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We report the results from a haloscope search for axion dark matter in the$3.3\text{-}4.2~{\mu}$eV mass range. This search excludes the axion-photoncoupling predicted by one of the benchmark models of "invisible" axion darkmatter, the KSVZ model. This sensitivity is achieved using a large-volumecavity, a superconducting magnet, an ultra low noise Josephson parametricamplifier, and sub-Kelvin temperatures. The validity of our detection procedureis ensured by injecting and detecting blind synthetic axion signals.

Search for "Invisible" Axion Dark Matter in the $3.3\text{-}4.2~{\mu}$eV Mass Range