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Oblique Propagation of Electrostatic Waves in a Magnetized Electron-Positron-Ion Plasma in the Presence of Heavy Particles

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dc.contributor.author Sarker, M.
dc.contributor.author Hossen, M. R.
dc.contributor.author Shah, M. G.
dc.contributor.author Hosen, B.
dc.contributor.author Mamun, A. A.
dc.date.accessioned 2018-09-05T06:12:15Z
dc.date.accessioned 2019-05-27T09:57:04Z
dc.date.available 2018-09-05T06:12:15Z
dc.date.available 2019-05-27T09:57:04Z
dc.date.issued 2018-04-06
dc.identifier.uri http://hdl.handle.net/20.500.11948/3064
dc.description.abstract A theoretical investigation is carried out to understand the basic features of nonlinear propagation of heavy ion-acoustic (HIA) waves subjected to an external magnetic field in an electron-positron-ion plasma that consists of cold magnetized positively charged heavy ion fluids and superthermal distributed electrons and positrons. In the nonlinear regime, the Korteweg-de Vries (K-dV) and modified K-dV (mK-dV) equations describing the propagation of HIA waves are derived. The latter admits a solitary wave solution with both positive and negative potentials (for K-dV equation) and only positive potential (for mK-dV equation) in the weak amplitude limit. It is observed that the effects of external magnetic field (obliqueness), superthermal electrons and positrons, different plasma species concentration, heavy ion dynamics, and temperature ratio significantly modify the basic features of HIA solitary waves. The application of the results in a magnetized EPI plasma, which occurs in many astrophysical objects (e.g. pulsars, cluster explosions, and active galactic nuclei) is briefly discussed. Full Text Link: https://doi.org/10.1515/zna-2017-0419 en_US
dc.language.iso en en_US
dc.publisher De Gruyter en_US
dc.subject HIA SWs en_US
dc.subject Obliquity on Magnetized Plasmas en_US
dc.subject Superthermality Effect en_US
dc.title Oblique Propagation of Electrostatic Waves in a Magnetized Electron-Positron-Ion Plasma in the Presence of Heavy Particles en_US
dc.type Article en_US


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