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- W4386285203 abstract "Abstract Detecting gravitational waves with frequencies higher than 10 kHz requires new strategies. In previous papers, we proposed magnon gravitational wave detectors and gave the first limit on gigahertz gravitational waves by reinterpreting the existing data from axion dark matter experiments. In this paper, we show that the sensitivity can be improved by constructing the detector specific to gravitational waves. In particular, we employ an infinite sum of terms in the expansion of Fermi normal coordinates to probe gravitational waves with a wavelength comparable to the detector size. As a consequence, we obtain sensitivity of around $$h_c sim 10^{-20}$$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mrow> <mml:msub> <mml:mi>h</mml:mi> <mml:mi>c</mml:mi> </mml:msub> <mml:mo>∼</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>-</mml:mo> <mml:mn>20</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> ." @default.
- W4386285203 created "2023-08-31" @default.
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- W4386285203 date "2023-08-30" @default.
- W4386285203 modified "2023-09-30" @default.
- W4386285203 title "Exploring high-frequency gravitational waves with magnons" @default.
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- W4386285203 doi "https://doi.org/10.1140/epjc/s10052-023-11876-2" @default.
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