Fermions tunneling from rotating stationary Kerr black hole with electric charge and magnetic charge

In this paper, the method of semi-classical fermion tunneling is extended to explore the fermion tunneling behavior of a Kerr-Newman-Kasuya black hole. Thus, the Hamilton-Jacobi equation in Kerr-Newman-Kasuya space-time is derived by the method presented in Refs. Lin and Yang (2009) [24-26], the Hawking temperature at the horizon and the tunneling probability of spin-1/2 fermions are finally obtained following the semi-classical quantum equation. The results indicate the common features of this black hole. (C) 2010 Elsevier B.V. All rights reserved.