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- W2115571128 abstract "The anomalies in positron fraction observed in PAMELA and total flux of electrons and positron reported by Fermi can be explained by a decaying dark matter. The agreement between astrophysical background and observed data in anti-proton indicates a lep-tophilic dark matter and constrains the hadronic decay branching ratios. In this work, we study the constrains on decaying rates of a dark matter to various 2-body final states using the Fermi and HESS gamma-ray data. We find that µ + µ - or τ + τ - final state is preferred to simultaneously explain the excesses and meet the gamma-ray constrains." @default.
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- W2115571128 date "2010-04-20" @default.
- W2115571128 modified "2023-10-02" @default.
- W2115571128 title "GAMMA-RAY CONSTRAINTS ON DECAYING DARK MATTER" @default.
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- W2115571128 doi "https://doi.org/10.1142/s0217732310000125" @default.
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