Influence of ambient temperature on cavitation bubble dynamics

We examine how ambient temperature $T$ (23–90 $^\circ \mathrm{C}$ ) alters the dynamics of spark-induced cavitation bubbles across a range of discharge energies. As $T$ rises, the collapse of an isolated spherical bubble weakens monotonically, as quantified by the Rayleigh collapse factor, minimum volume and maximum collapse velocity. When the bubble is generated near a rigid wall, the same thermal attenuation is reflected in reduced jet speed and diminished migration. Most notably, at $T \gtrsim 70\,^\circ \text{C}$ , we observe a previously unreported phenomenon: secondary cavitation nuclei appear adjacent to the primary bubble interface where the local pressure falls below the Blake threshold. The pressure reduction is produced by the over-expansion of the primary bubble itself, not by rarefaction waves as suggested in earlier work. Coalescence between these secondary nuclei and the parent bubble seeds pronounced surface wrinkles that intensify Rayleigh–Taylor instability and promote fission, providing an additional route for collapse strength attenuation. These findings clarify the inception mechanism of high-temperature cavitation and offer physical insight into erosion mitigation in heated liquids.

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Publication Details

Journal
Journal of Fluid Mechanics
Published
2025-11-20
DOI
https://doi.org/10.1017/jfm.2025.10838
Citations
6
Primary Topic
Ultrasound and Cavitation Phenomena
Type
article
Field-Weighted Citation Impact
3.11

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article

Influence of ambient temperature on cavitation bubble dynamics

Shao-Cong Pei, Tianyuan Zhang, A‐Man Zhang, Rui Han et al.
6 citations
Journal of Fluid Mechanics
Ultrasound and Cavitation Phenomena
3.11
article

Influence of ambient temperature on cavitation bubble dynamics

Shao-Cong Pei, Tianyuan Zhang, A‐Man Zhang, Rui Han, Shuai Li, Chang Liu
article en
6 citations

Abstract

We examine how ambient temperature $T$ (23–90 $^\circ \mathrm{C}$ ) alters the dynamics of spark-induced cavitation bubbles across a range of discharge energies. As $T$ rises, the collapse of an isolated spherical bubble weakens monotonically, as quantified by the Rayleigh collapse factor, minimum volume and maximum collapse velocity. When the bubble is generated near a rigid wall, the same thermal attenuation is reflected in reduced jet speed and diminished migration. Most notably, at $T \gtrsim 70\,^\circ \text{C}$ , we observe a previously unreported phenomenon: secondary cavitation nuclei appear adjacent to the primary bubble interface where the local pressure falls below the Blake threshold. The pressure reduction is produced by the over-expansion of the primary bubble itself, not by rarefaction waves as suggested in earlier work. Coalescence between these secondary nuclei and the parent bubble seeds pronounced surface wrinkles that intensify Rayleigh–Taylor instability and promote fission, providing an additional route for collapse strength attenuation. These findings clarify the inception mechanism of high-temperature cavitation and offer physical insight into erosion mitigation in heated liquids.

Journal of Fluid MechanicsVol. 1023
Harbin Engineering University (CN), Sanya University (CN)
National Natural Science Foundation of China, Harbin Engineering University
Openalex Percentile: Top 8%
Ultrasound and Cavitation Phenomena
3.11
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