{ "id": "hep-th/9610086", "version": "v2", "published": "1996-10-11T16:48:26.000Z", "updated": "1996-11-20T00:07:03.000Z", "title": "Entropy of Localized States and Black Hole Evaporation", "authors": [ "Ken D. Olum" ], "comment": "27 pages, ReVTeX, 5 postscript figures using epsf. Miscellaneous cleanups, one section rewritten for clarity", "journal": "Phys.Rev. D55 (1997) 6168-6180", "doi": "10.1103/PhysRevD.55.6168", "categories": [ "hep-th" ], "abstract": "We call a state \"vacuum-bounded\" if every measurement performed outside a specified interior region gives the same result as in the vacuum. We compute the maximum entropy of a vacuum-bounded state with a given energy for a one-dimensional model, with the aid of numerical calculations on a lattice. The maximum entropy is larger than it would be for rigid wall boundary conditions by an amount $\\delta S$ which for large energies is less than or approximately $(1/6) ln (L_in T)$, where L_in is the length of the interior region. Assuming that the state resulting from the evaporation of a black hole is similar to a vacuum-bounded state, and that the similarity between vacuum-bounded and rigid-wall-bounded problems extends from 1 to 3 dimensions, we apply these results to the black hole information paradox. We conclude that large amounts of information cannot be emitted in the final explosion of a black hole.", "revisions": [ { "version": "v2", "updated": "1996-11-20T00:07:03.000Z" } ], "analyses": { "subjects": [ "04.70.Dy", "05.30.-d" ], "keywords": [ "black hole evaporation", "localized states", "maximum entropy", "interior region", "rigid wall boundary conditions" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Phys. Rev. D" }, "note": { "typesetting": "RevTeX", "pages": 27, "language": "en", "license": "arXiv", "status": "editable", "inspire": 424476 } } }