3.II.18D3 . \mathrm{II} . 18 \mathrm{D}

Fluid Dynamics | Part IB, 2007

Given that the circulation round every closed material curve in an inviscid, incompressible fluid remains constant in time, show that the velocity field of such a fluid started from rest can be written as the gradient of a potential, ϕ\phi, that satisfies Laplace's equation.

A rigid sphere of radius a moves in a straight line at speed UU in a fluid that is at rest at infinity. Using axisymmetric spherical polar coordinates (r,θ)(r, \theta), with θ=0\theta=0 in the direction of motion, write down the boundary conditions on ϕ\phi and, by looking for a solution of the form ϕ=f(r)cosθ\phi=f(r) \cos \theta, show that the velocity potential is given by

ϕ=Ua3cosθ2r2\phi=\frac{-U a^{3} \cos \theta}{2 r^{2}}

Calculate the kinetic energy of the fluid.

A rigid sphere of radius aa and uniform density ρb\rho_{b} is submerged in an infinite fluid of density ρ\rho, under the action of gravity. Show that, when the sphere is released from rest, its initial upwards acceleration is

2(ρρb)gρ+2ρb\frac{2\left(\rho-\rho_{b}\right) g}{\rho+2 \rho_{b}}

[Laplace's equation for an axisymmetric scalar field in spherical polars is:

1r2r(r2ϕr)+1r2sinθθ(sinθϕθ)=0.]\left.\frac{1}{r^{2}} \frac{\partial}{\partial r}\left(r^{2} \frac{\partial \phi}{\partial r}\right)+\frac{1}{r^{2} \sin \theta} \frac{\partial}{\partial \theta}\left(\sin \theta \frac{\partial \phi}{\partial \theta}\right)=0 .\right]

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