Charged Rotating Black Hole in Three Spacetime Dimensions
Cristian Martinez, Claudio Teitelboim, Jorge Zanelli

TL;DR
This paper generalizes three-dimensional black holes to include electric charge, analyzes their properties, and explores how charge and angular momentum relate through Lorentz boosts, revealing some pathological features of charged solutions.
Contribution
It provides explicit solutions for charged rotating black holes in 3D, examines their stability, and clarifies how charge and angular momentum are interconnected via Lorentz transformations.
Findings
Inner horizon instability with small charge
Charged black holes can have arbitrarily negative mass
No upper bound on electric charge for these black holes
Abstract
The generalization of the black hole in three-dimensional spacetime to include an electric charge Q in addition to the mass M and the angular momentum J is given. The field equations are first solved explicitly when Q is small and the general form of the field at large distances is established. The total ``hairs'' M, J and Q are exhibited as boundary terms at infinity. It is found that the inner horizon of the rotating uncharged black hole is unstable under the addition of a small electric charge. Next it is shown that when Q=0 the spinning black hole may be obtained from the one with J=0 by a Lorentz boost in the plane. This boost is an ``illegitimate coordinate transformation'' because it changes the physical parameters of the solution. The extreme black hole appears as the analog of a particle moving with the speed of light. The same boost may be used when to…
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