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