2016; Physical and Mathematical Sciences, 50(3 (241): 11–14
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ON A POSSIBLE INFLATIONARY MODEL OF THE EARLY UNIVERSE

Avagyan Avagyan*

Received: 2025-02-10 · Published: 2016-10-26

© 2016 The Author(s) and the original publisher.

CC BY-NC 4.0 This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
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Original title
ON A POSSIBLE INFLATIONARY MODEL OF THE EARLY UNIVERSE
Author
Avagyan Avagyan
Published
2016-10-26
Licence
Creative Commons Attribution-NonCommercial 4.0 International
Original
https://doi.org/10.46991/PSYU:A/2016.50.3.011

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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