Critical phenomena in gravitational collapse

被引:100
作者
Gundlach C. [1 ,2 ]
机构
[1] Enrico Fermi Institute, University of Chicago, 5640 S Ellis Avenue, Chicago, 60637, IL
[2] University of Southampton, High field, Southampton
关键词
Black Hole Threshold; Choptuik; Critical Collapse; Discrete Self-similarity (DSS); Critical Solution;
D O I
10.12942/lrr-1999-4
中图分类号
学科分类号
摘要
As first discovered by Choptuik, the black hole threshold in the space of initial data for general relativity shows both surprising structure and surprising simplicity. Universality, power-law scaling of the black hole mass, and scale echoing have given rise to the term “critical phenomena". They are explained by the existence of exact solutions which are attractors within the black hole threshold, that is, attractors of codimension one in phase space, and which are typically self-similar. This review gives an introduction to the phenomena, tries to summarize the essential features of what is happening, and then presents extensions and applications of this basic scenario. Critical phenomena are of interest particularly for creating surprising structure from simple equations, and for the light they throw on cosmic censorship and the generic dynamics of general relativity. ©1999 Max-Planck-Gesellschaft and the authors.
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页数:58
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