Modulational instabilities in two-dimensional magnetized dust-lattice
Creators
- 1. Department of Physics, Faculty of Science, Arak-University, 38156-8-8349 Arak (Iran, Islamic Republic of)
Description
The transverse oscillations of paramagnetic dust grains in hexagonal dusty plasma crystal are discussed. The nonlinearity, which is related to the sheath electric/magnetic field(s) and to the weak inter grain interactions (magnetic dipole), is shown to lead to the generation of phase harmonics. In the case of propagating two-dimensional transverse dust-lattice modes in an arbitrary direction, it is shown the modulational instability of the carrier wave is due to self-interaction. The stability depends on the form of the electric field, the magnetic field, and the magnetic permeability of dust particles. The long term evolution of the modulated wave packet is described by a discrete nonlinear Schrodinger equation and it is solved numerically by Adomian decomposition method.
Additional details
Identifiers
- DOI
- 10.1063/1.3663842;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 11
- Journal Page Range
- p. 113705-113705.6
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44006567
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- DUSTS; ELECTRIC FIELDS; HARMONICS; MAGNETIC DIPOLES; MAGNETIC FIELDS; MAGNETIC MOMENTS; MAGNETIC SUSCEPTIBILITY; MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; PARAMAGNETISM; PLASMA; PLASMA INSTABILITY; PLASMA SHEATH; PLASMA WAVES; SCHROEDINGER EQUATION; TWO-DIMENSIONAL CALCULATIONS; WAVE PACKETS
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; DIPOLES; EQUATIONS; FLUID MECHANICS; HYDRODYNAMICS; INSTABILITY; MAGNETIC PROPERTIES; MAGNETISM; MECHANICS; MULTIPOLES; OSCILLATIONS; PARTIAL DIFFERENTIAL EQUATIONS; PHYSICAL PROPERTIES; WAVE EQUATIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics