Dirac dark matter, neutrino masses, and dark baryogenesis
Abstract
We present a gauged baryon number model as an example of models where all new fermions required to cancel out the anomalies help to solve phenomenological problems of the standard model (SM). Dark fermion doublets, along with the iso-singlet charged fermions, in conjunction with a set of SM-singlet fermions, participate in the generation of small neutrino masses through the Dirac-dark Zee mechanism. The other SM-singlets explain the dark matter in the Universe, while their coupling to an inert singlet scalar is the source of the violation. In the presence of a strong first-order electroweak phase transition, this "dark" violation allows for a successful electroweak baryogenesis mechanism.
Keywords
Cite
@article{arxiv.2205.05762,
title = {Dirac dark matter, neutrino masses, and dark baryogenesis},
author = {Diego Restrepo and Andrés Rivera and Walter Tangarife},
journal= {arXiv preprint arXiv:2205.05762},
year = {2022}
}
Comments
22 pages, 6 figures. Comments are welcome! v.3 matches the published version