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Geometry of Black Holes and Multi-Black-Holes in 2+1 dimensions
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Lecture given at ``Raychaudhuri session," ICGC-95 conference, Pune (India), December 1995. Contents: I. Introduction II. (2+1)-Dimensional Initial Values in Stereographic Projection A. The single, non-rotating black hole B. Non-rotating multi-black-holes C. ``Black Hole" Universe Initial Values III. Time Development: Enter the Raychaudhuri Equation IV. Time Development in Stereographic Projection A. The BTZ black hole spacetime B. Multi-Black-Hole Spacetimes V. Black Holes with Angular Momentum VI. Analogous 3+1-Dimensional Black Holes VII. Conclusions
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A Holographic Map from AdS$_3$ to CFT$_2$
Semiclassical pure AdS3 gravity states, labelled by fixed-area geodesic networks, are mapped to CFT2 primary states whose wavefunctions are networks of OPE coefficients.
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