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Proposed dark matter detectors with eV-scale sensitivities will detect alarge background of atomic (nuclear) recoils from coherent photon scattering.This background climbs steeply below $\sim10$~eVnr, far exceeding the decliningrate of low-energy Compton recoils. The upcoming generation of dark matterdetectors will not be limited by this background, but further development ofeV-scale and sub-eV detectors will require the use of low-$Z$ target materials,such as helium, to avoid a large rate of coherent photon scattering, or highlyefficient methods to reject photons when they scatter.

The coherent photon scattering background in sub-GeV/$c^2$ direct dark matter searches