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
- OpenAlex
- https://openalex.org/W1763748250
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:18095488
Keywords
Physics, Extremal black hole, Black hole (networking), de Sitter–Schwarzschild metric, Spacetime
References
Cited by
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- Gribov copies, BRST-exactness and Chern-Simons theory
- Positive energy of topologically massive gravity
- Power Structures in Finite Fields and the Riemann Hypothesis
- Quantum Gravity in Three Dimensions from Higher-Spin Holography
- On the Geometry of Space
- Hawking–Page phase transition in new massive gravity
- A Microscopic Theory of the Neutron
- The Dirac Equation and Its' Solutions
- Three Dimensional Charged Interior Solutions Admitting Conformal Killing Vectors
- Gravitational environments, flows and holographic fluids
- Nonlinear Electromagnetics in Flat and Curved Spacetime
- Analytic continuation of black hole entropy in Loop Quantum Gravity
- What after CERN? Opportunities from co-responding systems
- Quantization of BMS3 orbits: A perturbative approach
- A Mathematical Exploration of Low-Dimensional Black Holes
- Superradiance: Energy Extraction, Black-Hole Bombs and Implications for Astrophysics and Particle Physics
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