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

TL;DR

This paper investigates how electromagnetic fields influence energy density inhomogeneity in self-gravitating fluids within spherically symmetric spacetime, analyzing various fluid types and the role of charge.

Contribution

It formulates two key equations of the Weyl tensor to analyze energy density inhomogeneity in relativistic fluids with electromagnetic effects.

Findings

Electromagnetic fields affect energy density distribution.

Charge influences inhomogeneity in different fluid types.

Different fluid conditions alter the inhomogeneity behavior.

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.