Rastall gravity: accretion disk image in the context of radiation fields and visual transformations compared to Reissner-Nordström black hole

In this study, we investigated the astronomical implications of Rastall gravity, particularly its behavior amidst a radiation field compared to Reissner-Nordstrom (RN) black holes. We found a crucial correlation between the dynamics of the accretion disk and the parameters Q and N-r, which properly reflect the influence of spacetime metrics on the disk's appearance. Elevated electric charge Q causes contraction in the disk's orbit due to enhanced gravitational effects, while higher N(r )values lead to outward expansion, influenced by the attributes of the radiation field. Interestingly, the charged black holes surrounded by radiation fields exhibit distinct visual disparities from RN black holes. Brightness decreases and expansion occurs within the innermost stable circular orbit of the accretion disk with rising N(r )values. Our study also reveals the process by which the accretion disk transitions from a conventional disk-like structure to a hat-like form at different observation angles, with the redshift effect gradually intensifying. Moreover, the results of the considered Rastall gravity radiation field are consistent with the constraints of the gravitational lensing of the host galaxy on Rastall gravity parameters, thereby enhancing the consistency between theoretical predictions and actual observations.