On the problems of a very early universe

Physics

Scientific paper

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Scientific paper

Very early stages of an expanding universe or later stages of a collapsing universe are considered. Friedmann's universe is assumed to be filled with a nonlinear scalar field. In its development it passes the region near the classical singularity in a phase close to the de Sitter's one. Certain conditions necessary for providing the existence of a limiting energy density are taken into account in the formalism.

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