http://arxiv.org/abs/1412.7639
It has been shown that the gamma-ray flux observed by HESS from the J1745-290 Galactic Center source is well fitted as the secondary gamma-rays photons generated from Dark Matter annihilating into Standard Model particles in combination with a simple power law background. The neutrino flux expected from such Dark Matter source has been also analyzed. The main results of such analyses for 50 TeV Dark Matter annihilating into W+W- gauge boson and preliminary results for antiprotons are presented.
V. Gammaldi
Thu, 25 Dec 14
25/29
Comments: 5 pages, 3 figures, To appear on the proceeding of RICAP-14 “The Roma International Conference on Astroparticle Physics”
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