(1+2)-Dimensional model of the early universe

Physics

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Scientific paper

An anisotropic cosmological model is obtained by solving (1+3)-dimensional field equations. The topology of the model is R 1 ⊗ M 2 ⊗ S 1, where R 1 is the real line (time axis), M 2 is 2-dimensional space, and S 1 is the circle. Employing the method of Kaluza-Klein type compactification on S 1 and one-loop quantum correction to scalar fields, an effective (1+2)-dimensional gravity is obtained. The resulting (1+2)-dimensional cosmological model of the early universe is derived.

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