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Model of black hole evolution
Russo, J. G. (Jorge Guillermo)
Universitat de Barcelona
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.
11-05-2010
Relativitat general (Física)
Gravitació
Forats negres (Astronomia)
General relativity (Physics)
Gravitació
Black holes (Astronomy)
(c) The American Physical Society, 1996
Artículo
The American Physical Society
         

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