The shock-induced collapse of a pre-existing nucleus near a solid surface in the focal region of a lithotripter is investigated. The entire flow field of the collapse of a single gas bubble subjected to a lithotripter pulse is simulated using a high-order accurate shock- and interface-capturing scheme, and the wall pressure is considered as an indication of potential damage. Results from the computations show the same qualitative behavior as that observed in experiments: a re-entrant jet forms in the direction of propagation of the pulse and penetrates the bubble during collapse, ultimately hitting the distal side and generating a water-hammer shock. As a result of the propagation of this wave, wall pressures on the order of 1 GPa may be achieved for bubbles collapsing close to the wall. The wall pressure decreases with initial stand-off distance and pulse width and increases with pulse amplitude. For the stand-off distances considered in the present work, the wall pressure due to bubble collapse is larger than that due to the incoming shockwave; the region over which this holds may extend to ten initial radii. The present results indicate that shock-induced collapse is a mechanism with high potential for damage in shockwave lithotripsy.
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October 2008
October 01 2008
Shock-induced collapse of a gas bubble in shockwave lithotripsy
Eric Johnsen;
Eric Johnsen
a)
Division of Engineering and Applied Science,
California Institute of Technology
, Pasadena, California 91125
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Tim Colonius
Tim Colonius
b)
Division of Engineering and Applied Science,
California Institute of Technology
, Pasadena, California 91125
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a)
Electronic mail: johnsen@stanford.edu; present address: Center for Turbulence Research, Stanford University, CA 94305-3030.
b)
Electronic mail: colonius@caltech.edu
J. Acoust. Soc. Am. 124, 2011–2020 (2008)
Article history
Received:
April 23 2008
Accepted:
July 21 2008
Citation
Eric Johnsen, Tim Colonius; Shock-induced collapse of a gas bubble in shockwave lithotripsy. J. Acoust. Soc. Am. 1 October 2008; 124 (4): 2011–2020. https://doi.org/10.1121/1.2973229
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