Inflationary Butterfly Effect: Non-perturbative Dynamics From Small-Scale Features
Abstract
For the first time, we investigate the non-perturbative dynamics of single field inflation with a departure from slow-roll. Using simulations, we find that oscillatory features in the potential can drastically alter the course of inflation, with major phenomenological implications. In certain cases, the entire Universe gets trapped in a forever inflating de Sitter state. In others, only some regions get stuck in a false vacuum, offering an alternative channel for primordial black hole formation. Analogous to the flap of a butterfly, these results show that small-scale phenomena can have profound consequences on the evolution of the entire Universe. This demonstrates the necessity of a non-perturbative approach in the exploration of the small-scale physics of inflation, particularly in the regime relevant for gravitational-wave astronomy.
Cite
@article{arxiv.2403.12811,
title = {Inflationary Butterfly Effect: Non-perturbative Dynamics From Small-Scale Features},
author = {Angelo Caravano and Keisuke Inomata and Sébastien Renaux-Petel},
journal= {arXiv preprint arXiv:2403.12811},
year = {2024}
}
Comments
version published in PRL, minor modifications, 5 pages + Supplemental Material, 3 figures ; animations can be found at the following link https://github.com/caravangelo/Inflationary-Butterfly.git