Universality and Scaling at the Onset of Quantum Black Hole Formation

Preprint

21 January 1994

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.hep-th/9312017

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.

Keywords

SOLUTION DESCRIBING
CRITICAL THRESHOLD
HAWKING RADIATION
HOLE FORMATION
QUANTUM BLACK
FLUX EXCEEDS
UNIVERSALITY
EVAPORATION
BLACK HOLE

All Related Versions

Version 1, 1993-12-03, ArXiv
Version 2, 1993-12-04, ArXiv
Version 3, 1994-01-21, ArXiv
Published version: Physical Review Letters, 72 (11), 1584.

This publication has 0 references indexed in Scilit: