2006/02/28 by Satoshi Iso, Hiroshi Umetsu, Frank Wilczek
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Electrodynamics and Casimir Effect #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevlett.96.151302
published as Phys.Rev.Lett. 96 (2006) 151302 · 4 pages, typos corrected, references added, version to appear in Phys. Rev. Lett
openalex publication_date 2006/04/19 · arxiv created 2006/06/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Extending the method of Robinson and Wolczek, we show that in order to avoid a breakdown of general covariance and gauge invariance at the quantum level the total flux of charge and energy in each outgoing partial wave of a charged quantum field in a Reissner-Nordström black hole background must be equal to that of a (1 + 1)-dimensional blackbody at the Hawking temperature with the appropriate chemical potential.