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Highlights on gamma rays, neutrinos and antiprotons from TeV Dark Matter

By Gammaldi Viviana


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

Topics: Physics, QC1-999
Publisher: EDP Sciences
Year: 2016
DOI identifier: 10.1051/epjconf
OAI identifier: oai:doaj.org/article:0b7a7e9cdd394fab8ade7eaac7e532f9
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