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Journal Article | PUBDB-2024-07014 |
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2025
IOP Publ.
Bristol
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Please use a persistent id in citations: doi:10.1088/1361-6382/add8da doi:10.3204/PUBDB-2024-07014
Report No.: DESY-24-181; FERMILAB-PUB-24-0819-SQMS-TD; arXiv:2411.18346
Abstract: Heterodyne detection using microwave cavities is a promising method for detecting high-frequency gravitational waves (GWs) or ultralight axion dark matter. In this work, we report on studies conducted on a spherical 2-cell cavity developed by the MAGO collaboration for high-frequency GWs detection. Although fabricated around 20 years ago, the cavity had not been used since. Due to deviations from the nominal geometry, we conducted a mechanical survey and performed room-temperature plastic tuning. Measurements and simulations of the mechanical resonances and electromagnetic properties were carried out, as these are critical for estimating the cavity’s GW coupling potential. Based on these results, we plan further studies in a cryogenic environment. The cavity characterisation does not only provide valuable experience for a planned physics run but also informs the future development of improved cavity designs.
Keyword(s): General Relativity and Quantum Cosmology (gr-qc) ; Instrumentation and Methods for Astrophysics (astro-ph.IM) ; Instrumentation and Detectors (physics.ins-det) ; FOS: Physical sciences
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First characterisation of the MAGO cavity, a superconducting RF detector for kHz-MHz gravitational waves
[10.3204/PUBDB-2024-07925]
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