Anomaly analysis of Hawking radiation from 2+1 dimensional spinning black hole

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dc.creatorWei, Shao-Wen
dc.creatorLi, Ran
dc.creatorLiu, Yu-Xiao
dc.creatorRen, Ji-Rong
dc.date2009-04-19
dc.date2009-05-01
dc.date.accessioned2026-07-07T13:10:30Z
dc.date.available2026-07-07T13:10:30Z
dc.descriptionConsidering gravitational and gauge anomalies at the horizon, a new successful method that to derive Hawking radiations from black holes has been developed recently by Wilczek et al.. By using the dimensional reduction technique, we apply this method to a non-vacuum solution, the 2+1 dimensional spinning black hole. The Hawking temperature and angular velocity on the horizon are obtained. The results may partially imply that this method is independent of the gravity theory, the dimension of spacetime and the topological structure of the event horizon.
dc.descriptionv2: 5 pages, typos corrected, references added
dc.identifierhttps://arxiv.org/abs/0904.2915
dc.identifierhttp://arxiv.org/abs/0904.2915
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229027
dc.subjectHigh Energy Physics - Theory
dc.titleAnomaly analysis of Hawking radiation from 2+1 dimensional spinning black hole
dc.typetext

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