Direct and Indirect Detection of Dark Matter in D6 Flavor Symmetric Model
arXiv:1104.0367 · doi:10.1140/epjc/s10052-011-1688-0
Abstract
We study a fermionic dark matter in a non-supersymmetric extension of the standard model with a family symmetry based on D6xZ2xZ2. In our model, the final state of the dark matter annihilation is determined to be e+ e- by the flavor symmetry, which is consistent with the PAMELA result. At first, we show that our dark matter mass should be within the range of 230 GeV - 750 GeV in the WMAP analysis combined with mu to e gamma constraint. Moreover we simultaneously explain the experiments of direct and indirect detection, by simply adding a gauge and D6 singlet real scalar field. In the direct detection experiments, we show that the lighter dark matter mass ~ 230 GeV and the lighter standard model Higgs boson ~ 115 GeV is in favor of the observed bounds reported by CDMS II and XENON100. In the indirect detection experiments, we explain the positron excess reported by PAMELA through the Breit-Wigner enhancement mechanism. We also show that our model is consistent with no antiproton excess suggested by PAMELA.
20 pages, 9 figures, 2 tables, accepted version for publication in European Physical Journal C
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- Direct Detection of Leptophilic Dark Matter in a Model with Radiative Neutrino Masses
- Connecting neutrino physics with dark matter
- 3.5 keV X-ray Line Signal from Decay of Right-Handed Neutrino due to Transition Magnetic Moment
- Super Flavorsymmetry with Multiple Higgs Doublets
- Revisiting Discrete Dark Matter Model:θ_{13}\neq0 and ν_{R} Dark Matter
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