Using an information-theoretic bound on the halo velocity distribution, dark matter direct-detection limits vary from <10x to ~10,000x near threshold depending on the EFT operator, with higher velocity-weighting operators most affected.
Detecting Cold Dark Matter Candidates
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Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection
Using an information-theoretic bound on the halo velocity distribution, dark matter direct-detection limits vary from <10x to ~10,000x near threshold depending on the EFT operator, with higher velocity-weighting operators most affected.