Directional detection of galactic 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 that may be a powerful tool to identify genuine WIMP events as such. Directional detection strategy 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. 
F. Mayet (1), J. Billard (1) and D. Santos (1) ((1) LPSC Grenoble)
astro-ph.CO