Astrophysical uncertainties in dark matter halo models produce O(1% to 100%) fractional deviations in predicted single-phonon rates, but can be captured by parameter variations within the Standard Halo Model after rms-matching.
Phys. Rev. Lett. 123 (2019) 151802 [arXiv:1903.05101]. Y. Hochberg, et al.,\New Constraints on Dark Matter from Supercon- ducting Nanowires
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