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A M\"ossbauer Scheme to Probe Gravitational Waves
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A M\"ossbauer Scheme to Probe Gravitational Waves
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Under the local gravitational field, perturbations from high-frequency gravitational waves can cause a vertical shift of the M\"ossbauer resonance height. Considering a stationary scheme with the $^{109}$Ag isotope, we demonstrate that the extremely high precision of M\"ossbauer resonance allows for competitive gravitational wave sensitivity from KHz up to above MHz frequencies. M\"ossbauer resonance can offer a novel and small-sized alternative in the quest of multi-band gravitational wave searches. The presence of the static gravitational field plays essential role in the detection mechanism, isotope selection and sensitivity forecast. The proposed stationary scheme's sensitivity has the potential of significant improvement in a low-gravity environment.
Forward citations
Cited by 2 Pith papers
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Cavity Multimodes as an Array for High-Frequency Gravitational Waves
A 9-cell microwave cavity's 18 modes can act as a synthetic detector array that reconstructs the direction, polarization, and chirp of a high-frequency gravitational-wave signal.
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Searching for Ultralight Dark Matter with M{\"o}ssbauer Resonance
A stationary Mössbauer setup with 109Ag could probe ultralight scalar dark matter couplings down to roughly 10^-18 GeV^-1 (photon), 10^-21 (gluon), and 10^-22 (quark).
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