Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory

TL;DR

This paper enhances the Pinocchio code for fast halo catalog generation by incorporating third-order Lagrangian Perturbation Theory, significantly improving the accuracy of clustering statistics compared to previous versions.

Contribution

The paper introduces the use of 3rd-order LPT in Pinocchio, improving the accuracy of halo displacement and clustering predictions over earlier methods.

Findings

3LPT provides the best agreement with N-body simulations for halo displacements.

Using 3LPT, the halo power spectrum is recovered within 10% up to k~0.5 h/Mpc.

2LPT improves halo construction accuracy over Zeldovich approximation.

Abstract

We present the latest version of Pinocchio, a code that generates catalogues of DM haloes in an approximate but fast way with respect to an N-body simulation. This code version extends the computation of particle and halo displacements up to 3rd-order Lagrangian Perturbation Theory (LPT), in contrast with previous versions that used Zeldovich approximation (ZA). We run Pinocchio on the same initial configuration of a reference N-body simulation, so that the comparison extends to the object-by-object level. We consider haloes at redshifts 0 and 1, using different LPT orders either for halo construction - where displacements are needed to decide particle accretion onto a halo or halo merging - or to compute halo final positions. We compare the clustering properties of Pinocchio haloes with those from the simulation by computing the power spectrum and 2-point correlation function (2PCF) in real and redshift space (monopole and quadrupole), the bispectrum and the phase difference of halo distributions. We find that 2LPT and 3LPT give noticeable improvement. 3LPT provides the best agreement with N-body when it is used to displace haloes, while 2LPT gives better results for constructing haloes. At the highest orders, linear bias is typically recovered at a few per cent level. In Fourier space and using 3LPT for halo displacements, the halo power spectrum is recovered to within 10 per cent up to $k_{max}\sim0.5\ h/$Mpc. The results presented in this paper have interesting implications for the generation of large ensemble of mock surveys aimed at accurately compute covariance matrices for clustering statistics.