Accelerated Bayesian parameter estimation and model selection for gravitational waves with normalizing flows
Alicja Polanska, Thibeau Wouters, Peter T. H. Pang, Kaze K. W. Wong,, Jason D. McEwen

TL;DR
This paper introduces a high-performance, GPU-accelerated Bayesian inference pipeline using normalizing flows for gravitational wave data, significantly reducing computation time while maintaining accuracy.
Contribution
It develops an efficient, GPU-based Bayesian inference method with normalizing flows, integrating existing tools for faster gravitational wave parameter estimation and model selection.
Findings
GPU-based evidence estimates match traditional methods
Achieves 5-15x speedup in inference tasks
Open-source implementation ensures reproducibility
Abstract
We present an accelerated pipeline, based on high-performance computing techniques and normalizing flows, for joint Bayesian parameter estimation and model selection and demonstrate its efficiency in gravitational wave astrophysics. We integrate the Jim inference toolkit, a normalizing flow-enhanced Markov chain Monte Carlo (MCMC) sampler, with the learned harmonic mean estimator. Our Bayesian evidence estimates run on GPU are consistent with traditional nested sampling techniques run on CPU cores, while reducing the computation time by factors of and for -dimensional and -dimensional gravitational wave inference problems, respectively. Our code is available in well-tested and thoroughly documented open-source packages, ensuring accessibility and reproducibility for the wider research community.
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Taxonomy
TopicsMeteorological Phenomena and Simulations · Geophysics and Gravity Measurements · Fluid Dynamics and Turbulent Flows
