Costs of Bayesian Parameter Estimation in Third-Generation Gravitational Wave Detectors: an Assessment of Current Acceleration Methods
Qian Hu, John Veitch

TL;DR
This paper evaluates the computational costs of Bayesian parameter estimation for third-generation gravitational wave detectors, highlighting the need for more efficient methods due to the high data volume and computational demands.
Contribution
It systematically assesses the computational costs and compares acceleration techniques for Bayesian inference in 3G GW detectors, emphasizing their potential to reduce costs significantly.
Findings
Standard PE could require billions of CPU core hours for 3G data.
Acceleration methods can reduce this to less than a million core hours.
High-SNR scenarios require careful treatment of accelerated methods.
Abstract
Bayesian inference with stochastic sampling has been widely used to obtain the properties of gravitational wave (GW) sources. Although computationally intensive, its cost remains manageable for current second-generation GW detectors because of the relatively low event rate and signal-to-noise ratio (SNR). The third-generation (3G) GW detectors are expected to detect hundreds of thousands of compact binary coalescence (CBC) events every year with substantially higher SNR and longer signal duration, presenting significant computational challenges. In this study, we systematically evaluate the computational costs of CBC source parameter estimation (PE) in the 3G era by modeling the PE time cost as a function of SNR and signal duration. We examine the standard PE method alongside acceleration methods including relative binning, multibanding, and reduced order quadrature. We predict that PE…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Radio Astronomy Observations and Technology · Advanced Frequency and Time Standards
