Tunneling Effect Near Weakly Isolated Horizon

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dc.creatorWu, Xiaoning
dc.creatorGao, Sijie
dc.date2007-02-06
dc.date.accessioned2026-07-07T11:21:43Z
dc.date.available2026-07-07T11:21:43Z
dc.descriptionThe 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.
dc.description7 pages, accepted for publication in Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/0702033
dc.identifierhttp://arxiv.org/abs/gr-qc/0702033
dc.identifierPhys.Rev.D75:044027,2007
dc.identifierdoi:10.1103/PhysRevD.75.044027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194345
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTunneling Effect Near Weakly Isolated Horizon
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