Matrix method for perturbed black hole metric with discontinuity

DOI10.1088/1361-6382/AC95F1OpenAlexW4297520279MaRDI QIDQ5045972

Cheng-Gang Shao, Shui-Fa Shen, Wei-Liang Qian, Kai Lin, Yu Pan

Publication date: 8 November 2022

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2203.14320

zbMATH Keywords

perturbationblack holediscontinuitypseudospectrumquasinormal modesmatrix method

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Cites Work

• Quasinormal modes and shadow of a Schwarzschild black hole with GUP
• Quasinormal modes of black holes and black branes
• Black-hole spectroscopy: testing general relativity through gravitational-wave observations
• Quasinormal Modes of Dirty Black Holes
• A SELF-CONSISTENT MODEL OF THE BLACK HOLE EVAPORATION
• Quantifying excitations of quasinormal mode systems
• A Relativist's Toolkit
• 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
• A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes
• Time-delay interferometry

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