Abstract： We consider the resonant response of a Gaussian beam passing through a static magnetic field to a high-frequency relic gravitational wave (GW). It is found that under the synchroresonance condition, the first-order perturbative electromagnetic energy fluxes will contain a “left circularly wave” and a “right circularly wave”around the symmetrical axis of the Gaussian beam, but the perturbative effects produced by the + and x polarization of the GW have different physical behaviour. For the high-frequency relic GW with vg = 1010Hz, h = 10-30, recently expected by the quintessential inflationary models, the corresponding perturbative photon flux passing through the region 10-2m2 would be expected to be 104s-1, This is the largest perturbative photon flux we recently analysed and estimated using the typical laboratory parameters.
LI Fang-Yu;TANG Meng-Xi. Electrogravitational Resonance of a Gaussian Beam to a High-Frequency Relic Gravitational Wave[J]. 中国物理快报, 2001, 18(12): 1546-1549.
LI Fang-Yu, TANG Meng-Xi. Electrogravitational Resonance of a Gaussian Beam to a High-Frequency Relic Gravitational Wave. Chin. Phys. Lett., 2001, 18(12): 1546-1549.
2001, Vol. 18 
