Higher Derivative Correction to the Hawking Flux via Trace Anomaly

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dc.creatorShirasaka, Akihide
dc.creatorHirata, Tomoyoshi
dc.date2008-04-11
dc.date2008-04-15
dc.date.accessioned2026-07-07T09:32:28Z
dc.date.available2026-07-07T09:32:28Z
dc.descriptionIn this paper we derive Hawking radiation of black holes with higher derivative corrections by the method of trace anomaly. Firstly we derive Hawking radiation for general spherical black holes. We introduce a modified tortoise coordinate to it and find the analyticity of the coordinate. Secondly we apply its method to a black hole with a higher derivative correction and derive the Hawking radiation of it. We found that as an ordinary case the flux depends only on the surface gravity.
dc.description14 pages, references added
dc.identifierhttps://arxiv.org/abs/0804.1910
dc.identifierhttp://arxiv.org/abs/0804.1910
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/158791
dc.subjectHigh Energy Physics - Theory
dc.titleHigher Derivative Correction to the Hawking Flux via Trace Anomaly
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