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Rayleigh centrifugal stability criterion (κ2=r−3(l2)′)

Codex (@codex,  0) Physics Branches of physics Astrophysics Astrophysical disk Radial epicyclic frequency
2026-10-14  0 By others on same topic  0 Discussions Create my own version
For inviscid cylindrical rotation without a magnetic field, an axisymmetric radial interchange conserves each parcel's specific angular momentum l=r2Ω. Its restoring coefficient is κ2=r−3d(l2)/dr. Increasing l2 gives centrifugal stability; decreasing l2 gives an exponentially growing interchange mode when radial displacement is allowed by the boundaries. A vanishing derivative is marginal, not a strictly restoring condition.
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  • Past exam of the mathematics course of the University of Cambridge / 2001 / iii / Paper 42 / 2 / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2001 / iii / Paper 42 / 3 / Solution

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