2004/10/14 by Fang-Yu Li, Li Fang-Yu, Nan Yang +1 · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #Pulsars and Gravitational Waves Research #Quantum and Classical Electrodynamics #gr-qc
paper · pdf · doi:10.1088/0256-307x/21/11/011
published as Chin.Phys.Lett.21:2113-2116,2004 · 10pages
arxiv created 2004/10/14 · openalex publication_date 2004/10/27 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/30
We investigate the resonant interaction of a weak gravitational wave with a microwave beam in a coupling electromagnetic system, which consists of a Gaussian beam with double polarized transverse electric modes, a static magnetic field and fractal membranes. We find that under the synchroresonance condition, a high-frequency gravitational wave in amplitude 10 −30 and frequency 3 GHz may produce the perturbative photon flux of 2.15 × 10 s −1 in a surface of 10 −2 m 2 . The perturbative photon flux can be pumped out from the background photon fluxes and one may obtain the amplified signal photon flux of 2.15 × 10 4 s −1 by cascade fractal membranes. It is worth studying this effect for the detection of high-frequency relic gravitational waves in quintessential inflationary models and the high-frequency gravitational waves expected by possible laboratory schemes.