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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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Black Hole Shadows of Charged Spinning Black Holes

TL;DR: In this paper, the authors proposed a method for measuring the black hole charge by imaging a black hole shadow in a galactic center by future interferometers, which only assumes stationary black hole and general relativity.
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Spacetime approach to force-free magnetospheres

TL;DR: In this paper, the theory of force-free magnetospheres has been systematically developed from a spacetime perspective using a suite of spacetime tools and techniques (notably exterior calculus) and exact solutions that demonstrate the extraction and transport of the rotational energy of a compact object.
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First-Principles Plasma Simulations of Black-Hole Jet Launching

TL;DR: General-relativistic collisionless plasma simulations of Kerr-black-hole magnetospheres which begin from vacuum, inject e^{±} pairs based on local unscreened electric fields, and reach steady states with electromagnetically powered Blandford-Znajek jets and persistent current sheets are presented.
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The ‘Meissner effect’ and the Blandford–Znajek mechanism in conductive black hole magnetospheres

TL;DR: In this article, it was shown that conductivity dramatically changes the properties of axisymmetric electromagnetic solutions of black hole electrodynamics, and that even for a maximally rotating Kerr black hole, the magnetic field is pulled inside the event horizon.
Journal ArticleDOI

Kerr black holes in a magnetic universe

TL;DR: In this paper, exact expressions for the electromagnetic fields associated with arbitrarily charged Kerr-Newman black holes in a magnetic universe were presented. And for arbitrary charged black holes metrical corrections of order B0 are evaluated.
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