The early inflation phase in the evolution of the universe

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An anisotropic cosmological model with expansion and rotation with the Bianchi type IX metric has been constructed within the framework of the general relativity theory. The paper considers the first phase of the inflation of the Universe filled with a scalar field and an anisotropic liquid. In the approach implemented in this model, anisotropic fluid describes rotating dark energy.

Dark energy, first inflation, einstein equations

Короткий адрес: https://sciup.org/147245462

IDR: 147245462   |   DOI: 10.17072/1993-0550-2019-4-30-33

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