Directional detection of non-baryonic dark matter with MIMAC

Details Directional detection of non-baryonic dark matter with MIMAC Directional detection of non-baryonic dark matter with MIMAC

2010-08-27

arxiv.org/abs/1008.4712v2

Astronomy and Astrophysics

Astrophysics

Instrumentation and Methods for Astrophysics

4 pages, proc. of the 22nd Rencontres de Blois: Particle Physics and Cosmology, 15-20 July 2010, Blois, France

Scientific paper

Directional detection of non-baryonic Dark Matter is a promising search strategy for discriminating genuine WIMP events from background ones. However, carrying out such a strategy requires both a precise measurement of the energy down to a few keV and 3D reconstruction of tracks down to a few mm. To achieve this goal, the MIMAC project has been developed: it is based on a gaseous micro-TPC matrix, filled with 3He, CF4 and/or C4H10. Firsts results of low energy nuclei recoils obtained with a low energy neutron field are presented.

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