BullFrog: Multi-step perturbation theory as a time integrator for cosmological simulations
Cornelius Rampf, Florian List, Oliver Hahn

TL;DR
BullFrog introduces a multi-step perturbation time integrator for cosmological N-body simulations that converges rapidly to the exact solution, improving upon existing LPT-inspired methods without extra computational cost.
Contribution
The paper presents BullFrog, a second-order accurate integrator that automatically performs 2LPT steps, enhancing simulation accuracy without additional computational overhead.
Findings
BullFrog converges rapidly to the exact solution with increasing time steps.
It outperforms other LPT-inspired integrators like FastPM and COLA.
Implementation in existing N-body codes is straightforward.
Abstract
Modelling the cosmic large-scale structure can be done through numerical N-body simulations or by using perturbation theory. Here, we present an N-body approach that effectively implements a multi-step forward model based on Lagrangian Perturbation Theory (LPT) in a CDM Universe. This is achieved by introducing the second-order accurate BullFrog integrator, which automatically performs 2LPT time steps to second order without requiring the explicit computation of 2LPT displacements. Importantly, we show that BullFrog trajectories rapidly converge to the exact solution as the number of time steps increases, at any moment in time, even though 2LPT becomes invalid after shell-crossing. As a validation test, we compare BullFrog against other N-body integrators and high-order LPT, both for a realistic CDM cosmology and for simulations with a sharp UV cutoff in the initial…
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Taxonomy
TopicsNumerical methods for differential equations · Cosmology and Gravitation Theories · demographic modeling and climate adaptation
