Towards a Hartle-Hawking state for loop quantum gravity

Abstract

The Hartle-Hawking state is a proposal for a preferred initial state for quantum gravity, based on a path integral over all compact Euclidean four-geometries which have a given three-geometry as a boundary. The wave function constructed this way satisfies the (Lorentzian) Hamiltonian constraint of general relativity in ADM variables in a formal sense. In this article we mimic this procedure of constructing an initial state in terms of Ashtekar-Barbero variables, and observe that the wave function thus constructed does not satisfy the Lorentzian Hamiltonian constraint even in a formal sense. We also investigate this issue for the relativistic particle. We finally suggest a modification of the proposal that does satisfy the constraint at least in a formal sense and start to consider its implications in quantum cosmology. We find that for certain variables, and in the saddle point approximation, the state is very similar to the Ashtekar-Lewandowski state of loop quantum gravity.

21 pages, 3 figures, RevTex4-1, v2: 22 pages, no figures, mistake in calculation of cosmological on-shell action corrected, some clarifications added, typos removed, reference added

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Cited by in corpus (2)

• The no-boundary wave function for loop quantum cosmology
• Canonical analysis of covariant unimodular gravity and an extension of the Kodama state