Straightening the Density-Displacement Relation with a Logarithmic Transform
Bridget L. Falck, Mark C. Neyrinck, Miguel A. Aragon-Calvo, Guilhem, Lavaux, and Alexander S. Szalay

TL;DR
This paper demonstrates that using a logarithmic density variable improves the estimation of the Lagrangian displacement field in cosmological simulations, especially at nonlinear scales and low redshifts.
Contribution
It introduces and tests a logarithmic density transformation for better relation with displacement divergence, outperforming linear methods in certain regimes.
Findings
Logarithmic density relation is tighter at low redshifts.
Grid-based methods outperform tessellation in measuring fields.
Logarithmic transformation improves nonlinear scale estimations.
Abstract
We investigate the use of a logarithmic density variable in estimating the Lagrangian displacement field, motivated by the success of a logarithmic transformation in restoring information to the matter power spectrum. The logarithmic relation is an extension of the linear relation, motivated by the continuity equation, in which the density field is assumed to be proportional to the divergence of the displacement field; we compare the linear and logarithmic relations by measuring both of these fields directly in a cosmological N-body simulation. The relative success of the logarithmic and linear relations depends on the scale at which the density field is smoothed. Thus we explore several ways of measuring the density field, including Cloud-In-Cell smoothing, adaptive smoothing, and the (scale-independent) Delaunay tessellation, and we use both a Fourier space and a geometrical…
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