Gauge invariant perturbations of the Schwarzschild spacetime
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Publication:5369349
DOI10.1088/1361-6382/aa7f5bzbMath1372.83051arXiv1611.06214OpenAlexW3099937388MaRDI QIDQ5369349
Hector Chen, Jonathan E. Thompson, Bernard F. Whiting
Publication date: 17 October 2017
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1611.06214
perturbationSchwarzschildgauge invariantgravitational self-force problemRegge-Wheeler (RW) formalism
Black holes (83C57) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (5)
Gauge invariants of linearized gravity with a general background metric ⋮ Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory ⋮ Compatibility complex for black hole spacetimes ⋮ Master equations and stability of Einstein-Maxwell-scalar black holes ⋮ EZ gauge is singular at the event horizon
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- Energy and angular momentum of the weak gravitational waves on the Schwarzschild background. -- Quasilocal gauge-invariant formulation
- Effective source approach to self-force calculations
- High-order gauge-invariant perturbations of a spherical spacetime
- Gravitational Field of a Particle Falling in a Schwarzschild Geometry Analyzed in Tensor Harmonics
- Stability of a Schwarzschild Singularity
- Observables and gauge invariance in the theory of nonlinear spacetime perturbations
- Gauge-invariant non-spherical metric perturbations of Schwarzschild black-hole spacetimes
- The motion of point particles in curved spacetime
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