scientific article; zbMATH DE number 1515728

DOI<342::AID-ANDP342>3.0.CO;2-L 10.1002/(SICI)1521-3889(200005)9:3/5<342::AID-ANDP342>3.0.CO;2-LzbMath0972.83041MaRDI QIDQ4508100

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Publication date: 22 November 2001

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zbMATH Keywords

rotating starsperfect fluidsaxisymmetric stationary solutions

Mathematics Subject Classification ID

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)

Non-existence of stationary two-black-hole configurations: the degenerate case ⋮ On the balance problem for two rotating and charged black holes ⋮ A Physical Derivation of the Kerr–Newman Black Hole Solution ⋮ Stationary two-black-hole configurations: A non-existence proof ⋮ Stationary Black-Hole Binaries: A Non-existence Proof

Cites Work

• Conditions for Regularity on the Symmetry Axis in a Superposition of Two Kerr-NUT Solutions
• Asymptotically flat solutions to the Ernst equation with reflection symmetry
• General Relativity

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