Revisiting the model for radiative neutrino masses with dark matter in the $\mathrm{U(1)}_{B-L}$ gauge theory

TL;DR

This paper reevaluates a radiative neutrino mass model with dark matter within a gauged U(1)_{B-L} framework, considering recent experimental constraints and identifying viable parameter regions and testable scenarios.

Contribution

It provides updated analysis of the model's parameter space, introducing new benchmark scenarios compatible with current constraints and discussing their potential testability.

Findings

Allowed parameter regions under latest constraints

New benchmark scenarios for neutrino and scalar dark matter

Potential for future experimental verification

Abstract

The radiative seesaw model with gauged $\mathrm{U(1)}_{B-L}\times\mathbb{Z}_2$ extension is a well-motivated scenario which gives consistent predictions of active neutrino masses and the abundance of dark matter. Majorana masses of right-handed neutrinos, the lightest of which can be identified as dark matter, are given by the spontaneous breaking of the $\mathrm{U(1)}_{B-L}$ gauge symmetry. We revisit this model with the latest constraints from dark matter searches, neutrino oscillations, flavor experiments and collider experiments. We explore the feasible parameter space of this model, and find that there are still allowed regions under the latest experimental constraints. We present new viable benchmark scenarios for this model, i.e., the right-handed neutrino dark matter scenario and the scalar dark matter scenario. We also mention the testability of these benchmark scenarios at future experiments.