Cosmic Censorship in Two-Dimensional Gravity

Details Cosmic Censorship in Two-Dimensional Gravity Cosmic Censorship in Two-Dimensional Gravity

1992-09-04

arxiv.org/abs/hep-th/9209012v2

Phys.Rev.D47:533-539,1993

Physics

High Energy Physics

High Energy Physics - Theory

16 pages, 1 figure (not included), a few minor corrections added

Scientific paper

10.1103/PhysRevD.47.533

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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