Perturbation Theory of the Cosmological Log-Density Field

TL;DR

This paper develops a renormalized perturbation theory for the power spectrum of the log-density field in cosmology, providing a new analytic framework that aligns well with simulation data and addresses density smoothing.

Contribution

It introduces a novel perturbation theory formalism for the log-density power spectrum using renormalization and Taylor expansion, improving analysis of nonlinear regimes.

Findings

Perturbation theory results agree with simulations.

The formalism effectively handles density smoothing.

Logarithmic transformation closely relates to linear power spectrum.

Abstract

The matter density field exhibits a nearly lognormal probability density distribution (PDF) after entering into the nonlinear regime. Recently, it has been shown that the shape of the power spectrum of a logarithmically transformed density field is very close to the linear density power spectrum, motivating an analytic study of it. In this paper, we develop cosmological perturbation theory for the power spectrum of this field. Our formalism is developed in the context of renormalized perturbation theory, which helps to regulate the convergence behavior of the perturbation series, and of the Taylor- series expansion we use of the logarithmic mapping. This approach allows us to handle the critical issue of density smoothing in a straightforward way. We also compare our perturbative results with simulation measurements.