Tunnelling through black rings

dc.creatorZhao, Liu
dc.date2006-02-07
dc.date2006-02-08
dc.date.accessioned2026-07-07T12:53:47Z
dc.date.available2026-07-07T12:53:47Z
dc.descriptionHawking radiation of black ring solutions to 5-dimensional Einstein-Maxwell-dilaton gravity theory is analyzed by use of the Parikh-Wilczek tunnelling method. To get the correct tunnelling amplitude and emission rate, we adopted and developed the Angheben-Nadalini-Vanzo-Zerbini covariant approach to cover the effects of rotation and electronic discharge all at once, and the effect of back reaction is also taken into account. This constitute a unified approach to the tunnelling problem. Provided the first law of thermodynamics for black rings holds, the emission rate is proportional to the exponential of the change of Bekenstein-Hawking entropy. Explicit calculation for black ring temperatures agree exactly with the results obtained via the classical surface gravity method and the quasilocal formalism.
dc.description10 pages, V2: various modifications throughout the text, plus a lot of newly added references
dc.identifierhttps://arxiv.org/abs/hep-th/0602065
dc.identifierhttp://arxiv.org/abs/hep-th/0602065
dc.identifierCommun.Theor.Phys.47:835-842,2007
dc.identifierdoi:10.1088/0253-6102/47/5/014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223740
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTunnelling through black rings
dc.typetext

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