Maximal chirality transfer in the photon-graviton conversion in the early Universe

While photons and gravitons do not interact significantly, photons can be converted to gravitons in a background magnetic field---a phenomenon known as the Gertsenshtein effect. In this paper, we investigate whether chiral electromagnetic waves can be converted to chiral gravitational waves (GW) in the presence of primordial magnetic fields during the radiation-dominated epoch of the early Universe. We consider two situations wherein chirality is either present in the propagating electromagnetic waves or it exists in the background magnetic field. Our analysis shows that while the conversion probability increases with stronger magnetic fields, it remains insensitive to the chiral nature of the background magnetic field. Consequently, the net chirality parameter is independent of the chirality of the background field in both cases. Finally, we demonstrate that the present-day energy density of the produced chiral GWs peaks at a frequency of $\ensuremath{\sim}100\text{ }\text{ }\mathrm{GHz}$, and the corresponding characteristic strain can be sensitive to current and future missions designed to detect high-frequency GWs.