Inflation in a Bianchi-IX cosmological model. The roles of primordial shear and gauge fields

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Scientific paper

The role played by primordial anisotropy and gauge field configurations is investigated in the context of a model with an inflationary stage driven by a self-interacting complex scalar field. We find that, in general, both the anisotropy and the gauge field aid inflation and we try to understand, qualitatively, the reasons for such behaviour. Asymptotic inflationary solutions and their stability are investigated.

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