The Bisognano-Wichmann Theorem for Charged States and the Conformal Boundary of a Black Hole
Longo, Roberto
arXiv, 0001034 / Harvested from arXiv
Text on arXiv
Recent 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.
Publié le : 2000-01-21
Classification:  Mathematical Physics,  General Relativity and Quantum Cosmology,  High Energy Physics - Theory,  81T20 (Primary) 46L60 (Secondary) 
@article{0001034,
     author = {Longo, Roberto},
     title = {The Bisognano-Wichmann Theorem for Charged States and the Conformal
  Boundary of a Black Hole},
     journal = {arXiv},
     volume = {2000},
     number = {0},
     year = {2000},
     language = {en},
     url = {http://dml.mathdoc.fr/item/0001034}
}

Longo, Roberto. The Bisognano-Wichmann Theorem for Charged States and the Conformal
  Boundary of a Black Hole. arXiv, Tome 2000 (2000) no. 0, . http://gdmltest.u-ga.fr/item/0001034/