Highlights on gamma rays, neutrinos and antiprotons from TeV Dark Matter
  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. 
Viviana Gammaldi
astro-ph.HE astro-ph.CO hep-ph