Topologically Charged Holonomy corrected Schwarzschild black hole lensing

TL;DR

This paper explores how light bends around a topologically charged Holonomy corrected Schwarzschild black hole, providing analytical models for weak and strong gravitational lensing to aid observational detection.

Contribution

It introduces a novel black hole model with topological charge and Holonomy correction, analyzing its lensing effects in both weak and strong fields.

Findings

Derived analytical expressions for light deflection in both limits

Identified observable features for detecting such black holes

Modeled gravitational scenarios to verify characteristics

Abstract

In this paper, we theoretically investigate the deflection of light produced by a topologically charged Holonomy corrected Schwarzschild black hole. The study is carried out both in the weak field limit and in the strong field limit. We analytically deduced the expansions for light deflection in the two limits and, from them, we determined the observables in order to provide elements so that observational tools are able to identify these solutions. We model possible gravitational scenarios in order to verify the possible gravitational characteristics of the solution.