Published March 2004 | Version v1
Journal article

Dust acoustic solitary waves and double layers in a dusty plasma with two-temperature trapped ions

  • 1. Physics Department, Faculty of Science-Damietta, Mansoura University, Damietta El-Gedida, P.O. 34517 (Egypt)

Description

The combined effects of trapped ion distribution, two-ion-temperature, dust charge fluctuation, and dust fluid temperature are incorporated in the study of nonlinear dust acoustic waves in an unmagnetized dusty plasma. It is found that, owing to the departure from the Boltzmann ion distribution to the trapped ion distribution, the dynamics of small but finite amplitude dust acoustic waves is governed by a modified Korteweg-de Vries equation. The latter admits a stationary dust acoustic solitary wave solution, which has stronger nonlinearity, smaller amplitude, wider width, and higher propagation velocity than that involving adiabatic ions. The effect of two-ion-temperature is found to provide the possibility for the coexistence of rarefactive and compressive dust acoustic solitary structures and double layers. Although the dust fluid temperature increases the amplitude of the small but finite amplitude solitary waves, the dust charge fluctuation does the opposite effect. The present investigation should help us to understand the salient features of the nonlinear dust acoustic waves that have been observed in a recent numerical simulation study

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
11
Journal Issue
3
Journal Page Range
p. 926-933
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
35094755
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
DUSTS; ION ACOUSTIC WAVES; ION TEMPERATURE; KORTEWEG-DE VRIES EQUATION; PLASMA; PLASMA SHEATH; SOLITONS
Descriptors DEC
DIFFERENTIAL EQUATIONS; EQUATIONS; ION WAVES; PARTIAL DIFFERENTIAL EQUATIONS; PLASMA WAVES; QUASI PARTICLES

Optional Information

Notes
(c) 2004 American Institute of Physics.