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A Petrov type I cylindrically symmetric solution for perfect fluid in steady rigid body rotation

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Publication:4869478
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DOI10.1088/0264-9381/13/2/016zbMath0845.53062OpenAlexW1971427038MaRDI QIDQ4869478

William Davidson

Publication date: 11 March 1996

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/0264-9381/13/2/016


zbMATH Keywords

Einstein's equationsperfect fluidrigid body rotationstationary cylindrically symmetric solution


Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Exact solutions to problems in general relativity and gravitational theory (83C15)


Related Items (3)

Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα ⋮ Interior spacetimes sourced by stationary differentially rotating irrotational cylindrical fluids. Perfect fluids ⋮ Perfect fluid spacetimes with a purely magnetic Weyl tensor







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