Search for axion-like dark matter using solid-state nuclear magnetic resonance
Deniz Aybas, Janos Adam, Emmy Blumenthal, Alexander V. Gramolin,, Dorian Johnson, Annalies Kleyheeg, Samer Afach, John W. Blanchard, Gary P., Centers, Antoine Garcon, Martin Engler, Nataniel L. Figueroa, Marina Gil, Sendra, Arne Wickenbrock, Matthew Lawson, Tao Wang, Teng Wu

TL;DR
This study uses solid-state nuclear magnetic resonance to search for ultralight axion-like dark matter, setting new bounds on its interaction parameters within a specific mass range, and demonstrating the method's feasibility.
Contribution
The paper introduces a novel application of solid-state NMR for detecting axion-like dark matter and provides the first experimental bounds in this mass and frequency range.
Findings
Set upper bounds on axion-like couplings $g_d$ and $g_{aNN}$.
Calibrated the NMR detector and characterized nuclear spin properties.
Demonstrated the feasibility of using solid-state NMR for dark matter searches.
Abstract
We report the results of an experimental search for ultralight axion-like dark matter in the mass range 162 neV to 166 neV. The detection scheme of our Cosmic Axion Spin Precession Experiment (CASPEr) is based on a precision measurement of Pb solid-state nuclear magnetic resonance in a polarized ferroelectric crystal. Axion-like dark matter can exert an oscillating torque on Pb nuclear spins via the electric-dipole moment coupling , or via the gradient coupling . We calibrated the detector and characterized the excitation spectrum and relaxation parameters of the nuclear spin ensemble with pulsed magnetic resonance measurements in a 4.4 T magnetic field. We swept the magnetic field near this value and searched for axion-like dark matter with Compton frequency within a 1 MHz band centered at 39.65 MHz. Our measurements place the upper bounds…
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