Gauged model in light of muon anomaly, neutrino mass and dark matter phenomenology
arXiv:1607.04046 · doi:10.1016/j.nuclphysb.2017.02.010
Abstract
Gauged model has been advocated for a long time in light of muon anomaly, which is a more than discrepancy between the experimental measurement and the standard model prediction. We augment this model with three right-handed neutrinos and a vector-like singlet fermion to explain simultaneously the non-zero neutrino mass and dark matter content of the Universe, while satisfying anomalous muon constraints. It is shown that in a large parameter space of this model we can explain positron excess, observed at PAMELA, Fermi-LAT and AMS-02, through dark matter annihilation, while satisfying the relic density and direct detection constraints.
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