A Topologically Charged Black Hole in the Braneworld
Figure 1
as function of for different values of and . The intersections with the -axis give inner and outer horizons. In (a), we set , and (b) has . In both cases, values of give one horizon, while give two horizons or an extremal configuration , resembling the behaviour of Reissner-Nordström solution. Above this extremal value, there is no black hole. In (c), we consider the case, and the behaviour shows no black hole solution.
