Approximating non-Gaussian Bayesian partitions with normalising flows: statistics, inference and application to cosmology

Fuente: arXiv
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Autores principales: Röspel, Tobias, Schlosser, Adrian, Schäfer, Björn Malte
Formato: Preprint
Publicado: 2025
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author Röspel, Tobias
Schlosser, Adrian
Schäfer, Björn Malte
author_facet Röspel, Tobias
Schlosser, Adrian
Schäfer, Björn Malte
contents Subject of this paper is the simplification of Markov chain Monte Carlo sampling as used in Bayesian statistical inference by means of normalising flows, a machine learning method which is able to construct an invertible and differentiable transformation between Gaussian and non-Gaussian random distributions. We use normalising flows to compute Bayesian partition functions for non-Gaussian distributions and show how normalising flows can be employed in finding analytical expressions for posterior distributions beyond the Gaussian limit. Flows offer advantages for the numerical evaluation of the partition function itself, as well as for cumulants and for the information entropy. We demonstrate how normalising flows in conjunction with Bayes partitions can be used in inference problems in cosmology and apply them to the posterior distribution for the matter density $Ω_m$ and a dark energy equation of state parameter $w_0$ on the basis of supernova data.
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id arxiv_https___arxiv_org_abs_2501_04791
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Approximating non-Gaussian Bayesian partitions with normalising flows: statistics, inference and application to cosmology
Röspel, Tobias
Schlosser, Adrian
Schäfer, Björn Malte
Cosmology and Nongalactic Astrophysics
Instrumentation and Methods for Astrophysics
Subject of this paper is the simplification of Markov chain Monte Carlo sampling as used in Bayesian statistical inference by means of normalising flows, a machine learning method which is able to construct an invertible and differentiable transformation between Gaussian and non-Gaussian random distributions. We use normalising flows to compute Bayesian partition functions for non-Gaussian distributions and show how normalising flows can be employed in finding analytical expressions for posterior distributions beyond the Gaussian limit. Flows offer advantages for the numerical evaluation of the partition function itself, as well as for cumulants and for the information entropy. We demonstrate how normalising flows in conjunction with Bayes partitions can be used in inference problems in cosmology and apply them to the posterior distribution for the matter density $Ω_m$ and a dark energy equation of state parameter $w_0$ on the basis of supernova data.
title Approximating non-Gaussian Bayesian partitions with normalising flows: statistics, inference and application to cosmology
topic Cosmology and Nongalactic Astrophysics
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2501.04791