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We discuss first a method of measuring $\tau$ polarisation at the ILC usingthe 1--prong hadronic decays of the $\tau$. We then show in this contributionhow a study of the $\tilde \tau$ sector and particularly use of decay $\tau$polarisation can offer a very good handle for distinguishing between mSUGRA anda SUSY-GUT scenario, both of which can give rise to appropriate Dark Matter.

Distinguishing SUSY scenarios using \tau polarisation and \tilde\chi^0_1 Dark Matter