Slowly rotating perfect fluids with a cosmological constant

DOI10.1007/S10714-015-1982-5zbMath1338.83051arXiv1411.5486OpenAlexW2165798299MaRDI QIDQ276096

F. Blanchet-Sadri, M. Dambrine

Publication date: 27 April 2016

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

Full work available at URL: https://arxiv.org/abs/1411.5486

zbMATH Keywords

slow rotationcosmological constantHartle's formalismWahlquist's rotating perfect fluid interior solution

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) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Cites Work

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• An approximate global solution of Einstein's equation for a rotating compact source with linear equation of state
• Ellipsoidal space-times, sources for the Kerr metric
• Rotating Fields in General Relativity
• General Relativistic Gravitational Field of a Rigidly Rotating Disk of Dust: Solution in Terms of Ultraelliptic Functions
• Axistationary perfect fluids - a tetrad approach
• The Wahlquist metric cannot describe an isolated rotating body
• Source of the Kerr Metric

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