Effective Field Theory of Black Hole Echoes
arXiv:1808.00847 · doi:10.1007/JHEP09(2018)113
Abstract
Gravitational wave `echoes' during black-hole merging events have been advocated as possible signals of modifications to gravity in the strong-field (but semiclassical) regime. In these proposals the observable effect comes entirely from the appearance of nonzero reflection probability at the horizon, which vanishes for a standard black hole. We show how to apply EFT reasoning to these arguments, using and extending earlier work for localized systems that relates choices of boundary condition to the action for the physics responsible for these boundary conditions. EFT reasoning applied to this action argues that linear `Robin' boundary conditions dominate at low energies, and we determine the relationship between the corresponding effective coupling (whose value is the one relevant low-energy prediction of particular modifications to General Relativity for these systems) and the phenomenologically measurable near-horizon reflection coefficient. Because this connection involves only near-horizon physics it is comparatively simple to establish, and we do so for perturbations in both the Schwarzschild geometry (which is the one most often studied theoretically) and the Kerr geometry (which is the one of observational interest for post-merger ring down). In passing we identify the renormalization-group evolution of the effective couplings as a function of a regularization distance from the horizon, that enforces how physics does not depend on the precise position where the boundary conditions are imposed. We show that the perfect-absorber/perfect-emitter boundary conditions of General Relativity correspond to the only fixed points of this evolution. Nontrivial running of all other RG evolution reflects how modifications to gravity necessarily introduce new physics near the horizon.
arXiv commentv3: clarified role of IR Black Hole fixed point w.r.t. parameter ξ. v2: now published in JHEP; references added, changed definition of time delay and phase in echo spacing
References in corpus (38)
- The Confrontation between General Relativity and Experiment
- Testing General Relativity with Present and Future Astrophysical Observations
- Black Holes: Complementarity or Firewalls?
- Tests of general relativity from timing the double pulsar
- Evidence for Efimov quantum states in an ultracold gas of cesium atoms
- The fuzzball proposal for black holes: an elementary review
- Echoes of ECOs: gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale
- AdS/CFT duality and the black hole information paradox
- Testing General Relativity with Pulsar Timing
- Echoes from the Abyss: Tentative evidence for Planck-scale structure at black hole horizons
- Statistical interpretation of Bekenstein entropy for systems with a stretched horizon
- Echoes of Kerr-like wormholes
- A recipe for echoes from exotic compact objects
- Black Hole Based Tests of General Relativity
- Low significance of evidence for black hole echoes in gravitational wave data
- Efimov Physics in Cold Atoms
- Gravitational wave echoes through new windows
- Exotic Compact Objects and How to Quench their Ergoregion Instability
- Anomaly in conformal quantum mechanics: From molecular physics to black holes
- Analytical template for gravitational-wave echoes: signal characterization and prospects of detection with current and future interferometers
- Parameter estimation of gravitational wave echoes from exotic compact objects
- Black hole ringdown echoes and howls
- A morphology-independent data analysis method for detecting and characterizing gravitational wave echoes
- Black Hole Echology: The Observer's Manual
- Nonrelativistic inverse square potential, scale anomaly, and complex extension
- Black Hole Thermodynamics from Near-Horizon Conformal Quantum Mechanics
- Characterization of echoes: A Dyson-series representation of individual pulses
- Pauli Blocking Effect on Efimov States Near Feshbach Resonance
- Efimov physics from a renormalization group perspective
- Point-Particle Effective Field Theory I: Classical Renormalization and the Inverse-Square Potential
- Semiclassical Methods in Curved Spacetime and Black Hole Thermodynamics
- Effective Conformal Descriptions of Black Hole Entropy: A Review
- Point-Particle Effective Field Theory II: Relativistic Effects and Coulomb/Inverse-Square Competition
- Static Kerr Green's Function in Closed Form and an Analytic Derivation of the Self-Force for a Static Scalar Charge in Kerr Space-Time
- Point-Particle Effective Field Theory III: Relativistic Fermions and the Dirac Equation
- Conformal Tightness of Holographic Scaling in Black Hole Thermodynamics
- Fall to the Centre in Atom Traps and Point-Particle EFT for Absorptive Systems
- Conformal Enhancement of Holographic Scaling in Black Hole Thermodynamics: A Near-Horizon Heat-Kernel Framework
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- New Horizons for Fundamental Physics with LISA
- Phenomenological aspects of black holes beyond general relativity
- Ergoregion instability of exotic compact objects: electromagnetic and gravitational perturbations and the role of absorption
- Analytical model for gravitational-wave echoes from spinning remnants
- Echoes from Quantum Black Holes
- Black-hole microstate spectroscopy: ringdown, quasinormal modes, and echoes
- On Reflectivity of Quantum Black Hole Horizons
- Echoes from phantom wormholes
- On an alternative mechanism for the black hole echoes
- GW190521: Search for Echoes due to Stimulated Hawking Radiation from Black Holes
- Constraining Fundamental Physics with the Event Horizon Telescope
- Effective master equations for two accelerated qubits
- Quantum Hotspots: Mean Fields, Open EFTs, Nonlocality and Decoherence Near Black Holes
- Nonlinear treatment of a black hole mimicker ringdown
- Tidal response and near-horizon boundary conditions for spinning exotic compact objects
- Qubit Heating Near a Hotspot
- Testing the nature of dark compact objects with gravitational waves
- Mixing of gravitational wave echoes
- On echo intervals in gravitational wave echo analysis
- On Black Hole Echoes
- Near-horizon microstructure and superradiant instability of black holes
- Superradiant instabilities of massive bosons around exotic compact objects
- Duality between the quantum inverted harmonic oscillator and inverse square potentials
- Echoes from corpuscular black holes
- Echoes from beyond: Detecting gravitational-wave quantum imprints with LISA
- The Fredholm Approach to Charactize Gravitational Wave Echoes
- Reflecting boundary conditions in numerical relativity as a model for black hole echoes
- On the Interaction between Ultralight Bosons and Quantum-Corrected Black Holes
- Precision Nuclear-Spin Effects in Atoms: EFT Methods for Reducing Theory Errors
- Formulating the complete initial boundary value problem in numerical relativity to model black hole echoes
- Signatures of Quantum Gravity in Gravitational Wave Memory
- Superradiant instability of area quantized Kerr black hole with discrete reflectivity
- Influence Through Mixing: Hotspots as Benchmarks for Basic Black-Hole Behaviour
- Implications of the quantum nature of the black hole horizon on the gravitational-wave ringdown