The (2+1)-Dimensional Black Hole
arXiv:gr-qc/9506079 · doi:10.1088/0264-9381/12/12/005
Abstract
I review the classical and quantum properties of the (2+1)-dimensional black hole of Ba{ñ}ados, Teitelboim, and Zanelli. This solution of the Einstein field equations in three spacetime dimensions shares many of the characteristics of the Kerr black hole: it has an event horizon, an inner horizon, and an ergosphere; it occurs as an endpoint of gravitational collapse; it exhibits mass inflation; and it has a nonvanishing Hawking temperature and interesting thermodynamic properties. At the same time, its structure is simple enough to allow a number of exact computations, particularly in the quantum realm, that are impractical in 3+1 dimensions.
LaTeX, 34 pages, 4 figures in separate file
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Cited by in corpus (361)
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- Dynamical Black Holes in 2+1 Dimensions
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- Boosting thermodynamic performance by bending space-time
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- Noether Currents of Charged Spherical Black Holes
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- Entropy from AdS(3)/CFT(2)
- Dimension in a Radiative Stellar Atmosphere
- Four-dimensional anti-de Sitter black holes from a three-dimensional perspective: Full complexity
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- Grassmannians and conformal structure on absolutes
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- Structure of gravastars in the context of massive gravity
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- Analog model for the BTZ black hole
- An optical analogue for rotating BTZ black holes
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- Strings from 3D gravity: asymptotic dynamics of AdS gravity with free boundary conditions
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- Gravity From Topological Field Theory
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