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2023, no. 3-4


Sandakova O.V., Panov V.F., Kuvshinova E.V.

The first inflationary stage of the development of the Universe is considered for the Bianchi type IX metric for the case of hybrid inflation with two scalar fields with rotation. An anisotropic fluid and two scalar fields are used as sources of gravity at the inflation stage. An attempt has been made to compare different types of inflation - chaotic inflation, "new" inflation and hybrid inflation - for rotating models.

Keywords: Hybrid inflation, "new inflation", chaotic inflation, dark energy, cosmological model.

UDC: 530.12, 531.551

PACS: 04.20.-q, 98.80.-k, 98.80.Cq

DOI: 10.17238/issn2226-8812.2023.3-4.271-276

Please cite this article in English as:
Sandakova O.V., Panov V.F., Kuvshinova E.V. Various inflationary cosmological models with rotation. Space, Time and Fundamental Interactions, 2023, no. 3-4, pp. 271-276.