On a possible inflationary model of the early universe (Վաղ տիեզերքի հնարավոր ինֆլյացիոն մոդելի մասին)

Համառոտագիր

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 Λ, which is connected with the Hubble parameter by the power-law ϕ(Φ) = αH 4 . As a result, a stage of hybrid inflation is obtained, at the end of which the acceleration parameter becomes zero.