Location of Repository

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

By Gammaldi Viviana

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

Topics: Physics, QC1-999
Publisher: EDP Sciences
Year: 2016
DOI identifier: 10.1051/epjconf
OAI identifier: oai:doaj.org/article:0b7a7e9cdd394fab8ade7eaac7e532f9
Journal:
Download PDF:
Sorry, we are unable to provide the full text but you may find it at the following location(s):
  • https://doaj.org/toc/2100-014X (external link)
  • http://dx.doi.org/10.1051/epjc... (external link)
  • https://doaj.org/article/0b7a7... (external link)
  • Suggested articles


    To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.