Gauge-invariant non-spherical metric perturbations of Schwarzschild black-hole spacetimes

DOI10.1088/0264-9381/22/16/R01zbMath1078.83024arXivgr-qc/0502064OpenAlexW3099120147MaRDI QIDQ5693547

Luciano Rezzolla, Alessandro Nagar

Publication date: 26 September 2005

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0502064

zbMATH Keywords

Schwarzschild spacetimenon-spherical metric perturbationsnumerically generated spacetimes

Mathematics Subject Classification ID

Black holes (83C57) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (14)

Extraction of gravitational waves in numerical relativity ⋮ Extreme mass ratio inspirals with scalar hair ⋮ In horizon penetrating coordinates: Kerr black hole metric perturbation, construction and completion ⋮ Gauge invariant perturbations of the Schwarzschild spacetime ⋮ Multipole expansions for energy and momenta carried by gravitational waves ⋮ Stability of the Hayward black hole under electromagnetic perturbations ⋮ Characteristic evolution and matching ⋮ Characteristic evolution and matching ⋮ Gravitational waves from gravitational collapse ⋮ Characteristic evolution and matching ⋮ EZ gauge is singular at the event horizon ⋮ Quantum gravity on the black hole horizon ⋮ Stealth black hole perturbations in kinetic gravity braiding ⋮ Continuum and discrete initial-boundary value problems and Einstein's field equations

This page was built for publication: Gauge-invariant non-spherical metric perturbations of Schwarzschild black-hole spacetimes