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Please use this identifier to cite or link to this item: http://localhost:80/xmlui/handle/123456789/2008
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dc.contributor.authorSharif, M.-
dc.contributor.authorAzama, M.-
dc.date.accessioned2019-12-17T04:43:12Z-
dc.date.available2019-12-17T04:43:12Z-
dc.date.issued2013-01-01-
dc.identifier.issn22 050401-
dc.identifier.urihttp://142.54.178.187:9060/xmlui/handle/123456789/2008-
dc.description.abstractWe analyze the role of the electromagnetic field for the stability of a shearing viscous star with spherical symmetry. Matching conditions are given for the interior and the exterior metrics. We use a perturbation scheme to construct the collapse equation. The range of instability is explored in Newtonian and post Newtonian (pN) limits. We conclude that the electromagnetic field diminishes the effects of the shearing viscosity in the instability range and makes the system more unstable in both Newtonian and post Newtonian approximations.en_US
dc.language.isoen_USen_US
dc.publisherChinese Physical Society and IOP Publishing Ltden_US
dc.subjectNatural Scienceen_US
dc.subjectshearing viscous staren_US
dc.subjectelectromagnetic fielden_US
dc.titleThe stability of a shearing viscous star with an electromagnetic fielden_US
dc.typeArticleen_US
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