Hawking Radiation from a Vaidya Black Hole: A Semi-Classical Approach and Beyond

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dc.creatorSiahaan, Haryanto M.
dc.creatorTriyanta
dc.date2008-11-07
dc.date2008-11-19
dc.date.accessioned2026-07-07T10:19:06Z
dc.date.available2026-07-07T10:19:06Z
dc.descriptionWe derive the Hawking radiation for Vaidya black hole in the tunneling picture from the corresponding single particle action by the use of the radial null geodesic and the Hamilton-Jacobi method (beyond semi-classical approximation). Both results are then analyzed and compared.
dc.descriptionCorrected version of presented talk at 2nd ICMNS (October 28, 2008), Bandung, Indonesia. 13 pages, jhep style, v4: some minor corrections, references added
dc.identifierhttps://arxiv.org/abs/0811.1132
dc.identifierhttp://arxiv.org/abs/0811.1132
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/174385
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking Radiation from a Vaidya Black Hole: A Semi-Classical Approach and Beyond
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