A Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment
N. Du, N. Force, R. Khatiwada, E. Lentz, R. Ottens, L. J Rosenberg, G., Rybka, G. Carosi, N. Woolett, D. Bowring, A. S. Chou, A. Sonnenschein, W., Wester, C. Boutan, N.S. Oblath, R. Bradley, E. J. Daw, A. V. Dixit, J., Clarke, S. R. O'Kelley, N. Crisosto, J. R. Gleason, S. Jois

TL;DR
This paper reports a haloscope experiment that searches for invisible axion dark matter within a specific mass range, achieving unprecedented sensitivity and excluding certain theoretical models of axion-photon coupling.
Contribution
The study introduces a highly sensitive haloscope setup operating at sub-kelvin temperatures, enabling the exclusion of axion-photon couplings predicted by plausible invisible axion models.
Findings
Excluded axion-photon coupling range for 2.66-2.81 μeV mass
Achieved sensitivity surpassing previous experiments
Operated at sub-kelvin temperatures to reduce noise
Abstract
This Letter reports results from a haloscope search for dark matter axions with masses between 2.66 and 2.81 eV. The search excludes the range of axion-photon couplings predicted by plausible models of the invisible axion. This unprecedented sensitivity is achieved by operating a large-volume haloscope at sub-kelvin temperatures, thereby reducing thermal noise as well as the excess noise from the ultra-low-noise SQUID amplifier used for the signal power readout. Ongoing searches will provide nearly definitive tests of the invisible axion model over a wide range of axion masses.
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