Nonsteady dust charge variation induced ion acoustic monotonic shock structure in dusty plasma: Roles of ionization, ion loss, and collision
- 1. Centre for Plasma Studies, Faculty of Science, Jadavpur University, Kolkata 700 032 (India)
- 2. Department of Instrumentation Science, Jadavpur University, Kolkata-700 032 (India)
- 3. Government College of Engineering and Textile Technology, 4, Cantonment Road, Berhampore, Murshidabad 742101, West Bengal (India)
Description
The effects of nonsteady dust charge variation, ionization, ion loss, and collision on finite amplitude nonlinear ion acoustic wave are investigated in a complex (dusty) plasma. The dynamics of the nonlinear wave is governed by a Burger equation with linear damping or growth term. The anomalous dissipation originating from the nonsteady dust charge variation is responsible for the Burger term, whereas the other dissipative mechanisms (ionization, ion loss, and collision) are responsible for the linear damping (collision and ion loss are the dominant) or growth term (ionization is the dominant). Analytical approximate time evolution solution reveals that the wave possesses monotonic shock structure with exponentially growing or decaying wave amplitude. Its implications in gas discharge laboratory plasma are discussed
Additional details
Identifiers
- DOI
- 10.1063/1.2363171;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 13
- Journal Issue
- 10
- Journal Page Range
- p. 102312-102312.6
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38023265
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- AMPLITUDES; DAMPING; DUSTS; ELECTRON COLLISIONS; ION ACOUSTIC WAVES; ION COLLISIONS; IONIZATION; IONS; MATHEMATICAL SOLUTIONS; NONLINEAR PROBLEMS; PLASMA; SHOCK WAVES; VARIATIONS
- Descriptors DEC
- CHARGED PARTICLES; COLLISIONS; ION WAVES; PLASMA WAVES
Optional Information
- Notes
- (c) 2006 American Institute of Physics