Purely imaginary quasinormal modes of the Kerr geometry
arXiv:1603.09710 · doi:10.1088/0264-9381/33/24/245008
Abstract
We present a method for determining the purely imaginary quasinormal modes of the Kerr geometry. Such modes have previously been explored, but we show that prior results are incorrect. The method we present, based on the theory of Heun polynomials, is very general and can be applied to a broad class of problems, making it potentially useful to all branches of physics. Furthermore, our application provides an example where the method of matched asymptotic expansions seems to have failed. A deeper understanding of why it fails in this case may provide useful insights for other situations.
5 pages, 2 figures, submitted to Phys. Rev. Letters
References in corpus (3)
Cited by in corpus (15)
- Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (II) Ringdown
- Pseudospectrum and black hole quasi-normal mode (in)stability
- Love symmetry
- High-overtone fits to numerical relativity ringdowns: beyond the dismissed n=8 special tone
- Modes of the Kerr geometry with purely imaginary frequencies
- Parametrized Black Hole Quasinormal Ringdown Formalism for Higher Overtones
- Melting of heavy vector mesons and quasinormal modes in a finite density plasma from holography
- Spectroscopy of Kerr-AdS spacetime with the Heun function: Quasinormal modes, greybody factor, and evaporation
- From quasinormal modes of rotating black strings to hydrodynamics of a moving CFT plasma
- An unknown branch of the total-transmission modes for the Kerr-geometry
- Complete quasinormal modes of Type-D black holes
- Quasinormal ringing of thick braneworlds with a finite extra dimension
- Quasinormal modes of Dirac spinors in the background of rotating black holes in four and five dimensions
- Stable spontaneously-scalarized black holes in generalized scalar-tensor theories
- Pseudospectrum and (in)stability of black hole total transmission modes