Relationship between Hawking Radiation and Gravitational Anomalies

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dc.creatorRobinson, Sean P.
dc.creatorWilczek, Frank
dc.date2005-02-15
dc.date2005-08-23
dc.date.accessioned2026-07-07T11:30:09Z
dc.date.available2026-07-07T11:30:09Z
dc.descriptionWe show that in order to avoid a breakdown of general covariance at the quantum level the total flux in each outgoing partial wave of a quantum field in a black hole background must be equal to that of a (1+1)-dimensional blackbody at the Hawking temperature.
dc.description5 pages, 1 figure; v2: typo corrected, reference added; v3: comment added, minor editorial changes to agree with published version
dc.identifierhttps://arxiv.org/abs/gr-qc/0502074
dc.identifierhttp://arxiv.org/abs/gr-qc/0502074
dc.identifierPhys.Rev.Lett.95:011303,2005
dc.identifierdoi:10.1103/PhysRevLett.95.011303
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196931
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleRelationship between Hawking Radiation and Gravitational Anomalies
dc.typetext

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