Please use this identifier to cite or link to this item:
https://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: | https://hdl.handle.net/2445/12473 |
Related resource: | http://dx.doi.org/10.1103/PhysRevD.55.871 |
ISSN: | 0556-2821 |
Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
File | Description | Size | Format | |
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512112.pdf | 169.7 kB | Adobe PDF | View/Open |
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