Gravitational lensing by a black hole in effective loop quantum gravity

TL;DR

This paper investigates how quantum effects in effective loop quantum gravity influence gravitational lensing by black holes, revealing diverse black hole types, divergent bending behaviors, and potential signals for wormhole formation.

Contribution

It explores the impact of quantum parameters on light bending and image formation around black holes in loop quantum gravity, identifying conditions for different black hole and wormhole states.

Findings

Black holes can be Schwarzschild, regular, or wormholes depending on quantum parameters.

Strong bending angles exhibit logarithmic and non-logarithmic divergences.

Angular separation of relativistic images varies with quantum effects, indicating wormhole formation.

Abstract

It is well known that general relativity is an effective theory of gravity at low energy scale, and actually quantum effects cannot be ignored in the strong-field regime. As a strong gravitational object, black hole plays a key role in testing the quantum effects of gravity in the strong-field regime. In this paper, we focus on black hole in effective loop quantum gravity and investigate what the influences are of the quantum effects on the weak and strong bending angles of light rays. We find that this black hole could be a Schwarzschild black hole, a regular black hole, a one-way traversable wormhole, or a two-way traversable wormhole for the different values of the quantum parameter, and the strong bending angle for this compact object exhibits two different divergent behaviors, i.e., the logarithmic divergence and non-logarithmic divergence. There are a series of relativistic images on both sides of the optical axis. Only the outermost one can be resolved as a single image, and all others are packed together at the limiting angular position. It is interesting to note that the angular separation between the outermost relativistic image and the others initially increases and then decreases as the quantum parameter increases, indicating that there is a maximum in the angular separation. The maximum is reached after the black hole becomes a wormhole, which can be taken as a signal for the formation of the wormhole. Moreover, the limiting angular position decreases as the quantum parameter increases but a little bounce occurs after the formation of the wormhole, and the relative magnification in magnitudes first decreases and then increases as the quantum parameter increases.