期刊
CLASSICAL AND QUANTUM GRAVITY
卷 22, 期 12, 页码 R85-R123出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/22/12/R01
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In three spacetime dimensions, general relativity becomes a topological field theory, whose dynamics can be largely described holographically by a two-dimensional conformal field theory at the 'boundary' of spacetime. I review what is known about this reduction-mainly within the context of pure (2 + 1)dimensional gravity-and discuss its implications for our understanding of the statistical mechanics and quantum mechanics of black holes.
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