Higher-spin Currents and Thermal Flux from Hawking Radiation

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dc.creatorIso, Satoshi
dc.creatorMorita, Takeshi
dc.creatorUmetsu, Hiroshi
dc.date2007-01-30
dc.date2007-05-25
dc.date.accessioned2026-07-07T11:03:11Z
dc.date.available2026-07-07T11:03:11Z
dc.descriptionQuantum fields near black hole horizons can be described in terms of an infinite set of d=2 conformal fields. In this paper, by investigating transformation properties of general higher-spin currents under a conformal transformation, we reproduce the thermal distribution of Hawking radiation in both cases of bosons and fermions. As a byproduct, we obtain a generalization of the Schwarzian derivative for higher-spin currents.
dc.description4 pages, RevTex, accepted for publication in PRD
dc.identifierhttps://arxiv.org/abs/hep-th/0701272
dc.identifierhttp://arxiv.org/abs/hep-th/0701272
dc.identifierPhys.Rev.D75:124004,2007
dc.identifierdoi:10.1103/PhysRevD.75.124004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188501
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleHigher-spin Currents and Thermal Flux from Hawking Radiation
dc.typetext

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