Quantifying excitations of quasinormal mode systems

DOI10.1063/1.532698zbMath0946.83016arXivgr-qc/9810074OpenAlexW3105527557MaRDI QIDQ4701771

Richard H. Price, Hans-Peter Nollert

Publication date: 21 November 1999

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9810074

zbMATH Keywords

black holegravitational wavesexcitation coefficient

Mathematics Subject Classification ID

Black holes (83C57) Gravitational waves (83C35)

Related Items

High-order matrix method with delimited expansion domain ⋮ Matrix method for perturbed black hole metric with discontinuity ⋮ Quasinormal modes, echoes and the causal structure of the Green's function ⋮ Thermal ringdown of a Kerr black hole: overtone excitation, Fermi-Dirac statistics and greybody factor ⋮ An integer basis for celestial amplitudes ⋮ Pseudospectra of holographic quasinormal modes ⋮ MATCHING CHARACTERISTIC CODES: EXPLOITING TWO DIRECTIONS ⋮ Quasi-normal modes and gravitational wave astronomy ⋮ Quasinormal quantization in de Sitter spacetime ⋮ Quasi-normal modes of stars and black holes ⋮ Extreme gravity tests with gravitational waves from compact binary coalescences: II: Ringdown ⋮ Energy scales and black hole pseudospectra: the structural role of the scalar product

Cites Work

• Quasinormal modes of Schwarzschild black holes: Defined and calculated via Laplace transformation
• Stability of a Schwarzschild Singularity
• Model for the completeness of quasinormal modes of relativistic stellar oscillations
• Colliding black holes: The close limit
• Second-order perturbations of a Schwarzschild black hole
• The spectrum of radial adiabatic stellar oscillations