| Literature DB >> 16384462 |
Stephen D Hopkins1, Seth J Putterman, Brian A Kappus, Kenneth S Suslick, Carlos G Camara.
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 (approximately 10 ns), sharp thresholds, unstable translational motion, and implosions that are sufficiently weak that contributions from the van der Waals hard core are small.Entities:
Year: 2005 PMID: 16384462 DOI: 10.1103/PhysRevLett.95.254301
Source DB: PubMed Journal: Phys Rev Lett ISSN: 0031-9007 Impact factor: 9.161