The classical essence of black hole radiation

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dc.creatorNouri-Zonoz, M.
dc.creatorPadmanabhan, T.
dc.date1998-12-28
dc.date.accessioned2026-07-07T03:32:52Z
dc.date.available2026-07-07T03:32:52Z
dc.descriptionWe show that the mathematics of Hawking process can be interpreted classically as the Fourier analysis of an exponentially redshifted wave mode which scatters off the black hole and travels to infinity at late times. We use this method to derive the Planckian power spectrum for Schwarzchild, Reissner-Nordstrom and Kerr black holes.
dc.description5 pages, Revtex
dc.identifierhttps://arxiv.org/abs/gr-qc/9812088
dc.identifierhttp://arxiv.org/abs/gr-qc/9812088
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36395
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe classical essence of black hole radiation
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