Abstract
Coherent resonant conditions of a strong electromagnetic (EM) wave beam propagating in a static magnetic field to a standing gravitational wave (GW) are given. It is found that under the resonant conditions not only first-order perturbed energy fluxes (PEFs) propagating along the same and opposite directions to the background EM wave beam can be generated, but also radial and tangential PEFs which are perpendicular to the above directions can be produced. Such results might provide a new way to display the resonant response induced by the standing GW with h = 10-35 and λg = 0.1m at the level of the single photon avalanche effect.
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