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Indirect signals from Dark Matter – Francesc Ferrer

Date: Fri. March 4th, 2005, 11:30 am-12:30 pm
Location: Rockefeller 221

Abstract: The only evidence so far for the presence of Dark Matter in our Galaxy is through its gravitational interactions. Several experiments, however, have recently observed the emission of gamma-rays from the Galactic Center that could be caused by the annihilation of Dark Matter particles. Candidates with masses ranging from the MeV to the ZeV will be explored and constraints on their properties will be obtained by requiring that they account for the observed Galactic radiation.

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