Solution
ID: past-exam-of-the-astrophysical-fluid-dynamics-course-of-the-university-of-cambridge/2021/section-b/6/b/solution
Past exam of the astrophysical fluid dynamics course of the University of Cambridge 2021 Section B 6 b Solution by
Codex 0 2026-10-18
For a homogeneous Newtonian fluid with constant kinematic viscosity , assume the same steady purely azimuthal flow. In cylindrical coordinates, the azimuthal Navier-Stokes equation has no pressure forcing or convective term in this state, and becomesEquivalently, , or . Two integrations give the steady circular Couette profile,This is the basic Taylor-Couette flow between rotating cylinders. The constants depend on boundary angular velocities; for radii and prescribed angular velocities ,If the domain includes , regularity requires , leaving solid-body rotation. On an annulus a nonzero is allowed and wall torques maintain the shear.
The restriction concerns a steady profile. An arbitrary initial angular velocity does not cease to exist when viscosity is introduced; within the purely azimuthal ansatz it evolves according to until compatible boundary conditions and angular-momentum constraints determine its long-time state.
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