Sigma model of near-extreme rotating black holes and their microstates
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Publication:1571853
DOI10.1016/S0550-3213(98)00608-7zbMath0940.83017arXivhep-th/9806141MaRDI QIDQ1571853
Mirjam Cvetič, Arkady A. Tseytlin
Publication date: 12 July 2000
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/hep-th/9806141
Two-dimensional field theories, conformal field theories, etc. in quantum mechanics (81T40) Black holes (83C57)
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Cites Work
- Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravity
- Microscopic derivation of the Bekenstein-Hawking entropy formula for non-extremal black holes
- \(\text{AdS}_3\) black holes and a stringy exclusion principle
- Black hole entropy from near-horizon microstates
- Microscopic origin of the Bekenstein-Hawking entropy
- The string spectrum on the horizon of a non-extremal black hole
- Internal structure of black holes
- Infrared behavior of closed superstrings in strong magnetic and gravitational fields
- Strings as solitons \&\ black holes as strings
- Extremal black holes as fundamental strings
- \(D\)-brane approach to black hole quantum mechanics
- Extremal black hole entropy from conformal string sigma model
- Exact supersymmetric string solutions in curved gravitational backgrounds
- EXTREME DYONIC BLACK HOLES IN STRING THEORY
- Black hole in three-dimensional spacetime
- String theory formulation of the three-dimensional black hole
- Exact Four-Dimensional Dyonic Black Holes and Bertotti-Robinson Spacetimes in String Theory
- Dirichlet Branes and Ramond-Ramond Charges
- What we don't know about BTZ black hole entropy
- Two-dimensional models of black-hole evaporation
- D-branes and spinning black holes
- Closed superstrings in magnetic flux tube background
- Generalised chiral null models and rotating string backgrounds