Anomalies and de Sitter radiation from the generic black holes in de Sitter spaces

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dc.creatorJiang, Qing-Quan
dc.creatorWu, Shuang-Qing
dc.creatorCai, Xu
dc.date2007-05-26
dc.date.accessioned2026-07-07T10:35:57Z
dc.date.available2026-07-07T10:35:57Z
dc.descriptionRobinson-Wilczek's recent work shows that, the energy momentum tensor flux required to cancel gravitational anomaly at the event horizon of a Schwarzschild-type black hole has an equivalent form to that of a (1+1)-dimensional blackbody radiation at the Hawking temperature. Motivated by their work, Hawking radiation from the cosmological horizons of the general Schwarzschild-de Sitter and Kerr-de Sitter black holes, has been studied by the method of anomaly cancellation. The result shows that the absorbing gauge current and energy momentum tensor fluxes required to cancel gauge and gravitational anomalies at the cosmological horizon are precisely equal to those of Hawking radiation from it. It should be emphasized that the effective field theory for generic black holes in de Sitter spaces should be formulated within the region between the event horizon (EH) and the cosmological horizon (CH), to integrate out the classically irrelevant ingoing modes at the EH and the classically irrelevant outgoing modes at the CH, respectively.
dc.description14 pages without figure, use elsart.cls, to appear in Phys.Lett.B
dc.identifierhttps://arxiv.org/abs/0705.3871
dc.identifierhttp://arxiv.org/abs/0705.3871
dc.identifierPhys.Lett.B651:65-70,2007
dc.identifierdoi:10.1016/j.physletb.2007.06.003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179895
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAnomalies and de Sitter radiation from the generic black holes in de Sitter spaces
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