Horizon radiation reaction forces
arXiv:2007.00731 · doi:10.1007/JHEP10(2020)026
Abstract
Using Effective Field Theory (EFT) methods, we compute the effects of horizon dissipation on the gravitational interactions of relativistic binary black hole systems. We assume that the dynamics is perturbative, i.e it admits an expansion in powers of Newton's constant (post-Minkowskian, or PM, approximation). As applications, we compute corrections to the scattering angle in a black hole collision due to dissipative effects to leading PM order, as well as the post-Newtonian (PN) corrections to the equations of motion of binary black holes in non-relativistic orbits, which represents the leading order finite size effect in the equations of motion. The methods developed here are also applicable to the case of more general compact objects, eg. neutron stars, where the magnitude of the dissipative effects depends on non-gravitational physics (e.g, the equation of state for nuclear matter).
arXiv comment15 pages LaTex, 1 figure
References in corpus (43)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Tidal Love numbers of neutron stars
- Effective one-body approach to general relativistic two-body dynamics
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- New Developments in FeynCalc 9.0
- Transition from inspiral to plunge in binary black hole coalescences
- Relativistic theory of tidal Love numbers
- An Effective Field Theory of Gravity for Extended Objects
- Scattering Amplitudes and the Conservative Hamiltonian for Binary Systems at Third Post-Minkowskian Order
- Amplitudes, Observables, and Classical Scattering
- Black Hole Binary Dynamics from the Double Copy and Effective Theory
- From Scattering Amplitudes to Classical Potentials in the Post-Minkowskian Expansion
- Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory
- High-energy gravitational scattering and the general relativistic two-body problem
- Scattering of Spinning Black Holes from Exponentiated Soft Factors
- Classical Space-Times from the S Matrix
- From Boundary Data to Bound States
- Observables and amplitudes for spinning particles and black holes
- Scattering of two spinning black holes in post-Minkowskian gravity, to all orders in spin, and effective-one-body mappings
- Black-hole scattering with general spin directions from minimal-coupling amplitudes
- Classical and quantum scattering in post-Minkowskian gravity
- Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections
- Black hole stereotyping: Induced gravito-static polarization
- Dissipative Effects in the Worldline Approach to Black Hole Dynamics
- On Post-Minkowskian Hamiltonians in General Relativity
- From Boundary Data to Bound States II: Scattering Angle to Dynamical Invariants (with Twist)
- Energetics of two-body Hamiltonians in post-Minkowskian gravity
- Absorption of mass and angular momentum by a black hole: Time-domain formalisms for gravitational perturbations, and the small-hole/slow-motion approximation
- Spinning-black-hole scattering and the test-black-hole limit at second post-Minkowskian order
- Absorption Effects due to Spin in the Worldline Approach to Black Hole Dynamics
- Post-Minkowskian Scattering Angle in Einstein Gravity
- Radiation reaction and gravitational waves in the effective field theory approach
- Second-order Post-Minkowskian scattering in arbitrary dimensions
- Post-Newtonian Expansion of Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole :Effects of Black Hole Absorption
- Gravitational spin-orbit coupling in binary systems at the second post-Minkowskian approximation
- On the gravitational polarizability of black holes
- A Modern Approach to Superradiance
- Scattering of tidally interacting bodies in post-Minkowskian gravity
- Test black holes, scattering amplitudes and perturbations of Kerr spacetime
- From Scattering Amplitudes to Classical Physics: Universality, Double Copy and Soft Theorems
- An Effective Field Theory of Quantum Mechanical Black Hole Horizons
- An effective field theory approach to tidal dynamics of spinning astrophysical systems
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- Non-conservative effects on Spinning Black Holes from World-Line Effective Field Theory
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- Radiated momentum in the Post-Minkowskian worldline approach via reverse unitarity
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- Modeling horizon absorption in spinning binary black holes using effective worldline theory
- Gravitational Bremsstrahlung with tidal effects in the post-Minkowskian expansion
- Tidal response from scattering and the role of analytic continuation
- Scalar Love numbers and Love symmetries of 5-dimensional Myers-Perry black holes
- Quantum Hotspots: Mean Fields, Open EFTs, Nonlocality and Decoherence Near Black Holes
- Soft graviton exchange and the information paradox
- Qubit Heating Near a Hotspot
- Post-Newtonian templates for gravitational waves from compact binary inspirals
- Waveforms from Amplitudes
- Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results
- Quantum Effects for Black Holes with On-Shell Amplitudes
- Resummed energy loss in extreme-mass-ratio scattering using critical orbits
- Influence Through Mixing: Hotspots as Benchmarks for Basic Black-Hole Behaviour
- Gravitational Wave Signals from Finite Size Effects in Spinning Binary Inspirals Including Parity Violating Constituents