2008
DOI: 10.1063/1.2996964
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Dust Charge in Cryogenic Environment

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Cited by 8 publications
(8 citation statements)
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“…The microparticles in size of submicrometers to submillimeters have been called as dust grains or dust particles in the study of interstellar space as early as 1940s. Complex plasma has attracted much attention to the community of plasma physics [1][2][3][4], while recent advances in ultracold plasma [5][6][7][8][9] and cryogenic dusty plasma [10][11][12][13][14][15][16][17] challenge the basic understanding of plasmas. The Debye length, characterized by temperatures of electrons and ions, in a cryogenic plasma becomes much smaller than that in a conventional laboratory plasma and becomes comparable to the size of a dust particle.…”
Section: Introductionmentioning
confidence: 99%
“…The microparticles in size of submicrometers to submillimeters have been called as dust grains or dust particles in the study of interstellar space as early as 1940s. Complex plasma has attracted much attention to the community of plasma physics [1][2][3][4], while recent advances in ultracold plasma [5][6][7][8][9] and cryogenic dusty plasma [10][11][12][13][14][15][16][17] challenge the basic understanding of plasmas. The Debye length, characterized by temperatures of electrons and ions, in a cryogenic plasma becomes much smaller than that in a conventional laboratory plasma and becomes comparable to the size of a dust particle.…”
Section: Introductionmentioning
confidence: 99%
“…A neutral shadowing force (1) acts as an additional repulsion force and with Coulomb's force adds up to a greater net repulsion force causing a less dense system which was observed by Ishihara and his co-workers. 1) At the parameters of plasma in Refs. 2, 3 the strength of a neutral shadowing force is much less than that of Coulomb's force and shows no impact.…”
Section: Introductionmentioning
confidence: 99%
“…6,7) In this work we focus on the mean square displacement of dust particles (MSD), which characterizes the diffusion of particles. The MSD is calculated by performing a Langevin dynamics simulation taking into account the screened Coulomb interaction and neutral shadowing force (1).…”
Section: Introductionmentioning
confidence: 99%
“…A dusty plasma, being experimentally relatively easy realizable and observable, attracts interest as a system for investigation of many‐particle physics; e.g., waves and wakefield . Dusty plasma experiments were carried out under various conditions, including both terrestrial and space (microgravity) as well as cryogenic . It was found that in complex plasmas, interaction between particles deviates from the screened Coulomb potential due to a non‐equilibrium state of a plasma .…”
Section: Introductionmentioning
confidence: 99%