Lattice Simulations of Inflation
Angelo Caravano, Eiichiro Komatsu, Kaloian D. Lozanov, Jochen Weller

TL;DR
This paper demonstrates the use of lattice simulations to study the inflationary phase of the early universe, accurately reproducing known results for simple models and setting the stage for more complex future studies.
Contribution
It introduces lattice simulation techniques to analyze the inflationary universe, focusing on the scalar field perturbations during inflation, a novel application beyond reheating studies.
Findings
Successfully reproduces the nearly scale-invariant power spectrum for slow-roll inflation.
Accurately captures oscillatory features in the power spectrum for step potential models.
Establishes a foundation for future lattice-based studies of complex inflationary scenarios.
Abstract
The scalar field theory of cosmological inflation constitutes nowadays one of the preferred scenarios for the physics of the early universe. In this paper we aim at studying the inflationary universe making use of a numerical lattice simulation. Various lattice codes have been written in the last decades and have been extensively used for understating the reheating phase of the universe, but they have never been used to study the inflationary phase itself far from the end of inflation (i.e. about 50 e-folds before the end of inflation). In this paper we use a lattice simulation to reproduce the well-known results of some simple models of single-field inflation, particularly for the scalar field perturbation. The main model that we consider is the standard slow-roll inflation with an harmonic potential for the inflaton field. We explore the technical aspects that need to be accounted for…
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