Resonant Interaction Between a Weak Gravitational Wave and a Microwave Beam in the Double Polarized States Through a Static Magnetic Field

dc.creatorLi, Fang-Yu
dc.creatorYang, Nan
dc.date2004-10-14
dc.date.accessioned2026-07-07T11:42:58Z
dc.date.available2026-07-07T11:42:58Z
dc.descriptionWe investigate the resonant interaction to the weak gravitational waves in a coupling electromagnetic system, which consists of a Gaussian beam with the double polarized transverse electric modes, a static magnetic field and the fractal membranes. We find that under the syncroresonance condition a high-frequency GW (HFGW) of h=10^-30,v_g=3GHz may produce the perturbative photon flux (PPF) of 2.15*10/s in a surface of 0.01m^2. The PPF can be pumped out from the background photon fluxes and one might obtain the amplified signal photon flux of 2.15*10^4s^-1 by cascade fractal membranes. It appears to be worthwhile to study this effect for the detection of the high-frequency relic GWs in quintessential inflationary models and the HFGWs expected by possible laboratory schemes.
dc.description10pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0410060
dc.identifierhttp://arxiv.org/abs/gr-qc/0410060
dc.identifierChin.Phys.Lett.21:2113-2116,2004
dc.identifierdoi:10.1088/0256-307X/21/11/011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201074
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleResonant Interaction Between a Weak Gravitational Wave and a Microwave Beam in the Double Polarized States Through a Static Magnetic Field
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