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Microwave apparatus for gravitational waves observation

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arxiv gr-qc/0502054 v1 pith:ILOBUGLS submitted 2005-02-11 gr-qc

R. Ballantini , Ph. Bernard , S. Calatroni , E. Chiaveri , A. Chincarini , R.P. Croce , S. Cuneo , V. Galdi
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G. Gemme R. Losito R. Parodi E. Picasso V. Pierro I.M. Pinto A. Podesta' R. Vaccarone
This is my paper · ORCID
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keywords gravitationalmicrowavewavesactivitiesapparatuscavitiesdetectiondevelopment
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In this report the theoretical and experimental activities for the development of superconducting microwave cavities for the detection of gravitational waves are presented.

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Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Halbach Magnetic Weber Bars

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Halbach-array field gradients boost the displacement-to-flux readout of a resonant-sphere magnetic Weber bar, projecting ~10^-21/√Hz strain sensitivity near 10 kHz and ~5×10^-20/√Hz broadband at higher frequencies.

  2. Cavity Multimodes as an Array for High-Frequency Gravitational Waves

    hep-ph 2026-01 conditional novelty 6.0 of 10

    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.

  3. High-Frequency Gravitational Waves on BREAD

    hep-ph 2025-05 conditional novelty 6.0 of 10

    BREAD with single photon detectors could detect high-frequency gravitational waves at 0.05 to 200 THz, with projected strains as low as 1e-25 at 200 THz.

  4. Search for high-frequency gravitational waves via re-analysis of cavity axion data

    hep-ex 2025-11 unverdicted novelty 5.0 of 10

    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.

  5. Cryogenic RF characterization of the MAGO cavity for high-frequency gravitational-wave detection

    physics.ins-det 2026-07 unverdicted novelty 4.0 of 10

    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.

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