Electromagnetic Fields of Slowly Rotating Magnetized Gravastars
General Relativity and Quantum Cosmology
2010-04-20 v1 Solar and Stellar Astrophysics
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.
Cite
@article{arxiv.0902.0217,
title = {Electromagnetic Fields of Slowly Rotating Magnetized Gravastars},
author = {B. V. Turimov and B. J. Ahmedov and A. A. Abdujabbarov},
journal= {arXiv preprint arXiv:0902.0217},
year = {2010}
}
Comments
5 pages, 2 figures, accepted for publication to Mod. Phys. Lett. A