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.
CITATION STYLE
Mayet, F., Billard, J., & Santos, D. (2013). Directional detection of galactic dark matter. In Springer Proceedings in Physics (Vol. 148, pp. 117–121). Springer Science and Business Media, LLC. https://doi.org/10.1007/978-94-007-7241-0_18
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