# Perturbing Monopolar Force-Free Magnetospheres to Slowly Rotating Black   Holes

**Authors:** Kevin Thoelecke, Masaaki Takahashi, Sachiko Tsuruta

arXiv: 1901.01245 · 2019-03-15

## TL;DR

This paper investigates how frame-dragging influences force-free magnetospheres around slowly rotating black holes, revealing a bifurcation in magnetic field configurations due to perturbations in black hole spin.

## Contribution

It demonstrates that the common perturbed monopolar solution acts as a separatrix between two distinct classes of magnetic field structures influenced by frame-dragging effects.

## Key findings

- Perturbed monopolar solutions separate two magnetic field configurations.
- Frame-dragging alters toroidal magnetic fields and force balance.
- Magnetic field lines bend differently depending on solution class.

## Abstract

We study the effects of frame-dragging on the structure of force-free magnetospheres around rotating black holes. For slowly rotating black holes, analytic explorations often focus on transforming an exact force-free solution applicable to a static black hole into a solution approximately applicable to a slowly-rotating black hole via perturbations in black hole spin. We show that the single perturbed monopolar solution most commonly arrived at using such techniques is in fact a separatrix between two broad classes of solutions: those with poloidal magnetic fields that bend upwards towards the azimuthal axis and those that bend downwards towards the equatorial plane. This is because frame-dragging affects the toroidal magnetic field distributions, changing the force balance between poloidal magnetic field lines.

## Full text

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## Figures

2 figures with captions in the complete paper: https://tomesphere.com/paper/1901.01245/full.md

## References

13 references — full list in the complete paper: https://tomesphere.com/paper/1901.01245/full.md

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Source: https://tomesphere.com/paper/1901.01245