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Conformal Field Theory, (2+1)-Dimensional Gravity, and the BTZ Black Hole

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.

preprint2005arXivOpen access
S. Carlip
gr-qchep-th
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