masses will be generated via the O5 operator, and imposing that H does not carry a PQ charge (while L and/or NR do) the contribution to the neutrino masses from the O4 operator is automatically forbidden.

FRAMEWORK
NR þ X X1
RADIATIVE NEUTRINO MASSES AND AXION-WIMP DARK MATTER
A CASE STUDY
SUMMARY
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