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arXiv · 2607.28800

Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation

Drew Jamieson·Angelo Caravano·Eiichiro Komatsu
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Abstract

The cosmic web preserves a record of the physics that shaped the universe in its earliest moments, the period of exponential expansion known as cosmic inflation. However, if inflation involves significant nonlinear interactions, there are no direct theoretical predictions for the resulting cosmic web. We present the first simulation of the entire history of the universe, from deep in the inflationary epoch to the present-day cosmic structure. Applying this to axion-U(1) inflation, we find that early-universe interactions enhance small-scale structure at high redshift, imprinting the matter power spectrum and the mass function of dark matter halos with signatures of a modified primordial curvature power spectrum and non-Gaussianity. These signatures make high-redshift galaxy surveys, 21-cm observations, and line-intensity mapping promising probes of inflationary physics. More broadly, this ab initio approach provides a novel framework for mapping the signatures of nonlinear inflationary dynamics onto observable cosmic structures across cosmic time.

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Drew Jamieson, Angelo Caravano, Eiichiro Komatsu. 2026-07-30. Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation. https://arxiv.org/abs/2607.28800

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