Entropy of nonlinear black holes in quadratic gravity
Jerzy Matyjasek

TL;DR
This paper calculates the entropy of nonlinear black holes within quadratic gravity using Noether charge and Euclidean methods, focusing on extremal cases and boundary condition effects.
Contribution
It introduces a novel approach to compute black hole entropy in quadratic gravity coupled with nonlinear electrodynamics, emphasizing extremal configurations.
Findings
Entropy expression derived for nonlinear black holes in quadratic gravity.
Analysis of extremal black hole configurations.
Impact of boundary conditions on black hole parameters.
Abstract
Employing the Noether charge technique and Visser's Euclidean approach the entropy of the nonlinear black hole described by the perturbative solution of the system of coupled equations of the quadratic gravity and nonlinear electrodynamics is constructed. The solution is parametrized by the exact location of the event horizon and charge. Special emphasis in put on the extremal configuration. Consequences of the second choice of the boundary conditions, in which the solution is paramerized by the charge and the total mass as seen by a distant observer is briefly examined.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Pulsars and Gravitational Waves Research
