Black hole in three-dimensional spacetime.
@article{Baados1992BlackHI,
title={Black hole in three-dimensional spacetime.},
author={Ba{\~n}ados and Teitel'boim and Zanelli},
journal={Physical review letters},
year={1992},
volume={69 13},
pages={
1849-1851
}
}The standard Einstein-Maxwell equations in 2+1 spacetime dimensions, with a negative cosmological constant, admit a black hole solution. The 2+1 black hole---characterized by mass, angular momentum, and charge, defined by flux integrals at infinity---is quite similar to its 3+1 counterpart. Anti--de Sitter space appears as a negative energy state separated by a mass gap from the continuous black hole spectrum. Evaluation of the partition function yields that the entropy is equal to twice the…
2,182 Citations
2 + 1‐dimensional black holes with momentum and angular momentum
- PhysicsAnnalen der Physik
- 2000
Exact solutions of Einstein's equations in 2 + 1‐dimensional anti‐de Sitter space containing any number of black holes are described. In addition to the black holes these spacetimes can possess…
Black hole creation in 2 + 1 dimensions
- Physics
- 1999
When two point particles, coupled to three-dimensional gravity with a negative cosmological constant, approach each other with a sufficiently large centre-of-mass energy, then a BTZ black hole is…
2 + 1 black hole with a dynamical conical singularity
- Physics
- 1996
We find black hole solutions to Euclidean 2 + 1 gravity coupled to a relativistic particle which have a dynamical conical singularity at the horizon. These solutions mimic the tree level contribution…
Scale-dependent three-dimensional charged black holes in linear and non-linear electrodynamics
- Physics
- 2017
In the present work we study the scale dependence at the level of the effective action of charged black holes in Einstein–Maxwell as well as in Einstein–power-Maxwell theories in…
The (2 + 1)-dimensional black hole
- Physics
- 1995
I review the classical and quantum properties of the (2 + 1)-dimensional black hole of Banados, Teitelboim and Zanelli. This solution of the Einstein field equations in three spacetime dimensions…
References
SHOWING 1-9 OF 9 REFERENCES
Class
- Quantum Grav. 10: L54
- 1993
This makes the metric complex when J = 0. The Euclidean action is given by iI = −I Euc . Although correct in the case at hand, making imaginary a particular coordinate in a generally covariant theory
We thank E.Witten for pointing this out to us
Ann. Phy
- Ann. Phy
- 1984
That canonical conjugates in the sense of classical mechanics become thermodynamical conjugates has been noticed by
- Class
That the entropy may be written as a surface term on the horizon has been observed previously by
- Phy. Rev. Lett
- 1990
Electronic address: cecsnet@uchcecvm.bitnet
Phy. Rev. D
- Phy. Rev. D
- 1977