Principle of neutralino dark matter detection with neutrino telescopes and
predictions are reviewed. The future Antares detector is described. Prospection
in the CMSSM is exposed including comparison with experiment sensitivities of
both neutrino indirect detection and direct detection experiments. Results in
other frameworks are shortly surveyed. Models with a non negligible neutralino
higgsino fraction are promising for neutrino telescopes detection.Comment: Talk given at SUSY02, Desy, Hambourg, Germany June 17-2
