Authors: M Sharif Neelum Bashir
Publish Date: 2012/04/20
Volume: 44, Issue: 7, Pages: 1725-1737
Abstract
This paper is devoted to study the effects of electromagnetic field on the energy density inhomogeneity in the relativistic selfgravitating fluids for spherically symmetric spacetime Two important equations of the Weyl tensor are formulated which help to analyze the energy density inhomogeneity in this scenario We investigate two types of fluids ie nondissipative and dissipative The nondissipative fluid further includes dust locally isotropic and locally anisotropic charged fluids We explore the effects of different factors on energy density inhomogeneity in all these cases in particular the effect of charge
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