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Oscillations, Waves, and Interactions - GWDG

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140 W. Lauterborn et al.<br />

liquid<br />

κ<br />

pi<br />

Figure 1. Descriptors for a spherical bubble: bubble radius R(t), rest radius Rn, internal<br />

pressure pi, external pressure pe. Parameters of the liquid: density ρ, viscosity µ, <strong>and</strong><br />

surface tension σ. The bubble medium is characterized by the polytropic exponent κ.<br />

2.1 Bubble models<br />

To formulate a bubble model, various parameters of the liquid surrounding the bubble<br />

<strong>and</strong> of the gas <strong>and</strong> vapour contents inside the bubble need to be specified. For<br />

a spherical bubble the dependent variables can be condensed to just one, the bubble<br />

radius R whose variation with time t has to be determined, R(t). The model parameters<br />

as used here are given in Fig. 1. Besides R these are the radius of the bubble at<br />

rest, Rn, the external pressure in the liquid, pe, <strong>and</strong> the pressure inside the bubble,<br />

pi, further the polytropic exponent of the gas in the bubble, κ, <strong>and</strong> ρ, µ, <strong>and</strong> σ, the<br />

density, the viscosity, <strong>and</strong> the surface tension of the liquid, respectively.<br />

The simplest model is the Rayleigh model [2]:<br />

R<br />

R<br />

n<br />

σ<br />

p e<br />

ρ, µ<br />

ρR ¨ R + 3<br />

2 ρ ˙ R 2 = pi − pe , (1)<br />

where an overdot means differentiation with respect to time. The difference in pressure,<br />

pi−pe, drives the bubble motion. The form of the inertial terms on the left-h<strong>and</strong><br />

side is due to the spherical three-dimensional geometry that is transformed to one<br />

radial dimension in the differential equation. Both, pi <strong>and</strong> pe, become functions of<br />

radius R <strong>and</strong> time t, when gas <strong>and</strong> vapour fill the bubble, <strong>and</strong> when surface tension<br />

σ, liquid viscosity µ, <strong>and</strong> a sound field are taken into account. With these inclusions<br />

the Rayleigh model takes the form [3–6]:<br />

with<br />

ρR ¨ R + 3<br />

2 ρ ˙ R 2 = pgn<br />

� �3κ Rn<br />

+ pv − pstat −<br />

R<br />

2σ 4µ<br />

−<br />

R R ˙ R − p(t) , (2)<br />

pgn = 2σ<br />

Rn<br />

+ pstat − pv , (3)<br />

Rn being the equilibrium radius, pstat the static pressure, pv the (constant) vapour

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