Lightning-Fast Gravitational Wave Parameter Inference through Neural Amortization
arXiv:2010.12931
Abstract
Gravitational waves from compact binaries measured by the LIGO and Virgo detectors are routinely analyzed using Markov Chain Monte Carlo sampling algorithms. Because the evaluation of the likelihood function requires evaluating millions of waveform models that link between signal shapes and the source parameters, running Markov chains until convergence is typically expensive and requires days of computation. In this extended abstract, we provide a proof of concept that demonstrates how the latest advances in neural simulation-based inference can speed up the inference time by up to three orders of magnitude -- from days to minutes -- without impairing the performance. Our approach is based on a convolutional neural network modeling the likelihood-to-evidence ratio and entirely amortizes the computation of the posterior. We find that our model correctly estimates credible intervals for the parameters of simulated gravitational waves.
arXiv commentV1: First version; V2: Updated references; V3: Update references and camera-ready version; V4: Correct figure labels; V5: Updated references
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- Swift sky localization of gravitational waves using deep learning seeded importance sampling
- Neural Simulation-Based Inference of the Neutron Star Equation of State directly from Telescope Spectra
- Fast Likelihood-free Reconstruction of Gravitational Wave Backgrounds
- Simulation-based Inference for Gravitational-waves from Intermediate-Mass Binary Black Holes in Real Noise
- Arbitrary Marginal Neural Ratio Estimation for Simulation-based Inference
- Rapid Parameter Estimation for Merging Massive Black Hole Binaries Using Continuous Normalizing Flows
- Group equivariant neural posterior estimation
- Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses