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Oscillations, Waves, and Interactions - GWDG

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184 R. Mettin<br />

which is called the primary Bjerknes force.<br />

The st<strong>and</strong>ard discussion of this average considers weak bubble oscillations <strong>and</strong> a<br />

plane st<strong>and</strong>ing or travelling pressure wave [4,5]. Then the results can be captured by<br />

the relative phase of pressure <strong>and</strong> bubble oscillation, which depends on the bubble<br />

size R0 in relation to the linear resonance radius Rres: larger bubbles are attracted by<br />

pressure nodes, <strong>and</strong> smaller by the pressure antinodes. In propagating waves, bubbles<br />

around Rres feel a strong force in the wave’s direction, <strong>and</strong> the force diminishes for<br />

bubbles much smaller or much larger than the linear resonance size.<br />

In the case of strongly driven bubbles, which is typical for cavitating liquids, F B1<br />

becomes more complicated because of the anharmonic bubble oscillation. In particular,<br />

the collapse time of stronger <strong>and</strong> stronger exp<strong>and</strong>ing bubbles shifts to later<br />

instances, <strong>and</strong> thus the primary Bjerknes force in st<strong>and</strong>ing waves can change its sign<br />

at high pressure zones for small bubbles. This effect was first noted in the context of<br />

SBSL [36,37], <strong>and</strong> it is very important for cavitation fields: also bubbles <strong>and</strong> bubble<br />

clusters much smaller than the linear resonance radius can get expelled from pressure<br />

antinodes, <strong>and</strong> the high pressure regions may get depleted.<br />

Figure 10 shows for the two typical ultrasonic frequencies 20 kHz <strong>and</strong> 1 MHz the<br />

regions in R0 − pa parameter space where the bubbles are driven away from the<br />

pressure antinode due to the primary Bjerknes force. Here, pa is the local driving<br />

amplitude at the bubble’s position <strong>and</strong> can usually be identified with a spatial position<br />

in the st<strong>and</strong>ing wave. In the case of a traveling wave, the changes caused by<br />

nonlinear bubble oscillations are not so dramatic, although the forces can get much<br />

larger than for linear approximation, <strong>and</strong> also parameter combinations exist where<br />

the sign reverses, i. e., the bubbles feel a primary Bjerknes force against the wave<br />

direction [38].<br />

p a [kPa]<br />

200<br />

180<br />

160<br />

140<br />

120<br />

100<br />

80<br />

60<br />

40<br />

20<br />

20 kHz<br />

0<br />

0 20 40 60 80 100 120 140 160 180<br />

R0 [µm]<br />

p a [kPa]<br />

400<br />

350<br />

300<br />

250<br />

200<br />

150<br />

100<br />

50<br />

1 MHz<br />

0<br />

0 0.5 1 1.5 2<br />

R0 [µm]<br />

2.5 3 3.5 4<br />

Figure 10. Sign of the primary Bjerknes force in a st<strong>and</strong>ing sound wave in the parameter<br />

space of bubble equilibrium radius R0 <strong>and</strong> pressure amplitude pa. White areas indicate a<br />

force towards the high pressure regions, dark areas a force towards the pressure nodes. Left:<br />

f = 20 kHz, Rres = 138 µm; right: f = 1 MHz, Rres = 3.15 µm (water at normal conditions,<br />

κ = 1, σ = 0.07275 N/m).

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