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arXiv · 1204.4733

Predictive Discrete Dark Matter Model

M. S. Boucenna·S. Morisi·E. Peinado·Y. Shimizu·J. W. F. Valle
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Abstract

Dark Matter stability can be achieved through a partial breaking of a flavor symmetry. In this framework we propose a type-II seesaw model where left-handed matter transforms nontrivially under the flavor group Delta(54), providing correlations between neutrino oscillation parameters, consistent with the recent Daya-Bay and RENO reactor angle measurements, as well as lower bounds for neutrinoless double beta decay. The dark matter phenomenology is provided by a Higgs-portal.

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M. S. Boucenna, S. Morisi, E. Peinado, Y. Shimizu, J. W. F. Valle. 2012-06-28. Predictive Discrete Dark Matter Model. https://doi.org/10.1103/physrevd.86.073008

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