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arXiv · 1412.7639

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

Viviana Gammaldi
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Abstract

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.

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Viviana Gammaldi. 2014-12-24. Highlights on gamma rays, neutrinos and antiprotons from TeV Dark Matter. https://arxiv.org/abs/1412.7639

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