  The ANTARES neutrino telescope was completed in 2008 with the installation of
its twelfth line. Its scientific scope is very broad, but the two main goals
are the observation of astrophysical sources and the indirect detection of dark
matter. The latter is possible through neutrinos produced after the
annihilation of WIMPs, which would accumulate in sources like the Sun, the
Earth or the Galactic Centre. The neutralino, which arises in Supersymmetry
models, is one of the most popular WIMP candidates. KK particles, which appear
in Universal Extra Dimension models, are another one. Though in most models
these annihilations would not directly produce neutrinos, they are expected
from the decay of secondary particles. An important advantage of neutrino
telescopes with respect to other indirect searches (like gamma rays or cosmic
rays) is that a potential signal (for instance from the Sun) would be very
clean, since no other astrophysical explanations could mimic it (like pulsars
for the case of the positron excess seen by PAMELA). Moreover, the Galactic
Centre is accessible for ANTARES, being in the Northern Hemisphere. In this
talk I will present the results of the ANTARES telescope for dark matter
searches, which include neutralino and KK particles.
