A new class of relativistic perfect fluid cylinders with expansion proportional to shear scalar

DOI10.1007/S10509-010-0582-9zbMath1213.83047OpenAlexW2084523997MaRDI QIDQ535753

Sachin Kumar, Y. K. Gupta, Pratibha

Publication date: 13 May 2011

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

Full work available at URL: https://doi.org/10.1007/s10509-010-0582-9

zbMATH Keywords

general relativitycylindrical symmetryperfect fluids

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

Generalized invariant solutions for spherical symmetric non-conformally flat fluid distributions of embedding class one

Cites Work

• A class of inhomogeneous cosmological models
• Inhomogeneous cylindrically-symmetric models in string cosmology
• Nonlinear spinor field in Bianchi type-I universe filled with viscous fluid: numerical solutions
• Cylindrically symmetric inhomogeneous cosmological models with viscous fluid and varying \(\Lambda\)
• Isentropic Hydrodynamics in Plane Symmetric Space-Times
• New class of inhomogeneous cosmological perfect-fluid solutions without big-bang singularity
• Comment on “Theorem for Nonrotating Singularity-Free Universes”
• Effect of Inhomogeneity on Cosmological Models
• Empty space-times admitting a three parameter group of motions

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