All flow-stationary cylindrically symmetric solutions of the Einstein field equations for a rotating isentropic perfect fluid

DOI10.1016/0034-4877(78)90045-9zbMath0427.76099OpenAlexW2008714802MaRDI QIDQ1136582

Publication date: 1978

Published in: Reports on Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0034-4877(78)90045-9

zbMATH Keywords

Einstein field equations flow-stationary cylindrically symmetric solutions rotating isentropic perfect fluid

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (9)

Fully integrated interior solutions of GR for stationary rigidly rotating cylindrical perfect fluids ⋮ Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα ⋮ The parameters of the Lewis metric for the Weyl class ⋮ Homogeneous and hypersurface-homogeneous shear-free perfect fluids in general relativity ⋮ Type-N, shear-free, perfect-fluid spacetimes with a barotropic equation of state ⋮ A class of perfect fluid metrics with flat three-dimensional hypersurfaces ⋮ Classification of cylindrically symmetric static spacetimes according to their Ricci collineations ⋮ Shear-free perfect fluids with zero magnetic Weyl tensor ⋮ Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on uα and wα

Cites Work

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