Model of Evolution of the Universe with the Bianchi Type VIII Metric
- Authors: Panov V.F.1, Sandakova O.V.1, Yanishevsky D.M.1, Cheremnykh M.R.2
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Affiliations:
- Perm State National Research University
- Perm State Medical University Named after Academician E. A. Wagner of the Ministry of Healthcare of the Russian Federation
- Issue: Vol 61, No 9 (2019)
- Pages: 1629-1637
- Section: Article
- URL: https://bakhtiniada.ru/1064-8887/article/view/240963
- DOI: https://doi.org/10.1007/s11182-018-1580-6
- ID: 240963
Cite item
Abstract
An anisotropic cosmological model with expansion and rotation and the Bianchi type VIII metric has been constructed within the framework of general relativity theory. The first inflation stage of the Universe filled with a scalar field and an anisotropic fluid is considered. The model describes the Friedman stage of cosmological evolution with subsequent transition to accelerated exponential expansion observed in the present epoch. In the approach realized in the model, the anisotropic fluid describes the rotating dark energy.
About the authors
V. F. Panov
Perm State National Research University
Author for correspondence.
Email: panov@psu.ru
Russian Federation, Perm
O. V. Sandakova
Perm State National Research University
Email: panov@psu.ru
Russian Federation, Perm
D. M. Yanishevsky
Perm State National Research University
Email: panov@psu.ru
Russian Federation, Perm
M. R. Cheremnykh
Perm State Medical University Named after Academician E. A. Wagner of the Ministry of Healthcare of the Russian Federation
Email: panov@psu.ru
Russian Federation, Perm
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