Rotating and accelerating black holes with cosmological constant
arXiv:1606.02415 · doi:10.1103/PhysRevD.94.044001
Abstract
We propose a new form of the rotating C-metric with cosmological constant, which generalises the form found by Hong and Teo for the Ricci-flat case. This solution describes the entire class of spherical black holes undergoing rotation and acceleration in dS or AdS space-time. The new form allows us to identify the complete ranges of coordinates and parameters of this solution. We perform a systematic study of its geometrical and physical properties, and of the various limiting cases that arise from it.
arXiv comment36 pages, 5 figures; v2: references added; as accepted for publication in Phys. Rev. D
References in corpus (20)
- A new look at the Plebanski-Demianski family of solutions
- Stationary and Axisymmetric Solutions of Higher-Dimensional General Relativity
- Uniqueness theorem for 5-dimensional black holes with two axial Killing fields
- A new form of the C-metric
- Rotating Topological Black Holes
- Pair of accelerated black holes in an anti-de Sitter background: the AdS C-metric
- Accelerating black holes in anti-de Sitter universe
- Four-dimensional black holes with unusual horizons
- Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time
- Radiation from accelerated black holes in an anti-de Sitter universe
- A new form of the rotating C-metric
- Accelerated black holes in an anti-de Sitter universe
- Pair of accelerated black holes in a de Sitter background: the dS C-metric
- Rod-structure classification of gravitational instantons with U(1)xU(1) isometry
- Radiation from accelerated black holes in de Sitter universe
- Uniformly accelerating black holes in a de Sitter universe
- Deformed hyperbolic black holes
- A new form of the C-metric with cosmological constant
- Black holes with bottle-shaped horizons
- Domain Structure of Black Hole Space-Times with a Cosmological Constant