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arXiv · 1112.2926

Dark matter stability from non-Abelian discrete flavor symmetries

E. Peinado
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Abstract

We present a mechanism for the dark matter stability in the framework of a non-Abelian avour symmetry renormalizable model. The same non-abelian discrete avor symmetry which accounts for the observed pattern of neutrino oscillations, spontaneously breaks to a Z2 subgroup which renders DM stable. The simplest scheme leads to a scalar doublet DM potentially detectable in nuclear recoil experiments, inverse neutrino mass hierarchy, hence a neutrinoless double beta decay rate accessible to upcoming searches.

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E. Peinado. 2011-12-13. Dark matter stability from non-Abelian discrete flavor symmetries. https://doi.org/10.1088/1742-6596%2F375%2F1%2F012043

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