Some simple models for quark stars

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dc.creatorMaharaj, S. D.
dc.creatorSunzu, J. M.
dc.creatorRay, S.
dc.date2020-03-20T06:03:02Z
dc.date2020-03-20T06:03:02Z
dc.date2014
dc.date.accessioned2022-10-20T13:25:31Z
dc.date.available2022-10-20T13:25:31Z
dc.descriptionFull Text Article. Also available at: https://arxiv.org/abs/1412.8139
dc.descriptionWe find two new classes of exact solutions for the Einstein-Maxwell equations. The solutions are obtained by considering charged anisotropic matter with a linear equation of state consistent with quark stars. The field equations are integrated by specifying forms for the measure of anisotropy and a gravitational potential which are physically reasonable. The solutions found generalize the Mark-Harko model and the Komathiraj-Maharaj model. A graphical analysis indicates that the matter variables are well behaved.
dc.identifierMaharaj, S. D., Sunzu, J. M., & Ray, S. (2014). Some simple models for quark stars. The European Physical Journal Plus, 129 (1), 3.
dc.identifierhttps://arxiv.org/abs/1412.8139
dc.identifierhttp://hdl.handle.net/20.500.12661/2232
dc.identifier.urihttp://hdl.handle.net/20.500.12661/2232
dc.languageen
dc.publisherSpringer
dc.subjectEinstein-Maxwell equations
dc.subjectQuarks stars
dc.subjectRelativistic astrophysics
dc.subjectAnisotropy
dc.subjectCharged anisotropic matter
dc.subjectEinstein model
dc.subjectEinstein-Maxwell system
dc.subjectAnisotropic matter
dc.subjectStellar interior model
dc.subjectKomathiraj-Maharaj model
dc.titleSome simple models for quark stars
dc.typeArticle

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