The non-Kerr black hole with acceleration
arXiv:2106.02095 · doi:10.1140/epjc/s10052-021-09641-4
Abstract
The no-hair theorem can be tested in the strong gravity regime by using the top-bottom approach and the bottom-top approach. The non-Kerr spacetime of the later approach is an ideal framework to do the tests in the region very close to the black holes. In this work, we propose a non-Kerr black hole metric (and its charged extension) that is accelerating as well. These new objects are studied for their basic properties and thermodynamics.
References in corpus (17)
- The Confrontation between General Relativity and Experiment
- A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem
- Mapping spacetimes with LISA: inspiral of a test-body in a `quasi-Kerr' field
- General parametrization of axisymmetric black holes in metric theories of gravity
- Regular Black Hole Metric with Three Constants of Motion
- Tunnelling Methods and Hawking's radiation: achievements and prospects
- On generic parametrizations of spinning black-hole geometries
- Accelerating and rotating black holes
- Pair of accelerated black holes in a de Sitter background: the dS C-metric
- Tunneling of Dirac particles from accelerating and rotating black holes
- Radiation generated by accelerating and rotating charged black holes in (anti-)de Sitter space
- An exact solution for a rotating black hole in modified gravity
- Thermodynamics of accelerating and rotating black holes
- Quantum corrections to the entropy of charged rotating black holes
- Rotating charged black hole with Weyl corrections
- Charging the Johannsen-Psaltis spacetime
- Quantum corrections to the entropy of Einstein-Maxwell dilaton-axion black holes