Gravitational-wave surrogate models powered by artificial neural networks: The ANN-Sur for waveform generation
Sebastian Khan, Rhys Green

TL;DR
This paper introduces ANN-Sur, a neural network-based surrogate model for gravitational-wave waveform generation that significantly accelerates Bayesian inference processes in GW astronomy.
Contribution
The paper presents a novel neural network surrogate model, ANN-Sur, that efficiently generates gravitational-wave waveforms, outperforming existing methods in speed while maintaining high accuracy.
Findings
ANN-Sur achieves median mismatch of 2e-5.
Waveform generation on GPU takes only 0.4 ms.
Batch processing of 10^4 waveforms is possible in 163 ms.
Abstract
Inferring the properties of black holes and neutron stars is a key science goal of gravitational-wave (GW) astronomy. To extract as much information as possible from GW observations we must develop methods to reduce the cost of Bayesian inference. In this paper, we use artificial neural networks (ANNs) and the parallelisation power of graphics processing units (GPUs) to improve the surrogate modelling method, which can produce accelerated versions of existing models. As a first application of our method, ANN-Sur, we build a time-domain surrogate model of the spin-aligned binary black hole (BBH) waveform model SEOBNRv4. We achieve median mismatches of 2e-5 and mismatches no worse than 2e-3. For a typical BBH waveform generated from 12 Hz with a total mass of the original SEOBNRv4 model takes 1812 ms. Existing bespoke code optimisations (SEOBNRv4opt) reduced this to 91.6 ms…
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