Autoencoder based surrogate model for gravitational waves from BBH mergers

          @misc{ scivideos_oai:cds.cern.ch:3025600,
            doi = {},
            url = {https://videos.cern.ch/record/3025600},
            author = {},
            keywords = {},
            language = {en},
            title = {Autoencoder based surrogate model for gravitational waves from BBH mergers},
            publisher = {},
            year = {2026},
            month = {may},
            note = {oai:cds.cern.ch:3025600 see, \url{https://scivideos.org/cern-cds/3025600}}
          }
          

Abstract

The generation of accurate waveforms from binary black hole (BBH) mergers is a major effort in Gravitational-Wave Astronomy. In recent years, machine-learning-based surrogate models for BBH waveforms have been proposed. Those offer the potential to dramatically accelerate waveform generation while maintaining accuracy competitive with that of traditional waveform approximants. In this work, we investigate the viability of autoencoders as generative models for gravitational-wave signals from quasi-circular BBH mergers. We introduce AESur3dq8, a novel surrogate waveform model based on autoencoders that enables the rapid and accurate construction of large template banks, producing millions of waveforms in under a second using modest computational resources. The model is trained on the numerical-relativity-informed surrogate NRHybSur3dq8 and subsequently fine-tuned using the SXS catalog of BBH simulations. We demonstrate that waveforms generated by AESur3dq8 achieve mismatches of order $10^{-4}$ with respect to Numerical Relativity waveforms, and that parameter estimation performed with these templates yields results fully consistent with those reported by the LIGO-Virgo-KAGRA Collaboration for observed gravitational-wave events.

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