Thermodynamics of event horizons in (2+1)-dimensional gravity
- 15 March 1992
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 45 (6) , 2151-2154
- https://doi.org/10.1103/physrevd.45.2151
Abstract
Although gravity in 2+1 dimensions is very different in nature from gravity in 3+1 dimensions, it is shown that the laws of thermodynamics for event horizons can be manifested also for (2+1)-dimensional gravity. The validity of the classical laws of horizon mechanics is verified in general and exemplified for the (2+1)-dimensional analogues of Reissner-Nordström and Schwarzschild–de Sitter spacetimes. We find that the entropy is given by 1/4L, where L is the length of the horizon. A consequence of having consistent thermodynamics is that the second law fixes the sign of Newton’s constant to be positive.Keywords
This publication has 16 references indexed in Scilit:
- Stringy cosmic strings with horizonsPhysics Letters B, 1990
- A global string with an event horizonPhysics Letters B, 1990
- Einstein's theory in a three-dimensional space-timeGeneral Relativity and Gravitation, 1984
- Three-dimensional cosmological gravity: Dynamics of constant curvatureAnnals of Physics, 1984
- Three-dimensional Einstein gravity: Dynamics of flat spaceAnnals of Physics, 1984
- Spacetime foamNuclear Physics B, 1978
- Breakdown of predictability in gravitational collapsePhysical Review D, 1976
- Black holes and thermodynamicsPhysical Review D, 1976
- Generalized second law of thermodynamics in black-hole physicsPhysical Review D, 1974
- Black Holes and EntropyPhysical Review D, 1973