Do bubbles heat up as they collapse?

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    Bubbles Collapse Heat
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Discussion Overview

The discussion revolves around the phenomenon of bubble collapse, particularly in the context of cavitation bubbles and their potential to reach extremely high temperatures during this process. Participants explore the mechanisms behind this heating and the implications of bubble dynamics, referencing both theoretical and experimental aspects.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions the claim that bubbles can reach temperatures comparable to that of the sun, expressing confusion about the underlying mechanism.
  • Another participant explains that during the collapse of cavitation bubbles, the temperature can increase significantly, citing calculations that suggest maximum temperatures could be 4×104 times the ambient temperature, although various factors may affect this outcome.
  • A third participant supports the plausibility of high temperatures by comparing them to the sun's surface temperature, indicating that the calculated values align with this comparison.
  • Another participant presents a first principles approach, suggesting that as a bubble collapses, the internal pressure increases infinitely and that the process of gas condensing into the surrounding liquid contributes to heating, leading to the conclusion that the bubble could maintain a high temperature during collapse.

Areas of Agreement / Disagreement

Participants express varying levels of understanding and interpretation of the mechanisms involved in bubble collapse and heating. While some calculations suggest high temperatures are plausible, there is no consensus on the specifics of the mechanisms or the implications of these findings.

Contextual Notes

Participants acknowledge the complexity of bubble dynamics and the potential influence of various factors such as gas diffusion and liquid compressibility on the results. The discussion includes references to specialized literature and theoretical models, indicating a reliance on specific assumptions and conditions.

KingNothing
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In the video at http://www.spikedhumor.com/articles/108195/Real_Life_Creature_Assassin.html

they say something about the "bubbles momentarily reach the temperature of the sun". I don't understand this bit at all, or how this mechanism works.
 
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If you're referring to cavitation bubbles, it can increase in temperature quite a bit. Here is a great on-line reference for bubble dynamics and cavitation:

When a cavitation bubble grows from a small nucleus to many times its original size, the collapse will begin at a maximum radius, RM, with a partial pressure of gas, pGM, which is very small indeed. In a typical cavitating flow RM is of the order of 100 times the original nuclei size, Ro. Consequently, if the original partial pressure of gas in the nucleus was about 1 bar the value of pGM at the start of collapse would be about 10-6 bar. If the typical pressure depression in the flow yields a value for (p∞*-p∞(0)) of, say, 0.1 bar it would follow from Equation 2.38 that the maximum pressure generated would be about 1010 bar and the maximum temperature would be 4×104 times the ambient temperature! Many factors, including the diffusion of gas from the liquid into the bubble and the effect of liquid compressibility, mitigate this result. Nevertheless, the calculation illustrates the potential for the generation of high pressures and temperatures during collapse and the potential for the generation of shock waves and noise.

http://caltechbook.library.caltech.edu/1/04/chap3.htm#L1

Here is the TOC of the book:
http://caltechbook.library.caltech.edu/1/04/content.htm

This is a highly specialized field of study. I won't pretend to know anything except the very elemental aspects so I can't get into the deep physics of what is going on.
 
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The surface temperature of the sun is about 5800 degK i.e. about 20 times the ambient surface temperature of the earth, so FredGarvin's factor of "4x10^4 times the ambient temperature" is more than enough to make the initial statement plausible.
 
Just from first principles:

- as a bubble decreases to zero radius, the internal pressure increases infinitly (http://hyperphysics.phy-astr.gsu.edu/hbase/surten2.html#c2").

- the shrinking of the bubble involves the condensation of gas into the surrounding liquid, which is a heating process (opposite of evaporation).

From this I'm naively (neglecting the atomic scale) tempted to conclude that the bubble remains at a "boiling temperature" that with pressure goes also to infinity as the bubble collapses.
 
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