Absolute neutrino mass scale and dark matter stability from flavour symmetry

preprint2023arXivOpen access

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)Σ(81), which can also automatically protect dark matter stability. In addition, Σ(81)Σ(81) leads to striking predictions in the lepton sector: only Inverted Ordering is realised, the absolute neutrino mass scale is predicted to be mlightest≈7.5×10−4m_\text{lightest} \approx 7.5 \times 10^{-4} eV and the Majorana phases are correlated in such a way that ∣mee∣≈0.018|m_{ee}| \approx 0.018 eV. The model also leads to a strong correlation between the solar mixing angle θ12θ_{12} and δCPδ_{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.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.