arXiv (OAI Expanded)
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DANSur_HM: Modularly incorporating higher modes in a deep learning based gravitational-wave surrogate
Numerical relativity (NR) simulations provide the most faithful representation of the gravitational waves (GWs) emitted by binary black hole (BBH) systems during merger. In the context of GW astronomy, tasks such as parameter estimation can require vast numbers of waveform evaluations per second acr
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