Fast Bayesian gravitational wave parameter estimation using convolutional neural networks
M. Andr\'es-Carcasona, M. Martinez, Ll.M. Mir

TL;DR
This paper introduces a convolutional neural network method for rapid Bayesian gravitational wave parameter estimation, significantly reducing computation time while providing compatible posterior distributions and useful initial parameter indications.
Contribution
The paper presents a novel CNN-based approach that accelerates gravitational wave parameter estimation, enabling real-time analysis and initial parameter insights, which is a significant advancement over traditional Bayesian methods.
Findings
CNN produces posterior distributions compatible with traditional methods.
Inference speed is reduced by orders of magnitude.
Provides valuable initial parameter estimates for multi-messenger astronomy.
Abstract
The determination of the physical parameters of gravitational wave events is a fundamental pillar in the analysis of the signals observed by the current ground-based interferometers. Typically, this is done using Bayesian inference approaches which, albeit very accurate, are very computationally expensive. We propose a convolutional neural network approach to perform this task. The convolutional neural network is trained using simulated signals injected in a Gaussian noise. We verify the correctness of the neural network's output distribution and compare its estimates with the posterior distributions obtained from traditional Bayesian inference methods for some real events. The results demonstrate the convolutional neural network's ability to produce posterior distributions that are compatible with the traditional methods. Moreover, it achieves a remarkable inference speed, lowering by…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gaussian Processes and Bayesian Inference
