Non-Abelian gauge preheating
High Energy Physics - Phenomenology
2025-08-20 v2 Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
Abstract
We study preheating in models where a scalar inflaton is directly coupled to a non-Abelian gauge field. In particular, we examine inflation with a conformal, dilaton-like coupling to the non-Abelian sector. We describe a numerical scheme that combines lattice gauge theory with standard finite difference methods applied to the scalar field. We show that a significant tachyonic instability allows for efficient preheating, which is parametrically suppressed by increasing the non-Abelian self-coupling. Additionally, we comment on the technical implementation of the evolution scheme and setting initial conditions.
Cite
@article{arxiv.1708.02944,
title = {Non-Abelian gauge preheating},
author = {Peter Adshead and John T. Giblin and Zachary J. Weiner},
journal= {arXiv preprint arXiv:1708.02944},
year = {2025}
}
Comments
v2: 15 pages, 9 figures; references and minor clarifications added, matches PRD version