One-loop Quantum Holography for Higher Dimensional Black Holes
arXiv:hep-th/9811078 · doi:10.1016/S0370-2693(99)00099-4
Abstract
The one-loop quantum corrections to the free energy associated with scalar field in a higher dimensional static curved space-time is investigated making use of the conformal transformation method. For a space-time with bifurcate horizon, horizon divergences are accounted for choosing the Planck length as natural cutoff. The leading term in the high temperature quantum correction satifies holographically the "area law", like the tree level Bekenstein-Hawking term. Furthermore it is stressed that only for the asymptotically AdS black holes one may have a microscopic interpretation of the entropy also at quantum level.
Latex file, 7 pages. A reference added. To appear in Phys. Lett. B
References in corpus (7)
- Black Hole Entropy from Near-Horizon Microstates
- Black holes with unusual topology
- Thermodynamics of (3+1)-dimensional black holes with toroidal or higher genus horizons
- Mechanism of Generation of Black Hole Entropy in Sakharov's Induced Gravity
- The Bekenstein Formula and String Theory (N-brane Theory)
- Statistical Origin of Black Hole Entropy in Matrix Theory
- A New Approach to Black Hole Microstates