Fluid sources for Bianchi I and III space-times

DOI10.1063/1.527371zbMath0589.76147OpenAlexW2035689794MaRDI QIDQ3718429

J. P. Krisch, Selçuk Bayın

Publication date: 1986

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.527371

zbMATH Keywords

Einstein field equationscosmological modelsanalytic solutionsassociated fluid parametersBianchi III symmetrylocally rotationally symmetric solution

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (5)

Bianchi type VI0 space-times with perfect fluid source ⋮ Spatially homogeneous cosmological models of Bianchi type III ⋮ Spatially homogeneous cosmological models of Bianchi type III ⋮ Some new Bianchi type-I perfect fluid solutions ⋮ The LRS Bianchi type-I perfect fluids space-times

Cites Work

• Tilted electromagnetic Bianchi type III cosmological solution
• A class of homogeneous cosmological models

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