Page 13 - swp0000.dvi
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ABSTRACT


                  The properties of nonlinear dust-acoustic waves in an unmagnetized


            collisionless four-component dusty plasma system consisting of electrons,

           nonthermal ions, hot and cold dust species have been investigated. The basic

           set of fluid equations is reduced to a nonlinear Schrödinger equation via the

           derivative expansion method. The conditions on the coefficients of dispersion

           and nonlinear terms of this equation have been checked for both stable and

           unstable regions in our plasma system. It is found that the negative sign for the


           product of the coefficients of dispersion and nonlinear terms is required for the

           modulational stability of the waves while positive sign is allowed for a random

           perturbation of the amplitude leading to growing and a very huge wave may be

           created. Accordingly, the modulational instability, modulational instability

            growth rate and rational solution for rogue waves are discussed.


                  The      dependence         of     physical      characteristics        of    modulational

           instability,modulational instability growth rate and rogue waves amplitude on

           parameters like the population of nonthermal ions, the carrier wave number,the

           equilibrium density of hot dust grains and the charge numbers for negatively

           charged hot dust is investigated. On the other hand, under a suitable coordinate


           transformation in reductive perturbation theory, a three- dimensional cylindrical

           Kadomtsev-Petviashvili (3D-CKP) equation is obtained by reducing the system

           of equations. The effect of the nonthermal parameter, the negative charge number

           of hot and cold dust on the cylindrical solitary wave properties is investigated.

           Furthermore, the solitary wave profiles in both of the radial, axial, and polar

           coordinates are examined. The present investigation may be applicable in space

           plasma such as F-ring of Saturn.

           It is also found that the parameter of the population of nonthermal

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