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Several direct detection experiments, including recently CDMS-II, havereported signals consistent with 5 to 10 GeV dark matter (DM) that appear to bein tension with null results from XENON and LUX experiments; these indicate acareful review of the theoretical basis, including the galactic DM velocitydistribution function (VDF). We establish a VDF parameter space from DM-onlycosmological simulations and illustrate that seemingly contradictoryexperimental results can be made consistent within this parameter space. Futureexperimental limits should be reported after they are marginalized over a rangeof VDF parameters.

Connecting Direct Dark Matter Detection Experiments to Cosmologically Motivated Halo Models