Quantum Information and Quantum Black Holes

dc.creatorBekenstein, Jacob D.
dc.date2001-07-13
dc.date2002-05-28
dc.date.accessioned2026-07-07T03:26:05Z
dc.date.available2026-07-07T03:26:05Z
dc.descriptionFirst, the relation between black holes and limitations on information of other systems is developed. After reviewing the relation of entropy to information, we derive the entropy bound, review its applications to cosmology and its extensions to higher dimensions, and discuss why black holes behave as 1-D objects when emitting entropy. We also discuss fundamental limitations on the information of pulses in curved space, and on the rate of disposal of information into a black hole. We then move on to a discussion of quantum black holes motivated by the adiabatic invariance of horizon area of classical holes. We develop an algebraic formalism based on symmetry which gives information on the area (or mass) spectrum of quantum black holes, and on the degeneracy of the levels. This last turns out to be consistent with the horizon area-black hole entropy proportionality while leaving room for corrections.
dc.descriptionLectures delivered at NATO Advanced Study Institute as 17th course of the International School of Cosmology and Gravitation, Erice, 30 April-10 May, 2001, 26 pages, LaTeX209 with crckab.sty (provided)
dc.identifierhttps://arxiv.org/abs/gr-qc/0107049
dc.identifierhttp://arxiv.org/abs/gr-qc/0107049
dc.identifierin Advances in the Interplay between Quantum and Gravity Physics, ed. P. G. Bergmann and V. de Sabbata (Kluwer, Dordrecht 2002). pp. 1-26
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33958
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.subjectQuantum Physics
dc.titleQuantum Information and Quantum Black Holes
dc.typetext

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