Signal photon flux generated by high-frequency relic gravitational waves

The power spectrum of primordial tensor perturbations ${\mathcal{P}}_t$ increases rapidly in high frequency region if the spectral index $n_t>0$. It is shown that the amplitude of relic gravitational wave $h_t$($5\times {10}^9$Hz) varies from ${10}^{-36}$ to ${10}^{-25}$ while $n_t$ varies from $-6.25\times 10^{-3}$to$0.87$. High frequency gravitational waves detector that is proposed by F.-Y. Li detects gravitational waves through observing the perturbed photon flux that is generated by interaction between the relic gravitational waves and electromagnetic system. It is shown that the perturbative photon flux $N_x^1$($5\times {10}^9$Hz) varies from $1.40\times {10}^{-4}{\mathrm{s}}^{-1}$ to $2.85\times {10}^7{\mathrm{s}}^{-1}$ while $n_t$ varies from $-6.25\times {10}^{-3}$ to $0.87$. Correspondingly, the ratio of the transverse perturbative photon flux $N_x^1$ to the background photon flux varies from ${10}^{-28}$ to ${10}^{-16}$.