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- W2889404772 abstract "Recently, many studies indicate that the GeV gamma ray excess signal from the central Milky Way can be best explained by ∼40–50 GeV dark matter annihilating via the b b ¯ channel. However, this model appears to be disfavored by the recent Fermi-LAT data for dwarf spheroidal galaxies and the constraint from synchrotron radiation. In this article, we describe a consistent picture to relieve the tensions between the dark matter annihilation model and the observations. We show that a baryonic feedback process is the key to alleviate the tensions and the ∼40–50 GeV dark matter model is still the best one to account for the GeV gamma ray excess in the Milky Way." @default.
- W2889404772 created "2018-09-07" @default.
- W2889404772 creator A5061543393 @default.
- W2889404772 date "2018-08-29" @default.
- W2889404772 modified "2023-10-01" @default.
- W2889404772 title "Relieving Tensions Related to the Dark Matter Interpretation of the Fermi-LAT Data" @default.
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- W2889404772 doi "https://doi.org/10.3390/galaxies6030092" @default.
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