Cosmological Implication of Yang-Mills Field and its Chaotic Behavior

Physics

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Scientific paper

Studying Yang-Mills field and gravitational field in class A Bianchi spacetimes, we find that chaotic behavior appears in the late phase (the asymptotic future). At the same time, in the initial phase (near the initial singularity), we find a Mixmaster-like behavior in Bianchi I spacetime. Although this result may provide a counterexample to the BKL (Belinskii, Khalatnikov and Lifshitz) conjecture, we show that the BKL conjecture is still valid in Bianchi IX spacetime. We also analyze a multiplicative effect of two types of chaos, that is, chaos with the Yang-Mills field and that in vacuum Bianchi IX spacetime. In order to consider influence of such chaotic system upon cosmology, we also study the co-evolution of Yang-Mills fields and perfect fluids in Bianchi type I spacetime. We find that, whereas magnetic universes are strongly constrained by the microwave background anisotropy, Yang-Mills universes are principally constrained by primordial nucleosynthesis and the bound is comparatively weak, and ΩYM < 0.105Ωrad

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