ON A POSSIBLE INFLATIONARY MODEL OF THE EARLY UNIVERSE

Avagyan Avagyan

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Abstract

We consider the inflationary regime of the expansion of the Universe within the framework of the modified Jordan theory. In this model, a specific cosmological scalar is an analog of the Einstein cosmological constant L, which is connected with the Hubble parameter by the power-law φ(Φ)=αH4. As a result, a stage of hybrid inflation is obtained, at the end of which the acceleration parameter becomes zero.

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ON A POSSIBLE INFLATIONARY MODEL OF THE EARLY UNIVERSE

Abstract

Author(s)

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ON A POSSIBLE INFLATIONARY MODEL OF THE EARLY UNIVERSE

Abstract

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