Tunneling Effect Near Weakly Isolated Horizon
arXiv:gr-qc/0702033 · doi:10.1103/PhysRevD.75.044027
Abstract
The tunneling effect near a weakly isolated horizon (WIH) has been studied. By applying the null geodesic method of Parikh and Wilczek and Hamilton-Jacibi method of Angheben et al. to a weakly isolated horizon, we recover the semiclassical emission rate in the tunneling process. We show that the tunneling effect exists in a wide class of spacetimes admitting weakly isolated horizons. The general thermodynamic nature of WIH is then confirmed.
7 pages, accepted for publication in Physical Review D
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