Effective field theory for the perturbations of a slowly rotating black hole
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Publication:2085371
DOI10.1007/JHEP12(2021)183OpenAlexW3208873142WikidataQ125897278 ScholiaQ125897278MaRDI QIDQ2085371
Alessandro Podo, Luca Santoni, Lam Hui, Enrico Trincherini
Publication date: 14 October 2022
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2111.02072
Related Items (12)
Linear perturbations of Einstein-Gauss-Bonnet black holes ⋮ Generalized Regge-Wheeler equation from Effective Field Theory of black hole perturbations with a timelike scalar profile ⋮ Stability of hairy black holes in shift-symmetric scalar-tensor theories via the effective field theory approach ⋮ General effective field theory of teleparallel gravity ⋮ On the effective metric of axial black hole perturbations in DHOST gravity ⋮ Effective field theory of black hole perturbations with timelike scalar profile: formulation ⋮ An analytic approach to quasinormal modes for coupled linear systems ⋮ Black hole minimum size and scalar charge in shift-symmetric theories ⋮ Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory ⋮ Effective description of generalized disformal theories ⋮ Quasinormal modes from EFT of black hole perturbations with timelike scalar profile ⋮ Axial perturbations of black holes in scalar-tensor gravity: near-horizon behaviour
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