Космологическая модель V типа по Бьянки

Olga Sandakova; Elena Kuvshinova

doi:10.17072/1993-0550-2022-2-67-72

Bianchi Type V Cosmological Model

Authors

Olga Sandakova Perm State Univesity https://orcid.org/0000-0003-1768-7286
Elena Kuvshinova Perm State Univesity https://orcid.org/0000-0003-3432-8234

DOI:

https://doi.org/10.17072/1993-0550-2022-2-67-72

Keywords:

cosmological model, Einstein's system of equations, ideal fluid

Abstract

Within the framework of the general theory of relativity, a cosmological model of type V according to the Bianchi classification is constructed, where a non-interacting ideal fluid is used as a source of gravity. Two possible solutions have been found, the first of which describes the stage of early inflation of the evolution of the Universe.

References

Кувшинова Е. В., Сандакова О. В., Янишевский Д. М. Космологические модели с метрикой типа V по Бьянки // Известия высших учебных заведений. Физика. 2022. Т. 65, № 2. С. 43–47.

Гуц А. К. Топологическая структура Вселенной Геделя // Известия высших учебных заведений. Физика. 1980. № 6. С. 109–110.

Raval H. M. On a Godel-type Nonstatic Cosmological Solution for Matter in an Electromagnetic Field // Austral. J. Phys. 1967. Vol. 20, № 6. P. 663–673.

Bhardwaj V. K., Dixit A., Pradhan A. Bianchi type-V Transitioning model in Brans-Dicke theory with Observational Constraint // arxiv:2203/11426v2.

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Published

2022-07-05

How to Cite

Sandakova О. В., & Kuvshinova Е. В. (2022). Bianchi Type V Cosmological Model. BULLETIN OF PERM UNIVERSITY. MATHEMATICS. MECHANICS. COMPUTER SCIENCE, (2 (57), 67–72. https://doi.org/10.17072/1993-0550-2022-2-67-72