Gamma-Ray Excess and the Minimal Dark Matter Model
arXiv:1510.07562 · doi:10.1007/JHEP06(2016)008
Abstract
We point out that the gamma-ray excesses in the galactic center and in the dwarf galaxy Reticulum II can both be well explained within the simplest dark matter model. We find that the corresponding region of parameter space will be tested by direct and indirect dark matter searches in the near future.
6 pages, 8 figures; v2: new LUX bounds included, to appear in JHEP