A class of solutions of Einstein's equations for the interior of a rigidly rotating perfect fluid

DOI10.1007/BF00758118zbMath0637.53090OpenAlexW2068347400MaRDI QIDQ1098441

E. Kyriakopoulos

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1007/bf00758118

zbMATH Keywords

Einstein's equationsperfect fluid

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Applications of local differential geometry to the sciences (53B50)

Cites Work

• Relativistic, stationary, axisymmetric perfect fluids. I. Reduction to a system of two equations
• Relativistic, stationary, axisymmetric perfect fluids. II. Solutions with vanishing magnetic Weyl tensor
• Solutions of Einstein’s equations for the interior of a stationary axisymmetric perfect fluid

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