The non-linear dynamics of axion inflation: a detailed lattice study

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Hauptverfasser: Figueroa, Daniel G., Lizarraga, Joanes, Loayza, Nicolás, Urio, Ander, Urrestilla, Jon
Format: Preprint
Veröffentlicht: 2024
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author Figueroa, Daniel G.
Lizarraga, Joanes
Loayza, Nicolás
Urio, Ander
Urrestilla, Jon
author_facet Figueroa, Daniel G.
Lizarraga, Joanes
Loayza, Nicolás
Urio, Ander
Urrestilla, Jon
contents We study in detail the fully inhomogeneous non-linear dynamics of axion inflation, identifying three regimes: weak-, mild-, and strong-backreaction, depending on the duration of inflation. We use lattice techniques that explicitly preserve gauge invariance and shift symmetry, and which we validate against other computational methods of the linear dynamics and of the homogeneous backreaction regime. Notably, we demonstrate that the latter fails to accurately describe the truly local dynamics of strong backreaction. We investigate the convergence of simulations of local backreaction, determining the requirements to achieve an accurate description of the dynamics, and providing useful parametrizations of the delay of the end of inflation. Additionally, we identify key features emerging from a proper local treatment of strong backreaction: the dominance of magnetic energy against the electric counterpart, the excitation of the longitudinal mode, and the generation of a scale-dependent chiral (im)balance. Our results underscore the necessity to accurately capture the local nature of the non-linear dynamics of the system, in order to correctly assess phenomenological predictions, such as e.g. the production of gravitational waves and primordial black holes.
format Preprint
id arxiv_https___arxiv_org_abs_2411_16368
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The non-linear dynamics of axion inflation: a detailed lattice study
Figueroa, Daniel G.
Lizarraga, Joanes
Loayza, Nicolás
Urio, Ander
Urrestilla, Jon
Cosmology and Nongalactic Astrophysics
High Energy Physics - Lattice
High Energy Physics - Phenomenology
We study in detail the fully inhomogeneous non-linear dynamics of axion inflation, identifying three regimes: weak-, mild-, and strong-backreaction, depending on the duration of inflation. We use lattice techniques that explicitly preserve gauge invariance and shift symmetry, and which we validate against other computational methods of the linear dynamics and of the homogeneous backreaction regime. Notably, we demonstrate that the latter fails to accurately describe the truly local dynamics of strong backreaction. We investigate the convergence of simulations of local backreaction, determining the requirements to achieve an accurate description of the dynamics, and providing useful parametrizations of the delay of the end of inflation. Additionally, we identify key features emerging from a proper local treatment of strong backreaction: the dominance of magnetic energy against the electric counterpart, the excitation of the longitudinal mode, and the generation of a scale-dependent chiral (im)balance. Our results underscore the necessity to accurately capture the local nature of the non-linear dynamics of the system, in order to correctly assess phenomenological predictions, such as e.g. the production of gravitational waves and primordial black holes.
title The non-linear dynamics of axion inflation: a detailed lattice study
topic Cosmology and Nongalactic Astrophysics
High Energy Physics - Lattice
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2411.16368