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The recent WMAP data have confirmed that exotic dark matter together with thevacuum energy (cosmological constant) dominate in the flat Universe. The natureof the dark matter constituents cannot be determined till they are directlydetected. Recent developments in particle physics provide a number ofcandidates as constituents of dark matter, called Weakly Interacting MassiveParticles (WIMPs). Since these interact weakly and are of low energy theycannot excite the target and can only be detected via measuring the recoilingnucleus. For all WIMPs, including the most popular candidate, the lightestsupersymmetric particle (LSP), the relevant cross sections arise out of thefollowing mechanisms: i) The coherent mode, due to the scalar interaction. ii)The charge coherent mode, with only proton contribution, as in the recent caseof secluded dark matter scenario and iii) The spin contribution arising fromthe axial current. In this paper we will focus on the spin contribution, whichmaybe important, especially for light targets.

Searching for Dark Matter- Theoretical Rates and Exclusion Plots due to the Spin