Past exam of the mathematics course of the University of Cambridge 2014 iii Paper 77 2 b Solution Created 2026-10-03 Updated 2026-10-07
Scale time by , length by , velocity by , pressure by , and streamfunction by . Write , , and drop stars from dimensionless coordinates. The surface is and its material velocity in the sheet frame is . The no-slip boundary condition is thereforeThe stationary matrix identifies a preferred frame. In the sheet frame it translates with , so matrix-relative Brinkman velocity gives the consistent equationsEquivalently one may keep the printed right-hand side after defining ; then the far-field pressure has the gradient needed to balance that term. Using the printed equation with a uniform far-field flow and no such adjustment is inconsistent. The distinction first matters at second order, since the first-order swimming speed is zero. We solve the upper half-space; the lower half-space is its reflected counterpart.
Past exam of the mathematics course of the University of Cambridge 2014 iii Paper 77 2 e Solution Created 2026-10-03 Updated 2026-10-07
A Taylor expansion of the tangential no-slip boundary condition gives . Since ,For matrix-relative Brinkman velocity, the mean second-order tangential flow isThe mean tangential traction has no first-order geometric remainder: at the surface and , so the mean displaced-boundary and tilted-normal corrections cancel. Thus the force-free condition gives , hence . In the limit boundedness likewise excludes mean shear. The swimming speed of a Brinkman sheet is thereforeIt is larger than the simple-fluid speed by for fixed waveform and frequency. The matrix offers a reaction structure for the transverse stroke and more strongly confines the induced motion; it acts as a footing against which the wave pushes. This is a prescribed-stroke comparison, not a guarantee at fixed motor power. The small-amplitude expansion is at fixed ; a large- use also needs to control variation across the displaced boundary.