http://arxiv.org/abs/1701.07661
The dark matter spike induced by the adiabatic growth of a massive black hole in a cuspy environment, may explain the thermal dark matter density required to fit the cut-off in the HESSJ1745-290 gamma-ray spectra as TeV dark matter signal with a background component. The spike extension appears comparable with the HESS angular resolution.
V. Gammaldi, V. Avila-Reese, O. Valenzuela, et. al.
Fri, 27 Jan 17
34/54
Comments: 1 page, 1 figure. To appear on the proceedings of LARIM 2016 “XV Latin American Regional IAU Meeting”
You must be logged in to post a comment.