Prospects for the search of supersymmetric dark matter with HESS

Details Prospects for the search of supersymmetric dark matter with HESS Prospects for the search of supersymmetric dark matter with HESS

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003idm..conf..513g&link_type=abstract

THE IDENTIFICATION OF DARK MATTER. Proceedings of the Fourth International Workshop. Held 2 - 6 September 2002 in York, UK. Edit

Physics

Dark Matter, Experiments, Detection

Scientific paper

The H.E.S.S. sensitivity is presented for the first telescope already operating in Namibia and for the four telescopes of phase 1 that will take data in 2004. Located in the southern hemisphere at a latitude of 22 degrees, HESS can look at the galactic centre and many galactic sources. Its sensitivity to a point source at Zenith is 10-11 cm2.s-1 for an integrated spectrum above a threshold of 150 GeV for the first telescope and 2×10-11 cm2.s-1 above 80 GeV for four telescopes. We discuss the potential of HESS to detect γ-ray emission from neutralino annihilation at the galactic centre for several halos models and for the globular cluster Omega Centauri using a semi-analytical dynamical model. We scan supersymetric models in the CMSSM framework with the help of SUSPECT and DARKSUSY.

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