Reanalysis of CAPP-12T axion data sets 90% CL limits on HFGW strain down to 3.9e-21 at 5.311 GHz and excludes certain 10^{-6} solar mass black holes within 0.01 AU via superradiance interpretation.
Microwave apparatus for gravitational waves observation
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abstract
In this report the theoretical and experimental activities for the development of superconducting microwave cavities for the detection of gravitational waves are presented.
verdicts
UNVERDICTED 2representative citing papers
Cryogenic tests on the MAGO cavity achieved 11 kHz electromagnetic mode splitting and high Q factors at 2 K, while mechanical Q factors fell below theoretical expectations.
citing papers explorer
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Search for high-frequency gravitational waves via re-analysis of cavity axion data
Reanalysis of CAPP-12T axion data sets 90% CL limits on HFGW strain down to 3.9e-21 at 5.311 GHz and excludes certain 10^{-6} solar mass black holes within 0.01 AU via superradiance interpretation.
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Cryogenic RF characterization of the MAGO cavity for high-frequency gravitational-wave detection
Cryogenic tests on the MAGO cavity achieved 11 kHz electromagnetic mode splitting and high Q factors at 2 K, while mechanical Q factors fell below theoretical expectations.