Sigma Model on de Sitter Space
Peter C. Aichelburg, Christiane Lechner

TL;DR
This paper investigates static solutions of the SU(2) sigma model on de Sitter space, revealing a spectrum of solutions with finite energy that are linearly unstable, illustrating key features of non-linear matter-gravity systems.
Contribution
It provides a detailed analysis of spherically symmetric solutions in the sigma model on de Sitter space, highlighting their stability properties and solution structure.
Findings
Existence of a countable set of regular finite-energy solutions.
All solutions exhibit linear instability.
Number of unstable modes increases with energy.
Abstract
We discuss spherically symmetric, static solutions to the SU(2) sigma model on a de Sitter background. Despite of its simplicity this model reflects many of the features exhibited by systems of non-linear matter coupled to gravity e.g. there exists a countable set of regular solutions with finite energy; all of the solutions show linear instability with the number of unstable modes increasing with energy.
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