A Topologically Charged Rotating Black Hole in the Brane

Figure 2

Characteristic behaviour of the temperature of the black hole 𝑇 as a function of the horizon radius 𝑟₊ for different values of the parameter 𝛽. In the three plots, we use 𝑞=1 and 𝑎=1.25. The dotted line corresponds to the temperature 𝑇_KN for the conventional Kerr-Newman solution (i.e., 𝛽=0).