A Note on the Semi-Classical Approximation in Quantum Gravity

Abstract

We re-examine the semiclassical approximation to quantum gravity in the canonical formulation, focusing on the definition of a quasiclassical state for the gravitational field. It is shown that a state with classical correlations must be a superposition of states of the form $e^{iS}$. In terms of a reduced phase space formalism, this type of state can be expressed as a coherent superposition of eigenstates of operators that commute with the constraints and so correspond to constants of the motion. Contact is made with the usual semiclassical approximation by showing that a superposition of this kind can be approximated by a WKB state with an appropriately localised prefactor. A qualitative analysis is given of the effects of geometry fluctuations, and the possibility of a breakdown of the semiclassical approximation due to interference between neighbouring classical trajectories is discussed. It is shown that a breakdown in the semiclassical approximation can be a coordinate dependent phenomenon, as has been argued to be the case close to a black hole horizon.

Latex with 3 figures. About 30 pages

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• Noether symmetric $f(R)$ quantum cosmology and its classical correlations
• WKB Approaches to Restore Time in Quantum Cosmology: Predictions and Shortcomings
• Quantum Gravity and Turning Points in the Semiclassical Approximation
• Time dependent perturbation theory from Wheeler De Witt solutions
• Black hole thermodynamics from quantum gravity
• The Background Field Approximation in (quantum) cosmology
• Classical and Quantum Mechanics of Black Holes in Generic 2-D Dilaton Gravity
• Time dependent Green functions from Wheeler De Witt solutions
• Massive Dilaton and Topological Gravity
• Semi-classical predictions of cosmological wave-packets from ridge-lines