Vlasov Perturbation Theory applied to $\Lambda$CDM
Mathias Garny, Dominik Laxhuber, Roman Scoccimarro

TL;DR
This paper extends perturbation theory for cosmological matter distribution by incorporating velocity dispersion effects, leading to more accurate, cutoff-independent predictions of the matter power spectrum in $\Lambda$CDM models, validated against simulations.
Contribution
It introduces Vlasov Perturbation Theory (VPT) with velocity dispersion, providing a stable, efficient alternative to standard methods for modeling non-linear cosmic structures.
Findings
VPT agrees with simulations up to missing three-loop effects.
Treating dispersion as a free parameter yields stable predictions.
Two-loop power spectrum is robust to neglecting higher cumulants.
Abstract
We apply the framework of Vlasov Perturbation Theory (VPT) to the two-loop matter power spectrum within CDM cosmologies. The main difference to Standard Perturbation Theory (SPT) arises from taking the velocity dispersion tensor into account, and the resulting screening of the backreaction of UV modes renders loop integrals cutoff-independent. VPT is informed about non-perturbative small scale dynamics via the average value of the dispersion generated by shell-crossing, which impacts the evolution of perturbations on weakly non-linear scales. When using an average dispersion from halo models, the VPT power spectrum agrees with the one from the simulation, up to differences from missing three-loop contributions. Alternatively, treating the average dispersion as free parameter we find a remarkably stable prediction of the matter power spectrum from collisionless dynamics at…
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Taxonomy
TopicsGas Dynamics and Kinetic Theory
