Extending the domain of validity of the Lagrangian approximation
Sharvari Nadkarni-Ghosh, David F. Chernoff

TL;DR
This paper analyzes the convergence of Lagrangian Perturbation Theory (LPT) in cosmology, identifying its limitations and proposing a re-expansion method with controlled time steps to improve its predictive accuracy.
Contribution
It provides a formal structure for LPT series, explains convergence limitations, and introduces a re-expansion technique with a time step control strategy to extend LPT validity.
Findings
LPT convergence is limited by the analyticity of the exact solution.
Re-expanding LPT in multiple steps improves its predictive range.
A recipe for time step control enhances LPT re-expansion accuracy.
Abstract
We investigate convergence of Lagrangian Perturbation Theory (LPT) by analyzing the model problem of a spherical homogeneous top-hat in an Einstein-deSitter background cosmology. We derive the formal structure of the LPT series expansion, working to arbitrary order in the initial perturbation amplitude. The factors that regulate LPT convergence are identified by studying the exact, analytic solution expanded according to this formal structure. The key methodology is to complexify the exact solution, demonstrate that it is analytic and apply well-known convergence criteria for power series expansions of analytic functions.This analysis fully explains the previously reported observation that LPT fails to predict the evolution of an underdense, open region beyond a certain time. It also implies the existence of other examples, including overdense, closed regions, for which LPT predictions…
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