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Inertial shocks in surface waves and collapsing bubbles

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Book cover Bubble Dynamics and Interface Phenomena

Part of the book series: Fluid Mechanics and Its Applications ((FMIA,volume 23))

Abstract

There exists a class of analytic, free-surface flows which describes qualitatively the highly-accelerated re-entrant jets seen in bubble generation and collapse. In semi-Langrangian coordinates such a flow is given by

$$ x + iy = ({F_1}\sin \omega - i{G_1}\cos {\rm{ }}\omega ) + {1 \over 2}({F_2}\sin 2\omega - i{\rm{ }}{G_2}{\rm{ }}\cos {\rm{ }}2\omega ) $$

where ? is a complex parameter, real at the free surface. The coefficients F 1, G 1, F 2 and G 2 are real functions of the time t only, related by a set of nonlinear, ordinary differential equations, so as to satisfy appropriate boundary conditions and conditions of regularity in the fluid. A wide variety of such flows exists, depending on the initial conditions. One remarkable feature of many of the flows is the occurrence of a sudden “inertial shock” at a critical time t = t o. This usually happens when the surface locally has the form of a rectangular hyperbola — as in the previously known “Dirichlet hyperbola”. The phenomenon is illustrated by the behaviour of the inwards acceleration y tt at the point ? = 0 on the free surface (the tip of the jet). The acceleration becomes infinite like (tt o)−4/3, near the instant t o.

Solutions also exist with two jets directed inwards from opposite sides of the bubble — or indeed any number of such jets per bubble.

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© 1994 Springer Science+Business Media Dordrecht

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Longuet-Higgins, M.S. (1994). Inertial shocks in surface waves and collapsing bubbles. In: Blake, J.R., Boulton-Stone, J.M., Thomas, N.H. (eds) Bubble Dynamics and Interface Phenomena. Fluid Mechanics and Its Applications, vol 23. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0938-3_36

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  • DOI: https://doi.org/10.1007/978-94-011-0938-3_36

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4404-2

  • Online ISBN: 978-94-011-0938-3

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