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Relativistic compact anisotropic charged stellar models with Chaplygin equation of state

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dc.contributor.authorBhar, Piyali
dc.contributor.authorMurad, Mohammad Hassan
dc.contributor.departmentDepartment of Mathematics and Natural Sciences
dc.date.accessioned2016-11-09T10:16:35Z
dc.date.available2016-11-09T10:16:35Z
dc.date.copyright2016
dc.date.issued2016
dc.descriptionThis article was published in the Astrophys Space Sci [© Springer Science+Business Media Dordrecht 2016] and the definite version is available at : http://10.1007/s10509-016-2923-9 The Journal's website is at: http://link.springer.com/article/10.1007/s10509-016-2923-9en_US
dc.description.abstractThis paper presents a new model of static spherically symmetric relativistic charged stellar objects with locally anisotropic matter distribution together with the Chaplygin equation of state. The interior spacetime has been matched continuously to the exterior Reissner–Nordström geometry. Different physical properties of the stellar model have been investigated, analyzed, and presented graphically.en_US
dc.description.versionPublished
dc.format.extent10 pages
dc.identifier.citationBhar, P., & Murad, M. H. (2016). Relativistic compact anisotropic charged stellar models with Chaplygin equation of state. Astrophysics and Space Science, 361, 334. doi:10.1007/s10509-016-2923-9en_US
dc.identifier.doi10.1007/s10509-016-2923-9
dc.identifier.urihttp://hdl.handle.net/10361/6805
dc.language.isoenen_US
dc.publisher© Springer Science+Business Media Dordrecht 2016en_US
dc.relation.urihttp://link.springer.com/article/10.1007/s10509-016-2923-9
dc.subjectGeneral relativityen_US
dc.subjectRelativistic astrophysicsen_US
dc.subjectExact solutionen_US
dc.subjectAnisotropic fluid sphereen_US
dc.subjectCharged fluid sphereen_US
dc.subjectCompact starsen_US
dc.subjectRelativistic starsen_US
dc.subjectEquation of stateen_US
dc.titleRelativistic compact anisotropic charged stellar models with Chaplygin equation of stateen_US
dc.typeArticleen_US

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