Abstract
The spectral shape and observed sonoluminescence emission from Xe bubbles in concentrated sulfuric acid is consistent only with blackbody emission from a spherical surface that fills the bubble. The interior of the observed 7000 K blackbody must be at least 4 times hotter than the emitting surface in order that the equilibrium light-matter interaction length be smaller than the radius. Bright emission is correlated with long emission times (∼10ns), sharp thresholds, unstable translational motion, and implosions that are sufficiently weak that contributions from the van der Waals hard core are small.
| Original language | English (US) |
|---|---|
| Article number | 254301 |
| Journal | Physical review letters |
| Volume | 95 |
| Issue number | 25 |
| DOIs | |
| State | Published - Dec 16 2005 |
ASJC Scopus subject areas
- General Physics and Astronomy
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