Fluxes of Higher-spin Currents and Hawking Radiations from Charged Black Holes

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dc.creatorIso, Satoshi
dc.creatorMorita, Takeshi
dc.creatorUmetsu, Hiroshi
dc.date2007-05-24
dc.date.accessioned2026-07-07T10:55:47Z
dc.date.available2026-07-07T10:55:47Z
dc.descriptionThis is an extended version of the previous paper (hep-th/0701272). Quantum fields near horizons can be described in terms of an infinite set of two-dimensional conformal fields. We first generalize the method of Christensen and Fulling to charged black holes to derive fluxes of energy and charge. These fluxes can be obtained by employing a conformal field theory technique. We then apply this technique to obtain the fluxes of higher-spin currents and show that the thermal distribution of Hawking radiation from a charged black hole can be completely reproduced by investigating transformation properties of the higher-spin currents under conformal and gauge transformations.
dc.description15 pages
dc.identifierhttps://arxiv.org/abs/0705.3494
dc.identifierhttp://arxiv.org/abs/0705.3494
dc.identifierPhys.Rev.D76:064015,2007
dc.identifierdoi:10.1103/PhysRevD.76.064015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186194
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFluxes of Higher-spin Currents and Hawking Radiations from Charged Black Holes
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