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The halo independent comparison of direct dark matter detection dataeliminates the need to make any assumption on the uncertain local dark matterdistribution and is complementary to the usual data comparison which requiredassuming a dark halo model for our galaxy. The method, initially proposed forWIMPs with spin-independent contact interactions, has been generalized to anyother interaction and applied to recent data on "Light WIMPs".

Halo-Independent analysis of direct dark matter detection data for any WIMP interaction