The stability of a differentially rotating cylinder of an incompressible perfect fluid
The stability criterion for differentially rotating fluid cylinders given by Goldreich, Goodman & Narayan is re-examined. A rotation law of the form $\Omega_0\propto r^{-q}$ is assumed for the unperturbed state, where Ω0, r and q are the angular velocity, the distance from the central star and a...
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Published in: | Monthly notices of the Royal Astronomical Society Vol. 234; no. 1; pp. 107 - 114 |
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Main Authors: | , |
Format: | Journal Article |
Language: | English |
Published: |
Oxford, UK
Oxford University Press
01-09-1988
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Online Access: | Get full text |
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Summary: | The stability criterion for differentially rotating fluid cylinders given by Goldreich, Goodman & Narayan is re-examined. A rotation law of the form $\Omega_0\propto r^{-q}$ is assumed for the unperturbed state, where Ω0, r and q are the angular velocity, the distance from the central star and a constant, respectively. We find that, even for$q\gt\sqrt 3$ a cylinder of an incompressible fluid is unstable provided that the half thickness of the cylinder, a is finite. The growth rate of a small perturbation is proportional to a2 as long as a≪3−q2. |
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Bibliography: | Present address: Department of Applied Physics, Tokyo Institute of Technology, Ookayama 2-12-1, Meguro-ku, Tokyo 152, Japan. istex:23C1666B229DC0948F8A15EB55BF4BE4070F3050 ark:/67375/HXZ-QPFKQ6F9-S |
ISSN: | 0035-8711 1365-2966 |
DOI: | 10.1093/mnras/234.1.107 |