Charged anisotropic models for quark stars

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dc.creatorSunzu, J. M.
dc.creatorMaharaj, S. D.
dc.creatorRay, S.
dc.date2020-03-19T11:41:51Z
dc.date2020-03-19T11:41:51Z
dc.date2014
dc.date.accessioned2022-10-20T13:25:30Z
dc.date.available2022-10-20T13:25:30Z
dc.descriptionAbstract. Full Text Article also available at: https://link.springer.com/article/10.1007/s10509-014-1918-7
dc.descriptionWe perform a detailed physical analysis for a class of exact solutions for the Einstein-Maxwell equations. The linear equation of state consistent with quark stars has been incorporated in the model. The physical analysis of the exact solutions is performed by considering the charged anisotropic stars for the particular nonsingular exact model obtained by Maharaj, Sunzu and Ray. In performing such an analysis we regain masses obtained by previous researchers for isotropic and anisotropic matter. It is also indicated that other masses and radii may be generated which are in acceptable ranges consistent with observed values of stellar objects. A study of the mass-radius relation indicates the effect of the electromagnetic field and anisotropy on the mass of the relativistic star
dc.identifierSunzu, J. M., Maharaj, S. D., & Ray, S. (2014). Charged anisotropic models for quark stars. Astrophysics and Space Science, 352(2), 719-727.
dc.identifierhttp://hdl.handle.net/20.500.12661/2215
dc.identifier.urihttp://hdl.handle.net/20.500.12661/2215
dc.languageen
dc.publisherSpringer
dc.subjectEinstein-Maxwell equations
dc.subjectCharged anisotropic stars
dc.subjectQuark stars
dc.subjectAnisotropic matter
dc.subjectAnisotropy
dc.subjectLinear equation
dc.subjectGravitating matter
dc.subjectPressure anisotropy
dc.titleCharged anisotropic models for quark stars
dc.typeArticle

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