The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial \u3bd\u3bcs with energies between 1011 eV and 10 18 eV, \u3bd\u3bcs emitted from point sources and \u3bd\u3bcs from dark matter annihilation in the Earth and the Sun
