Expectation value of the horizon area for thermal equilibrium black holes
- 1 June 1991
- journal article
- Published by IOP Publishing in Classical and Quantum Gravity
- Vol. 8 (6) , L119-L123
- https://doi.org/10.1088/0264-9381/8/6/001
Abstract
Using a Euclidean path integral representation for the canonical ensemble partition function the author calculates the average value and fluctuations of the horizon area for thermal equilibrium black holes.Keywords
This publication has 7 references indexed in Scilit:
- Thermodynamic ensembles and gravitationClassical and Quantum Gravity, 1990
- Action Principle and Partition Function for the Gravitational Field in Black-Hole TopologiesPhysical Review Letters, 1988
- Black-hole thermodynamics and the Euclidean Einstein actionPhysical Review D, 1986
- Action integrals and partition functions in quantum gravityPhysical Review D, 1977
- Particle creation by black holesCommunications in Mathematical Physics, 1975
- Black Holes and EntropyPhysical Review D, 1973
- Role of Conformal Three-Geometry in the Dynamics of GravitationPhysical Review Letters, 1972