Cosmological structure formation with augmented Lagrangian perturbation theory

We present a new fast and efficient approach to model structur e formation with Augmented Lagrangian Perturbation Theory (ALPT). Our method is based on splitting the displacement field into a long and a short-range component. The l ong-range component is computed by second order LPT (2LPT). This approximation contains a tidal nonlocal and nonlinear term. Unfortunately, 2LPT fails on small scales due to severe shell crossing and a crude quadratic behaviour in the low density regime. The spherical collapse (SC) approximation has been recently reported to correct for both effects by adding an ideal collapse truncation. However, this approach fails to reproduce the structures on lar ge scales where it is significantly less correlated with the N -body result than 2LPT or linear LPT (the Zeldovich approximation). We propose to combine both approximations using for the short-range displacement field the SC solution. A Gaussian filter with a smoothing radius rS is used to separate between both regimes. We use the result of 25 dark matter only N -body simulations to benchmark at z = 0 the different approximations: 1st, 2nd, 3rd order LPT, SC an d our novel combined ALPT model. This comparison demonstrates that our method improves previous approximations at all scales showing �25% and �75% higher correlation than 2LPT with the N -body solution at k = 1 and 2 h Mpc 1 , respectively. We conduct a parameter study to determine the optimal range of smoothing radii and find that the maximum cor relation is achieved with rS = 4 5 h 1 Mpc. This structure formation approach could be used for various purposes, such as setting-up initial conditions for N -body simulations, generating mock galaxy catalogues, cosmic web analysis or for reconstructions of the pr imordial density fluctuations.