Path integrals and instantons in quantum gravity: Minisuperspace models
- 15 June 1996
- journal article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 53 (12) , 6979-6990
- https://doi.org/10.1103/physrevd.53.6979
Abstract
While there does not at this time exist a complete canonical theory of full 3+1 quantum gravity, there does appear to be a satisfactory canonical quantization of minisuperspace models. The method requires no `choice of time variable' and preserves the systems' explicit reparametrization invariance. In the following study, this canonical formalism is used to derive a path integral for quantum minisuperspace models. As it comes from a well-defined canonical starting point, the measure and contours of integration are specified by this construction. The properties of the resulting path integral are analyzed, both exactly and in the semiclassical limit. Particular attention is paid to the role of the (unbounded) Euclidean action and Euclidean instantons are argued to contribute as $e^{-|S_E|/\hbar}$.Comment: 23 pages, ReVTeX, minor changes: clarifying Comments and references adde
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This publication has 50 references indexed in Scilit:
- Decay of magnetic fields in Kaluza-Klein theoryPhysical Review D, 1995
- Pair creation of extremal black holes and Kaluza-Klein monopolesPhysical Review D, 1994
- Semiclassical Wheeler wormhole productionPhysics Letters B, 1991
- THE CONFORMAL FACTOR AND THE COSMOLOGICAL CONSTANTInternational Journal of Modern Physics A, 1990
- Conformal rotation in Bianchi type-I quantum cosmologyPhysical Review D, 1989
- The quantum state of the universeNuclear Physics B, 1984
- Wave function of the UniversePhysical Review D, 1983
- Instability of the Kaluza-Klein vacuumNuclear Physics B, 1982
- Path integrals and the indefiniteness of the gravitational actionNuclear Physics B, 1978
- Quantum Theory of Gravity. I. The Canonical TheoryPhysical Review B, 1967