Hawking radiation and Quasinormal modes

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dc.creatorYoon, SangChul
dc.date2005-10-03
dc.date2005-10-05
dc.date.accessioned2026-07-07T06:21:05Z
dc.date.available2026-07-07T06:21:05Z
dc.descriptionThe spectrum of Hawking radiation by quantum fields in the curved spacetime is continuous, so the explanation of Hawking radiation using quasinormal modes can be suspected to be impossible. We find that quasinormal modes do not explain the relation between the state observed in a region far away from a black hole and the short distance behavior of the state on the horizon.
dc.description6 pages, references added
dc.identifierhttps://arxiv.org/abs/gr-qc/0510009
dc.identifierhttp://arxiv.org/abs/gr-qc/0510009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95488
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking radiation and Quasinormal modes
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