Hypothesis
Ultralow-mass axion-like dark matter would induce an oscillating neutron electric dipole moment or an axion-wind spin-precession effect visible in the ratio of ultracold-neutron and ¹⁹⁹Hg precession frequencies.
What failed
No signal consistent with dark matter was observed for axion masses from 10⁻²⁴ to 10⁻¹⁷ eV.
Broken assumption
Axion-like dark matter in this mass range couples to nucleons or gluons strongly enough to show up in spin-precession measurements.
Why
No signal was present at the experiment's sensitivity; the null result sets the first laboratory limits on axion–gluon coupling, up to 1,000 times tighter than astrophysical limits.
From the published paper: Abel et al. reroDoc Digital Library, 2017. ↗CC BY