TL;DR
This paper demonstrates that using third-order Lagrangian perturbation theory (3LPT) for initial conditions significantly reduces errors in cosmological N-body simulations, enabling more accurate modeling of large-scale structures at later starting redshifts.
Contribution
The study introduces and validates the use of 3LPT for initial conditions, showing it suppresses truncation errors and improves simulation accuracy compared to lower-order methods.
Findings
3LPT reduces truncation errors by an order of magnitude.
Late initialization with 3LPT achieves near-continuum accuracy at z=0.
Discreteness errors decay over time and are amplified when starting early.
Abstract
Inaccuracies in the initial conditions for cosmological N-body simulations could easily be the largest source of systematic error in predicting the non-linear large-scale structure. From the theory side, initial conditions are usually provided by using low-order truncations of the displacement field from Lagrangian perturbation theory, with the first and second-order approximations being the most common ones. Here we investigate the improvement brought by using initial conditions based on third-order Lagrangian perturbation theory (3LPT). We show that with 3LPT, truncation errors are vastly suppressed, thereby opening the portal to initializing simulations accurately as late as z=12 (for the resolution we consider). We analyse the competing effects of perturbative truncation and particle discreteness on various summary statistics. Discreteness errors are essentially decaying modes and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Code & Models
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
