The linear stability of Reissner-Nordström spacetime: the full subextremal range \(|Q|
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Publication:2216774
DOI10.1007/s00220-020-03893-zzbMath1468.35200arXiv1910.05630OpenAlexW2979748734MaRDI QIDQ2216774
Publication date: 17 December 2020
Published in: Communications in Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1910.05630
Related Items (9)
Stable black holes: in vacuum and beyond ⋮ Precise late-time asymptotics of scalar field in the interior of a subextreme Kerr black hole and its application in Strong Cosmic Censorship conjecture ⋮ Peeling for tensorial wave equations on Schwarzschild spacetime ⋮ Price's law for spin fields on a Schwarzschild background ⋮ Sharp decay for Teukolsky equation in Kerr spacetimes ⋮ Conformal scattering theories for tensorial wave equations on Schwarzschild spacetime ⋮ Conformal scattering theory for the linearized gravity fields on Schwarzschild spacetime ⋮ Uniform energy bound and Morawetz estimate for extreme components of spin fields in the exterior of a slowly rotating Kerr black hole. I: Maxwell field ⋮ Sharp decay estimates for massless Dirac fields on a Schwarzschild background
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Stability and instability of extreme Reissner-Nordström black hole spacetimes for linear scalar perturbations. I
- Stability and instability of extreme Reissner-Nordström black hole spacetimes for linear scalar perturbations. II
- The global stability of Minkowski space-time in harmonic gauge
- 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
- The spin \(\pm 1\) Teukolsky equations and the Maxwell system on Schwarzschild
- Boundedness and decay for the Teukolsky system of spin \(\pm 2\) on Reissner-Nordström spacetime: the case \(|Q| \ll M\)
- Nonlinear scalar perturbations of extremal Reissner-Nordström spacetimes
- Boundedness and decay for the Teukolsky equation on Kerr spacetimes. I: The case \(|a|\ll M\)
- Mathematical problems of general relativity. I.
- The linear stability of the Schwarzschild solution to gravitational perturbations
- The linear stability of Reissner-Nordström spacetime for small charge
- Mode stability of the Kerr black hole
- A new physical-space approach to decay for the wave equation with applications to black hole spacetimes
- Stability of a Schwarzschild Singularity
- DECAY OF THE MAXWELL FIELD ON THE SCHWARZSCHILD MANIFOLD
- The red‐shift effect and radiation decay on black hole spacetimes
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- 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
- Analysis of linear waves near the Cauchy horizon of cosmological black holes
- Note on the Kerr Spinning-Particle Metric
- Exact Space-Times in Einstein's General Relativity
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