TL;DR
Simulation-Based Inference (SBI) for non-Gaussian likelihoods faces similar covariance estimation issues as traditional methods, including inflated posterior variance, but can still accurately recover the true posterior with sufficient simulations.
Contribution
This paper demonstrates that SBI does not circumvent covariance estimation problems and quantifies the inflation of posterior variance compared to traditional Gaussian likelihood methods.
Findings
SBI suffers from posterior variance inflation similar to covariance estimation.
Neither linear nor neural network compression methods avoid covariance issues in SBI.
SBI can recover the true posterior with enough simulations despite limitations.
Abstract
Making inferences about physical properties of the Universe requires knowledge of the data likelihood. A Gaussian distribution is commonly assumed for the uncertainties with a covariance matrix estimated from a set of simulations. The noise in such covariance estimates causes two problems: it distorts the width of the parameter contours, and it adds scatter to the location of those contours which is not captured by the widths themselves. For non-Gaussian likelihoods, an approximation may be derived via Simulation-Based Inference (SBI). It is often implicitly assumed that parameter constraints from SBI analyses, which do not use covariance matrices, are not affected by the same problems as parameter estimation with a covariance matrix estimated from simulations. We investigate whether SBI suffers from effects similar to those of covariance estimation in Gaussian likelihoods. We use…
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