Stability of hairy black holes in shift-symmetric scalar-tensor theories via the effective field theory approach

DOI10.1088/1475-7516/2023/04/035zbMath1522.83202arXiv2208.02823OpenAlexW4365451873MaRDI QIDQ6040463

Sam S. C. Wong, Justin Khoury, Mark Trodden, Toshifumi Noumi

Publication date: 17 May 2023

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

Full work available at URL: https://arxiv.org/abs/2208.02823

zbMATH Keywords

exact solutionsmodified gravityblack holes and black hole thermodynamics in GR and beyondgravitational waves in GR and beyond: theory

Mathematics Subject Classification ID

Black holes (83C57) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Gravitational waves (83C35) Classification theory, stability, and related concepts in model theory (03C45) Effective quantum field theories (81T12)

Related Items (4)

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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