Kinetic instability of the dust acoustic mode in inhomogeneous, partially magnetized plasma with both positively and negatively charged grains
Creators
- 1. Centre for Plasma Astrophysics, Celestijnenlaan 200B, 3001 Leuven (Belgium) and Leuven Mathematical Modeling and Computational Science Research Centre (LMCC), Celestijnenlaan 200B, 3001 Leuven (Belgium)
Description
A purely kinetic instability of the dust acoustic mode in inhomogeneous plasmas is discussed. In the presence of a magnetic field, electrons and ions may be magnetized while at the same time dust grains may remain unmagnetized. Although the dynamics of the light species is strongly affected by the magnetic field, the dust acoustic mode may still propagate in practically any direction. The inhomogeneity implies a source of free energy for an instability that develops through the diamagnetic drift effects of the magnetized species. It is shown that this may be a powerful mechanism for the excitation of dust acoustic waves. The analysis presented in the work is also directly applicable to plasmas containing both positive and negative ions and electrons, provided that at least one of the two ion species is unmagnetized.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics (Print)
- Journal Volume
- 82
- Journal Issue
- 2
- Journal Page Range
- p. 026411-026411.5
- ISSN
- 1539-3755
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42058325
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ANIONS; DUSTS; ELECTRONS; EXCITATION; FREE ENERGY; INHOMOGENEOUS PLASMA; MAGNETIC FIELDS; PLASMA DIAMAGNETISM; PLASMA DRIFT; PLASMA INSTABILITY; PLASMA WAVES; SOUND WAVES
- Descriptors DEC
- CHARGED PARTICLES; DIAMAGNETISM; ELEMENTARY PARTICLES; ENERGY; ENERGY-LEVEL TRANSITIONS; FERMIONS; INSTABILITY; IONS; LEPTONS; MAGNETISM; PHYSICAL PROPERTIES; PLASMA; THERMODYNAMIC PROPERTIES
Optional Information
- Notes
- (c) 2010 The American Physical Society