A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field

DOI10.1007/BF00643932zbMath0714.76122MaRDI QIDQ751444

Atul Tyagi, Raj Bali

Publication date: 1990

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

zbMATH Keywords

electromagnetic field tensorexpanding, shearing, non-rotating universeplane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field

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 (7)

A plane-symmetric magnetized inhomogeneous cosmological models of perfect fluid distribution with variable magnetic permeability in Lyra geometry ⋮ Plane symmetric inhomogeneous cosmological models with a perfect fluid in general relativity ⋮ EVOLUTION OF EXPANSION-FREE SELF-GRAVITATING FLUIDS AND PLANE SYMMETRY ⋮ Thermodynamical behavior of inhomogeneous universe with varying \(\Lambda \) in presence of electromagnetic field ⋮ Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable \(\Lambda\) ⋮ PLANE-SYMMETRIC INHOMOGENEOUS VISCOUS FLUID COSMOLOGICAL MODELS WITH ELECTROMAGNETIC FIELD ⋮ Cylindrically symmetric inhomogeneous cosmological models with viscous fluid and varying \(\Lambda\)

Cites Work

• A class of inhomogeneous cosmological models
• The Large Scale Structure of Space-Time
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• Unnamed Item

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