Narrow-gap centrifugal stability equation

ID: narrow-gap-centrifugal-stability-equation

For axisymmetric inviscid modes between impermeable cylinders in a thin annulus, let and . The linear azimuthal equation gives and the axial equation gives , where is the kinematic pressure perturbation. Thin-gap incompressibility implies . Eliminating it from the radial equation gives the title equation with . If a plus sign is used for the potential, its coefficient must be defined as , the negative of the usual Rayleigh discriminant.

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