Paper 3, Section II, D

Fluid Dynamics
Part IB, 2009

Starting from Euler's equations for an inviscid incompressible fluid of density ρ\rho with no body force, undergoing irrotational motion, show that the pressure pp is given by

pρ+ϕt+12(ϕ)2=F(t)\frac{p}{\rho}+\frac{\partial \phi}{\partial t}+\frac{1}{2}(\nabla \phi)^{2}=F(t)

for some function F(t)F(t), where ϕ\phi is the velocity potential.

The fluid occupies an infinite domain and contains a spherical gas bubble of radius R(t)R(t) in which the pressure is pgp_{g}. The pressure in the fluid at infinity is pp_{\infty}.

Show that

R¨R+32R˙2=pgpρ\ddot{R} R+\frac{3}{2} \dot{R}^{2}=\frac{p_{g}-p_{\infty}}{\rho}

The bubble contains a fixed mass MM of gas in which

pg=C(M/R3)2p_{g}=C\left(M / R^{3}\right)^{2}

for a constant CC. At time t=0,R=R0,R˙=0t=0, R=R_{0}, \dot{R}=0 and pg=p/2p_{g}=p_{\infty} / 2. Show that

R˙2R3=pρ[R03R063R323R3]\dot{R}^{2} R^{3}=\frac{p_{\infty}}{\rho}\left[R_{0}^{3}-\frac{R_{0}^{6}}{3 R^{3}}-\frac{2}{3} R^{3}\right]

and deduce that the bubble radius oscillates between R0R_{0} and R0/21/3R_{0} / 2^{1 / 3}.