The Bisognano-Wichmann Theorem for Charged States and the Conformal Boundary of a Black Hole

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dc.creatorLongo, Roberto
dc.date2000-01-21
dc.date.accessioned2026-07-07T04:27:36Z
dc.date.available2026-07-07T04:27:36Z
dc.descriptionRecent applications of Operator Algebras to Quantum Field Theory on a Curved Spacetime show that the incremental entropy associated with a quantum black hole, due the addition of a short range charge, is quantized proportionally to the logarithm of an integer. This talk first reviews the case of a Rindler black hole and then sketches the case of a spacetime with bifurcate Killing horizon and charges localizable on the horizon. An important tool is the construction of the conformal symmetries on the horizon.
dc.descriptionAMS-LaTeX, 7 pages. talk delivered at the conference on ``Mathematical Physics and Quantum Field Theory'', Berkeley, 11-13 June 1999. Electronic Journal of Differential Equations (to appear)
dc.identifierhttps://arxiv.org/abs/math-ph/0001034
dc.identifierhttp://arxiv.org/abs/math-ph/0001034
dc.identifierElectr. J. Diff. Eq., Conf. 04, (2000), 159-164
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/56478
dc.subjectMathematical Physics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.subject81T20 (Primary) 46L60 (Secondary)
dc.titleThe Bisognano-Wichmann Theorem for Charged States and the Conformal Boundary of a Black Hole
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