English

Absolute neutrino mass scale and dark matter stability from flavour symmetry

High Energy Physics - Phenomenology 2023-01-10 v2

Abstract

We explore a simple but extremely predictive extension of the scotogenic model. We promote the scotogenic symmetry Z2\mathbb{Z}_2 to the flavour non-Abelian symmetry Σ(81)\Sigma(81), which can also automatically protect dark matter stability. In addition, Σ(81)\Sigma(81) leads to striking predictions in the lepton sector: only Inverted Ordering is realised, the absolute neutrino mass scale is predicted to be mlightest7.5×104m_\text{lightest} \approx 7.5 \times 10^{-4} eV and the Majorana phases are correlated in such a way that mee0.018|m_{ee}| \approx 0.018 eV. The model also leads to a strong correlation between the solar mixing angle θ12\theta_{12} and δCP\delta_{CP}, 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