What does the N-point function hierarchy of the cosmological matter density field really measure ?
Julien Carron, Istv\'an Szapudi

TL;DR
This paper investigates the limitations of N-point functions in fully describing the cosmological matter density field, using the lognormal model to reveal how hierarchy probes different evolution equations and undergoes a transition to disorder.
Contribution
It provides an exact characterization of the joint information of all N-point correlators for the lognormal field, highlighting the non-perturbative effects and the nonlinear 'wrapping' transformation.
Findings
Hierarchy probes a diffusion equation on a compact torus.
The field undergoes a sharp transition to disorder, losing initial condition memory.
The lognormal model captures the nonlinear evolution beyond perturbative regimes.
Abstract
The cosmological dark matter field is not completely described by its hierarchy of -point functions, a non-perturbative effect with the consequence that only part of the theory can be probed with the hierarchy. We give here an exact characterization of the joint information of the full set of -point correlators of the lognormal field. The lognormal field is the archetypal example of a field where this effect occurs, and, at the same time, one of the few tractable and insightful available models to specify fully the statistical properties of the evolved matter density field beyond the perturbative regime. Nonlinear growth in the Universe in that model is set letting the log-density field probability density functional evolve keeping its Gaussian shape, according to the diffusion equation in Euclidean space. We show that the hierarchy probes a different evolution equation, the…
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