Bianchi type II cosmological model of the Universe’s evolution

DOI10.1142/S0219887818500160zbMath1381.83152WikidataQ108969512 ScholiaQ108969512MaRDI QIDQ4600598

D. M. Yanishevsky, E. V. Kuvshinova, O. V. Sandakova, V. F. Panov

Publication date: 11 January 2018

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

rotationcosmological modeldark energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

Related Items (4)

On the quantum birth of the universe with a Bianchi type-IX metric in the presence of an anisotropic fluid, a scalar field, and pure radiation ⋮ Evolution of a cosmological model with rotation with a Bianchi type-IX metric ⋮ A cosmological scenario with rotation ⋮ Model of evolution of the Universe with the Bianchi type VIII metric

Cites Work

• Unnamed Item
• Modern cosmological data and rotation of the Universe
• Erratum: The Vaidya–Patel solution with Robertson–Walker metric as a rotating inflationary scenario [J. Math. Phys. 2 9, 1514 (1988)]
• Dynamical importance of vorticity and shear in the universe

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