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arXiv · 2512.20592

Signatures of High-Frequency Gravitational Waves in Electromagnetic Cavities

Sebastian Schenk·Kristof Schmieden·Pedro Schwaller
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Abstract

Similar to axions, gravitational waves (GW) can induce oscillating electromagnetic fields inside electromagnetic cavities. We explore their experimental sensitivity to monochromatic and non-monochromatic GW signals, using the total deposited energy as a primary measure. Focusing on cylindrical and spherical cavities, we present the coupling coefficients of GWs to the dominant electromagnetic resonances in transverse-traceless gauge, which is most appropriate in this regime. By considering the superposition of degenerate modes, we further examine their angular sensitivity. In addition, we calculate the response of a spherical cavity to non-monochromatic GWs emitted by primordial black hole mergers. We find that, for transient signals, a high quality factor with $Q \gtrsim 10^5$ does not necessarily enhance experimental sensitivity. In fact, even in the most optimistic scenario, only mergers within the solar system yield an observable energy deposit in the cavity.

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Sebastian Schenk, Kristof Schmieden, Pedro Schwaller. 2025-12-23. Signatures of High-Frequency Gravitational Waves in Electromagnetic Cavities. https://arxiv.org/abs/2512.20592

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