Hawking Radiation as Tunnelling in Static Black Holes

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dc.creatorLiu, Wenbiao
dc.date2005-12-16
dc.date.accessioned2026-07-07T06:53:57Z
dc.date.available2026-07-07T06:53:57Z
dc.descriptionHawking radiation can usefully be viewed as a semi-classical tunnelling process that originates at the black hole horizon. The conservation of energy implies the effect of self-gravitation. For a static black hole, a generalized Painleve coordinate system is introduced, and Hawking radiation as tunnelling under the effect of self-gravitation is investigated. The corrected radiation is consistent with the underlying unitary theory.
dc.identifierhttps://arxiv.org/abs/gr-qc/0512098
dc.identifierhttp://arxiv.org/abs/gr-qc/0512098
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/105773
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking Radiation as Tunnelling in Static Black Holes
dc.typetext

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