2015
DOI: 10.1007/s10509-015-2475-4
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Nonlinear dust acoustic rogue waves in a two temperature charged dusty grains plasma

Abstract: The properties of nonlinear dust-acoustic rogue 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 Schrodinger equation. The dependence of the rogue wave properties on the ion energetic population parameter is discussed. The results of the present investigation could be applicable in Saturn F-ring.

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Cited by 16 publications
(14 citation statements)
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“…The results of our present investigation will be useful in understanding the propagation of DAWs, MI of DARWs, and finally the generation of the DARWs in space plasma medium (viz. Saturn F-ring [1], circum-solar dust grains [2], and interstellar molecular clouds [3], etc.) and also laboratory DP (viz.…”
Section: Resultsmentioning
confidence: 99%
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“…The results of our present investigation will be useful in understanding the propagation of DAWs, MI of DARWs, and finally the generation of the DARWs in space plasma medium (viz. Saturn F-ring [1], circum-solar dust grains [2], and interstellar molecular clouds [3], etc.) and also laboratory DP (viz.…”
Section: Resultsmentioning
confidence: 99%
“…Now-a-days, scientist are enthralled by the natural elegance of dusty plasmas (DP) because of their existence in space (viz. Saturn F-ring [1], circum-solar dust grains [2], and interstellar molecular clouds [3], etc.) and enormous application in laboratory (viz.…”
Section: Introductionmentioning
confidence: 99%
“…To study the MI of DAWs, we will derive the NLSE by employing the standard multiple scale (reductive perturbation) technique . Let A be the state (column) vector ( n d , u d , ϕ ) T , describing the system's state at a given position x and instant t. We shall consider small deviations from the equilibrium state A (0) = (1, 0, 0) T by taking …”
Section: Derivation Of Nlsementioning
confidence: 99%
“… A=A()0+ϵA()1+ϵ2A()2+=A()0+false∑n=1ϵnA()n, where ϵ ≪ 1 is a smallness parameter. In the standard multiple scale (reductive perturbation) technique, the stretched (slow) space and time variables are commonly used by many authors as follows: ξ=ϵxvgt,τ=ϵ2t, where v g is the group velocity in the x direction. We assume that all perturbed states depend on the fast scales via the phase θ 1 = kx − ωt only, while the slow scales enter the argument of the l th harmonic amplitude Al()n, which is allowed to vary along x , A()n=false∑l=Al()nξτeilkxωitalict. …”
Section: Derivation Of Nlsementioning
confidence: 99%
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