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Uncertainty-aware and Data-efficient Cosmological Emulation using Gaussian Processes and PCA
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Uncertainty-aware and Data-efficient Cosmological Emulation using Gaussian Processes and PCA
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Bayesian parameter inference is one of the key elements for model selection in cosmological research. However, the available inference tools require a large number of calls to simulation codes which can lead to high and sometimes even infeasible computational costs. In this work we propose a new way of emulating simulation codes for Bayesian parameter inference. In particular, this novel approach emphasizes the uncertainty-awareness of the emulator, which allows to state the emulation accuracy and ensures reliable performance. With a focus on data efficiency, we implement an active learning algorithm based on a combination of Gaussian Processes and Principal Component Analysis. We find that for an MCMC analysis of Planck and BAO data on the $\Lambda$CDM model (6 model and 21 nuisance parameters) we can reduce the number of simulation calls by a factor of $\sim$500 and save about $96\%$ of the computational costs.
Forward citations
Cited by 2 Pith papers
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CMBolic: Symbolic emulators for the Cosmic Microwave Background. I. Lensing
CMBolic supplies analytic emulators for CMB lensing spectra achieving 0.27-0.32% mean fractional error, validated against CLASS on ACT DR6 and Planck lensing data.
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SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
SPT-3G delivers the most precise CMB EE and TE spectra at high multipoles to date, giving LCDM parameters with H0 = 66.66 ± 0.60 km/s/Mpc from ground-based data alone and reaching Planck-level constraints when combine...
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