Modeling an isotropic charged relativistic matter with linear equation of state.

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dc.contributor.authorDanford, Petro
dc.date.accessioned2019-08-19T08:15:59Z
dc.date.available2019-08-19T08:15:59Z
dc.date.issued2016
dc.descriptionDissertation (MSc Mathematics)en_US
dc.description.abstractWe find new exact solutions to Einstein-Maxwell field equation for charged anisotropy stellar bodies. We are considering the stellar object that is anisotropic and charged with linear equation of state consistent with quark stars. We have new choice of measure of anisotropy and adopted Sunzu’s metric function. The solutions are obtained after considering the transformed Einstein-Maxwell field equations for charged anisotropic matter. In our models we regain previous anisotropic and isotropic results as a special case. Exact solutions regained in our models are those by Sunzu, Maharaj and Ray and those by Komathiraj and Maharaj. We have considered the space time geometry to be static spherically symmetry. The exact solutions to the Einstein-Maxwell field equations corresponding to our models are found explicitly in terms of elementary functions namely simple algebraic functions. The obtained graphical plots and physical analyses for the gravitational potentials, the matter variables and the electric field are well behaved.en_US
dc.identifier.citationDanford, P. (2016). Modeling anisotropic charged relativistic matter with linear equation of state. Dodoma: The University of Dodoma.en_US
dc.identifier.urihttp://hdl.handle.net/20.500.12661/869
dc.publisherThe University of Dodomaen_US
dc.subjectLinear equationen_US
dc.subjectModeling anisotropic charged equationen_US
dc.subjectModeling linear equationen_US
dc.subjectCharged anisotropy stellar bodiesen_US
dc.subjectAnisotropic linear equationen_US
dc.subjectCharged matteren_US
dc.subjectStellar objecten_US
dc.subjectEinstein-Maxwell field equationsen_US
dc.titleModeling an isotropic charged relativistic matter with linear equation of state.en_US
dc.typeDissertationen_US
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