Black holes with constant topological Euler density
arXiv:1609.07933 · doi:10.1209/0295-5075/115/60002
Abstract
A class of four dimensional spherically symmetric and static geometries with constant topological Euler density is studied. These geometries are shown to solve the coupled Einstein-Maxwell system when non-linear Born-Infeld-like electrodynamics is employed.
7 pages, REVTeX 4, 1 figure, to appear in EPL
References in corpus (23)
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics
- Regular Magnetic Black Holes and Monopoles from Nonlinear Electrodynamics
- On non-abelian generalisation of Born-Infeld action in string theory
- Twenty Years of the Weyl Anomaly
- Regular black holes with a nonlinear electrodynamics source
- Construction of cosmologically viable f(G) gravity models
- Higher-dimensional charged black holes solutions with a nonlinear electrodynamics source
- Dark energy problem: from phantom theory to modified Gauss-Bonnet gravity
- Generalized Vaidya Solutions
- Black hole solutions in Euler-Heisenberg theory
- Action and Entropy of Extreme and Non-Extreme Black Holes
- Topology, Entropy and Witten Index of Dilaton Black Holes
- Asymptotic Reissner-Nordstrom black holes
- Born-Infeld black hole in the isolated horizon framework
- Second Order Scalar Invariants of the Riemann Tensor: Applications to Black Hole Spacetimes
- Exact solutions for null fluid collapse
- Action and entropy of black holes in spacetimes with a cosmological constant
- Entropy and Topology for Gravitational Instantons
- A nongravitational wormhole
- Topological Static Spherically Symmetric vacuum Solutions in Gravity
- Geometry and topology of two kinds of extreme Reissner-Nordstrm-anti-de Sitter black holes
- Euler numbers of four-dimensional rotating black holes with the Euclidean signature
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- Scale-dependent (2+1) - dimensional electrically charged black holes in Einstein-power-Maxwell theory
- Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density
- Four-Dimensonal Gauss-Bonnet Gravity Without Gauss-Bonnet Coupling to Matter - Spherically Symmetric Solutions, Domain Walls and Spacetime Singularities
- Gauss-Bonnet Gravity in Without Gauss-Bonnet Coupling to Matter - Cosmological Implications