Modulation Instability and Dust-Ion-Acoustic Rogue Waves in Electron-Positron-Ion-Dust Magnetized Plasmas
A realistic multicomponent collisionless complex magnetized dusty plasma system consisting of warm ions, <inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula>-distributed positrons and electrons, and immobile dust grains is considered to st...
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Published in | IEEE transactions on plasma science Vol. 48; no. 7; pp. 2591 - 2600 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
New York
IEEE
01.07.2020
The Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
Subjects | |
Online Access | Get full text |
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Summary: | A realistic multicomponent collisionless complex magnetized dusty plasma system consisting of warm ions, <inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula>-distributed positrons and electrons, and immobile dust grains is considered to study the modulational instability (MI) (stable/unstable frequency regimes) of dust-ion-acoustic waves (DIAWs). By employing the reductive perturbation method, a 3-D nonlinear Schrödinger equation (NLSE), which leads to the MI of DIAWs, is derived. Furthermore, the NLSE gives a special type of 3-D rogue wave (RW) solution. It is observed that the spectral index <inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula> plays a crucial role on the behavior of DIAWs. The basic properties like amplitude and width of the first- and second-order dust-ion-acoustic RWs are affected by the key complex magneto-plasma configuration parameters, such as spectral index <inline-formula> <tex-math notation="LaTeX">\kappa </tex-math></inline-formula>, temperature ratio, number densities of magneto-plasma species, and ion cyclotron frequency <inline-formula> <tex-math notation="LaTeX">(\omega _{ci}) </tex-math></inline-formula>. The implication of our results for space and laboratory plasmas is briefly discussed. |
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ISSN: | 0093-3813 1939-9375 |
DOI: | 10.1109/TPS.2020.3002424 |