Published December 28, 2009
| Version v1
Journal article
Head-on collision of ion-acoustic solitary waves in a Thomas-Fermi plasma containing degenerate electrons and positrons
Creators
- 1. Theoretical Physics Group, Physics Department, Faculty of Science, Mansoura University, Damietta-Branch, New Damietta 34517, Damietta (Egypt)
- 2. Department of Physics, Faculty of Science-Port Said, Suez Canal University (Egypt)
- 3. Institut fuer Theoretische Physik IV, Fakultaet fuer Physik und Astronomie, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)
Description
Head-on collision between two ion acoustic solitary waves in a Thomas-Fermi plasma containing degenerate electrons and positrons is investigated using the extended Poincare-Lighthill-Kuo (PLK) method. The results show that the phase shifts due to the collision are strongly dependent on the positron-to-electron number density ratio, the electron-to-positron Fermi temperature ratio and the ion-to-electron Fermi temperature ratio. The present study might be helpful to understand the excitation of nonlinear ion-acoustic solitary waves in a degenerate plasma such as in superdense white dwarfs.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physleta.2009.10.060Additional details
Identifiers
- DOI
- 10.1016/j.physleta.2009.10.060;
- PII
- S0375-9601(09)01356-5;
Publishing Information
- Journal Title
- Physics Letters. A
- Journal Volume
- 374
- Journal Issue
- 2
- Journal Page Range
- p. 290-293
- ISSN
- 0375-9601
- CODEN
- PYLAAG
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41108058
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- COLLISIONS; ELECTRON DENSITY; ELECTRONS; EXCITATION; NONLINEAR PROBLEMS; PHASE SHIFT; PLASMA; POSITRONS; SOUND WAVES; THOMAS-FERMI MODEL; WHITE DWARF STARS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; ATOMIC MODELS; DWARF STARS; ELEMENTARY PARTICLES; ENERGY-LEVEL TRANSITIONS; FERMIONS; LEPTONS; MATHEMATICAL MODELS; MATTER; STARS
Optional Information
- Copyright
- Copyright (c) 2009 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.