Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1896696 | Journal of Geometry and Physics | 2010 | 5 Pages |
Abstract
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], [25] and [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.
Related Topics
Physical Sciences and Engineering
Mathematics
Mathematical Physics
Authors
Juan Yang, Shu-Zheng Yang,