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• W2912342940 abstract "Electromagnetic radiation with angular frequency equal to half the axion mass stimulates the decay of cold dark matter axions and produces an echo, i.e., faint electromagnetic radiation traveling in the opposite direction. We propose to search for axion dark matter by sending out to space a powerful beam of microwave radiation and listening for its echo. We estimate the sensitivity of this technique in the isothermal and caustic ring models of the Milky Way halo and find it to be a promising approach to axion, or axionlike, dark matter detection." @default.
• W2912342940 created "2019-02-21" @default.
• W2912342940 creator A5021426023 @default.
• W2912342940 creator A5046128831 @default.
• W2912342940 date "2019-09-27" @default.
• W2912342940 modified "2023-10-18" @default.
• W2912342940 title "Production and Detection of an Axion Dark Matter Echo" @default.
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• W2912342940 doi "https://doi.org/10.1103/physrevlett.123.131804" @default.
• W2912342940 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/31697522" @default.
• W2912342940 hasPublicationYear "2019" @default.
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