Dark matter stability from non-Abelian discrete flavor symmetries

Details Dark matter stability from non-Abelian discrete flavor symmetries Dark matter stability from non-Abelian discrete flavor symmetries

2011-12-13

arxiv.org/abs/1112.2926v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 3 figures. To appear in the TAUP 2011 proceedings

Scientific paper

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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