Caltech Water-Ice Dusty Plasma Experiment Upgrade and Analysis of Creation of Hot Electron Tail and its Effect on Dust Charging
POSTER
Abstract
The Caltech water-ice dusty plasma experiment has water vapor injected into a capacitively coupled RF plasma with LN2-cooled electrodes. Water ice grains form spontaneously in the weakly-ionized plasma with extremely cold background gas. The experiment is undergoing a significant upgrade wherein the RF electrodes will be cooled by a liquid helium cryocooler to enable lower and more controlled temperatures. Status of this upgrade will be reported.
The electron energy distribution in a weakly-ionized dusty plasma depends on a competition between electron creation by ionization, electron cooling by collisions with neutrals, and electron loss via recombination. Free electrons created by ionization have energy of a few eV but then cool down to a small fraction of an eV via collisions with the cold neutrals. There is thus a steady-state hot “tail” of energetic just-created free electrons coexisting with a much larger population of cold electrons. Detailed computations of the collision cascade show that the hot tail can be so large as to substantially increase the dust grain charge.
The electron energy distribution in a weakly-ionized dusty plasma depends on a competition between electron creation by ionization, electron cooling by collisions with neutrals, and electron loss via recombination. Free electrons created by ionization have energy of a few eV but then cool down to a small fraction of an eV via collisions with the cold neutrals. There is thus a steady-state hot “tail” of energetic just-created free electrons coexisting with a much larger population of cold electrons. Detailed computations of the collision cascade show that the hot tail can be so large as to substantially increase the dust grain charge.
Presenters
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André Nicolov
Caltech
Authors
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André Nicolov
Caltech
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Paul M Bellan
Caltech