Dark Higgs Channel for FERMI GeV γγ-ray Excess

preprint2016arXivOpen access

Abstract

Dark Higgs is very generic in dark matter models where DM is stabilized by some spontaneously broken dark gauge symmetries. Motivated by the FERMI observation of ∼\simGeV scale γγ-ray excess from the galactic center (GC), we investigate a scenario that a pair of dark matter XX annihilates into a pair of dark Higgs H2H_2, which subsequently decays into standard model particles through its mixing with SM Higgs boson. Besides the two-body decay of H2H_2, we also include multibody decay channels of the dark Higgs. We find that the best-fit point is around MX≃95.0M_X\simeq 95.0GeV, MH2≃86.7M_{H_2}\simeq 86.7GeV, ⟨σv⟩≃4.0×10−26cm3/s\langle σv\rangle\simeq 4.0\times 10^{-26}\textrm{cm}^3\textrm{/s} and gives a p-value ≃0.40\simeq 0.40. Implication of this result is described in the context of dark matter models with dark gauge symmetries. Since such a dark Higgs boson is very difficult to produce at colliders, indirect DM detections of cosmic γγ-rays could be an important probe of dark sectors, complementary to collider searches.

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