A note on non-linear electrodynamics, regular black holes and the entropy function
Kevin Goldstein, Hossein Yavartanoo

TL;DR
This paper investigates regular black holes in non-linear electrodynamics coupled with gravity, demonstrating that the entropy function formalism accurately reproduces their near-horizon geometry and entropy, countering recent claims.
Contribution
It shows that the entropy function formalism applies to regular black holes in non-linear electrodynamics, confirming its validity beyond traditional singular solutions.
Findings
Entropy function reproduces near horizon geometry
Correct entropy calculation for regular black holes
Counteracts recent claims in the literature
Abstract
We examine four dimensional magnetically charged extremal black holes in certain non-linear U(1) gauge theories coupled to two derivative gravity. For a given coupling, one can tune the magnetic charge (or vice versa) so that the curvature singularity at the centre of the space-time is cancelled. Since these solutions have a horizon but no singularity, they have been called regular black holes. Contrary to recent claims in the literature, we find that the entropy function formalism reproduces the near horizon geometry and gives the correct entropy for these objects.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Pulsars and Gravitational Waves Research
