Tunneling Effect Near Weakly Isolated Horizon

Details Tunneling Effect Near Weakly Isolated Horizon Tunneling Effect Near Weakly Isolated Horizon

2007-02-06

arxiv.org/abs/gr-qc/0702033v1

Phys.Rev.D75:044027,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, accepted for publication in Physical Review D

Scientific paper

10.1103/PhysRevD.75.044027

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.

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