TL;DR
This paper demonstrates that simulation-based inference with neural network compressed summaries can nearly match the exact Bayesian posteriors in cosmological field analysis, offering a computationally efficient alternative to traditional likelihood methods.
Contribution
It introduces a neural network-based summary statistic approach that retains all information and enables nearly lossless, scalable inference in cosmological data analysis, bypassing complex likelihood evaluations.
Findings
Neural network summaries do not lose information compared to full field analysis.
Simulation-based inference with these summaries nearly recovers exact posteriors.
Implicit inference is computationally cheaper than explicit likelihood methods.
Abstract
We present a comparison of simulation-based inference to full, field-based analytical inference in cosmological data analysis. To do so, we explore parameter inference for two cases where the information content is calculable analytically: Gaussian random fields whose covariance depends on parameters through the power spectrum; and correlated lognormal fields with cosmological power spectra. We compare two inference techniques: i) explicit field-level inference using the known likelihood and ii) implicit likelihood inference with maximally informative summary statistics compressed via Information Maximising Neural Networks (IMNNs). We find that a) summaries obtained from convolutional neural network compression do not lose information and therefore saturate the known field information content, both for the Gaussian covariance and the lognormal cases, b) simulation-based inference using…
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