The stability of a shearing viscous star with an electromagnetic field

dc.contributor.author	Sharif, M.
dc.contributor.author	Azama, M.
dc.date.accessioned	2019-12-17T04:43:12Z
dc.date.available	2019-12-17T04:43:12Z
dc.date.issued	2013-01-01
dc.identifier.issn	22 050401
dc.identifier.uri	http://142.54.178.187:9060/xmlui/handle/123456789/2008
dc.description.abstract	We 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.iso	en_US	en_US
dc.publisher	Chinese Physical Society and IOP Publishing Ltd	en_US
dc.subject	Natural Science	en_US
dc.subject	shearing viscous star	en_US
dc.subject	electromagnetic field	en_US
dc.title	The stability of a shearing viscous star with an electromagnetic field	en_US
dc.type	Article	en_US