Abstract
We consider the resonant response of a Gaussian beam passing through astatic magnetic field to a high-frequency relic gravitational wave (GW).It is found that under the synchroresonance condition, the first-orderperturbative electromagnetic energy fluxes will contain a ``left circularwave'' and a ``right circular wave'' around the symmetrical axis of theGaussian beam, but the perturbative effects produced by the + and ×polarization of the GW have a different physical behaviour. For thehigh-frequency relic GW with νg = 1010 Hz, h = 10-30,recently expected by the quintessential inflationary models, thecorresponding perturbative photon flux passing through the region10-2 m2 would be expected to be 104 s-1. This is the largestperturbative photon flux we have recently analysed and estimated using thetypical laboratory parameters.
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