Some simple models for quark stars

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dc.contributor.authorMaharaj, S. D.
dc.contributor.authorSunzu, J. M.
dc.contributor.authorRay, S.
dc.date.accessioned2020-03-20T06:03:02Z
dc.date.available2020-03-20T06:03:02Z
dc.date.issued2014
dc.descriptionFull Text Article. Also available at: https://arxiv.org/abs/1412.8139en_US
dc.description.abstractWe 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.en_US
dc.identifier.citationMaharaj, S. D., Sunzu, J. M., & Ray, S. (2014). Some simple models for quark stars. The European Physical Journal Plus, 129 (1), 3.en_US
dc.identifier.urihttps://arxiv.org/abs/1412.8139
dc.identifier.urihttp://hdl.handle.net/20.500.12661/2232
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectEinstein-Maxwell equationsen_US
dc.subjectQuarks starsen_US
dc.subjectRelativistic astrophysicsen_US
dc.subjectAnisotropyen_US
dc.subjectCharged anisotropic matteren_US
dc.subjectEinstein modelen_US
dc.subjectEinstein-Maxwell systemen_US
dc.subjectAnisotropic matteren_US
dc.subjectStellar interior modelen_US
dc.subjectKomathiraj-Maharaj modelen_US
dc.titleSome simple models for quark starsen_US
dc.typeArticleen_US
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