Structure and thermodynamics of charged nonrotating black holes in higher dimensions

TL;DR

This paper investigates the structure and thermodynamics of charged black holes in higher-dimensional spacetimes within nonlinear electrodynamics coupled to General Relativity, classifying solutions and deriving key thermodynamic relations.

Contribution

It provides a classification of nonlinear electrodynamics models supporting black hole solutions and derives general thermodynamic formulas, including the extremal black hole condition and Smarr relation.

Findings

Classified families of nonlinear electrodynamics supporting black holes.

Derived the general extremal black hole equation.

Established a universal Smarr formula for these solutions.

Abstract

We analyze the structural and thermodynamic properties of $D$-dimensional ($D \geq 4$), asymptotically flat or Anti-de-Sitter, electrically charged black hole solutions, resulting from the minimal coupling of general nonlinear electrodynamics to General Relativity. This analysis deals with static spherically symmetric (elementary) configurations with spherical horizons. Our methods are based on the study of the behaviour (in vacuum and on the boundary of their domain of definition) of the Lagrangian density functions characterizing the nonlinear electrodynamic models in flat spacetime. These functions are constrained by some admissibility conditions endorsing the physical consistency of the corresponding theories, which are classified in several families, some of them supporting elementary solutions in flat space which are non topological solitons. This classification induces a similar one for the elementary black hole solutions of the associated gravitating nonlinear electrodynamics, whose geometrical structures are thoroughly explored. A consistent thermodynamic analysis can be developed for the subclass of families whose associated black hole solutions behave asymptotically as the Schwarzschild metric (in absence of a cosmological term). In these cases we obtain the behaviour of the main thermodynamic functions, as well as important finite relations among them. In particular, we find the general equation determining the set of extreme black holes for every model, and a general Smarr formula, valid for the set of elementary black hole solutions of such models. We also consider the one-parameter group of scale transformations, which are symmetries of the field equations of any nonlinear electrodynamics in flat spacetime.