Post-collapse Lagrangian perturbation theory in three dimensions
Shohei Saga, Stéphane Colombi, Atsushi Taruya, Cornelius Rampf, Abineet Parichha
TL;DR
This work introduces three-dimensional post-collapse perturbation theory (PCPT) for cold dark matter, extending the one-dimensional framework to realistic 3D pancake-like collapse. It combines high-order Lagrangian perturbation theory for the pre-collapse background with a perturbative, analytically tractable backreaction treatment derived from a reduced one-dimensional Poisson problem along the collapse axis, yielding explicit corrections to displacement and velocity shortly after shell-crossing. Validation against high-resolution ColDICE Vlasov-Poisson simulations shows PCPT accurately captures early multistream dynamics and caustic structure, outperforming standard LPT in the post-collapse regime. The approach provides a deterministic bridge between Zel'dovich flow and nonlinear multi-stream evolution, with implications for understanding the initial stages of halo formation, while acknowledging limitations related to symmetry, transverse corrections, and LPT convergence that guide future refinements.
Abstract
The gravitational collapse of collisionless matter leads to shell-crossing singularities that challenge the applicability of standard perturbation theory. Here, we present the first fully perturbative approach in three dimensions by using Lagrangian coordinates that asymptotically captures the highly nonlinear nature of matter evolution after the first shell-crossing. This is made possible essentially thanks to two basic ingredients: (1) We employ high-order standard Lagrangian perturbation theory to evolve the system until shell-crossing, and (2) we exploit the fact that the density caustic structure near the first shell-crossing begins generically with pancake formation. The latter property allows us to exploit largely known one-dimensional results to determine perturbatively the gravitational backreaction after collapse, yielding accurate solutions within our post-collapse perturbation theory (PCPT) formalism. We validate the PCPT predictions against high-resolution Vlasov-Poisson simulations and demonstrate that PCPT provides a robust framework for describing the early stages of post-collapse dynamics.
