A comparison between the detection of gamma rays and positrons in Supersymmetric Models

Details A comparison between the detection of gamma rays and positrons in Supersymmetric Models A comparison between the detection of gamma rays and positrons in Supersymmetric Models

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..878...53m&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 2nd International Conference on The Dark Side of the Universe DSU 2006. AIP Conference Proceedin

Computer Science

Dark Matter, Supersymmetric Models

Scientific paper

We present the indirect detection of neutralino dark matter using positrons and gamma rays from its annihilation in the galactic halo. Considering the HESS data as the spectrum constituting the gamma-ray background, we compare the prospects for the experiments GLAST and PAMELA in a general supergravity framework with non-universal scalar and gaugino masses. We show that with a boost factor of about 10, PAMELA will be competitive with GLAST for typical NFW cuspy profiles.

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