Learning Inspiral-Merger-Ringdown Waveforms from a Post-Newtonian Baseline
gr-qc, astro-ph.HE
Submitted: 2026-09-24
Updated: 2026-09-24
Terminology
Sources
- Effective one-body approach to general relativistic two-body dynamics
- Transition from inspiral to plunge in binary black hole coalescences
- Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism
- Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins
- Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
- Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
- Fast and accurate prediction of numerical relativity waveforms from binary black hole coalescences using surrogate models
- A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
- Surrogate models for precessing binary black hole simulations with unequal masses
- Statistical Gravitational Waveform Models: What to Simulate Next?
- Reduced-order modeling with artificial neurons for gravitational-wave inference
- Regression methods in waveform modeling: a comparative study
- Machine Learning Gravitational Waves from Binary Black Hole Mergers
- Gravitational-wave surrogate models powered by artificial neural networks: The ANN-Sur for waveform generation
- Accelerating multimodal gravitational waveforms from precessing compact binaries with artificial neural networks
- Interpretable AI forecasting for numerical relativity waveforms of quasi-circular, spinning, non-precessing binary black hole mergers
- A Deep Learning Powered Numerical Relativity Surrogate for Binary Black Hole Waveforms
- Learning orbital dynamics of binary black hole systems from gravitational wave measurements
- Learning Post-Newtonian Corrections from Numerical Relativity
- KAN: Kolmogorov-Arnold Networks
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