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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...
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