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It is usually assumed that dark matter direct detection is sensitive to a large fraction of the dark matter (DM) velocity distribution.
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J. Hisano, S. Matsumoto, M. Nagai, O. Saito, and M. Senami, Non-perturbative Effect on Thermal Relic Abundance of Dark Matter
2007
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M. Cirelli, A. Strumia, and M. Tamburini, Cosmology and Astrophysics of Minimal Dark Matter
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2009
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S. Chang, G. D. Kribs, D. Tucker-Smith, and N. Weiner, Inelastic Dark Matter in Light of DAMA/LIBRA
2009
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