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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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Charged Compact Binary Coalescence Signal and Electromagnetic Counterpart of Plunging BH-NS mergers

TL;DR: In this paper, the authors developed a general theory of cCBC for any mass and amount of charge for each member of a compact binary coalescence and showed that if at least one of the members of a BH-NS merger is charged, the inspiral of the two members would generate a Poynting flux with an increasing power, giving rise to a brief electromagnetic counterpart temporally associated with the chirp signal of the merger (with possibly a small temporal offset), which they termed as the {\em charged Compact Binary Coalescence} (cCBC) signal
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On the GeV Emission of the Type I BdHN GRB 130427A

TL;DR: The inner engine of a binary-driven hypernova (BdHN) is composed of a Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field aligned with the BH rotation axis, and surrounded by an ionized plasma of extremely low density.
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Mass of Kerr-Newman black holes in an external magnetic field

TL;DR: In this article, the first law and Smarr formula for black holes in a magnetic field was clarified and the unique mass which is integrable and reduces to the Kerr-Newman mass in the absence of magnetic fields was defined.
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