Cosmological models with Yang-Mills fields
E. Elizalde, A. J. Lopez-Revelles, S. D. Odintsov, S. Yu. Vernov

TL;DR
This paper explores cosmological models with SU(2) Yang-Mills fields, demonstrating that minimal coupling models lack de Sitter solutions, while non-minimal coupling models can produce de Sitter solutions without a cosmological constant.
Contribution
It introduces a reconstruction program for Yang-Mills cosmological models and compares minimal and non-minimal coupling effects on de Sitter solutions.
Findings
Minimal coupling models lack de Sitter solutions.
Non-minimal coupling models can produce de Sitter solutions without a cosmological constant.
A reconstruction method for Yang-Mills cosmological models is proposed.
Abstract
Cosmological models with an SU(2) Yang-Mills field are studied. For a specific model with a minimally coupled Yang-Mills Lagrangian, which includes an arbitrary function of the second-order term and a fourth-order term, a corresponding reconstruction program is proposed. It is shown that the model with minimal coupling has no de Sitter solutions, for any nontrivial function of the second-order term. To get de Sitter solutions, a gravitational model with nonminimally coupled Yang-Mills fields is then investigated. It is shown that the model with non-minimal coupling has in fact a de Sitter solution, even in absence of the cosmological constant term.
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