A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes

DOI10.1142/S0217732317501346zbMath1371.83104arXiv1703.06439OpenAlexW2599575748MaRDI QIDQ5363885

Elcio Abdalla, Wei-Liang Qian, Kai Lin, Alan B. Pavan

Publication date: 2 October 2017

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1703.06439

zbMATH Keywords

Taylor seriesKerr black holequasinormal modesTeukolsky equationKerr-Sen black hole

Mathematics Subject Classification ID

Black holes (83C57)

Related Items (6)

High-order matrix method with delimited expansion domain ⋮ Matrix method for perturbed black hole metric with discontinuity ⋮ Gravitational quasinormal modes of a parametrized Schwarzschild metric ⋮ Charged scalar fields around Einstein-power-Maxwell black holes ⋮ Quasinormal modes of the BTZ black hole under scalar perturbations with a non-minimal coupling: exact spectrum ⋮ Quasinormal Modes of the Planar Black Holes of a Particular Lovelock Theory

Cites Work

• Quasinormal modes of Hayward regular black hole
• Dynamical behavior and nonminimal derivative coupling scalar field of Reissner-Nordström black hole with a global monopole
• Detection of gravitational waves from black holes: is there a window for alternative theories?
• Quasinormal modes of black holes and black branes
• On an expansion method for black hole quasinormal modes and Regge poles
• Massive complex scalar field in the Kerr–Sen geometry: Exact solution of wave equation and Hawking radiation
• Quasinormal modes: the characteristic `sound' of black holes and neutron stars
• A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes
• Quasi-normal modes of stars and black holes

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