Non-linear charged planar black holes in four-dimensional Scalar-Gauss-Bonnet theories
arXiv:2205.09282 · doi:10.1103/PhysRevD.106.024017
Abstract
In this work, we consider the recently proposed well-defined theory that permits a healthy limit of the Einstein-Gauss-Bonnet combination, which requires the addition of a scalar degree of freedom. We continue the construction of exact, hairy black hole solutions in this theory in the presence of matter sources, by considering a nonlinear electrodynamics source, constructed through the Plebański tensor and a precise structural function . Computing the thermodynamic quantities with the Wald formalism, we identify a region in parameter space where the hairy black holes posses well-defined, non-vanishing, finite thermodynamic quantities, in spite of the relaxed asymptotic approach to planar AdS. We test its local stability under thermal and electrical fluctuations and we also show that a Smarr relation is satisfied for these black hole configurations.
10 pages, 3 figures, Accepted for publication in Physical Review D
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- Exploring the shear viscosity in four-dimensional planar black holes beyond General Relativity
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- Scaling symmetry, Smarr relation, and the extended first law in lower-dimensional Lovelock gravity
- Thermodynamics of Flat 4D Einstein-Gauss-Bonnet Black Hole with Rényi Entropy: An RPST-like formalism
- New brane-like solutions in modified four-dimensional Einstein-Gauss-Bonnet gravity