2013
DOI: 10.1088/0256-307x/30/11/115201
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Cluster Rotation in an Unmagnetized Dusty Plasma

Abstract: Rotation of dust clusters in an unmagnetized dusty plasma under different gas pressures is experimentally studied. Clusters containing different numbers of charged dust grains are found in different horizontal planes. The mechanism behind the dust rotation is investigated by using molecular dynamics simulations. The experimental and simulation results show that the radial confinement potential plays an important role in determining the properties of the cluster rotation under given gas pressure or temperature.

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Cited by 12 publications
(5 citation statements)
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“…We are interested in long and narrow two-row crystals because they are suitable for FELs. [25] Narrow two-row crystals have strong transverse electric field that is essential for an electrostatic wiggler in FEL. On the other side, narrowing is equivalent to a small quantity of b, and small b leads to crystals with only one row.…”
Section: Crystals With Arbitrary Shapementioning
confidence: 99%
See 1 more Smart Citation
“…We are interested in long and narrow two-row crystals because they are suitable for FELs. [25] Narrow two-row crystals have strong transverse electric field that is essential for an electrostatic wiggler in FEL. On the other side, narrowing is equivalent to a small quantity of b, and small b leads to crystals with only one row.…”
Section: Crystals With Arbitrary Shapementioning
confidence: 99%
“…We restrict this study to the 2D case and assume that grain levitation occurs at a definite height above the lower electrode in the plasma sheath due to the balance between grain weight and sheath field. [25][26][27] In the horizontal direction, there are two forces: screened Coulomb force and confinement force. The first force is formulated in the next section and rigid walls are used as the second confinement force.…”
Section: Introductionmentioning
confidence: 99%
“…The two-dimensional zigzag transitions have been studied in dusty plasmas confined by a biharmonic potential well created by a rectangular depression between four conducting bars placed on the RF powered electrode [32]. It has been shown that the properties of dust cluster rotation in a non-magnetized dusty plasma is highly dependent on the characteristics of the parabolic radial confinement potential [33,34].…”
Section: Introductionmentioning
confidence: 99%
“…[6][7][8][9][10][11][12] As dust is a common species in a wide range of space and astrophysical plasmas, such as the cometary tails, interstellar clouds, Earth mesosphere and ionosphere, Saturn's rings, the gossamer ring of Jupiter, and in laboratory experiments, [5,[13][14][15] the study of dust-plasma interaction has become a hub of interest for recent research in plasma physics. [16,17] The propagation of a solitary wave is important as it describes the characteristic nature of the interaction of the wave with the plasma constituents. However, once the ion velocity approaches to the velocity of light, the amplitude, width, and energy of the wave will each experience a drastic modification as the relativistic effect becomes dominant.…”
Section: Introductionmentioning
confidence: 99%