Black hole in three-dimensional spacetime.

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Summary

The standard Einstein-Maxwell equations in 2+1 spacetime dimensions, with a negative cosmological constant, admit a black hole solution that appears as a negative energy state separated by a mass gap from the continuous black hole spectrum.

Type
article
Published
1992-04-29
Cited by
2,302
References
12
Access
Open access

Keywords

Physics, Extremal black hole, Black hole (networking), de Sitter–Schwarzschild metric, Spacetime

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