Signal photon flux generated by high-frequency relic gravitational waves

TL;DR

This paper explores the potential detection of high-frequency relic gravitational waves through their interaction with electromagnetic systems, showing how photon flux varies with different spectral indices and proposing a detection method.

Contribution

It demonstrates a novel detection approach for high-frequency relic gravitational waves via perturbed photon flux measurements, with detailed flux variation analysis.

Findings

Perturbed photon flux varies significantly with spectral index n_t.

The flux ratio ranges from 10^{-28} to 10^{-16}.

Amplitude of relic gravitational waves at 5 GHz varies from 10^{-36} to 10^{-25}.

Abstract

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 $h_t$($5\times10^9$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 $N_x^1$($5\times10^9$Hz) varies from $1.40\times10^{-4}\rm s^{-1}$ to $2.85\times10^{7}\rm s^{-1}$ 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 $10^{-16}$.