Journal
UNIVERSE
Volume 8, Issue 11, Pages -Publisher
MDPI
DOI: 10.3390/universe8110556
Keywords
quantum cosmology; WKB approximation; minisuperspace dynamics; canonical methods of quantization; Born-Oppenheimer separation
Funding
- TAsP INFN initiative
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This article analyzes the possibility of separating a gravity-matter system into a quasi-classical state and a small quantum subset using a WKB expansion of dynamics and considering the Bianchi universe minisuperspace. It discusses the validity of the approximation scheme for the Bianchi I model and explores applications for the quantum subsystem in the Bianchi IX model.
In this review, we analyse different aspects concerning the possibility to separate a gravity-matter system into a part which lives close to a quasi-classical state and a small quantum subset. The considered approaches are all relying on a WKB expansion of the dynamics by an order parameter and the natural arena consists of the Bianchi universe minisuperspace. We first discuss how, limiting the WKB expansion to the first order of approximation, it is possible to recover for the quantum subsystem a Schrodinger equation, as written on the classical gravitational background. Then, after having tested the validity of the approximation scheme for the Bianchi I model, we give some applications for the quantum subsystem in the so-called corner configuration of the Bianchi IX model. We individualize the quantum variable in the small one of the two anisotropy degrees of freedom. The most surprising result is the possibility to obtain a non-singular Bianchi IX cosmology when the scenario is extrapolated backwards in time. In this respect, we provide some basic hints on the extension of this result to the generic cosmological solution. In the last part of the review, we consider the same scheme to the next order of approximation identifying the quantum subset as made of matter variables only. This way, we are considering the very fundamental problem of non-unitary morphology of the quantum gravity corrections to quantum field theory discussing some proposed reformulations. Instead of constructing the time dependence via that one of the classical gravitational variables on the label time as in previous works, we analyse a recent proposal to construct time by fixing a reference frame. This scheme can be reached both introducing the so-called kinematical action, as well as by the well-known Kuchar-Torre formulation. In both cases, the Schrodinger equation, amended for quantum gravity corrections, has the same morphology and we provide a cosmological implementation of the model, to elucidate its possible predictions.
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