On the effective metric of axial black hole perturbations in DHOST gravity

DOI10.1088/1475-7516/2022/08/040OpenAlexW4280507292MaRDI QIDQ5101146

Hugo Roussille, David Langlois, Karim Noui

Publication date: 2 September 2022

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

Full work available at URL: https://arxiv.org/abs/2205.07746

zbMATH Keywords

modified gravityGauss-Bonnet-Lovelock-Horndeski-Palatini etc. gravity theoriesgravitational waves in GR and beyond: theory

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Gravitational waves (83C35) Matrix models and tensor models for quantum field theory (81T32)

Related Items (4)

Generalized Regge-Wheeler equation from Effective Field Theory of black hole perturbations with a timelike scalar profile ⋮ An analytic approach to quasinormal modes for coupled linear systems ⋮ Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory ⋮ Axial perturbations of black holes in scalar-tensor gravity: near-horizon behaviour

Cites Work

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• Quasi-normal modes of stars and black holes

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