Are eikonal quasinormal modes linked to the unstable circular null geodesics?

DOI10.1016/j.physletb.2017.06.015zbMath1372.83045arXiv1705.05928OpenAlexW2616547010MaRDI QIDQ2410202

Zdeněk Stuchlík, Roman A. Konoplya

Publication date: 17 October 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1705.05928

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Equations of motion in general relativity and gravitational theory (83C10)

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Cites Work

• Symmetric solutions to the maximally Gauss-Bonnet extended Einstein equations
• Master Equations for Gravitational Perturbations of Static Lovelock Black Holes in Higher Dimensions
• Lyapunov timescales and black hole binaries
• The Einstein Tensor and Its Generalizations
• Schwarzschild field inn dimensions and the dimensionality of space problem
• Quasi-normal modes of stars and black holes
• Upper bound on the radii of black-hole photonspheres
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