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In this paper we discuss the dynamics of the cosmological Bartnick-McKinnonanalogue with $n=1$ and $\Lambda=\Lambda_{reg}(n)$ . We derive boundaryconditions from energy considerations. Numerical simulations are carried out toshow the existence of a non-stationary solution.

Numerical Simulations of a Spherically Symmetric Yang-Mills system on a de Sitter Manifold