Absolute neutrino mass scale and dark matter stability from flavour symmetry
Abstract
We explore a simple but extremely predictive extension of the scotogenic model. We promote the scotogenic symmetry to the flavour non-Abelian symmetry , which can also automatically protect dark matter stability. In addition, leads to striking predictions in the lepton sector: only Inverted Ordering is realised, the absolute neutrino mass scale is predicted to be eV and the Majorana phases are correlated in such a way that eV. The model also leads to a strong correlation between the solar mixing angle and , which may be falsified by the next generation of neutrino oscillation experiments. The setup is minimal in the sense that no additional symmetries or flavons are required.
Keywords
Cite
@article{arxiv.2204.12517,
title = {Absolute neutrino mass scale and dark matter stability from flavour symmetry},
author = {Salvador Centelles Chuliá and Ricardo Cepedello and Omar Medina},
journal= {arXiv preprint arXiv:2204.12517},
year = {2023}
}
Comments
19 pages, 6 figures, 1 Table. v2: Additional comments about flavour symmetry breaking, FCNCs, and dark matter were added, also an Appendix concerning the scalar sector was included. This document matches the published version