Solution generating with perfect fluids

DOI10.1023/A:1018882615955zbMath0872.53058arXivgr-qc/9611052OpenAlexW1636036996MaRDI QIDQ1357822

David Garfinkle, J. P. Kirsch, E. N. Glass

Publication date: 19 October 1997

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9611052

zbMATH Keywords

symmetryEinstein equationsenergy-momentum tensorKilling vector

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (5)

On the connection between cosmological parameters and peculiar motion in a G2 massless scalar field spacetime ⋮ Adding twist to anisotropic fluids ⋮ Physically viable rotating mass solutions surrounding Kerr black holes ⋮ Spikes and matter inhomogeneities in massless scalar field models ⋮ GENERATING ANISOTROPIC FLUIDS FROM VACUUM ERNST EQUATIONS

Cites Work

• Unnamed Item
• A Petrov type-III perfect fluid solution of Einstein's equations
• Spatially homogeneous and inhomogeneous cosmologies with equation of state p=mu
• Plane symmetric self-gravitating fluids with pressure equal to energy density
• Cylindrically symmetric static perfect fluids
• Symmetries of Einstein’s field equations with a perfect fluid source as examples of Lie–Bäcklund symmetries
• New Solutions of the Einstein-Maxwell Equations from Old
• A Method for Generating Solutions of Einstein's Equations
• The Large Scale Structure of Space-Time

This page was built for publication: Solution generating with perfect fluids