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Solitons in magnetized plasma with electron inertia under weakly relativistic effect

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dc.contributor.authorKalita, Jyotishmita
dc.contributor.authorDas, Ranjan Kumar
dc.contributor.authorHosseini, K.
dc.contributor.authorBaleanu, Dumitru I.
dc.contributor.authorSalahshour, Soheil
dc.contributor.institutionKalita, Jyotishmita, Department of Mathematics, Gauhati University, Guwahati, India
dc.contributor.institutionDas, Ranjan Kumar, Department of Mathematics, Arya Vidyapeeth College, Guwahati, India
dc.contributor.institutionHosseini, K., Department of Mathematics, Near East University TRNC, Mersin, Turkey
dc.contributor.institutionBaleanu, Dumitru I., Department of Mathematics, Çankaya Üniversitesi, Ankara, Turkey, Institute for Space Sciences, Bucharest, Bucharest, Romania, Department of Medical Research, China Medical University, Taichung, Taiwan
dc.contributor.institutionSalahshour, Soheil, Department of Mathematics, Near East University TRNC, Mersin, Turkey, Faculty of Engineering and Natural Sciences, Bahçeşehir Üniversitesi, Istanbul, Turkey
dc.date.accessioned2025-10-05T15:06:01Z
dc.date.issued2023
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. © 2023 Elsevier B.V., All rights reserved.
dc.identifier.doi10.1007/s11071-022-08015-z
dc.identifier.endpage3711
dc.identifier.issn0924090X
dc.identifier.issn1573269X
dc.identifier.issue4
dc.identifier.scopus2-s2.0-85140829653
dc.identifier.startpage3701
dc.identifier.urihttps://doi.org/10.1007/s11071-022-08015-z
dc.identifier.urihttps://hdl.handle.net/20.500.14719/8135
dc.identifier.volume111
dc.language.isoen
dc.publisherSpringer Science and Business Media B.V.
dc.relation.sourceNonlinear Dynamics
dc.subject.authorkeywordsEnergy Integral
dc.subject.authorkeywordsMach Number
dc.subject.authorkeywordsMagnetic Field
dc.subject.authorkeywordsSagdeev Potential
dc.subject.authorkeywordsSolitary Waves
dc.subject.authorkeywordsAerodynamics
dc.subject.authorkeywordsElectromagnetic Wave Propagation In Plasma
dc.subject.authorkeywordsMach Number
dc.subject.authorkeywordsMagnetic Fields
dc.subject.authorkeywordsMagnetoplasma
dc.subject.authorkeywordsElectron Inertia
dc.subject.authorkeywordsEnergy
dc.subject.authorkeywordsEnergy Integral
dc.subject.authorkeywordsMagnetic-field
dc.subject.authorkeywordsMagnetized Plasmas
dc.subject.authorkeywordsRelativistic Effects
dc.subject.authorkeywordsRelativistic Plasmas
dc.subject.authorkeywordsRelativistic Soliton
dc.subject.authorkeywordsRelativistics
dc.subject.authorkeywordsSagdeev Potential
dc.subject.authorkeywordsSolitons
dc.subject.indexkeywordsAerodynamics
dc.subject.indexkeywordsElectromagnetic wave propagation in plasma
dc.subject.indexkeywordsMach number
dc.subject.indexkeywordsMagnetic fields
dc.subject.indexkeywordsMagnetoplasma
dc.subject.indexkeywordsElectron inertia
dc.subject.indexkeywordsEnergy
dc.subject.indexkeywordsEnergy integral
dc.subject.indexkeywordsMagnetic-field
dc.subject.indexkeywordsMagnetized plasmas
dc.subject.indexkeywordsRelativistic effects
dc.subject.indexkeywordsRelativistic plasmas
dc.subject.indexkeywordsRelativistic soliton
dc.subject.indexkeywordsRelativistics
dc.subject.indexkeywordsSagdeev potential
dc.subject.indexkeywordsSolitons
dc.titleSolitons in magnetized plasma with electron inertia under weakly relativistic effect
dc.typeArticle
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dspace.entity.typePublication
local.indexed.atScopus
person.identifier.scopus-author-id57946122900
person.identifier.scopus-author-id57199967532
person.identifier.scopus-author-id36903183800
person.identifier.scopus-author-id7005872966
person.identifier.scopus-author-id23028598900

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