Natural explanation for 130 GeV photon line within vector boson dark matter model

preprint2013arXivOpen access

Abstract

We present a dark matter model for explaining the observed 130 GeV photon line from the galaxy center. The dark matter candidate is a vector boson of mass mVm_V with a dimensionless coupling to the photon and ZZ boson. The model predicts a double line photon spectrum at energies equal to mVm_V and mV(1−mZ2/4mV2)m_V(1-m_Z^2/4m_V^2) originating from the dark matter annihilation. The same coupling leads to a mono-photon plus missing energy signal at the LHC. The entire perturbative parameter space can be probed by the 14 TeV LHC run. The model has also a good prospect of being probed by direct dark matter searches as well as the measurement of the rates of h→γγh \to γγ and h→Zγh \to Z γ at the LHC.

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