Effects of Electromagnetic Field on the Structure of Massive Compact Objects

Abstract

This paper encompasses a set of stellar equations that administer the formation and evolution of self-gravitating, dissipative spherically symmetric fluid distributions having anisotropic stresses in the presence of electromagnetic field. The Riemann tensor is split orthogonally to procure five scalar functions named as structure scalars which are then utilized in the stellar equations. It is shown that some basic fluid properties such as energy density inhomogeneity, pressure anisotropy and heat flux are interlinked with the obtained scalars. Further, it is shown that all the solutions to Einstein equations can be written in terms of these five scalars keeping in view the static case.

24 pages

References in corpus (4)

• Electrically Charged Strange Quark Stars
• Construction of Charged Cylindrical Gravastar-like Structures
• On the Role of $f(G,T)$ Terms in Structure Scalars
• Shear-free axially symmetric dissipative fluids

Cited by in corpus (6)

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• Role of Structure Scalars on the evolution of Compact Objects in Palatini $f(R)$ Gravity
• Influence of $f(\mathcal{R},\mathcal{T},\mathcal{Q})$ Gravity on Cylindrical Collapse
• Influence of Electromagnetic Field on Hyperbolically Symmetric Source
• Thermoelectric Conduction in General Relativity: A Causal, Stable, and Well Posed Theory