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- W3100543384 abstract "A bstract We propose an approach to search for axion dark matter with a specially designed superconducting radio frequency cavity, targeting axions with masses m a ≲ 10 − 6 eV. Our approach exploits axion-induced transitions between nearly degenerate resonant modes of frequency ∼ GHz. A scan over axion mass is achieved by varying the frequency splitting between the two modes. Compared to traditional approaches, this allows for parametrically enhanced signal power for axions lighter than a GHz. The projected sensitivity covers unexplored parameter space for QCD axion dark matter for 10 − 8 eV ≲ m a ≲ 10 − 6 eV and axion-like particle dark matter as light as m a ∼ 10 − 14 eV." @default.
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- W3100543384 date "2020-07-01" @default.
- W3100543384 modified "2023-10-16" @default.
- W3100543384 title "Axion dark matter detection by superconducting resonant frequency conversion" @default.
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- W3100543384 doi "https://doi.org/10.1007/jhep07(2020)088" @default.
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