Effective Field Theory for the Perturbations of a Slowly Rotating Black Hole
arXiv:2111.02072 · doi:10.1007/JHEP12(2021)183
Abstract
We develop the effective theory for perturbations around black holes with scalar hair, in two directions. First, we show that the scalar-Gauss--Bonnet theory, often used as an example exhibiting scalar black hole hair, can be deformed by galileon operators leading to order unity changes to its predictions. The effective theory for perturbations thus provides an efficient framework for describing and constraining broad classes of scalar-tensor theories, of which the addition of galileon operators is an example. Second, we extend the effective theory to perturbations around an axisymmetric, slowly rotating black hole, at linear order in the black hole spin. We also discuss the inclusion of parity-breaking operators in the effective theory.
References in corpus (67)
- Quasinormal modes of black holes and black branes
- The galileon as a local modification of gravity
- The Effective Field Theory of Inflation
- Causality, Analyticity and an IR Obstruction to UV Completion
- Chern-Simons Modification of General Relativity
- Chern-Simons Modified General Relativity
- Dilatonic Black Holes in Higher Curvature String Gravity
- Black hole hair in generalized scalar-tensor gravity
- Dressing a black hole with a time-dependent Galileon
- Black hole hair in generalized scalar-tensor gravity: An explicit example
- Dynamical Chern-Simons Modified Gravity I: Spinning Black Holes in the Slow-Rotation Approximation
- A no-hair theorem for the galileon
- Black hole ringdown: the importance of overtones
- Regular Black Hole Metric with Three Constants of Motion
- Perturbations of slowly rotating black holes: massive vector fields in the Kerr metric
- Perturbed black holes in Einstein-dilaton-Gauss-Bonnet gravity: Stability, ringdown, and gravitational-wave emission
- Black-Hole Solutions with Scalar Hair in Einstein-Scalar-Gauss-Bonnet Theories
- Slowly Rotating Black Holes in Dynamical Chern-Simons Gravity: Deformation Quadratic in the Spin
- Asymptotically flat black holes in Horndeski theory and beyond
- Advanced Methods in Black-Hole Perturbation Theory
- Slowly rotating black holes in alternative theories of gravity
- Gravitational signature of Schwarzschild black holes in dynamical Chern-Simons gravity
- Black holes and binary mergers in scalar Gauss-Bonnet gravity: scalar field dynamics
- The Kerr Metric
- The effects of Chern-Simons gravity on bodies orbiting the Earth
- Fundamental physics implications on higher-curvature theories from the binary black hole signals in the LIGO-Virgo Catalog GWTC-1
- Parametrized black hole quasinormal ringdown. I. Decoupled equations for nonrotating black holes
- Black hole perturbation in the most general scalar-tensor theory with second-order field equations I: The odd-parity sector
- Black hole perturbation in the most general scalar-tensor theory with second-order field equations II: the even-parity sector
- An effective formalism for testing extensions to General Relativity with gravitational waves
- Improved gravitational-wave constraints on higher-order curvature theories of gravity
- Rotating black hole in extended Chern-Simons modified gravity
- Static response and Love numbers of Schwarzschild black holes
- Parametrized black hole quasinormal ringdown. II. Coupled equations and quadratic corrections for nonrotating black holes
- How do Black Holes Spin in Chern-Simons Modified Gravity?
- Perturbations of Schwarzschild black holes in Dynamical Chern-Simons modified gravity
- Weakly Broken Galileon Symmetry
- Effective Field Theory of Black Hole Quasinormal Modes in Scalar-Tensor Theories
- Gravitational ringing of rotating black holes in higher-derivative gravity
- Quasinormal modes of slowly-rotating black holes in dynamical Chern-Simons gravity
- Ringing of rotating black holes in higher-derivative gravity
- Parametrized ringdown spin expansion coefficients: a data-analysis framework for black-hole spectroscopy with multiple events
- Perturbations of Schwarzschild Black Holes in Chern-Simons Modified Gravity
- Fundamental theorem on gauge fixing at the action level
- Eikonal quasinormal modes of black holes beyond General Relativity
- Hairy black holes in DHOST theories: Exploring disformal transformation as a solution-generating method
- The Darboux transformation in black hole perturbation theory
- Analytical computation of quasi-normal modes of slowly-rotating black-holes in dCS gravity
- LISA parameter estimation and source localization with higher harmonics of the ringdown
- Stealth Schwarzschild solution in shift symmetry breaking theories
- General theories of linear gravitational perturbations to a Schwarzschild Black Hole
- Inflation from Minkowski Space
- Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky
- Asymptotically flat, parameterized black hole metric preserving Kerr symmetries
- Spinning black holes in shift-symmetric Horndeski theory
- A Parametrized post-Einsteinian Framework for Gravitational Wave Bursts
- Eikonal quasinormal modes of black holes beyond general relativity III: scalar Gauss-Bonnet gravity
- Scalar Deformations of Schwarzschild Holes and Their Stability
- Eikonal quasinormal modes of black holes beyond general relativity II: generalised scalar-tensor perturbations
- Behind Horndeski: Structurally Robust Higher Derivative EFTs
- Stable wormholes in scalar-tensor theories
- Parametrizing and constraining scalar corrections to general relativity
- Hairy Black-holes in Shift-symmetric Theories
- More about stable wormholes in beyond Horndeski theory
- Black Hole Ringdown as a Probe for Dark Energy
- Stability analysis of Schwarzschild black holes in dynamical Chern-Simons gravity
- Black hole perturbations of massive and partially massless spin-2 fields in (anti) de Sitter spacetime
Cited by in corpus (27)
- Generation and propagation of nonlinear quasi-normal modes of a Schwarzschild black hole
- Black-hole ringdown as a probe of higher-curvature gravity theories
- Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory
- Effective Field Theory of Black Hole Perturbations with Timelike Scalar Profile: Formulation
- Quasinormal Modes from EFT of Black Hole Perturbations with Timelike Scalar Profile
- Generalized Regge-Wheeler Equation from Effective Field Theory of Black Hole Perturbations with a Timelike Scalar Profile
- Quasi-normal modes of non-separable perturbation equations: the scalar non-Kerr case
- Black hole hairs in scalar-tensor gravity and the lack thereof
- Tidal Love Numbers from EFT of Black Hole Perturbations with Timelike Scalar Profile
- Effective description of generalized disformal theories
- Vanishing of Quadratic Love Numbers of Schwarzschild Black Holes
- Stability of Hairy Black Holes in Shift-Symmetric Scalar-Tensor Theories via the Effective Field Theory Approach
- General Effective Field Theory of Teleparallel Gravity
- Linear perturbations of Einstein-Gauss-Bonnet black holes
- On the effective metric of axial black hole perturbations in DHOST gravity
- Consistency of matter coupling in modified gravity
- Testing the Speed of Gravity with Black Hole Ringdown
- How Do Axisymmetric Black Holes Grow Monopole and Dipole Hair?
- Black hole minimum size and scalar charge in shift-symmetric theories
- Ringdowns for black holes with scalar hair: the large mass case
- An analytic approach to quasinormal modes for coupled linear systems
- Causality and Stability from Acoustic Geometry
- Exact solution for rotating black holes in parity-violating gravity
- Axial perturbations of black holes in scalar-tensor gravity: near-horizon behaviour
- Axial Gravitational Perturbations of Slowly-Rotating Compact Objects in General Relativity and Beyond
- Superradiant instability in slowly rotating Kerr-Newman black holes
- On the logarithmic Love number of black holes beyond general relativity