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dc.contributor.authorMurad, Mohammad Hassan
dc.contributor.authorFatema, Saba
dc.date.accessioned2018-10-16T06:21:26Z
dc.date.available2018-10-16T06:21:26Z
dc.date.issued2013-12-06
dc.identifier.urihttp://hdl.handle.net/20.500.11948/3397
dc.description.abstractIn this work a new family of relativistic models of electrically charged compact star has been obtained by solving Einstein–Maxwell field equations with preferred form of one of the metric potentials and a suitable form of electric charge distribution function. The resulting equation of state (EOS) has been calculated. The relativistic stellar structure for matter distribution obtained in this work may reasonably models an electrically charged compact star whose energy density associated with the electric fields is on the same order of magnitude as the energy density of fluid matter itself (e.g. electrically charged bare strange stars). Based on the analytic model developed in the present work, the values of the relevant physical quantities have been calculated by assuming the estimated masses and radii of some well known strange star candidates like X-ray pulsar Her X-1, millisecond X-ray pulsar SAX J 1808.4-3658, and 4U 1820-30. Full Text Link: https://doi.org/10.1007/s10509-013-1722-9en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectGeneral relativityen_US
dc.subjectEinstein–Maxwellen_US
dc.subjectReissner–Nordströmen_US
dc.subjectRelativistic Astrophysicsen_US
dc.subjectSchwarzschild coordinatesen_US
dc.subjectCharged fluid sphereen_US
dc.subjectCompact staren_US
dc.subjectRelativistic staren_US
dc.subjectEquation of stateen_US
dc.titleSome static relativistic compact charged fluid spheres in general relativityen_US
dc.typeArticleen_US


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