Resonant flow instability of space-charge waves in self-gravitating Lorentzian dusty plasma columns

Author:

Lee Myoung-Jae12,Jung Young-Dae34

Affiliation:

1. Department of Physics, Hanyang University, Seoul 04763, South Korea.

2. Research Institute for Natural Sciences, Hanyang University, Seoul 04763, South Korea.

3. Department of Applied Physics and Department of Bionanotechnology, Hanyang University, Ansan, Kyunggi-Do 15588, South Korea.

4. Department of Electrical and Computer Engineering, MC 0407, University of California, San Diego, 9500 Gilman Drive, La Jolla, California 92093-0407, USA.

Abstract

The dispersion characteristics and the resonant instability mode of the space-charge wave are investigated in a streaming Lorentzian dusty plasma column by using the normal mode analysis. The result shows that the non-thermal character of the Lorentzian cylindrical dusty plasma enhances the unstable property of the space-charge wave due to the beam–plasma interaction. It is found that the resonant growth rates of the space-charge wave increase with an increase of the harmonic-order of the root of the Bessel function. It is also found that the influence of the self-gravitation enhances the resonant growth rate of the space-charge wave of the Lorentzian cylindrical dusty plasma. In addition, it is found the resonant growth rate decreases with an increase of the radius of the dusty plasma column. The variation of the resonant instability mode due to the non-thermal character and geometric effects is also discussed.

Publisher

Canadian Science Publishing

Subject

General Physics and Astronomy

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