Effects of Electromagnetic Field on Energy Density Inhomogeneity in Self-Gravitating Fluids

Abstract

This paper is devoted to study the effects of electromagnetic field on the energy density inhomogeneity in the relativistic self-gravitating 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, i.e., non-dissipative and dissipative. The non-dissipative 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.

16 pages, no figure

References in corpus (6)

• Nonadiabatic charged spherical gravitational collapse
• On the Role of Electric Charge and Cosmological Constant in Structure Scalars
• Why Gravitational Contraction Must be Accompanied by Emission of Radiation Both in Newtonian and Einstein Gravity
• Charged Cylindrical Collapse of Anisotropic Fluid
• Dynamics of Non-adiabatic Charged Cylindrical Gravitational Collapse
• Dynamics of Charged Plane Symmetric Gravitational Collapse

Cited by in corpus (3)

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