Holographic Einstein Rings of AdS Black Holes in Horndeski Theory

TL;DR

This paper explores how holographic Einstein rings around AdS black holes in Horndeski theory are affected by various physical parameters, using wave optics and geometric optics, providing insights into spacetime geometry and dual strongly coupled systems.

Contribution

It presents a detailed analysis of holographic Einstein rings in Horndeski theory, highlighting the influence of physical parameters and comparing wave optics with geometric optics predictions.

Findings

Holographic Einstein rings are sensitive to observer position and black hole parameters.

Variations in parameters can deform rings into bright spots.

Wave optics and geometric optics results strongly agree.

Abstract

By utilizing the AdS/CFT correspondence and wave optics techniques, we conducted an extensive study of the imaging properties of holographic Einstein rings in the context of Anti-de Sitter (AdS) black holes (BHs) in Horndeski theory. Our results indicate that the optical characteristics of these holographic Einstein rings are significantly influenced by the observer's position, the physical parameters of the BH, the nature of the wave source, and the configuration of the optical system. Specifically, when the observer is positioned at the north pole of the AdS boundary, the holographic image prominently displays a ring structure aligning with the BH's photon sphere. We thoroughly analyzed how various physical parameters -- including the observation position, event horizon radius, temperature, and the parameter $\gamma$ in Horndeski theory -- affect the holographic Einstein rings. These parameters play a crucial role in determining the rings' radius and brightness, with variations potentially causing the ring structures to deform or even transform into bright spots. Furthermore, our comparative analysis between wave optics and geometric optics reveals a strong agreement in predicting the positions and brightnesses of both the photon ring and the Einstein ring. This research offers new insights into the spacetime geometry of BHs in Horndeski theory and proposes a promising framework for exploring the gravitational duals of strongly coupled systems.