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Beyond semiclassical time

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arxiv 2205.09147 v1 pith:D2RAQWJN submitted 2022-05-18 gr-qc hep-thquant-ph

classification gr-qchep-thquant-ph
keywords timesemiclassicalborn-oppenheimerorderquantumrelatedtheoryamplitudes
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We show that the usual Born-Oppenheimer type of approximation used in quantum gravity, in which a semiclassical time parameter emerges from a weak-coupling expansion of the Wheeler-DeWitt constraint, leads to a unitary theory at least up to the next-to-leading order in minisuperspace models. As there are no unitarity-violating terms, this settles the issue of unitarity at this order, which has been much debated in the literature. Furthermore, we also show that the conserved inner product is gauge-fixed in the sense that the measure is related to the Faddeev-Popov determinant associated with the choice of semiclassical time as a reparametrization gauge. This implies that the Born-Oppenheimer approach to the problem of time is, in fact, an instance of a relational quantum theory, in which transition amplitudes can be related to conditional probabilities.

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  1. Cosmological perturbations meet Wheeler DeWitt

    hep-th 2024-12 conditional novelty 6.0 of 10

    The semiclassical Wheeler-DeWitt wavefunction matches the perturbation-theory wavefunction of cosmology up to a specific phase and normalization, verified in exponential-potential and slow-roll mini-superspace models.

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