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Journal ArticleDOI

Black hole in a uniform magnetic field

Robert M. Wald
- 15 Sep 1974 - 
- Vol. 10, Iss: 6, pp 1680-1685
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TLDR
In this paper, the authors derived the solution for the electromagnetic field occurring when a stationary, axisymmetric black hole is placed in an originally uniform magnetic field aligned along the symmetry axis of the black hole.
Abstract
Using the fact that a Killing vector in a vacuum spacetime serves as a vector potential for a Maxwell test field, we derive the solution for the electromagnetic field occurring when a stationary, axisymmetric black hole is placed in an originally uniform magnetic field aligned along the symmetry axis of the black hole. It is shown that a black hole in a magnetic field will selectively accrete charges until its charge becomes $Q=2{\mathrm{Bb}}_{0}J$, where ${B}_{0}$ is the strength of the magnetic field and $J$ is the angular momentum of the black hole. As a by-product of the analysis given here, we prove that the gyromagnetic ratio of a slightly charged, stationary, axisymmetric black hole (not assumed to be Kerr) must have the value $g=2$.

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Citations
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A coupled guiding center-Boris particle pusher for magnetized plasmas in compact-object magnetospheres.

TL;DR: In this article, a coupled pusher is proposed to simulate the motion of relativistic charged particles in magnetospheres of compact objects, typically filled with highly magnetized collisionless plasmas, based on a dynamic switch between the full system of equations of motion and a guiding center approximation.
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Near-horizon Structure of Escape Zones of Electrically Charged Particles around Weakly Magnetized Rotating Black Hole. II. Acceleration and Escape in the Oblique Magnetosphere

TL;DR: In this paper, the authors investigated the effect of a large-scale magnetic field on the dynamics of charged particles near a rotating black hole and found that breaking the axial symmetry substantially increases the fraction of escaping orbits and allows the acceleration to ultrarelativistic velocities.

Carrollian motion in magnetized black hole horizons

TL;DR: In this paper , the authors revisited the motion of massless particles with anyonic spin in the horizon of Kerr-Newman geometry and showed that the previously computed magnetic field is not invariant under Carroll diffeomorphisms and found another result which respects these symmetries of the horizon.
Book ChapterDOI

Black Holes and Superradiant Instabilities

TL;DR: In this paper, the authors look at the main cause of several important instabilities in BH spacetimes, such as hairy BH solutions and rotational energy from the BH, spinning it down.
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