Slowly, rotating non-stationary, fluid solutions of Einstein's equations and their match to Kerr empty space-time

DOI10.1023/A:1022332824643zbMath1039.83016arXivgr-qc/0202065MaRDI QIDQ1868460

Ronald J. Wiltshire

Publication date: 27 April 2003

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0202065

zbMATH Keywords

junction conditionfluid sourcerotating solution

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items

Revisiting the Darmois and Lichnerowicz junction conditions, Robertson-Walker fluid sources endowed with rotation characterised by quadratic terms in angular velocity parameter

Cites Work

• Geometry of general hypersurfaces in spacetime: junction conditions
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• The Mass-Particle in an Expanding Universe
• The Wahlquist metric cannot describe an isolated rotating body
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