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Mirror dark matter offers a framework to explain the existing dark matterdirect detection experiments. Here we confront this theory with the most recentexperimental data, paying attention to the various known systematicuncertainties, in quenching factor, detector resolution, galactic rotationalvelocity and velocity dispersion. We perform a detailed analysis of the DAMAand CoGeNT experiments assuming a negligible channeling fraction and find thatthe data can be fully explained within the mirror dark matter framework. Wealso show that the mirror dark matter candidate can explain recent data fromthe CDMS/Ge, EdelweissII and CRESSTII experiments and we point out ways inwhich the theory can be further tested in the near future.

A comprehensive analysis of the dark matter direct detection experiments in the mirror dark matter framework