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The MIMAC project aims to provide a nominal fluorine detector for directionaldetection of galactic dark matter recoil events. Its expected behavior reachesan important part of the predicted spin dependent elastic scatteringinteractions of the supersymmetric neutralino with protons. Hence, theparameter space in the MSSM and the NMSSM models with neutralino dark mattercould be probed by such experimental efforts. In particular, a good sensitivityto spin dependent interactions tackles parameter space regions to which thepredictions on spin independent interactions and indirect signatures are farbelow current and projected experiments.

MIMAC potential discovery and exclusion of neutralinos in the MSSM and NMSSM