Statistical Origin of Black Hole Entropy in Matrix Theory
arXiv:hep-th/9802173 · doi:10.1103/PhysRevLett.81.256
Abstract
The statistical entropy of black holes in M-theory is considered. Assuming Matrix theory is the discretized light-cone quantization of a theory with eleven-dimensional Lorentz invariance, we map the counting problem onto the original Gibbons-Hawking calculation of the thermodynamic entropy.
9 pages, harvmac, (v2 References added, typo fixed), (v3 Some clarifying comments added.)
References in corpus (15)
- Self-Interaction and Gauge Invariance
- Why is the Matrix Model Correct?
- Mechanism of Generation of Black Hole Entropy in Sakharov's Induced Gravity
- Schwarzschild Black Holes from Matrix Theory
- Matrix Theory
- Constraints From Extended Supersymmetry in Quantum Mechanics
- Linearized supergravity from Matrix theory
- Long-distance interactions of branes: correspondence between supergravity and super Yang-Mills descriptions
- Interactions of type IIB D-branes from D-instanton matrix model
- Schwarzchild Black Holes in Matrix Theory II
- Why Matrix Theory is Hard
- Schwarzschild Black Holes in Various Dimensions from Matrix Theory
- Comments on Black Holes in Matrix Theory
- Matrix Schwarzschild Black Holes in Large N limit
- Renormalization of Higher Derivative Operators in the Matrix Model
Cited by in corpus (6)
- Black hole entropy from non-perturbative gauge theory
- AdS/CFT and the Information Paradox
- Stretched horizons, quasiparticles and quasinormal modes
- Conservation of Supergravity Currents from Matrix Theory
- Near-Extremal Black Hole Evaporation in Asymptotically Flat Spacetime
- One-loop Quantum Holography for Higher Dimensional Black Holes