Paper 1, Section II, B

Fluid Dynamics
Part IB, 2014

Consider the purely two-dimensional steady flow of an inviscid incompressible constant density fluid in the absence of body forces. For velocity u\mathbf{u}, the vorticity is ×u=ω=(0,0,ω)\boldsymbol{\nabla} \times \mathbf{u}=\boldsymbol{\omega}=(0,0, \omega). Show that

u×ω=[pρ+12u2]\mathbf{u} \times \boldsymbol{\omega}=\boldsymbol{\nabla}\left[\frac{p}{\rho}+\frac{1}{2}|\mathbf{u}|^{2}\right]

where pp is the pressure and ρ\rho is the fluid density. Hence show that, if ω\omega is a constant in both space and time,

12u2+ωψ+pρ=C,\frac{1}{2}|\mathbf{u}|^{2}+\omega \psi+\frac{p}{\rho}=C,

where CC is a constant and ψ\psi is the streamfunction. Here, ψ\psi is defined by u=×Ψ\mathbf{u}=\boldsymbol{\nabla} \times \boldsymbol{\Psi}, where Ψ=(0,0,ψ)\boldsymbol{\Psi}=(0,0, \psi).

Fluid in the annular region a<r<2aa<r<2 a has constant (in both space and time) vorticity ω\omega. The streamlines are concentric circles, with the fluid speed zero on r=2ar=2 a and V>0V>0 on r=ar=a. Calculate the velocity field, and hence show that

ω=2V3a\omega=\frac{-2 V}{3 a}

Deduce that the pressure difference between the outer and inner edges of the annular region is

Δp=(1516ln218)ρV2\Delta p=\left(\frac{15-16 \ln 2}{18}\right) \rho V^{2}

[Hint: Note that in cylindrical polar coordinates (r,ϕ,z)(r, \phi, z), the curl of a vector field A(r,ϕ)=[a(r,ϕ),b(r,ϕ),c(r,ϕ)]\mathbf{A}(r, \phi)=[a(r, \phi), b(r, \phi), c(r, \phi)] is

×A=[1rcϕ,cr,1r((rb)raϕ)]\boldsymbol{\nabla} \times \mathbf{A}=\left[\frac{1}{r} \frac{\partial c}{\partial \phi},-\frac{\partial c}{\partial r}, \frac{1}{r}\left(\frac{\partial(r b)}{\partial r}-\frac{\partial a}{\partial \phi}\right)\right]