Electromagnetic-gravitational perturbations of Kerr–Newman spacetime: The Teukolsky and Regge–Wheeler equations
From MaRDI portal
Publication:5075545
DOI10.1142/S0219891622500011zbMath1486.83004arXiv2002.07228OpenAlexW3092806338WikidataQ115245139 ScholiaQ115245139MaRDI QIDQ5075545
Publication date: 16 May 2022
Published in: Journal of Hyperbolic Differential Equations (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2002.07228
Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)
Related Items (3)
Stable black holes: in vacuum and beyond ⋮ Scalar QNM Spectra of Kerr and Reissner-Nordström revealed by eigenvalue repulsions in Kerr-Newman ⋮ A scale-critical trapped surface formation criterion for the Einstein-Maxwell system
Cites Work
- Unnamed Item
- Unnamed Item
- Decay for solutions of the wave equation on Kerr exterior spacetimes. III: The full subextremalcase \(|a| < M\).
- Mode stability for the Teukolsky equation on extremal and subextremal Kerr spacetimes
- Uniform energy bound and Morawetz estimate for extreme components of spin fields in the exterior of a slowly rotating Kerr black hole. II: linearized gravity
- Hidden symmetries and decay for the wave equation on the Kerr spacetime
- The global non-linear stability of the Kerr-de Sitter family of black holes
- Non-linear stability of the Kerr-Newman-de Sitter family of charged black holes
- Boundedness and decay for the Teukolsky system of spin \(\pm 2\) on Reissner-Nordström spacetime: the case \(|Q| \ll M\)
- Linear stability of Schwarzschild spacetime: decay of metric coefficients
- Boundedness and decay for the Teukolsky equation on Kerr spacetimes. I: The case \(|a|\ll M\)
- The linear stability of the Schwarzschild solution to gravitational perturbations in the generalised wave gauge
- Quantitative mode stability for the wave equation on the Kerr spacetime
- The linear stability of the Schwarzschild solution to gravitational perturbations
- The linear stability of Reissner-Nordström spacetime for small charge
- Linear stability of slowly rotating Kerr black holes
- Mode stability of the Kerr black hole
- A new physical-space approach to decay for the wave equation with applications to black hole spacetimes
- A Local Energy Estimate on Kerr Black Hole Backgrounds
- Stability of a Schwarzschild Singularity
- The red‐shift effect and radiation decay on black hole spacetimes
- Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations
- Boundedness and decay for the Teukolsky equation of spin ±1 on Reissner–Nordström spacetime: the $\boldsymbol{ \newcommand{\e}{{\rm e}} \ell=1}$ spherical mode
- Lectures on black holes and linear waves
- Exact Space-Times in Einstein's General Relativity
This page was built for publication: Electromagnetic-gravitational perturbations of Kerr–Newman spacetime: The Teukolsky and Regge–Wheeler equations
