@Article{CentellesChulia_etal2022,
author="Centelles Chulia, S.
and Cepedello, R.
and Medina, O.",
title="Absolute neutrino mass scale and dark matter stability from flavour symmetry",
journal="Journal of High Energy Physics",
year="2022",
publisher="Springer",
volume="10",
number="10",
pages="080--23pp",
optkeywords="Discrete Symmetries; Flavour Symmetries; Neutrino Mixing; Particle Nature of Dark Matter",
abstract="We explore a simple but extremely predictive extension of the scotogenic model. We promote the scotogenic symmetry Z(2) to the flavour non-Abelian symmetry sigma(81), which can also automatically protect dark matter stability. In addition, sigma(81) leads to striking predictions in the lepton sector: only Inverted Ordering is realised, the absolute neutrino mass scale is predicted to be m(lightest)approximate to 7.5x10(-4) eV and the Majorana phases are correlated in such a way that vertical bar m(ee)vertical bar approximate to 0.018 eV. The model also leads to a strong correlation between the solar mixing angle theta(12) and 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.",
optnote="WOS:000867661300002",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=5387), last updated on Mon, 24 Oct 2022 07:04:22 +0000",
issn="1029-8479",
doi="10.1007/JHEP10(2022)080",
opturl="https://arxiv.org/abs/2204.12517",
opturl="https://doi.org/10.1007/JHEP10(2022)080",
language="English"
}