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We consider the perturbative photon flows (PPFs, i.e., electromagnetic (EM)counterparts) generated by the EM resonance response to high-frequencygravitational waves (HFGWs) with additional polarization states in a rotatinglaboratory frame system. It is found that when the propagating direction ofHFGWs and the symmetrical axis of the laboratory frame system are the same, thePPFs have the maximum value. In this case, using the rotation (the rotation ofthe azimuth $\phi$) of the EM detection system, all six possible polarizationstates of HFGWs can be separated and displayed. For the current experimentalconditions, it is quite prospective to detect the PPFs generated by the HFGWspredicted in the braneworld models, the primordial black hole theories, theinteraction mechanism between astrophysical plasma and intense EM radiation,etc., due to the large amplitudes (or high spectral densities) and spectralcharacteristics of these HFGWs. Detecting the primordial HFGWs from inflationfaces great challenges at present, but it is not impossible.

Electromagnetic counterparts of high-frequency gravitational waves in a rotating laboratory frame system and their detection