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It is broadly believed that quasinormal modes cannot tell the black-hole near-horizon geometry, because usually the low-lying modes are determined by the scattering of perturbations around the peak of the effective potential.
Semiclassically weak reflections above analytic and non-analytic potential barriers
M. V. Berry · 1982
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An Analytic representation for the quasi normal modes of Kerr black holes
E. W. Leaver · 1985
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Initial results in Prony analysis of power system response signals
J.F. Hauer, C.J. Demeure, and L.L. Scharf · 1990
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Quasinormal modes of Schwarzschild black holes: The determination of quasinormal frequencies with very large imaginary parts
Hans-Peter Nollert · 1993
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Late time behavior of stellar collapse and explosions: 1. Linearized perturbations
Carsten Gundlach, Richard H. Price, and Jorge Pullin · 1994
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About the significance of quasinormal modes of black holes
Hans-Peter Nollert · 1996
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Scattering by black holes: A Simulated potential approach
J. M. Aguirregabiria and C. V. Vishveshwara · 1996
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TOPICAL REVIEW: Quasinormal modes: the characteristic ‘sound’ of black holes and neutron stars
Hans-Peter Nollert · 1999
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Quasinormal modes of stars and black holes
Kostas D. Kokkotas and Bernd G. Schmidt · 1999
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Massive scalar field quasi-normal modes of higher dimensional black holes
Alexander Zhidenko · 2006
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Quasi-Normal Modes of Brane-Localised Standard Model Fields. II. Kerr Black Holes
P. Kanti, R. A. Konoplya, and A. Zhidenko · 2006
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On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA
Emanuele Berti, Vitor Cardoso, and Clifford M. Will · 2006
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Wormholes as black hole foils
Thibault Damour and Sergey N. Solodukhin · 2007
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Quasinormal frequencies of D-dimensional Schwarzschild black holes: Evaluation via continued fraction method
Andrzej Rostworowski · 2007
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Quasinormal modes of black holes and black branes
Emanuele Berti, Vitor Cardoso, and Andrei O. Starinets · 2009
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Linear perturbations of black holes: stability, quasi-normal modes and tails
Alexander Zhidenko · 2009
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The Einstein Telescope: A third-generation gravitational wave observatory
M. Punturo et al · 2010
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Quasinormal modes of black holes: From astrophysics to string theory
R. A. Konoplya and A. Zhidenko · 2011
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Thin-disc theory with a non-zero-torque boundary condition and comparisons with simulations: Thin-disc theory and simulations
Robert F. Penna, Aleksander Sądowski, and Jonathan C. McKinney · 2011
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Foundations of Black Hole Accretion Disk Theory
Marek A. Abramowicz and P. Chris Fragile · 2013
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New parametrization for spherically symmetric black holes in metric theories of gravity
Luciano Rezzolla and Alexander Zhidenko · 2014
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Gravitational wave detector with cosmological reach
Sheila Dwyer, Daniel Sigg, Stefan W. Ballmer, Lisa Barsotti, Nergis Mavalvala, and Matthew Evans · 2015
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Is the gravitational-wave ringdown a probe of the event horizon?
Vitor Cardoso, Edgardo Franzin, and Paolo Pani · 2016
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Wormholes versus black holes: quasinormal ringing at early and late times
R. A. Konoplya and A. Zhidenko · 2016
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General parametrization of axisymmetric black holes in metric theories of gravity
Roman Konoplya, Luciano Rezzolla, and Alexander Zhidenko · 2016
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Laser Interferometer Space Antenna
Pau Amaro-Seoane et al · 2017
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Binary Black Hole Mergers in the first Advanced LIGO Observing Run
B. P. Abbott et al · 2018
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Axisymmetric black holes allowing for separation of variables in the Klein-Gordon and Hamilton-Jacobi equations
Gravitational Wave Signatures of Black Hole Quasinormal Mode Instability
José Luis Jaramillo, Rodrigo Panosso Macedo, and Lamis Al Sheikh · 2022
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Destabilizing the Fundamental Mode of Black Holes: The Elephant and the Flea
Mark Ho-Yeuk Cheung, Kyriakos Destounis, Rodrigo Panosso Macedo, Emanuele Berti, and Vitor Cardoso · 2022
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Stability of the fundamental quasinormal mode in time-domain observations against small perturbations
Emanuele Berti, Vitor Cardoso, Mark Ho-Yeuk Cheung, Francesco Di Filippo, Francisco Duque, Paul Martens, and Shinji Mukohyama · 2022
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Thermal ringdown of a Kerr black hole: overtone excitation, Fermi-Dirac statistics and greybody factor
Naritaka Oshita · 2023
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Neural posterior estimation with guaranteed exact coverage: The ringdown of GW150914
Marco Crisostomi, Kallol Dey, Enrico Barausse, and Roberto Trotta · 2023
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R. A. Konoplya, Z. Stuchlík, and A. Zhidenko · 2018
Cited alongside, same era.
Black Hole Ringdown: The Importance of Overtones
Matthew Giesler, Maximiliano Isi, Mark A. Scheel, and Saul Teukolsky · 2019
Cited alongside, same era.
Testing the no-hair theorem with GW150914
Maximiliano Isi, Matthew Giesler, Will M. Farr, Mark A. Scheel, and Saul A. Teukolsky · 2019
Cited alongside, same era.
First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
Kazunori Akiyama et al · 2019
Cited alongside, same era.
General parametrization of black holes: The only parameters that matter
R. A. Konoplya and A. Zhidenko · 2020
Cited alongside, same era.
Ease of excitation of black hole ringing: Quantifying the importance of overtones by the excitation factors
Naritaka Oshita · 2021
Cited alongside, same era.
High-overtone fits to numerical relativity ringdowns: Beyond the dismissed n=8 special tone
Xisco Jiménez Forteza and Pierre Mourier · 2021
Cited alongside, same era.
Multimode Quasinormal Spectrum from a Perturbed Black Hole
Collin D. Capano, Miriam Cabero, Julian Westerweck, Jahed Abedi, Shilpa Kastha, Alexander H. Nitz, Yi-Fan Wang, Alex B. Nielsen, and Badri Krishnan · 2023
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Nonlinear Effects in Black Hole Ringdown
Mark Ho-Yeuk Cheung et al · 2023
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Nonlinearities in Black Hole Ringdowns
Keefe Mitman et al · 2023
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Slowly decaying ringdown of a rapidly spinning black hole: Probing the no-hair theorem by small mass-ratio mergers with LISA
Naritaka Oshita and Daichi Tsuna · 2023
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Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory
R. A. Konoplya · 2023
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Quasinormal modes of renormalization group improved Dymnikova regular black holes
R. A. Konoplya, Z. Stuchlik, A. Zhidenko, and A. F. Zinhailo · 2023
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Bardeen spacetime as a quantum corrected Schwarzschild black hole: Quasinormal modes and Hawking radiation
R. A. Konoplya, D. Ovchinnikov, and B. Ahmedov · 2023
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Quasinormal modes in higher-derivative gravity: Testing the black hole parametrization and sensitivity of overtones
R. A. Konoplya · 2023
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Extremal Kerr Black Holes as Amplifiers of New Physics
Gary T. Horowitz, Maciej Kolanowski, Grant N. Remmen, and Jorge E. Santos · 2023
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On the physical significance of black hole quasinormal mode spectra instability
Vitor Cardoso, Shilpa Kastha, and Rodrigo Panosso Macedo · 2024
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Quasinormal modes and their excitation beyond general relativity
Hector O. Silva, Giovanni Tambalo, Kostas Glampedakis, Kent Yagi, and Jan Steinhoff · 2024
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Long-lived quasinormal modes and oscillatory tails of the Bardeen spacetime
S. V. Bolokhov · 2024
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Overtones’ outburst of asymptotically AdS black holes
R. A. Konoplya and A. Zhidenko · 2024
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Quasinormal modes of a regular black hole with sub-Planckian curvature
Dan Zhang, Huajie Gong, Guoyang Fu, Jian-Pin Wu, and Qiyuan Pan · 2024
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Probing the Effective Quantum Gravity via Quasinormal Modes and Shadows of Black Holes
R. A. Konoplya and O. S. Stashko · 2024
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Black Hole in the Quantum Oppenheimer-Snyder model: long lived modes and the overtones’ behavior
A. F. Zinhailo · 2024
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