TY - JOUR
T1 - Plasma line emission during single-bubble cavitation
AU - Flannigan, David J.
AU - Suslick, Kenneth S.
PY - 2005/7/22
Y1 - 2005/7/22
N2 - Emission lines from transitions between high-energy states of noble-gas atoms (Ne, Ar, Kr, and Xe) and ions (Ar+, Kr+, and Xe+) formed and excited during single-bubble cavitation in sulfuric acid are reported. The excited states responsible for these emission lines range 8.3 eV (for Xe) to 37.1 eV (for Ar+) above the respective ground states. Observation of emission lines allows for identification of intracavity species responsible for light emission; the populated energy levels indicate the plasma generated during cavitation is comprised of highly energetic particles.
AB - Emission lines from transitions between high-energy states of noble-gas atoms (Ne, Ar, Kr, and Xe) and ions (Ar+, Kr+, and Xe+) formed and excited during single-bubble cavitation in sulfuric acid are reported. The excited states responsible for these emission lines range 8.3 eV (for Xe) to 37.1 eV (for Ar+) above the respective ground states. Observation of emission lines allows for identification of intracavity species responsible for light emission; the populated energy levels indicate the plasma generated during cavitation is comprised of highly energetic particles.
UR - http://www.scopus.com/inward/record.url?scp=27144458372&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=27144458372&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.95.044301
DO - 10.1103/PhysRevLett.95.044301
M3 - Article
C2 - 16090812
AN - SCOPUS:27144458372
SN - 0031-9007
VL - 95
JO - Physical review letters
JF - Physical review letters
IS - 4
M1 - 044301
ER -