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The most recent results from direct searches for dark matter particles in the galactic halo are examined in terms of an effective Minimal Supersymmetric extension of the Standard Model at the electroweak scale without gaugino masses unification.
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The class of models discussed in Ref. bcfs represents a quite exhaustive summary of dark matter distributions functions as possible departures from the isothermal sphere model. Notice, however, that it does not include the possibility of non–thermal components in the f ( v → ) f(\vec{v}) , which could in principle modify the high–velocity tail of the velocity DF (see for instance: A. Helmi, S.D.M. White, V. Springel, Phys. Rev. D 66
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For a general overview about experiments for direct detection of relic particles, see, for instance, the review talks given by P. Belli and by G. Gerbier (D. Bauer) at TAUP 2007, Sendai, Japan, September 2007 and the contributions presented in the relevant Workshop sessions at the same Conference (see: http://www.awa.tohoku.ac.jp/taup2007/ and forthcoming proceedings)
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