  Dark matter detection experiments are getting ever closer to the sensitivity
needed to detect the primary particle physics candidates for nonbaryonic dark
matter. Indirect detection methods include searching for antimatter and gamma
rays, in particular gamma ray lines, in cosmic rays and high-energy neutrinos
from the centre of the Earth or Sun caused by accretion and annihilation of
dark matter particles. A review is given of recent progress, both on the
theoretical and experimental sides.
