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Realistic relativistic stellar anisotropic models with equation of state

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dc.creator Thomas, Mashiku
dc.date 2018-10-15T16:54:47Z
dc.date 2018-10-15T16:54:47Z
dc.date 2017
dc.date.accessioned 2021-05-06T12:58:58Z
dc.date.available 2021-05-06T12:58:58Z
dc.identifier Thomas, M. (2017). Realistic relativistic stellar anisotropic models with equation of state, Dodoma: The University of Dodoma
dc.identifier http://hdl.handle.net/20.500.12661/504
dc.identifier.uri http://hdl.handle.net/20.500.12661/504
dc.description Dissertation (MSc Mathematics)
dc.description We obtain new exact solutions to the Einstein field equations for anisotropic neutral stellar objects. In our dissertation, we are considering a quadratic equation of state and a choice of measure of anisotropy and metric function adopted from Sunzu’s work. We transform the Einstein field equations for neutral anisotropic matter by adopting the Durgapal and Bannerji’s new variables. We generate the exact solution and hence obtain the gravitational potentials and matter variables from the general differential equation of the model. In our models, we regain the previous anisotropic and isotropic results generated by Sunzu as a special case. It is interesting that our results agree with Minkowski spacetime and earlier Einstein model. The physical analysis of the plots reveals that gravitational potentials and matter variables are well behaved in the interior of the stellar objects. In our model, we generate finite masses which are consistent with astronomical objects found by other researchers.
dc.language en
dc.publisher The University of Dodoma
dc.subject Anisotropic
dc.subject Einstein field
dc.subject Durgapal
dc.subject Bannerji’s variables
dc.subject Isotropic
dc.subject Sunzu
dc.subject Finite masses
dc.subject Minkowski spacetime
dc.subject Anisotropy
dc.subject Stellar anisotropic models
dc.subject Stellar objects
dc.title Realistic relativistic stellar anisotropic models with equation of state
dc.type Dissertation


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