Vlasov Perturbation Theory and the role of higher cumulants
Mathias Garny, Roman Scoccimarro

TL;DR
This paper introduces a new Vlasov Perturbation Theory that incorporates higher cumulants of the phase-space distribution, improving the understanding of collisionless dark matter dynamics in cosmology.
Contribution
The authors develop a high-order cumulant hierarchy approach to Vlasov Perturbation Theory, extending beyond standard perturbation theory and analyzing its impact on cosmological structure formation.
Findings
Higher cumulants have minor effects on power spectra at weakly non-linear scales.
Spurious exponential growth is eliminated under certain scalar-mode constraints.
Loop corrections in VPT are finite for hierarchical initial spectra.
Abstract
We develop a new approach to Vlasov Perturbation Theory (VPT) that solves for the hierarchy of cumulants of the phase-space distribution function to arbitrarily high truncation order in the context of cosmological structure formation driven by collisionless dark matter. We investigate the impact of higher cumulants on density and velocity power spectra as well as the bispectrum, and compare to scale-free -body simulations. While there is a strong difference between truncation at the first cumulant, i.e. standard perturbation theory (SPT), and truncation at the second (i.e. including the velocity dispersion tensor), the third cumulant has a small quantitative impact and fourth and higher cumulants only have a minor effect on these summary statistics at weakly non-linear scales. We show that spurious exponential growth is absent in vector and tensor modes if scalar-mode constraints on…
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