Abstract
We present an exact solution of a rotating dyon black hole in the Tomimatsu-Sato-Yamazaki space-time and study its special case, i.e., the exact rotating dyon solution for which the space-time metric takes the Kerr-Newman form. This solution is characterized by four physical parameters (mass M, angular momentum S, electric charge Q, and magnetic charge Φ), represents a black hole, and reduces to the rotating monopole in the case Q=0.

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