Bayesian and frequentist investigation of prior effects in EFTofLSS analyses of full-shape BOSS and eBOSS data
Emil Brinch Holm, Laura Herold, Th\'eo Simon, Elisa G. M. Ferreira,, Steen Hannestad, Vivian Poulin, Thomas Tram

TL;DR
This paper compares Bayesian and frequentist methods in analyzing cosmological data with EFTofLSS, revealing prior dependence issues and emphasizing the importance of combining approaches for accurate inference.
Contribution
It introduces a frequentist profile likelihood approach to assess prior effects in EFTofLSS analyses, providing a more prior-independent perspective on cosmological parameter constraints.
Findings
Bayesian constraints depend on priors and show volume effects.
Frequentist intervals are wider and prior-independent.
Future data will reconcile Bayesian and frequentist results.
Abstract
Previous studies based on Bayesian methods have shown that the constraints on cosmological parameters from the Baryonic Oscillation Spectroscopic Survey (BOSS) full-shape data using the Effective Field Theory of Large Scale Structure (EFTofLSS) depend on the choice of prior on the EFT nuisance parameters. In this work, we explore this prior dependence by adopting a frequentist approach based on the profile likelihood method, which is inherently independent of priors, considering data from BOSS, eBOSS and Planck. We find that the priors on the EFT parameters in the Bayesian inference are informative and that prior volume effects are important. This is reflected in shifts of the posterior mean compared to the maximum likelihood estimate by up to 1.0 {\sigma} (1.6 {\sigma}) and in a widening of intervals informed from frequentist compared to Bayesian intervals by factors of up to 1.9 (1.6)…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Monetary Policy and Economic Impact
