Some analytical models of anisotropic strange stars

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dc.contributor.authorMurad, Mohammad Hassan
dc.date.accessioned2016-11-09T09:21:14Z
dc.date.available2016-11-09T09:21:14Z
dc.date.issued2016
dc.descriptionThis article was published in the Astrophysics and Space Science [© Springer Science+Business Media Dordrecht 2015] and the definite version is available at : http://10.1007/s10509-015-2582-2 The Journal's website is at: http://link.springer.com/article/10.1007/s10509-015-2582-2
dc.description.abstractOver the years of the concept of local isotropy has become a too stringent condition in modeling relativistic self-gravitating objects. Taking local anisotropy into consideration, in this work, some analytical models of relativistic anisotropic charged strange stars have been developed. The Einstein–Maxwell gravitational field equations have been solved with a particular form of one of the metric potentials. The radial pressure and the energy density have been assumed to follow the usual linear equation of state of strange quark matter, the MIT bag model.
dc.identifier.citationMurad, Mohammad Hassan. (2016). Some analytical models of anisotropic strange stars. Astrophysics and Space Science, 361(01), 20. doi:10.1007/s10509-015-2582-2
dc.identifier.otherhttps://dspace.bracu.ac.bd/server/api/core/items/8e589644-2e4e-428f-8736-3a5a4fd80a71
dc.identifier.urihttp://hdl.handle.net/10361/6804
dc.language.isoen
dc.publisher© Springer Science+Business Media Dordrecht 2015
dc.sourceBRAC University Institutional Repository
dc.subjectGeneral relativity
dc.subjectEinstein–Maxwell
dc.subjectExact solution
dc.subjectReissner–Nordström
dc.subjectSchwarzschild
dc.subjectCoordinates
dc.subjectCharged fluid sphere
dc.subjectPerfect fluid sphere
dc.subjectAnisotropic fluid sphere
dc.subjectCompact star
dc.subjectStrange star
dc.subjectRelativistic star
dc.subjectEquation of state
dc.titleSome analytical models of anisotropic strange stars
dc.typeArticle

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