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dc.contributor.authorVerheest, F.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-09-21T11:04:12Z
dc.date.accessioned2021-02-12T09:28:56Z-
dc.date.available2015-09-21T11:04:12Z
dc.date.available2021-02-12T09:28:56Z-
dc.date.issued2005
dc.identifier.citationNew Journal of Physics, v.7, 2005, doi: 10.1088/1367-2630/7/1/094en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/451-
dc.description.abstractThe equal charge-to-mass ratio for both species in pair plasmas induces a decoupling of the linear eigenmodes between waves that are charge neutral or non-neutral, also at oblique propagation with respect to a static magnetic field. While the charge-neutral linear modes have been studied in greater detail, including their weakly and strongly nonlinear counterparts, the non-neutral mode has received less attention. Here the nonlinear evolution of a solitary non-neutral mode at oblique propagation is investigated in an electron?positron plasma. Employing the framework of reductive perturbation analysis, a modified Korteweg?de Vries equation (with cubic nonlinearity) for the lowest-order wave magnetic field is obtained. In the linear approximation, the non-neutral mode has its magnetic component orthogonal to the plane spanned by the directions of wave propagation and of the static magnetic field. The linear polarization is not maintained at higher orders. The results may be relevant to the microstructure in pulsar radiation or to the subpulses.en_US
dc.language.isoenen_US
dc.subjectMagnetic fielden_US
dc.subjectNonlinear pair plasmasen_US
dc.subjectSolitary Alfven modesen_US
dc.subjectAlfven wavesen_US
dc.titleOblique non-neutral solitary Alfven modes in weakly nonlinear pair plasmasen_US
dc.typeArticleen_US
dc.identifier.accession090956
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