摘要
Gravitational waves can generate electromagnetic effects inside a strong electric or magnetic field within the Standard Model and general relativity. Here we propose using a quarterly split cavity and LC (inductor and capacitor) resonance circuit to detect a high-frequency gravitational wave from 0.1 MHz to GHz. We perform a full 3D simulation of the cavity's signal for sensitivity estimate. Our sensitivity depends on the coherence timescale of the high-frequency gravitational wave sources and the volume size of the split cavity. We discuss the resonant measurement schemes for narrow-band gravitational wave sources and also a nonresonance scheme for broadband signals. For a meter-sized split cavity under a 14 Tesla magnetic field, the LC resonance enhanced sensitivity to the gravitational wave strain is expected to reach h∼10-20 around 10 MHz.
源语言 | 英语 |
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文章编号 | 084004 |
期刊 | Physical Review D |
卷 | 109 |
期 | 8 |
DOI | |
出版状态 | 已出版 - 15 4月 2024 |