Hawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies

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dc.creatorJiang, Qing-Quan
dc.creatorWu, Shuang-Qing
dc.date2006-12-30
dc.date2007-01-19
dc.date.accessioned2026-07-07T11:23:33Z
dc.date.available2026-07-07T11:23:33Z
dc.descriptionRobinson-Wilczek's recent work, which treats Hawking radiation as a compensating flux to cancel gravitational anomaly at the horizon of a Schwarzschild-type black hole, is extended to study Hawking radiation of rotating black holes in anti-de Sitter spaces, especially that in dragging coordinate system, via gauge and gravitational anomalies. The results show that in order to restore gauge invariance and general coordinate covariance at the quantum level in the effective field theory, the charge and energy flux by requiring to cancel gauge and gravitational anomalies at the horizon, must have a form equivalent to that of a $(1+1)$-dimensional blackbody radiation at Hawking temperature with an appropriate chemical potential.
dc.description15 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0701002
dc.identifierhttp://arxiv.org/abs/hep-th/0701002
dc.identifierPhys.Lett.B647:200-206,2007
dc.identifierdoi:10.1016/j.physletb.2007.01.058
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194927
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies
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