Strong Field Scattering of Black Holes: Assessing Resummation Strategies
arXiv:2411.09652 · doi:10.1103/PhysRevD.111.064048
Abstract
Recent developments in post-Minkowksian (PM) calculations have led to a fast-growing body of weak-field perturbative information. As such, there is major interest within the gravitational wave community as to how this information can be used to improve the accuracy of theoretical waveform models. In this work, we build on recent efforts to validate high-order PM calculations using numerical relativity simulations. We present a new set of high-energy scattering simulations for equal-mass, non-spinning binary black holes, further expanding the existing suite of NR simulations. We outline the basic features of three recently proposed resummation schemes (the -resummed model, the model and the SEOB-PM model) and compare the analytical predictions to our NR data. Each model is shown to demonstrate pathological behaviour at high energies, with common features such as PM hierarchical shifts and divergences. The NR data can also be used to calibrate pseudo-5PM corrections to the scattering angle or EOB radial potentials. In each case, we argue that including higher-order information improves the agreement between the analytical models and NR, though the extent of improvement depends on how this information is incorporated and the choice of analytical baseline. Finally, we demonstrate that further resummation of the EOB radial potentials could be an effective strategy to improving the model agreement.
30 pages, 19 figures, 8 tables
References in corpus (52)
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- New Relations for Gauge-Theory Amplitudes
- Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes
- Scattering Amplitudes and the Conservative Hamiltonian for Binary Systems at Third Post-Minkowskian Order
- Black Hole Binary Dynamics from the Double Copy and Effective Theory
- Black holes and the double copy
- Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory
- IMRPhenomXHM: A multi-mode frequency-domain model for the gravitational wave signal from non-precessing black-hole binaries
- Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
- Post-Minkowskian Effective Field Theory for Conservative Binary Dynamics
- Conservative Dynamics of Binary Systems to Third Post-Minkowskian Order from the Effective Field Theory Approach
- Classical black hole scattering from a worldline quantum field theory
- Scattering Amplitudes and Conservative Binary Dynamics at
- From Boundary Data to Bound States
- 4-OGC: Catalog of gravitational waves from compact-binary mergers
- Classical and quantum scattering in post-Minkowskian gravity
- Scattering Amplitudes, the Tail Effect, and Conservative Binary Dynamics at
- Effective one body approach to the dynamics of two spinning black holes with next-to-leading order spin-orbit coupling
- Classical Gravitational Bremsstrahlung from a Worldline Quantum Field Theory
- The Eikonal Approach to Gravitational Scattering and Radiation at
- Dynamics of Binary Systems to Fourth Post-Minkowskian Order from the Effective Field Theory Approach
- A new effective-one-body description of coalescing nonprecessing spinning black-hole binaries
- Radiative contribution to classical gravitational scattering at the third order in
- From Boundary Data to Bound States II: Scattering Angle to Dynamical Invariants (with Twist)
- High-spin binary black hole mergers
- The high-energy collision of two black holes
- New binary black hole mergers in the LIGO--Virgo O3a data
- A faithful analytical effective one body waveform model for spin-aligned, moderately eccentric, coalescing black hole binaries
- Conservative Dynamics of Binary Systems at Fourth Post-Minkowskian Order in the Large-eccentricity Expansion
- Radiation Reaction and Gravitational Waves at Fourth Post-Minkowskian Order
- SEOBNRv5PHM: Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes
- Laying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes
- Radiation Reaction from Soft Theorems
- A multipolar effective one body waveform model for spin-aligned black hole binaries
- Cross section, final spin and zoom-whirl behavior in high-energy black hole collisions
- Effective one body multipolar waveform model for spin-aligned, quasi-circular, eccentric, hyperbolic black hole binaries
- Effective-one-body multipolar waveforms for eccentric binary black holes with non-precessing spins
- Gravitational Bremsstrahlung in the Post-Minkowskian Effective Field Theory
- High-velocity collision of two black holes
- Post-Minkowskian Scattering Angle in Einstein Gravity
- Radiation-Reaction in the Effective Field Theory Approach to Post-Minkowskian Dynamics
- Radiated Angular Momentum and Dissipative Effects in Classical Scattering
- A tale of two exponentiations in supergravity at subleading level
- The Third RIT binary black hole simulations catalog
- Strong-field scattering of two black holes: Numerical Relativity meets Post-Minkowskian gravity
- Radiated momentum and radiation-reaction in gravitational two-body scattering including time-asymmetric effects
- Eccentric binary black holes: Comparing numerical relativity and small mass-ratio perturbation theory
- Post-Minkowskian Theory Meets the Spinning Effective-One-Body Approach for Two-Body Scattering
- Radiation-reaction and angular momentum loss at the second Post-Minkowskian order
- Black hole scattering near the transition to plunge: Self-force and resummation of post-Minkowskian theory
- Mapping eccentricity evolutions between numerical relativity and effective-one-body gravitational waveforms
Cited by in corpus (8)
- The Science of the Einstein Telescope
- Highly accurate simulations of asymmetric black-hole scattering and cross validation of effective-one-body models
- Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results
- Strong Field Scattering of Two Black Holes: Exploring Gauge Flexibility
- Black-hole scattering with numerical relativity: Self-force extraction and post-Minkowskian validation
- Gravitational scattering of two neutron stars
- Analytic structure of the high-energy gravitational amplitude: multi-H diagrams and classical 5PM logarithms
- Parameter control for binary black hole initial data