# Singlet-Doublet Dirac Dark Matter and Neutrino Masses

## TL;DR

This paper proposes a model extending the Standard Model to include a Dirac dark matter candidate and generate neutrino masses radiatively, analyzing its phenomenology against current experimental constraints.

## Contribution

It introduces a novel singlet-doublet Dirac dark matter model with radiative neutrino mass generation, expanding the viable parameter space beyond Majorana dark matter scenarios.

## Key findings

- Dark matter mass up to 1.1 TeV is viable
- Broader parameter space than Majorana models
- Consistent with direct, indirect, and collider searches

## Abstract

We examine an extension of the Standard Model that addresses the dark matter puzzle and generates Dirac neutrinos masses through the radiative seesaw mechanism. The new field content includes a scalar field that plays an important role in setting the relic abundance of dark matter. We analyze the phenomenology in the light of direct, indirect, and collider searches of dark matter. In this framework, the dark matter candidate is a Dirac particle that is a mixture of new singlet-doublet fields with mass $m_{\chi_1^0}\lesssim 1.1\,\text{TeV}$. We find that the allowed parameter space of this model is broader than the well-known Majorana dark matter scenario.