Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory
DOI10.1088/1475-7516/2023/07/001zbMath1528.83029arXiv2305.09187OpenAlexW4382988572MaRDI QIDQ6116488
Publication date: 18 July 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.09187
gravitymodified gravityGauss-Bonnet-Lovelock-Horndeski-Palatini etc. gravity theoriesgravitational waves in GR and beyond: theory
Black holes (83C57) Applications of differential geometry to physics (53Z05) Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Electromagnetic theory (general) (78A25) Gravitational waves (83C35) Systems of nonlinear higher-order PDEs (35G50) Effective quantum field theories (81T12)
Related Items (2)
Cites Work
- Grey-body factors and Hawking radiation of black holes in \(4D\) Einstein-Gauss-Bonnet gravity
- Effective field theory of black hole quasinormal modes in scalar-tensor theories
- Effective field theory for the perturbations of a slowly rotating black hole
- Are eikonal quasinormal modes linked to the unstable circular null geodesics?
- Further clarification on quasinormal modes/circular null geodesics correspondence
- Effective field theory of cosmological perturbations
- Gravitational radiation from dynamical black holes
- Quasi-normal modes of Schwarzschild–de Sitter black holes
- Existence and instability of hairy black holes in shift-symmetric Horndeski theories
- Generalized Regge-Wheeler equation from Effective Field Theory of black hole perturbations with a timelike scalar profile
- Quasinormal ringing of regular black holes in asymptotically safe gravity: the importance of overtones
- Black hole perturbations in DHOST theories: master variables, gradient instability, and strong coupling
- Higher derivative scalar tensor theory in unitary gauge
- On the effective metric of axial black hole perturbations in DHOST gravity
- Effective field theory of black hole perturbations with timelike scalar profile: formulation
- Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
- Quasinormal modes of Kerr–de Sitter black holes via the Heun function
- Quasi-normal modes of the scalar hairy black hole
- How general is the strong cosmic censorship bound for quasinormal modes?
- Stability of hairy black holes in shift-symmetric scalar-tensor theories via the effective field theory approach
- Thermal ringdown of a Kerr black hole: overtone excitation, Fermi-Dirac statistics and greybody factor
- Quasinormal modes from EFT of black hole perturbations with timelike scalar profile
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