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Cosmic Censorship in Two-Dimensional Gravity

1992/09/22 by Jorge G. Russo, J. Russo, Leonard Susskind +3 · 14 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Electrodynamics and Casimir Effect #hep-th

paper · pdf · doi:10.1103/physrevd.47.533

published as Phys.Rev.D47:533-539,1993 · 16 pages, 1 figure (not included), a few minor corrections added

arxiv created 1992/09/22 · openalex publication_date 1993/01/15 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/04

Abstract

A weak version of the cosmic censorship hypothesis is implemented as a set of boundary conditions on exact semi-classical solutions of two-dimensional dilaton gravity. These boundary conditions reflect low-energy matter from the strong coupling region and they also serve to stabilize the vacuum of the theory against decay into negative energy states. Information about low-energy incoming matter can be recovered in the final state but at high energy black holes are formed and inevitably lead to information loss at the semi-classical level.

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