Charged anisotropic models via embedding

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dc.contributor.authorMathias, Alberto K.
dc.contributor.authorMaharaj, Sunil D.
dc.contributor.authorSunzu, Jefta M.
dc.contributor.authorMkenyeleye, Jason M.
dc.date.accessioned2022-11-30T07:17:42Z
dc.date.available2022-11-30T07:17:42Z
dc.date.issued2021
dc.descriptionAbstract. Full Text Article Available at: https://link.springer.com/article/10.1007/s12043-021-02207-9en_US
dc.description.abstractWe generate exact solutions to the Einstein–Maxwell field equations by analysing the embedding condition. We obtain a relationship between gravitational potentials that helps to solve the embedding condition and integrate the field equations. Our choice of the measure of anisotropy and electric field are physically realistic. Our model contains several previously known solutions as special cases. These include the investigations of interior Schwarzchild metric, Finch and Skea, Hansraj and Maharaj, Feroze and Siddiqui, and Manjonjo, Maharaj and Moopanar. We also describe the structure and properties of the relativistic star by including graphical representations. Our analysis shows that the body is stable, all energy conditions are satisfied, the regularity condition is not violated, forces under equilibrium condition are balanced, all matter variables are well behaved and the matching conditions are satisfied at the boundary of the relativistic star.en_US
dc.identifier.citationMathias, A. K., Maharaj, S. D., Sunzu, J. M., & Mkenyeleye, J. M. (2021). Charged anisotropic models via embedding. Pramana, 95(4), 1-13.en_US
dc.identifier.otherURL: https://link.springer.com/article/10.1007/s12043-021-02207-9
dc.identifier.urihttp://hdl.handle.net/20.500.12661/3570
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectEinstein–Maxwellen_US
dc.subjectEinstein–Maxwell fielden_US
dc.subjectField equationsen_US
dc.subjectAnisotropic modelsen_US
dc.subjectEmbedding conditionen_US
dc.subjectElectric fielden_US
dc.titleCharged anisotropic models via embeddingen_US
dc.typeArticleen_US
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