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Solitons in magnetized plasma with electron inertia under weakly relativistic effect

dc.contributor.authorKalita, J.
dc.contributor.authorDas, R.
dc.contributor.authorHosseini, K.
dc.contributor.authorBaleanu, Dumitru
dc.contributor.authorSalahshour, S.
dc.contributor.authorID56389tr_TR
dc.date.accessioned2024-01-24T11:59:00Z
dc.date.available2024-01-24T11:59:00Z
dc.date.issued2023
dc.departmentÇankaya Üniversitesi, Fen - Edebiyat Fakültesi, Matematik Bölümüen_US
dc.description.abstractIn this relativistic consideration, the energy integral unlike others has been derived in a weakly relativistic plasma in terms of Sagdeev potential. Both compressive and rarefactive subsonic solitary waves are found to exist, depending on wave speeds in various directions of propagation. It is found that compressive relativistic solitons have potential depths that are higher than non-relativistic solitons in all directions of propagation, allowing for the presence of denser plasma particles in the potential well. Furthermore, it shows how compressive soliton amplitude grows as the propagation direction gets closer to the magnetic field’s direction.en_US
dc.description.publishedMonth2
dc.identifier.citationKalita J.;...et.al. (2023). "Solitons in magnetized plasma with electron inertia under weakly relativistic effect", Nonlinear Dynamics, Vol.111, No.4, ppç3701-3711.en_US
dc.identifier.doi10.1007/s11071-022-08015-z
dc.identifier.endpage3711en_US
dc.identifier.issn0924090X
dc.identifier.issue4en_US
dc.identifier.startpage3701en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12416/6979
dc.identifier.volume111en_US
dc.language.isoenen_US
dc.relation.ispartofNonlinear Dynamicsen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectEnergy Integralen_US
dc.subjectMach Numberen_US
dc.subjectMagnetic Fielden_US
dc.subjectSagdeev Potentialen_US
dc.subjectSolitary Wavesen_US
dc.titleSolitons in magnetized plasma with electron inertia under weakly relativistic effecttr_TR
dc.titleSolitons in Magnetized Plasma With Electron Inertia Under Weakly Relativistic Effecten_US
dc.typeArticleen_US
dspace.entity.typePublication

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