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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.
Relativitat general (Física)
Forats negres (Astronomia)
General relativity (Physics)
Black holes (Astronomy)
(c) The American Physical Society, 1996
The American Physical Society

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