Model of Evolution of the Universe with the Bianchi Type VIII Metric
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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.
Keywordsaccelerated cosmological expansion dust-like matter dark energy inflation
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- 2.A. Payez, J. R. Cudell, and D. Hutsemekers, New constraints on very light pseudoscalars, arXiv: 1204.6614 [astro-ph] (2012).Google Scholar
- 3.M. J. Longo, Detection of a dipole in the handedness of spiral galaxies with redshifts z ~ 0.04, arXiv: 1104.2815 [astro-ph] (2011).Google Scholar
- 11.M. L. Filchenkov and Yu. P. Laptev, Quantum Gravitation. From Microworld to Megaworld [in Russian], Lenand, Moscow (2016).Google Scholar
- 13.V. F. Panov and Yu. G. Sbytov, Zh. Eksp. Teor. Fiz., 114, No. 3, 769–776 (1998).Google Scholar