Search for Supersymmetric Dark Matter in M31 with CELESTE

Details Search for Supersymmetric Dark Matter in M31 with CELESTE Search for Supersymmetric Dark Matter in M31 with CELESTE

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1705n&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Under the assumption that the dark matter is composed of the lightest stable supersymmetric particle, assumed to be the neutralino, the feasibility of its indirect detection by the CELESTE experiment via the observation of a continuous gamma-ray signal due to neutralino annihilation within M31 is examined. The dark matter halo modelling in M31 is addressed and predictions are made in the framework of mSUGRA models.

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