In horizon penetrating coordinates: Kerr black hole metric perturbation, construction and completion
From MaRDI portal
Publication:6086655
DOI10.1088/1361-6382/ad0495arXiv2309.09474OpenAlexW4387734962MaRDI QIDQ6086655
Dejan Stojkovic, Unnamed Author
Publication date: 10 November 2023
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2309.09474
Kerr spacetimeconfluent Heun equationlinear perturbationTeukolsky equationhorizon penetrating coordinates
Black holes (83C57) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Cites Work
- Unnamed Item
- Unnamed Item
- Effective state, Hawking radiation and quasi-normal modes for Kerr black holes
- Detection of gravitational waves from black holes: is there a window for alternative theories?
- On the derivatives of the Heun functions
- Black holes, hidden symmetries, and complete integrability
- Perturbations of the Kerr spacetime in horizon-penetrating coordinates
- Stability of a Schwarzschild Singularity
- Classes of exact solutions to the Teukolsky master equation
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Space–times admitting Killing–Yano tensors. I
- Space—times admitting Killing—Yano tensors. II
- Teukolsky formalism for nonlinear Kerr perturbations
- The Kerr metric
- Gauge-invariant non-spherical metric perturbations of Schwarzschild black-hole spacetimes
- Exact Space-Times in Einstein's General Relativity
- General Relativity