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This Letter reports on a cavity haloscope search for dark matter axions in the Galactic halo in the mass range 2.81-3.31 μeV. This search utilizes the combination of a low-noise Josephson parametric amplifier and a large-cavity haloscope to achieve unprecedented sensitivity across this mass range. This search excludes the full range of axion-photon coupling values predicted in benchmark models of the invisible axion that solve the strong CP problem of quantum chromodynamics.
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T. Braine
Pacific Northwest National Laboratory
R. Cervantes
Ford Motor Company (United States)
N. Crisosto
University of Washington
Physical Review Letters
University of California, Berkeley
University of Washington
University of Chicago
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Braine et al. (Wed,) studied this question.
synapsesocial.com/papers/6a1a965f49c3147e1045c6fe — DOI: https://doi.org/10.1103/physrevlett.124.101303