Constrained probability distributions of correlation functions
David Keitel, Peter Schneider

TL;DR
This paper derives the exact probability distribution functions for correlation functions of Gaussian random fields, improving the statistical modeling used in cosmology beyond Gaussian approximations.
Contribution
It provides an analytic derivation of the univariate and bivariate distributions of correlation functions, including a closed-form in a special case, enhancing data analysis accuracy.
Findings
Derived exact univariate and bivariate distributions
Presented mode expansions and a closed-form solution in a special case
Discussed moments and approximation methods like Edgeworth expansion
Abstract
Context: Two-point correlation functions are used throughout cosmology as a measure for the statistics of random fields. When used in Bayesian parameter estimation, their likelihood function is usually replaced by a Gaussian approximation. However, this has been shown to be insufficient. Aims: For the case of Gaussian random fields, we search for an exact probability distribution of correlation functions, which could improve the accuracy of future data analyses. Methods: We use a fully analytic approach, first expanding the random field in its Fourier modes, and then calculating the characteristic function. Finally, we derive the probability distribution function using integration by residues. We use a numerical implementation of the full analytic formula to discuss the behaviour of this function. Results: We derive the univariate and bivariate probability distribution function of…
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