Hawking radiation and Hawking flux from spherical reduction

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dc.creatorKummer, W.
dc.creatorVassilevich, D. V.
dc.date2000-09-14
dc.date.accessioned2026-07-07T03:25:15Z
dc.date.available2026-07-07T03:25:15Z
dc.descriptionUsing heat kernel techniques we show that the relation between Hawking temperature and radiation flux known from Einstein gravity in D dimensions can be reproduced from the spherically reduced action. A recent controversy regarding the D=2 anomaly for that case is discussed. The generalized effective Polyakov action in the presence of a dilaton field is presented.
dc.descriptionInvited Talk at Parallel Session "Black Hole Thermodynamics" of 9th Marcel Grossmann Conference Rome, 2-8 July 2000, 6 p
dc.identifierhttps://arxiv.org/abs/gr-qc/0009051
dc.identifierhttp://arxiv.org/abs/gr-qc/0009051
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33637
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking radiation and Hawking flux from spherical reduction
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