Static black holes and strictly static spacetimes in Einstein-Gauss-Bonnet gravity with gauge field
arXiv:1406.3914 · doi:10.1103/PhysRevD.89.124022
Abstract
We examine strictly static asymptotically flat spacetimes in Einstein-Gauss-Bonnet gravity with U(1) gauge field, revealing that, up to small curvature corrections, confomally flat slices of the spacetime in question are of Minkowski origin. We consider uncharged and charged black hole solutions in the theory, showing that, up to the small curvature limit, they are diffeomorphic to Schwarzschild_Tangherlini or Reissner-Nordstrom solutions, respectively.
8 pagers, RevTex, to be published in Phys.Rev.D15
References in corpus (12)
- A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric
- Uniqueness theorem for 5-dimensional black holes with two axial Killing fields
- Black Holes in the Dilatonic Einstein-Gauss-Bonnet Theory in Various Dimensions I -- Asymptotically Flat Black Holes --
- A Uniqueness theorem for 5-dimensional Einstein-Maxwell black holes
- Classification of Static Charged Black Holes in Higher Dimensions
- Boundary Value Problem for Black Rings
- Horizons of radiating black holes in Einstein gauss-bonnet gravity
- Uniqueness theorem for stationary black ring solution of -models in five dimensions
- Uniqueness Theorem for Stationary Axisymmetric Black Holes in Einstein-Maxwell-axion-dilaton Gravity
- Uniqueness of charged static asymptotically flat black holes in dynamical Chern-Simons gravity
- Complex scalar field in strictly stationary Einstein-Maxwell-axion-dilaton spacetime with negative cosmological constant
- Mass angular momentum and charge inequalities for black holes in Einstein-Maxwell-axion-dilaton gravity
Cited by in corpus (4)
- Expanded evasion of the black hole no-hair theorem in dilatonic Einstein-Gauss-Bonnet theory
- Uniqueness of photon sphere for Einstein-Maxwell-dilaton black holes with arbitrary coupling constant
- Uniqueness of dilaton Melvin-Schwarzschild solution
- Uniqueness of dark matter magnetized static black hole spacetime