Subtleties in the quasi-classical calculation of Hawking radiation

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dc.creatorAkhmedov, Emil T.
dc.creatorPilling, Terry
dc.creatorSingleton, Douglas
dc.date2008-05-17
dc.date2008-10-02
dc.date.accessioned2026-07-07T13:11:59Z
dc.date.available2026-07-07T13:11:59Z
dc.descriptionhe quasi-classical method of deriving Hawking radiation is investigated. In order to recover the original Hawking temperature one must take into account a previously ignored contribution coming from the temporal part of the action. This contribution plus a contribution coming from the spatial part of the action gives the correct temperature.
dc.description6 pages revtex. Honorable Mention in 2008 GRF essay contest, typos fixed, sign errors corrected. To be published in Special Issue of IJMPD
dc.identifierhttps://arxiv.org/abs/0805.2653
dc.identifierhttp://arxiv.org/abs/0805.2653
dc.identifierInt.J.Mod.Phys.D17:2453-2458,2008
dc.identifierdoi:10.1142/S0218271808013947
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229458
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleSubtleties in the quasi-classical calculation of Hawking radiation
dc.typetext

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