A gravitationally non-degenerate cosmological model with expanding and shearing viscous fluid in general relativity

DOI10.1007/BF00643823zbMath0633.76134MaRDI QIDQ1096510

Deepak Raj Jain, Raj Bali

Publication date: 1987

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

shear viscositycosmological modelbehaviour of viscosityrate of expansion

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)

Five dimensional bulk viscous string cosmological models in Saez and Ballester theory of gravitation ⋮ Five dimensional bulk viscous cosmological model with wet dark fluid in general relativity ⋮ Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant ⋮ Plane symmetric viscous fluid cosmological models with varying \(\Lambda\)-term ⋮ FRW bulk viscous cosmology in multi dimensional space-time

Cites Work

• Unnamed Item
• Topology and cosmology

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