The temperature in Hawking radiation as tunneling

Simple item page
dc.creatorZhang, Baocheng
dc.creatorCai, Qing-yu
dc.creatorZhan, Ming-sheng
dc.date2009-01-06
dc.date.accessioned2026-07-07T12:55:24Z
dc.date.available2026-07-07T12:55:24Z
dc.descriptionThe quasi-classical method of deriving Hawking radiation under the consideration of canonical invariance is investigated. We find that the horizon should be regarded as a two-way barrier and the ingoing amplitude should be calculated according to the negative energy particles tunneling into the black hole because of the whole space-time interchange and thus the standard Hawking temperature is recovered. We also discuss the advantage of the Painlevé coordinates in Hawking radiation as tunneling.
dc.identifierhttps://arxiv.org/abs/0901.0591
dc.identifierhttp://arxiv.org/abs/0901.0591
dc.identifierPhys.Lett.B671:310-313,2009
dc.identifierdoi:10.1016/j.physletb.2008.12.019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224242
dc.subjectHigh Energy Physics - Theory
dc.titleThe temperature in Hawking radiation as tunneling
dc.typetext

Files

Collections

arXiv