Figure 9

Figure 9: The ADM mass as a function of the horizon radius RD of static spherically symmetric solutions to the Einstein-Yang-Mills system (in units provided by the Yang-Mills coupling constant). Numerical plots for the colorless (n = 0) and families of colored black holes (n = 1,2) are shown. (Note that the y-axis begins at M = 0.7 rather than at M = 0.)