Xiang-Qian Li, Ge-Rui Chen
Published 2015-07-13Version 1
In this paper, we investigate the Hawking radiation of massive spin-1 particles from 4-dimensional Kerr and Kerr-Newman black holes. By applying the Hamilton-Jacobi ansatz and the WKB approximation to the field equations of the massive bosons in Kerr and Kerr-Newman space-time, the quantum tunneling method is successfully implemented. As a result, we obtain the tunneling rate of the emitted vector particles and recover the standard Hawking temperature of both the two black holes.
Nonextensive entropies impact onto thermodynamics and phase structure of Kerr-Newman black holes
More on scattering of Chern-Simons vortices
Kerr-Newman black holes from $\mathcal{N}=1^*$
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