Active Galactic Nuclei (AGN) significantly impacts galaxy evolution through feedback driven by relativistic jets. At higher redshifts, these jets are thought to produce strong X-ray emissions via inverse Compton scattering of Cosmic Microwave Background (IC/CMB) photons. As CMB photon density rises with redshift, this process becomes more prominent and may explain enhanced X-ray output from AGN jets in the early universe. Understanding this effect is key to revealing how AGN influences their surroundings and shapes galactic evolution.