Generative adversarial network for stellar core-collapse gravitational waves
Tarin Eccleston, Matthew C. Edwards

TL;DR
This paper introduces a deep learning-based emulator for stellar core-collapse gravitational wave signals, enabling rapid and realistic waveform generation by learning from existing simulation data.
Contribution
A novel deep convolutional GAN trained on waveform data to efficiently generate realistic core-collapse gravitational wave signals.
Findings
The DCGAN accurately captures key features of the waveforms.
The emulator produces realistic signals with core-collapse, bounce, and ringdown features.
It serves as a phenomenological model for gravitational waves from stellar core-collapse.
Abstract
We present a rapid stellar core-collapse waveform emulator built using a deep convolutional generative adversarial network (DCGAN). The DCGAN was trained on the Richers \textit{et al.~}\cite{richers:2017} waveform catalogue to learn the structure of rotating stellar core-collapse gravitational-wave signals and generate realistic waveforms. We show that the DCGAN learns the distribution of the training data reasonably well, and that the waveform emulator produces signals that appear to have the key features of core-collapse, bounce, early post-bounce, and ringdown oscillations of the early proto-neutron star. The pre-trained DCGAN can therefore be used as a phenomenological model for rotating stellar core-collapse gravitational-waves.
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Taxonomy
TopicsStatistical and numerical algorithms · Time Series Analysis and Forecasting · Gamma-ray bursts and supernovae
