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Dynamical quasinormal mode excitation

Marina De Amicis ^1,*, Enrico Cannizzaro², Gregorio Carullo ^1,3,†, and Laura Sberna ⁴

¹Center of Gravity, Niels Bohr Institute, Blegdamsvej 17, 2100 Copenhagen, Denmark
²CENTRA, Departamento de Fisica, Instituto Superior Técnico—IST, Universidade de Lisboa—UL, Avenida Rovisco Pais 1, 1049 Lisboa, Portugal
³School of Physics and Astronomy and Institute for Gravitational Wave Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, United Kingdom
⁴School of Mathematical Sciences, University of Nottingham, University Park, Nottingham NG7 2RD, United Kingdom

^*Contact author: mdeamicis@perimeterinstitute.ca
^†Contact author: g.carullo@bham.ac.uk

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Articles Citing

Dynamical quasinormal mode excitation

Green function of the Pöschl-Teller potential

Novel Ringdown Tests of General Relativity with Black Hole Graybody Factors

Quasinormal Modes Ratios as Agnostic Test of General Relativity

Singular structures and causality of the Schwarzschild Green’s function in the frequency domain

Beyond quasinormal modes: A complete mode decomposition of black hole perturbations

Pole structure of the Kerr Green’s function

Quasinormal ringing of Kerr black holes. III. Excitation coefficients for equatorial inspirals from the innermost stable circular orbit

Modeling the merger-ringdown of an eccentric test-mass inspiral into a Kerr black hole using the effective-one-body framework

Ringdown modeling for effective-one-body waveforms in the test-mass limit for eccentric equatorial orbits around a Kerr black hole

Bilinear products and the orthogonality of quasinormal modes on hyperboloidal foliations

Shaping black hole resonances: Black hole ringdown as a spectral filtering process

Resonance in black hole ringdown: Benchmarking quasinormal mode excitation and extraction

Quasinormal mode ringing of binary black hole mergers in scalar-Gauss-Bonnet gravity

Gravitational waves from the late inspiral, transition, and plunge of small-mass-ratio eccentric binaries

Decomposition of the Schwarzschild Green’s function

GW250114 reveals signatures of post-merger black-hole horizon

Eccentricity in disguise? Insights from GW231123 and numerically simulated binary black hole merger signals

Constraining the swift memory burden effect with GW250114-like events

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