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This Letter reports the results from a haloscope search for dark matter axions with masses between 2.66 and 2.81 μeV. 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 subkelvin temperatures, thereby reducing thermal noise as well as the excess noise from the ultralow-noise superconducting quantum interference device 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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Du et al. (Mon,) studied this question.
synapsesocial.com/papers/69d6af1efca0359822aa802e — DOI: https://doi.org/10.1103/physrevlett.120.151301
N. Du
Lawrence Livermore National Laboratory
Nicholas Force
University of Washington
Rakshya Khatiwada
IIT Research Institute
Physical Review Letters
University of California, Berkeley
University of Washington
University of Chicago
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