Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/12475
Title: Quantum black holes: Nonperturbative corrections and no-veil scenario
Author: Russo, J. G. (Jorge Guillermo)
Keywords: Relativitat general (Física)
Gravitació
General relativity (Physics)
Gravitation
Issue Date: 1994
Publisher: The American Physical Society
Abstract: A common belief is that further quantum corrections near the singularity of a large black hole should not substantially modify the semiclassical picture of black hole evaporation; in particular, the outgoing spectrum of radiation should be very close to the thermal spectrum predicted by Hawking. In this paper we explore a possible counterexample: in the context of dilaton gravity, we find that nonperturbative quantum corrections which are important in strong-coupling regions may completely alter the semiclassical picture, to the extent that the presumptive spacelike boundary becomes timelike, changing in this way the causal structure of the semiclassical geometry. As a result, only a small fraction of the total energy is radiated outside the fake event horizon; most of the energy comes in fact at later retarded times and there is no problem of information loss. This may constitute a general characteristic of quantum black holes, that is, quantum gravity might be such as to prevent the formation of global event horizons.
Note: Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.49.5266
It is part of: Physical Review D, 1994, vol. 49, núm. 10, p. 5266-5277
URI: http://hdl.handle.net/2445/12475
ISSN: 0556-2821
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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