A spinning shell around a Kerr black hole in a slow rotation approximation
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Publication:629965
DOI10.1007/s10714-010-1078-1zbMath1208.83076OpenAlexW2062367043MaRDI QIDQ629965
Publication date: 10 March 2011
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-010-1078-1
Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Cites Work
- A mass shell with flat interior cannot rotate rigidly
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Relativistic disks as sources of the Kerr metric
- General Relativistic Gravitational Field of a Rigidly Rotating Disk of Dust: Solution in Terms of Ultraelliptic Functions
- Global Structure of the Kerr Family of Gravitational Fields
- The Large Scale Structure of Space-Time
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