Holographic Einstein Ring of a Charged Rastall AdS Black Hole with Bulk Electromagnetic Field

TL;DR

This paper explores the holographic imaging of Einstein rings around a charged Rastall AdS black hole, analyzing how various parameters affect the response function and ring characteristics within the AdS/CFT framework.

Contribution

It introduces a detailed holographic model of Einstein rings in a charged Rastall AdS black hole, linking optical features with black hole parameters and response functions.

Findings

Einstein ring appears with concentric stripes at the north pole.

Ring transforms into a bright spot when the observer moves away.

Shadow radius decreases with increasing Rastall parameter .

Abstract

We study the Einstein images of a charged Rastall AdS black hole (BH) within the fabric of AdS/CFT correspondence. Considering the holographic setup, we analyze the amplitude of the total response function for various values of model parameters. With an increase in parameter $\lambda$ and temperature $T$, the amplitude of the response function is decreased, while it is increased with the increase of the electric charge $e$ and chemical potential $\mu$. The influence of frequency $\omega$ also plays an important role in the bulk field, as it is found that the decreasing $\omega$ leads to an increase in the periods of the waves, which means that the amplitude of the response function also depends on the wave source. The relation between $T$ to the inverse of the horizon $r_{h}$ for the parameter $\lambda$ is interpreted under fixed values of other involved parameters. These, in turn, affect the behavior of the response function and the Einstein ring, which may be used to differentiate the present work from previous studies. Via a special optical system, we construct the holographic images of the BH in bulk. The obtained results show that the Einstein ring always appears with concentric stripes at the position of the north pole, and this ring transforms into the luminosity-deformed ring or bright light spot when the distant observer lies away from the north pole. Moreover, from the brightness profiles, it is observed that as $\lambda$ grows, the shadow radius is significantly decreased, while the brightness of the ring is negligibly changed. We further investigate the influence of $T$ and $\mu$ on the ring radius. These results reveal that the increasing values of $T$ lead to an increase in the shadow radius and decrease as the values of $\mu$ grow. Finally, we finish this work with a discussion of the Einstein ring radius obtained by geometric optics, which is consistent with wave optics.