Abstract
Under current LHC and dark matter constraints, the general NMSSM can have self-interacting dark matter to explain the cosmological small structure. In this scenario, the dark matter is the light singlino-like neutralino () which self-interacts through exchanging the light singlet-like scalars (). These light scalars and neutralinos inevitably interact with the 125 GeV SM-like Higgs boson (), which cause the Higgs exotic decays . We first demonstrate the parameter space required by the explanation of the cosmological small structure and then display the Higgs exotic decays. We find that in such a parameter space the Higgs exotic decays can have branching ratios of a few percent, which should be accessible in the future colliders.
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