Entropy in the RST Model
arXiv:gr-qc/9412065 · doi:10.1103/PhysRevD.52.2239
Abstract
The RST Model is given boundary term and Z-field so that it is well-posed and local. The Euclidean method is described for general theory and used to calculate the RST intrinsic entropy. The evolution of this entropy for the shockwave solutions is found and obeys a second law.
10 pages, minor revisions, published version in Latex
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- Unveiling horizons in quantum critical collapse
- Two-dimensional quantum-corrected black hole in a finite size cavity
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- Note on explicit form of entanglement entropy in the RST model
- Evaporation and Antievaporation instabilities
- Quantum-Corrected Bondi Mass for 2D Hawking Radiation