Show simple item record

dc.contributor.authorMurad, Mohammad Hassan
dc.contributor.authorFatema, Saba
dc.date.accessioned2018-10-15T06:06:36Z
dc.date.available2018-10-15T06:06:36Z
dc.date.issued2012-12-18
dc.identifier.urihttp://hdl.handle.net/20.500.11948/3393
dc.description.abstractThis paper presents a family of two-parametric interior solutions of Einstein–Maxwell field equations in general relativity for a static spherically symmetric distribution of a charged perfect fluid with particular form of charge distribution. This class of solutions gives us wide range of parameters, n and K, for which the solutions are well behaved hence, suitable for modeling of compact star (e. g. bare strange quark star). The mass of star is maximized with all degree of suitability by assuming the stellar “surface” density equal to strange (quark) matter density at zero pressure. It is hoped that our investigation may be of some help in connection of some study of stellar structure. Full Text Link: https://doi.org/10.1007/s10509-012-1320-2en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectGeneral relativityen_US
dc.subjectExact solutionen_US
dc.subjectStatic spherically symmetric metricen_US
dc.subjectCharged fluid sphereen_US
dc.subjectCompact objecten_US
dc.subjectCurvature coordinatesen_US
dc.subjectReissener–Nordströmen_US
dc.titleA family of well behaved charge analogues of Durgapal’s perfect fluid exact solution in general relativity IIen_US
dc.typeArticleen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record