Quark star model with charged anisotropic matter

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dc.creatorSunzu, J. M.
dc.creatorMaharaj., S. D.
dc.creatorRay, S.
dc.date2020-03-20T06:01:21Z
dc.date2020-03-20T06:01:21Z
dc.date2014
dc.date.accessioned2022-10-20T13:25:31Z
dc.date.available2022-10-20T13:25:31Z
dc.descriptionFull Text Article. Also available at: 10.1007/s10509-014-2131-4
dc.descriptionWe find two new classes of exact solutions to the Einstein-Maxwell system of equations. The matter distribution satisfies a linear equation of state consistent with quark matter. The field equations are integrated by specifying forms for the measure of anisotropy and a gravitational potential which are physically reasonable. The first class has a constant potential and is regular in the stellar interior. It contains the familiar Einstein model as a limiting case and we can generate finite masses for the star. The second class has a variable potential and singularity at the center. A graphical analysis indicates that the matter variables are well behaved.
dc.identifierSunzu, J. M., Maharaj, S. D., & Ray, S. (2014). Quark star model with charged anisotropic matter. Astrophysics and Space Science, 354(2), 517-524.
dc.identifier10.1007/s10509-014-2131-4
dc.identifierhttp://hdl.handle.net/20.500.12661/2231
dc.identifier.urihttp://hdl.handle.net/20.500.12661/2231
dc.languageen
dc.publisherSpringer
dc.subjectGravitational potential
dc.subjectLinear equation
dc.subjectQuark matter
dc.subjectAnisotropy
dc.subjectIsotropic
dc.subjectEinstein-Maxwell equations
dc.subjectEinstein-Maxwell system
dc.subjectEinstein model
dc.titleQuark star model with charged anisotropic matter
dc.typeArticle

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