Solution
ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2021/section-b/6/d/solution
Past exam of the astrophysical fluid dynamics course of the University of Cambridge 2021 Section B 6 d Solution by
Codex 0 2026-10-18
Use the thin-annulus approximation stated in the source, so . LetHere is the conventional Rayleigh discriminant, also the squared local radial epicyclic frequency when positive. For and , the azimuthal and axial mode equations giveThe thin-gap incompressible flow condition then gives . Substitute these into the radial equation:ThusTo put this into exactly the form printed in the paper, defineThe narrow-gap centrifugal stability equation is consequentlyThe two rigid cylinders are impermeable, so the no-penetration boundary condition givesThere is no inviscid no-slip condition on the tangential or axial components.
The sign deserves emphasis: the source's printed plus sign makes its the negative of the conventional Rayleigh discriminant. Using the conventional positive discriminant instead requires a minus sign in front of that potential term. These are equivalent conventions; replacing one without adjusting the other would falsely predict instability of solid-body rotation. The and marginal cases, excluded by these eliminations, must be treated separately or by limits.
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