Astronomy & Space

Cavity Multimodes as an Array for High-Frequency Gravitational Waves

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This study demonstrates that multiple electromagnetic modes within a single microwave cavity can detect and characterize high-frequency gravitational waves when operated in a magnetic field. Using a 9-cell cavity design, researchers showed that 18 nearly degenerate modes can work together like an array of detectors, enabling localization of gravitational wave sources and reconstruction of signal properties including polarization and frequency drift. The multi-mode approach enhances sensitivity analogously to having a network of independent detectors, making detection of astrophysical sources such as binary systems theoretically feasible.


This work provides a practical pathway for detecting gravitational waves at higher frequencies than current detectors like LIGO can measure, potentially opening a new observational window in astrophysics. The use of existing particle accelerator cavity technology makes implementation more feasible and cost-effective than building entirely new detector arrays.


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arXiv:2601.03341v3 Announce Type: replace-cross
Abstract: Microwave cavities operated in the presence of a background magnetic field provide a promising avenue for detecting high-frequency gravitational waves (HFGWs). We demonstrate for the first time that the distinct antenna patterns of multiple electromagnetic modes within a single cavity enable localization and reconstruction of key properties of an incoming HFGW signal, including its polarization ratio and frequency drift rate. Using a 9-cell cavity commonly employed in particle accelerators as a representative example, we analyze the time-domain response of 18 nearly degenerate modes, which can be sequentially excited by a frequency-drifting signal. The sensitivity is further enhanced by the number of available modes, in close analogy to the scaling achieved by a network of independent detectors, enabling sensitivity to astrophysically plausible binary sources.

Source: Cavity Multimodes as an Array for High-Frequency Gravitational Waves