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Black Hole Evaporation in 1+1 Dimensions | | J. Russo
; L. Susskind
; L. Thorlacius
; | | Date: |
30 Dec 1991 | | Journal: | Phys.Lett. B292 (1992) 13-18 | | Subject: | hep-th | | Abstract: | The formation and quantum mechanical evaporation of black holes in two spacetime dimensions can be studied using effective classical field equations, recently introduced by Callan {it et al.} We find that gravitational collapse always leads to a curvature singularity, according to these equations, and that the region where the quantum corrections introduced by Callan {it et al.} could be expected to dominate is on the unphysical side of the singularity. The model can be successfully applied to study the back-reaction of Hawking radiation on the geometry of large mass black holes, but the description breaks down before the evaporation is complete. | | Source: | arXiv, hep-th/9201074 | | Services: | Forum | Review | PDF | Favorites | |
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