2001
DOI: 10.1080/09500340117525
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Sonoluminescence: how bubbles glow

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Cited by 44 publications
(16 citation statements)
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“…This imprecise nomenclature arose from acoustics being mainly used to generate the cavitation in the early decades (Marinesco & Trillat 1933;Jarman 1960;Knapp, Daily & Hammett 1970). The current debate on the commonality of the sources of the various luminescences calls this nomenclature into question (Barber et al 1992;Matula & Roy 1997;Blake 1999;Leighton, Cox & Phelps 2000;Hammer & Frommhold 2001).…”
Section: Introductionmentioning
confidence: 99%
“…This imprecise nomenclature arose from acoustics being mainly used to generate the cavitation in the early decades (Marinesco & Trillat 1933;Jarman 1960;Knapp, Daily & Hammett 1970). The current debate on the commonality of the sources of the various luminescences calls this nomenclature into question (Barber et al 1992;Matula & Roy 1997;Blake 1999;Leighton, Cox & Phelps 2000;Hammer & Frommhold 2001).…”
Section: Introductionmentioning
confidence: 99%
“…The £ value in normal ionisation translates to the gas being ~ 13.5% ionised at 10000 K and ~ 37% ionised at 20000 K. This corresponds to slightly more ionisation (and, hence, more energy involvement) at a given temperature threshold than SL research suggests [2,9]. However, other effects such as chemical reactions (which, at bubble collapse, absorb heat energy in a similar way to ionisation) have not been included in this model, so a conservative £ estimate was used to accommodate them.…”
Section: Ionisation Parameters Following the Derivation And Implementmentioning
confidence: 97%
“…The only adjustable parameters in the comparison are the ambient radii and forcing pressures of the bubbles. From Hammer and Frommhold (2001). sured values, and is an indication that the modeling overestimates the amount of water vapor in the bubble.…”
Section: Figmentioning
confidence: 97%
“…Depending on the actual temperatures achieved during collapse, different excitations become dominant in the compressed gas, so that ''thermal emission'' can refer to a large variety of different processes. As temperatures increase from several hundred to many thousand kelvin, those processes can be, among others, molecular recombination (Saksena and Nyborg, 1970), collision-induced emission (Frommhold and Atchley, 1994), molecular emission (Didenko et al, 2000b), excimers (Hammer and Frommhold, 2001), atomic recombination (Hilgenfeldt et al, 1999b), radiative attachment of ions (Hammer and Frommhold, 2001), neutral and ion bremsstrahlung (Moss et al, 1997;Xu et al, 1998;Hilgenfeldt et al, 1999b), or emission from confined electrons in voids (Bernstein and Zakin, 1995). The uncertainty about the precise temperatures of SBSL bubbles (see Sec.…”
Section: B Sbsl: a Multitude Of Theoriesmentioning
confidence: 99%