Electromagnetic Fields of Slowly Rotating Magnetized 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 $a$ at the equatorial plane.

5 pages, 2 figures, accepted for publication to Mod. Phys. Lett. A

References in corpus (5)

• Dynamics of dark energy
• How to tell a gravastar from a black hole
• Gravastars supported by nonlinear electrodynamics
• On the ergoregion instability in rotating gravastars
• Van der Waals quintessence stars

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