Monte Carlo simulation of electron-ion recombination at high pressure
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Cited by (11)
Electron Collision Data for Plasma Chemistry Modeling
2000, Advances in Atomic, Molecular and Optical PhysicsCitation Excerpt :It was found experimentally by Warman et al. (1979) and by Armstrong et al. (1982) that in some molecular gases at pressures ranging from 100 torr to several atmospheres, the dissociative recombination rate coefficient is enhanced by termolecular effects. This was simulated for electrons in H2O, NH3, and CO2 by Morgan and Bardsley (1983) and by Morgan (1984a, 1984b) using numerical Monte Carlo techniques. The effect comes about because of the large low-energy inelastic collision cross sections in these gases.
Electron-ion recombination in condensed nonpolar media
1993, Nuclear Inst. and Methods in Physics Research, AElectron-Ion and Ion-Ion Recombination
2006, Springer HandbooksElectron-Ion Recombination in Condensed Matter: Geminate and Bulk Recombination Processes
2003, Charged Particle and Photon Interactions with Matter: Chemical, Physicochemical, and Biological Consequences with ApplicationsElectron-ion recombination rate constant in dense gaseous argon and krypton
1999, Journal of Chemical Physics
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