A model problem for quasinormal ringdown of asymptotically flat or extremal black holes
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Publication:5141088
DOI10.1063/5.0024699zbMath1455.83015arXiv1910.08481OpenAlexW3093869563WikidataQ113281474 ScholiaQ113281474MaRDI QIDQ5141088
Dejan Gajic, Claude M. Warnick
Publication date: 17 December 2020
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1910.08481
Black holes (83C57) Wave equation (35L05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (7)
Hidden spectral symmetries and mode stability of subextremal Kerr(-de Sitter) black holes ⋮ Characteristic approach to the soliton resolution ⋮ Analyticity of quasinormal modes in the Kerr and Kerr-De Sitter spacetimes ⋮ Outgoing solutions via Gevrey-2 properties ⋮ Quasinormal modes in extremal Reissner-Nordström spacetimes ⋮ Existence of zero-damped quasinormal frequencies for nearly extremal black holes ⋮ Energy scales and black hole pseudospectra: the structural role of the scalar product
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- An introduction to partial differential equations
- Outgoing solutions via Gevrey-2 properties
- Boundedness and growth for the massive wave equation on asymptotically anti-de Sitter black holes
- On quasinormal modes of asymptotically anti-de Sitter black holes
- A new physical-space approach to decay for the wave equation with applications to black hole spacetimes
- A global definition of quasinormal modes for Kerr–AdS black holes
- Mathematical Theory of Scattering Resonances
- Horizon instability of extremal black holes
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