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Charged anisotropic models in finch-skea spacetime / Rabia Naeem

By: Material type: TextTextPublication details: Lahore : Division of Science & Technology, University of Education, 2018Description: 71 p. CDISBN:
  • hbk
Subject(s): DDC classification:
  • 511.5 C377
Summary: 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.
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Theses Theses UE-Central Library 511.5 C377 (Browse shelf(Opens below)) Not for loan TTH114

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.

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