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Electrostatic Solitary Pulses in a Dusty Electronegative Magnetoplasma

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dc.contributor.author Banik, S.
dc.contributor.author Amina, M.
dc.contributor.author Ema, S. A.
dc.contributor.author Hossen, M. R.
dc.contributor.author Mamun, A. A.
dc.date.accessioned 2019-05-09T09:34:50Z
dc.date.accessioned 2019-05-27T09:57:09Z
dc.date.available 2019-05-09T09:34:50Z
dc.date.available 2019-05-27T09:57:09Z
dc.date.issued 2018-11-22
dc.identifier.issn 1063-780X
dc.identifier.uri http://hdl.handle.net/20.500.11948/3539
dc.description.abstract The nonlinear characteristics of dust-electron-acoustic (DEA) waves in a dusty electronegative magneto plasma system consisting of nonextensive hot electrons, inertial cold electrons, positively charged static ions, and negatively charged immobile dust grains has been investigated. In this observation, the well-known reductive perturbation technique is employed to determine different types of nonlinear dynamical equations, namely, magnetized Korteweg–de Vries (KdV), magnetized modified KdV (mKdV), and magnetized Gardner equations. The stationary solitary wave and double layer solution of these three equations, which describe the characteristics of solitary waves and double layers of DEA waves, are obtained and numerically analyzed. It is noticed that various plasma parameters (viz., hot electron nonextensivity, positive ion-to-cold electron number density ratio, dust-to-cold electron number density ratio, etc.) significantly affect the basic properties of DEA solitary waves (DEASWs) and Gardner solitons (GSs). The prodigious results found from this theoretical investigation may be useful for researchers to investigate the nonlinear structures in various space and laboratory plasmas. en_US
dc.language.iso en_US en_US
dc.publisher Pleiades Publishing en_US
dc.subject Electrostatic en_US
dc.subject Electronegative en_US
dc.subject Magnetoplasma en_US
dc.subject Solitary Pulses en_US
dc.title Electrostatic Solitary Pulses in a Dusty Electronegative Magnetoplasma en_US
dc.type Article en_US


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