Maeda-Dadhich Solutions as Real Black Holes
arXiv:1503.06780 · doi:10.1103/PhysRevD.92.104046
Abstract
A four-dimensional static Schwarzschild-like solution obtained in [3]-[6] in the frames of the Einstein-Gauss-Bonnet gravity at the Kaluza-Klein split is analyzed. The matter in these solutions is created by auxiliary dimensions. The main goal of our work is to study physically sensible characteristics, which could be observable. Study of the perturbed equations demonstrates their stability under linear perturbations. The specific combinations of the parameters, permitting to construct black hole-like objects with one or two horizons or naked singularities are determined. Stable orbits of test particles around these black holes are presented. We show the exotic thermodynamical properties of the solution, when the Hawking evaporation law has the behavior opposite to usual one in General Relativity.
References in corpus (8)
- Jet Launching Structure Resolved Near the Supermassive Black Hole in M87
- Time delay and magnification centroid due to gravitational lensing by black holes and naked singularities
- Circular motion of neutral test particles in Reissner-Nordström spacetime
- Constraints on a charge in the Reissner--Nordström metric for the black hole at the Galactic Center
- Matter without matter: novel Kaluza-Klein spacetime in Einstein-Gauss-Bonnet gravity
- Kaluza-Klein black hole with negatively curved extra dimensions in string generated gravity models
- Quasinormal modes for the scattering on a naked Reissner-Nordstrom singularity
- Origin of matter out of pure curvature