Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries
Christopher Whittall, Geraint Pratten

TL;DR
This paper introduces a neural network surrogate model for precessing binary black hole gravitational waveforms, significantly accelerating waveform generation while maintaining accuracy for Bayesian analysis.
Contribution
It develops a new neural network-based surrogate for the SEOBNRv5PHM waveform model, extending coverage to precessing binaries with high mass ratios.
Findings
Surrogate is 5 times faster than the original model on CPU.
Surrogate achieves nearly 1000 times speed-up on GPU for batch evaluations.
Faithfulness validated through Bayesian parameter inference with real and simulated data.
Abstract
Gravitational waveform templates are a key ingredient for the detection and characterization of gravitational waves emitted by compact binary mergers in the universe. These templates must be physically accurate and extensive, but also highly computationally efficient, two requirements that are often in tension. One solution to this problem is the development of surrogate models, which are fast, data-driven models trained to predict the output of a slower, physically realistic waveform model. In this article we build on existing work to incorporate machine learning techniques into the conventional reduced order surrogate framework, with a focus on extending coverage to waveform models that describe generically precessing quasicircular binaries. In particular, we present SEOBNRv5PHM_NNSur7dq10, a reduced order neural network surrogate of the SEOBNRv5PHM waveform model, valid up to mass…
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