Publication Date:
2018-08-30
Description:
Galaxies, Vol. 6, Pages 92: Relieving Tensions Related to the Dark Matter Interpretation of the Fermi-LAT Data Galaxies doi: 10.3390/galaxies6030092 Authors: Man Ho Chan 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.
Electronic ISSN:
2075-4434
Topics:
Physics
