Nonideal dusty plasma expansion

M. Djebli; R. Annou; T. H. Zerguini

doi:10.1063/1.1699324

Nonideal dusty plasma expansion

Physics of Plasmas ◽

10.1063/1.1699324 ◽

2004 ◽

Vol 11 (5) ◽

pp. 2267-2271 ◽

Cited By ~ 4

Author(s):

M. Djebli ◽

R. Annou ◽

T. H. Zerguini

Keyword(s):

Dusty Plasma ◽

Plasma Expansion

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Dusty plasma expansion with a variable charge in a spherical configuration

Physics of Plasmas ◽

10.1063/1.1358890 ◽

2001 ◽

Vol 8 (5) ◽

pp. 1493-1496 ◽

Cited By ~ 9

Author(s):

M. Djebli ◽

R. Annou ◽

T. H. Zerguini

Keyword(s):

Dusty Plasma ◽

Plasma Expansion ◽

Variable Charge

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Charge evolution in dusty plasma expansion with negative ions

Physics of Plasmas ◽

10.1063/1.1627329 ◽

2003 ◽

Vol 10 (12) ◽

pp. 4910-4912 ◽

Cited By ~ 22

Author(s):

M. Djebli

Keyword(s):

Dusty Plasma ◽

Negative Ions ◽

Plasma Expansion

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Opposite polarity dusty plasma expansion in Earth’s mesosphere

Astrophysics and Space Science ◽

10.1007/s10509-014-2075-8 ◽

2014 ◽

Vol 353 (2) ◽

pp. 413-416 ◽

Cited By ~ 5

Author(s):

S. K. El-Labany ◽

H. N. Abd El-Razek ◽

G. A. El-Gamish

Keyword(s):

Dusty Plasma ◽

Opposite Polarity ◽

Plasma Expansion

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Self-similar expansion of adiabatic electronegative dusty plasma

Journal of Plasma Physics ◽

10.1017/s0022377817000836 ◽

2017 ◽

Vol 83 (6) ◽

Cited By ~ 1

Author(s):

M. Shahmansouri ◽

A. Bemooni ◽

A. A. Mamun

Keyword(s):

Dusty Plasma ◽

Dusty Plasmas ◽

Adiabatic Index ◽

The Self ◽

Charged Dust ◽

Plasma Expansion ◽

Plasma Parameters ◽

Dust Temperature ◽

Self Similar ◽

Expansion Of Space

The self-similar expansion of an adiabatic electronegative dusty plasma (consisting of inertialess adiabatic electrons, inertialess adiabatic ions and inertial adiabatic negatively charged dust fluids) is theoretically investigated by employing the self-similar approach. It is found that the effects of the plasma adiabaticity (represented by the adiabatic index $\unicode[STIX]{x1D6FE}$) and dusty plasma parameters (determined by dust temperature and initial dust population) significantly modify the nature of the plasma expansion. The implications of our results are expected to play an important role in understanding the physics of the expansion of space and laboratory electronegative dusty plasmas.

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