Numerical computation of quasinormal modes in the first-order approach to black hole perturbations in modified gravity

DOI10.1088/1475-7516/2024/01/054WikidataQ129334801 ScholiaQ129334801MaRDI QIDQ6497814

David Langlois, Hugo Roussille, Karim Noui

Publication date: 6 May 2024

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

zbMATH Keywords

exact solutionsmodified gravityblack holes and black hole thermodynamics in GR and beyondGauss-Bonnet-Lovelock-Horndeski-Palatini etc. gravity theoriesgravitational waves in GR and beyond: theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Cites Work

• Extreme gravity tests with gravitational waves from compact binary coalescences: II: Ringdown
• Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
• Disforming the Kerr metric
• ADVANCED METHODS IN BLACK-HOLE PERTURBATION THEORY
• Stability of a Schwarzschild Singularity
• Quasinormal modes of black holes and black branes
• Quasinormal modes: the characteristic `sound' of black holes and neutron stars
• Asymptotically flat black holes in Horndeski theory and beyond
• On rotating black holes in DHOST theories
• Linear perturbations of Einstein-Gauss-Bonnet black holes
• Hairy black holes in DHOST theories: exploring disformal transformation as a solution generating method
• General Relativity solutions with stealth scalar hair in quadratic higher-order scalar-tensor theories
• Regular black holes via the Kerr-Schild construction in DHOST theories
• Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
• Dark energy and modified gravity in degenerate higher-order scalar–tensor (DHOST) theories: A review
• Computational Aspects of Three-Term Recurrence Relations
• Quasi-normal modes of stars and black holes
• An analytic approach to quasinormal modes for coupled linear systems

This page was built for publication: Numerical computation of quasinormal modes in the first-order approach to black hole perturbations in modified gravity