Local, Non-Geodesic, Timelike Currents in the Force-Free Magnetosphere of a Kerr Black Hole

Abstract

In this paper, we use previously developed exact solutions to present some of the curious features of a force-free magnetosphere in a Kerr background. More precisely, we obtain a hitherto unseen timelike current in the force-free magnetosphere that does not flow along a geodesic. The electromagnetic field in this case happens to be magnetically dominated. This too is a feature that has entered the literature for the first time. Changing the sign of a single parameter in our solutions generates a spacelike current that creates an electromagnetic field that is electrically dominated.

References in corpus (2)

• Electromagnetic power of merging and collapsing compact objects
• Magnetohydrodynamics in stationary and axisymmetric spacetimes: a fully covariant approach

Cited by in corpus (1)

• The Non-Null and Force-Free Electromagnetic Field