Spectral Problems for Quasinormal Modes of Black Holes
arXiv:2111.15197 · doi:10.3390/universe7120476
Abstract
This is an unconventional review article on spectral problems in black hole perturbation theory. Our purpose is to explain how to apply various known techniques in quantum mechanics to such spectral problems. The article includes analytical/numerical treatments, semiclassical perturbation theory, the (uniform) WKB method and useful mathematical tools: Borel summations, Padé approximants, etc. The article is not comprehensive, but rather looks into a few examples from various points of view. The techniques in this article are widely applicable to many other examples.
This is a contribution to the special issue "Black Hole Physics and Beyond: From the Ringdown Analysis with Gravitational Waves" (Editors: Hiroyuki Nakano and Nami Uchikata) in Universe. V2: Published version. V3: Minor revision
References in corpus (9)
- Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
- Quasi-Normal Modes and Gravitational Wave Astronomy
- Quasinormal ringing of Kerr black holes: The excitation factors
- Gravitational ringing of rotating black holes in higher-derivative gravity
- Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity
- Isomonodromy, Painlevé Transcendents and Scattering off of Black Holes
- A simple test for stability of black hole by -deformation
- Semi-analytic expressions for quasinormal modes of slowly rotating Kerr black holes
- Master Functions and Equations for Perturbations of Vacuum Spherically-Symmetric Spacetimes