Charged anisotropic models in finch-skea spacetime
Rabia Naeem MS Mathmatics, 2014-2018, Supervised by Dr. Muhammad Azam
Charged anisotropic models in finch-skea spacetime / Rabia Naeem - Lahore : Division of Science & Technology, University of Education, 2018 - 71 p. CD
In this thesis, some models of exact solutions have been explored for the static,
spherically symmetric relativistic compact object with charged anisotropic fluid which
admits the generalized polytropic equation of state (GPEoS). The system of EinsteinMaxwell equations have solved under the well-known transformation of metric functions presented by Durgapal and Bannerji (1983). The Finch-Skea spacetime geometry has been considered which is physically acceptable. The models obtained for
the certain values of polytropic index. For the specific values of parameter, we have
demonstrated the graphical behavior of mass, matter density, tangential pressure,
radial pressure, anisotropy and speed of sound. Graphical analysis revealed that all
required physical attributes are accomplished by our uncharged astrophysical models.
hbk
Mathmatics--Charged Anisotropic Models--Finch-SKEA--Spacetime
511.5 / C377
Charged anisotropic models in finch-skea spacetime / Rabia Naeem - Lahore : Division of Science & Technology, University of Education, 2018 - 71 p. CD
In this thesis, some models of exact solutions have been explored for the static,
spherically symmetric relativistic compact object with charged anisotropic fluid which
admits the generalized polytropic equation of state (GPEoS). The system of EinsteinMaxwell equations have solved under the well-known transformation of metric functions presented by Durgapal and Bannerji (1983). The Finch-Skea spacetime geometry has been considered which is physically acceptable. The models obtained for
the certain values of polytropic index. For the specific values of parameter, we have
demonstrated the graphical behavior of mass, matter density, tangential pressure,
radial pressure, anisotropy and speed of sound. Graphical analysis revealed that all
required physical attributes are accomplished by our uncharged astrophysical models.
hbk
Mathmatics--Charged Anisotropic Models--Finch-SKEA--Spacetime
511.5 / C377
