Constraints on axionlike dark matter with masses down to 10-23 eV/c2

Abstract

We analyzed an 6.7-year span of data from a rotating torsion-pendulum containing ≈ 1023 polarized electrons to search for the "wind" arising from ultralight, axionlike dark matter with masses between 10-23 and 10-18 eV/c2. Over most of this range we obtain a 95\% confidence limit F a/C e ≥ 1 × 1015 eV on the axionlike decay constant.

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