Indirect Search for Dark Matter with the ANTARES Neutrino Telescope

Indirect search for Dark Matter trapped inside celestial bodies is one of the main physics goals of neutrino telescopes. The expected sensitivity of ANTARES with its data recorded in 2007 and 2008 to detect the flux of neutrinos originating from Dark Matter annihilations inside the Sun is presented. A comparison to current limits coming from direct detection experiments and other indirect detection experiments is shown with regards to the predictions of popular models such as the CMSSM and the Minimal Universal Dimension model.