Quark star models with logarithmic anisotropy

dc.contributor.authorJuma, Mahamudu
dc.contributor.authorMkenyeleye, Jason M.
dc.contributor.authorSunzu, Jefta M.
dc.date.accessioned2023-05-25T07:41:05Z
dc.date.available2023-05-25T07:41:05Z
dc.date.issued2022
dc.descriptionAbstract. Full text article available at https://link.springer.com/article/10.1007/s12043-022-02338-7en_US
dc.description.abstractNew models for the charged anisotropic stellar object were generated using the Einstein–Maxwell field equations. A new choice of pressure anisotropy in logarithmic form was used to generate a quark star model. Anisotropic and isotropic models were regained as a special case. We regained anisotropic models found by Maharaj, Sunzu and Ray; Abdalla, Sunzu and Mkenyeleye; and Sunzu and Danford. The isotropic models regained include the performance by Mak and Harko, and Maharaj and Komathiraj. Physical analysis showed that matter variables and the gravitational potentials are well behaved. Our model does satisfy the energy conditions and stability condition.en_US
dc.identifier.citationJuma, M., Mkenyeleye, J. M., & Sunzu, J. M. (2022). Quark star models with logarithmic anisotropy. Pramana, 96(2), 88.en_US
dc.identifier.otherURL:https://link.springer.com/article/10.1007/s12043-022-02338-7
dc.identifier.urihttp://hdl.handle.net/20.500.12661/3969
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectQuark star modelsen_US
dc.subjectlogarithmic anisotropyen_US
dc.subjectAnisotropic stellar objecten_US
dc.subjectAnisotropicen_US
dc.subjectIsotropic modelsen_US
dc.titleQuark star models with logarithmic anisotropyen_US
dc.typeArticleen_US
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