Quantum kinematics of spacetime. II. A model quantum cosmology with real clocks
- 15 November 1988
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 38 (10) , 2985-2999
- https://doi.org/10.1103/physrevd.38.2985
Abstract
Nonrelativistic model quantum cosmologies are studied in which the basic time variable is the position of a clock indicator and the time parameter of the Schrödinger equation is an unobservable label. Familiar Schrödinger-Heisenberg quantum mechanics emerges if the clock is ideal—arbitrarily accurate for arbitrarily long times. More realistically, however, the usual formulation emerges only as an approximation appropriate to states of this model universe in which part of the system functions approximately as an ideal clock. It is suggested that the quantum kinematics of spacetime theories such as general relativity may be analogous to those of this model. In particular it is suggested that our familiar notion of time in quantum mechanics is not an inevitable property of a general quantum framework but an approximate feature of specific initial conditions.Keywords
This publication has 35 references indexed in Scilit:
- “Time” replaced by quantum correlationsInternational Journal of Theoretical Physics, 1984
- Evolution without evolution: Dynamics described by stationary observablesPhysical Review D, 1983
- Measurement of time by quantum clocksAmerican Journal of Physics, 1980
- The time of arrival in quantum mechanics II. The individual measurementAnnals of Physics, 1969
- The time of arrival in quantum mechanics I. Formal considerationsAnnals of Physics, 1969
- Quantum Theory of Gravity. I. The Canonical TheoryPhysical Review B, 1967
- Über quantenmechanische ZeitoperatorenAnnalen der Physik, 1962
- Heisenberg representation in classical general relativityIl Nuovo Cimento (1869-1876), 1961
- Relativistic Invariance and Quantum PhenomenaReviews of Modern Physics, 1957
- Relativity quantum mechanics with an application to compton scatteringProceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character, 1926