Dark matter searches with H.E.S.S.

Details Dark matter searches with H.E.S.S. Dark matter searches with H.E.S.S.

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1223..140o&link_type=abstract

SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA-RAY EXPERIMENTS: Proceedings of the 7th Workshop on Gamma-Ray Physics in th

Physics

Astronomical Telescopes, Dark Matter, Clusters Of Galaxies, Galactic Centre, Black Holes, Radio Galaxies, X- And Gamma-Ray Telescopes And Instrumentation, Dark Matter, Small And Compact Galaxy Groups, Galactic Halo, Galactic Center, Bar, Circumnuclear Matter, And Bulge, Radio Galaxies

Scientific paper

Astrophysical observations require the existence of non-baryonic dark matter (DM). If the dark matter particle has a mass in the TeV range and decays or annihilates via the weak interaction, very high energy (VHE) γ-ray telescopes like H.E.S.S., MAGIC and VERITAS are well-suited to search for dark matter signals, as photons produced in dark matter annihilations allow directional back-tracking to their source. Dark matter searches and related observations performed by the H.E.S.S. collaboration are summarized here.

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