Published November 2011
| Version v1
Journal article
Acoustic double layer structures in dense magnetized electron-positron-ion plasmas
Creators
- 1. Department of Physics and Applied Mathematics, PIEAS, P. O. Nilore, Islamabad 44000 (Pakistan)
- 2. Theoretical Plasma Physics Division, PINSTECH, P. O. Nilore, Islamabad 44000 (Pakistan)
Description
The acoustic double layer structures are studied using quantum hydrodynamic model in dense magnetized electron-positron-ion plasmas. The extended Korteweg-de Vries is derived using reductive perturbation method. It is found that increase in the ion concentration in dense magnetized electron-positron plasmas increases the amplitude as well as the steepness of the double layer structure. However, increase in the magnetic field strength and decrease in the obliqueness of the nonlinear acoustic wave enhances only the steepness of the double layer structures. The numerical results have also been shown by using the data of the outer layer regions of white dwarfs given in the literature.
Additional details
Identifiers
- DOI
- 10.1063/1.3655438;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 11
- Journal Page Range
- p. 112506-112506.8
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44006536
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AMPLITUDES; ELECTRONS; HYDRODYNAMICS; ION ACOUSTIC WAVES; IONS; KORTEWEG-DE VRIES EQUATION; LAYERS; MAGNETIC FIELDS; NONLINEAR PROBLEMS; PLASMA; PLASMA SHEATH; PLASMA SIMULATION; POSITRONS; SOUND WAVES; WHITE DWARF STARS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; CHARGED PARTICLES; DIFFERENTIAL EQUATIONS; DWARF STARS; ELEMENTARY PARTICLES; EQUATIONS; FERMIONS; FLUID MECHANICS; ION WAVES; LEPTONS; MATTER; MECHANICS; PARTIAL DIFFERENTIAL EQUATIONS; PLASMA WAVES; SIMULATION; STARS
Optional Information
- Notes
- (c) 2011 American Institute of Physics