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Applicant:
Central University of Tamil Nadu 
Author:
L.Kavitha, C.Lavanya, V.Senthil Kumar, D.Gopi and A.Pasqua 
Corresponding Authors:
L. Kavitha 
DOI #:
doi.org/10.1063/1.4945609 
Title:
Perturbed soliton excitations of Rao dust Alfven waves in magnetized dusty plasmas 
Journal:
Physics of Plasma 
Year:
2016 
Volume:
23 
Page:
043702 
Keywords:
Solitons; propagation dynamics; perturbation method 
Abstract:
We investigate the propagation dynamics of the perturbed soliton excitations in a three component fully ionized dusty magnetoplasma consisting of electrons, ions, and heavy charged dust particulates. We derive the governing equation of motion for the two dimensional Rao-dust magnetohydrodynamic (R-D-MHD) wave by employing the inertialess electron equation of motion, inertial ion equation of motion, the continuity equations in a plasma with immobile charged dust grains, together with the Maxwell's equations, by assuming quasi neutrality and neglecting the displacement current in Ampere's law. Furthermore, we assume the massive dust particles are practically immobile since we are interested in timescales much shorter than the dusty plasma period, thereby neglecting any damping of the modes due to the grain charge fluctuations. We invoke the reductive perturbation method to represent the governing dynamics by a perturbed cubic nonlinear Schrödinger (pCNLS) equation. We solve the pCNLS, along the lines of Kodama-Ablowitz multiple scale nonlinear perturbation technique and explored the R-D-MHD waves as solitary wave excitations in a magnetized dusty plasma. Since Alfvén waves play an important role in energy transport in driving field-aligned currents, particle acceleration and heating, solar flares, and the solar wind, this representation of R-D-MHD waves as soliton excitations may have extensive applications to study the lower part of the earth's ionosphere. 
Entered by:
Kavitha Louis on 2020-09-03 
 
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