LRS Bianchi type-V universes filled with matter and radiation

DOI10.1007/BF00651674zbMath0547.76139MaRDI QIDQ799221

N. E. Zubov

Publication date: 1983

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

zbMATH Keywords

perfect fluidstress-energy tensorBianchi type-V universesnon-isotropic metrics

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (12)

Bianchi V cosmology with a specific Hubble parameter ⋮ Bianchi type V barotropic perfect fluid cosmological model in Lyra geometry ⋮ 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 ⋮ Bianchi type V universe models with specific expansion anisotropy ⋮ THE BIANCHI TYPE V MAGNETIZED STRING DUST COSMOLOGICAL MODEL IN GENERAL RELATIVITY ⋮ Bianchi V cosmological model in Palatini \(f(R)\) gravity ⋮ 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 ⋮ Inhomogeneous generalizations of Bianchi type-VI\(_ h\) universes with co-moving perfect fluid and radiation ⋮ Bianchi type V cosmological models with constant deceleration parameter in general relativity

Cites Work

• Tilted electromagnetic Bianchi type \(VI_ 0 \)cosmological model
• Exact Bianchi type \(VI_ 0 \)cosmological models with matter and an electromagnetic field

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