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Holonomy corrected Schwarzschild black hole lensing

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arxiv 2309.05106 v2 pith:BLN66M3G submitted 2023-09-10 gr-qc

A. R. Soares , C. F. S. Pereira , R. L. L. Vitória This is my paper · ORCID
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keywords schwarzschildblackcorrectedfieldholeholonomylensinglimit
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In the present work, we theoretically investigate gravitational lensing in the spacetime of a holonomy corrected Schwarzschild black hole. Analytical expressions for the light deflection angle are obtained in both the weak field limit and the strong field limit. Furthermore, we analyze observables, such as relativistic images and magnifications, and compare the results with those expected in a Schwarzschild spacetime. We discuss the possibilities and difficulties of investigating such a solution in practice.

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Cited by 1 Pith paper

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  1. Analyzing Deflection Angles and Photon Sphere Dynamics of Magnetically Charged Black Holes in Nonlinear Electrodynamic

    gr-qc 2025-02 reject novelty 4.0 of 10

    A new closed-form weak deflection angle and shadow analysis for a magnetically charged NED black hole, with strong-field results that reduce to Schwarzschild after a mass redefinition.

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