Force-free electrodynamics near rotation axis of a Kerr black hole
Gianluca Grignani, Troels Harmark, Marta Orselli

TL;DR
This paper investigates force-free electrodynamics near the rotation axis of Kerr black holes, revealing restrictions on solutions and providing insights into the limitations of existing models like the Blandford-Znajek monopole.
Contribution
It introduces a systematic asymptotic analysis near the rotation axis, highlighting constraints on magnetosphere solutions and challenging assumptions in prior models.
Findings
Regularity conditions restrict solutions near the axis.
Solutions cannot connect smoothly to static monopoles as rotation vanishes.
Provides evidence of issues with Blandford-Znajek monopole asymptotics.
Abstract
Despite their potential importance for understanding astrophysical jets, physically realistic exact solutions for magnetospheres around Kerr black holes have not been found, even in the force-free approximation. Instead approximate analytical solutions such as the Blandford-Znajek (split-)monopole, as well as numerical solutions, have been constructed. In this paper we consider a new approach to the analysis and construction of such magnetospheres. We consider force-free electrodynamics close to the rotation axis of a magnetosphere surrounding a Kerr black hole assuming axisymmetry. This is the region where the force-free approximation should work the best, and where the jets are located. We perform a systematic study of the asymptotic region with (split-)monopole, paraboloidal and vertical asymptotic behaviors. Imposing asymptotics similar to a (split-)monopole, we find under certain…
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