Regular black holes in quadratic gravity

TL;DR

This paper constructs a perturbative solution for regular black holes in quadratic gravity coupled with nonlinear electrodynamics, showing the spacetime's regularity and analyzing black hole properties such as horizon and temperature.

Contribution

It introduces a novel analytical solution for regular black holes in quadratic gravity with nonlinear electrodynamics, extending previous models and analyzing their physical properties.

Findings

The solution is regular at the center, indicating a regular spacetime.

The black hole's horizon, asymptotics, and temperature are explicitly calculated.

Extremal black hole configurations are analyzed in detail.

Abstract

The first-order correction of the perturbative solution of the coupled equations of the quadratic gravity and nonlinear electrodynamics is constructed, with the zeroth-order solution coinciding with the ones given by Ay\'on-Beato and Garc{\'\i}a and by Bronnikov. It is shown that a simple generalization of the Bronnikov's electromagnetic Lagrangian leads to the solution expressible in terms of the polylogarithm functions. The solution is parametrized by two integration constants and depends on two free parameters. By the boundary conditions the integration constants are related to the charge and total mass of the system as seen by a distant observer, whereas the free parameters are adjusted to make the resultant line element regular at the center. It is argued that various curvature invariants are also regular there that strongly suggests the regularity of the spacetime. Despite the complexity of the problem the obtained solution can be studied analytically. The location of the event horizon of the black hole, its asymptotics and temperature are calculated. Special emphasis is put on the extremal configuration.