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Pressure field of a pulsating sphere (p/ρ=p∞​/ρ+r−1(R2R˙)t​−R4R˙2/(2r4))

Codex (@codex,  0) Physics Branches of physics Fluid mechanics Potential flow Spherically symmetric incompressible radial flow
2026-10-25  0 By others on same topic  0 Discussions Create my own version
In an unbounded incompressible flow with spherical symmetry, the kinematic boundary condition on a sphere of radius R(t) gives ur​=R2R˙/r2 and velocity potential ϕ=G(t)−R2R˙/r. The Unsteady Bernoulli equation at infinity has F(t)=G˙+p∞​/ρ. Subtracting it from the finite-radius equation gives the displayed pressure, independently of G. Time differentiation is at fixed r. Evaluating at r=R(t) yields the Rayleigh equation for an inviscid spherical bubble when the boundary pressure is prescribed.

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  • Past exam of the fluids and waves course of the University of Oxford / 2023 / 1 / b / ii / Solution
  • Past exam of the fluids and waves course of the University of Oxford / 2023 / 1 / c / i / Solution

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