Directional detection of Dark Matter
  Directional detection is a promising Dark Matter search strategy. Taking
advantage on the rotation of the Solar system around the galactic center
through the Dark Matter halo, it allows to show a direction dependence of WIMP
events. It requires the simultaneous measurement of the energy and the 3D track
of low energy recoils, which is a common challenge for all current projects of
directional detectors. The third CYGNUS workshop on directional dark matter
detection has brought together the scientific community working on both
theoretical and experimental aspects of the subject. In this paper, we give an
introductory revue of directional detection of Dark Matter, focusing on the
main recent progresses.
