Electromagnetic Fields of Slowly Rotating Magnetized Gravastars
B.V. Turimov, B.J. Ahmedov, A.A. Abdujabbarov
TL;DR
This paper models the magnetic field of a slowly rotating gravastar with a highly magnetized shell, providing solutions to Maxwell's equations in this context.
Contribution
It presents a novel analytical approach to understanding the magnetic field configuration of gravastars, incorporating rotation and internal structure.
Findings
Derived magnetic field solutions for a rotating gravastar
Modeling of the gravastar shell as a perfect highly magnetized fluid
Analysis of dipolar magnetic field penetration in gravastars
Abstract
We study the dipolar magnetic field configuration and present solutions of Maxwell equations in the internal background spacetime of a a slowly rotating gravastar. The shell of gravastar where magnetic field penetrated is modeled as sphere consisting of perfect highly magnetized fluid with infinite conductivity. Dipolar magnetic field of the gravastar is produced by a circular current loop symmetrically placed at radius at the equatorial plane.
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