EFTofLSS meets simulation-based inference: $\sigma_8$ from biased tracers
Beatriz Tucci, Fabian Schmidt

TL;DR
This paper demonstrates how simulation-based inference can be used to estimate the cosmological parameter sigma_8 from biased tracers in large-scale structure, bypassing the need for explicit likelihood functions.
Contribution
It introduces a method combining EFT-based forward modeling with neural density estimation for sigma_8 inference from power spectrum and bispectrum data.
Findings
Covariance form impacts inference more than non-Gaussianity at certain scales.
Simulation-based inference matches traditional methods when covariance is accurately modeled.
The approach is effective for scales up to 0.2h/Mpc.
Abstract
Cosmological inferences typically rely on explicit expressions for the likelihood and covariance of the data vector, which normally consists of a set of summary statistics. However, in the case of nonlinear large-scale structure, exact expressions for either likelihood or covariance are unknown, and even approximate expressions can become very cumbersome, depending on the scales and summary statistics considered. Simulation-based inference (SBI), in contrast, does not require an explicit form for the likelihood but only a prior and a simulator, thereby naturally circumventing these issues. In this paper, we explore how this technique can be used to infer from a Lagrangian effective field theory (EFT) based forward model for biased tracers. The power spectrum and bispectrum are used as summary statistics to obtain the posterior of the cosmological, bias and noise parameters…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Computational Physics and Python Applications · Cosmology and Gravitation Theories
