Published November 2011
| Version v1
Journal article
Arbitrary amplitude ion-acoustic waves in a multicomponent plasma with superthermal species
Creators
- 1. Department of Physics, Faculty of Science, Port Said University, Port Said 42521 (Egypt)
- 2. International Center for Advanced Studies in Physical Sciences, Faculty of Physics and Astronomy, Ruhr University Bochum, D-44780 Bochum (Germany)
Description
Properties of fully nonlinear ion-acoustic waves in a multicomponent plasma consisting of warm positive ions, superthermal electrons, as well as positrons, and dust impurities have been investigated. By using the hydrodynamic model for ions and superthermal electron/positron distribution, a Sagdeev potential has been derived. Existence conditions for large amplitude solitary and shock waves are presented. In order to show that the characteristics of the solitary and shock waves are influenced by the plasma parameters, the relevant numerical analysis of the Sagdeev potential is presented. The nonlinear structures, as predicted here, may be associated with the electrostatic perturbations in interstellar medium.
Additional details
Identifiers
- DOI
- 10.1063/1.3656979;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 11
- Journal Page Range
- p. 112105-112105.8
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44006516
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AMPLITUDES; CATIONS; DISTURBANCES; DUSTS; ELECTRONS; INTERSTELLAR SPACE; ION ACOUSTIC WAVES; NONLINEAR PROBLEMS; NUMERICAL ANALYSIS; PLASMA; PLASMA IMPURITIES; POSITRONS; POTENTIALS; SHOCK WAVES; SOLITONS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; CHARGED PARTICLES; ELEMENTARY PARTICLES; FERMIONS; IMPURITIES; ION WAVES; IONS; LEPTONS; MATHEMATICS; MATTER; PLASMA WAVES; QUASI PARTICLES; SPACE
Optional Information
- Notes
- (c) 2011 American Institute of Physics