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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/12477
Cosmic censorship in two-dimensional gravity
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A weak version of the cosmic censorship hypothesis is implemented as a set of boundary conditions on exact semiclassical 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 semiclassical level.
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RUSSO, J. G. (Jorge Guillermo), SUSSKIND, Leonard and THORLACIUS, Lárus. Cosmic censorship in two-dimensional gravity. Physical Review D. 1993. Vol. 47, num. 2, pags. 533-539. ISSN 0556-2821. [consulted: 10 of August of 2026]. Available at: https://hdl.handle.net/2445/12477