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• W1965663638 abstract "We investigate homogeneous and isotropic cosmological solutions supported by the SU(2) gauge field governed by the Born-Infeld Lagrangian. In the framework of the Friedmann-Robertson-Walker cosmology with or without the cosmological constant $ensuremath{lambda},$ we derive dynamical systems that give a rather complete description of the space of solutions. For $ensuremath{lambda}=0$ the effective equation of state $ensuremath{varepsilon}(p)$ is shown to interpolate between $p=ensuremath{-}ensuremath{varepsilon}/3$ in the regime of the strong field and $p=ensuremath{varepsilon}/3$ for the weak field. Correspondingly, the universe starts with zero acceleration and gradually enters the decelerating regime, asymptotically approaching the Tolman solution." @default.
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• W1965663638 date "2002-03-15" @default.
• W1965663638 modified "2023-09-26" @default.
• W1965663638 title "Non-Abelian Born-Infeld cosmology" @default.
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• W1965663638 doi "https://doi.org/10.1103/physrevd.65.084007" @default.
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