Time in quantum theory, the Wheeler-DeWitt equation and the Born-Oppenheimer approximation
Alexander Yu. Kamenshchik, Alessandro Tronconi, Tereza Vardanyan and, Giovanni Venturi

TL;DR
This paper compares gauge-fixing and Born-Oppenheimer approaches to the Wheeler-DeWitt equation in quantum cosmology, showing they yield similar results in a simple model and discussing the broader problem of time in quantum theories.
Contribution
It provides a comparative analysis of two methods for introducing time in quantum cosmology and explores their implications and similarities in a simplified setting.
Findings
Both approaches produce similar predictions in the tested model.
The paper discusses the problem of time in quantum mechanics.
It examines the classical-quantum correspondence in cosmological contexts.
Abstract
We compare two different approaches to the treatment of the Wheeler-DeWitt equation and the introduction of time in quantum cosmology. One approach is based on the gauge-fixing procedure in theories with first-class constraints, while the other uses the Born-Oppenheimer method. We apply both to a very simple cosmological model and observe that they give similar predictions. We also discuss the problem of time in non-relativistic quantum mechanics and some questions concerning the correspondence between classical and quantum theories.
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