Bianchi type V perfect-fluid space-times

DOI10.1007/BF00675107zbMath0702.76129OpenAlexW2006618136MaRDI QIDQ915613

Shri Ram

Publication date: 1990

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00675107

zbMATH Keywords

solutionsEinstein field equationsBianchi type V space-timesenergy- momentum tensor is of perfect fluid type

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 (11)

Bianchi type V universe models with specific expansion anisotropy ⋮ Bianchi type V cosmological models with varying cosmological term ⋮ THE BIANCHI TYPE V MAGNETIZED STRING DUST COSMOLOGICAL MODEL IN GENERAL RELATIVITY ⋮ Stiff domain walls in creation-field cosmology ⋮ Bianchi type V viscous fluid cosmological models in presence of decaying vacuum energy ⋮ Bianchi type-V cosmological model with purely magnetic solution ⋮ Inflationary scenario in Bianchi type V space-time for a barotropic fluid distribution with variable bulk viscosity and vacuum energy density ⋮ Bianchi type-V bulk viscous fluid string dust cosmological model in general relativity ⋮ Bianchi type I universe with constant deceleration parameter in creation-field cosmology ⋮ Bianchi type V cosmological models with constant deceleration parameter in general relativity ⋮ Bianchi type-I string cosmological model in creation-field

Cites Work

• Zero-curvature FRW models and Bianchi I space-time as solutions of the same equation
• On the Relation between the Expansion and the Mean Density of the Universe

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