Hessling's Quantum Equivalence Principle and the Temperature of an Extremal Reissner-Nordström Black Hole

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dc.creatorMoretti, Valter
dc.date1995-10-10
dc.date.accessioned2026-07-07T03:30:52Z
dc.date.available2026-07-07T03:30:52Z
dc.descriptionThe Hessling improvement of the Haag, Narnhofer and Stein principle is analysed in the case of a massless scalar field propagating outside of an extremal R-N black hole. It is found that this sort of ``Quantum (Einstein's) Equivalence Principle'' selects only the R-N vacuum as a physically sensible state, i.e., it selects the temperature $T=0$ only.
dc.description8 pages, standard LaTex, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9510016
dc.identifierhttp://arxiv.org/abs/gr-qc/9510016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35671
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleHessling's Quantum Equivalence Principle and the Temperature of an Extremal Reissner-Nordström Black Hole
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