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Article

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Published version

Publication date

1996

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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/12473

Model of black hole evolution

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http://dx.doi.org/10.1103/PhysRevD.55.871

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.

Subject

Relativitat general (Física), Gravitació, Forats negres (Astronomia)

Subject (English)

General relativity (Physics), Gravitació, Black holes (Astronomy)

Citation

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Articles publicats en revistes (Física Quàntica i Astrofísica)

Citation

RUSSO, J. G. (Jorge Guillermo). Model of black hole evolution. Physical Review D. 1996. Vol. 55, num. núm 2, pags. 871-877. ISSN 0556-2821. [consulted: 14 of August of 2026]. Available at: https://hdl.handle.net/2445/12473

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