We construct static axially symmetric solutions of SU(2) Einstein-Yang-Millsdilaton theory. Like their spherically symmetric counterparts, these solutions are nonsingular and asymptotically flat. The solutions are characterized by the winding number n and the node number k of the gauge field functions. For fixed n with increasing k the solutions tend to “extremal” Einstein-Maxwell-dilaton black...

We construct new black hole solutions in Einstein-Yang-Mills theory. They are static, axially symmetric and asymptotically flat. They are characterized by their horizon radius and a pair of integers (k, n), where k is related to the polar angle and n to the azimuthal angle. The known spherically and axially symmetric EYM black holes have k = 1. For k > 1, pairs of new black hole solutions appea...

The grey body radiation spectrum from various types of black holes is an interesting topic, both at the fundamental level and at the experimental (astrophysical) one. In a previous paper, I have applied the modified Moebius transform (henceforth MMT) due to Chen to the so-called distorted black holes, a terminology used by Geroch and Hartle to denote axially symmetric black hole Einstein soluti...