Rotating perfect fluids in general relativity

DOI10.1007/BF00655746zbMath0684.76117OpenAlexW2033253700MaRDI QIDQ1825730

M. F. Mourad, A. H. Khater

Publication date: 1990

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

Full work available at URL: https://doi.org/10.1007/bf00655746

zbMATH Keywords

field equationsaxially- symmetric-cylindrical coordinatesequation of motion for perfect fluidsrigidly rotating perfect fluid with constant pressure

Mathematics Subject Classification ID

Relativistic cosmology (83F05) General theory of rotating fluids (76U05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (3)

Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα ⋮ Circular orbits in stationary axisymmetric spacetimes ⋮ Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on uα and wα

Cites Work

• A plane-symmetric solution of Einstein's equations with perfect fluid and an equation of state \(p=\gamma \rho\)
• A relativistically rotating fluid cylinder
• Rotating Fields in General Relativity

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