Universality and Scaling at the Onset of Quantum Black Hole Formation
arXiv:hep-th/9312017 · doi:10.1103/PhysRevLett.72.1584
Abstract
In certain two-dimensional models, collapsing matter forms a black hole if and only if the incoming energy flux exceeds the Hawking radiation rate. Near the critical threshold, the black hole mass is given by a universal formula in terms of the distance from criticality, and there exists a scaling solution describing the formation and evaporation of an arbitrarily small black hole.
9 pages, 3 figures (uuencoded)
References in corpus (6)
Cited by in corpus (31)
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