Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/12473
Title: Model of black hole evolution
Author: Russo, J. G. (Jorge Guillermo)
Keywords: Relativitat general (Física)
Gravitació
Forats negres (Astronomia)
General relativity (Physics)
Gravitació
Black holes (Astronomy)
Issue Date: 1996
Publisher: The American Physical Society
Abstract: We investigate a model where the quantum dynamics of black hole evaporation is determined by imposing a boundary on the apparent horizon with suitable boundary conditions. An unconventional scenario for the evolution emerges: only an insignificant fraction of energy of order (mG)-1 is radiated out; the outgoing wave carries a very small part of the quantum-mechanical information of the collapsed body, the bulk of the information remaining in the final stable black hole geometry.
Note: Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.55.871
It is part of: Physical Review D, 1996, vol. 55, núm 2, p. 871-877
URI: http://hdl.handle.net/2445/12473
ISSN: 0556-2821
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

Files in This Item:
File Description SizeFormat 
512112.pdf169.7 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.