2019
DOI: 10.1515/zna-2019-0223
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Gauge Fixing and the Semiclassical Interpretation of Quantum Cosmology

Abstract: We make a critical review of the semiclassical interpretation of quantum cosmology and emphasise that it is not necessary to consider that a concept of time emerges only when the gravitational field is (semi)classical. We show that the usual results of the semiclassical interpretation, and its generalisation known as the Born-Oppenheimer approach to quantum cosmology, can be obtained by gauge fixing, both at the classical and quantum levels. By 'gauge fixing' we mean a particular choice of the time coordinate,… Show more

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Cited by 18 publications
(54 citation statements)
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“…(56) together with (48) implies that sgn(ṫ) = −sgn(p t ) = σ = const., which leads to |t(b) − t(a)| = σ(t(b) − t(a)). Using (56) and (57), we can now insert the relational solution (50) in the integrand of (47) to obtain the on-shell action:…”
Section: On-shell Action and The Hamilton-jacobi Constraintmentioning
confidence: 99%
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“…(56) together with (48) implies that sgn(ṫ) = −sgn(p t ) = σ = const., which leads to |t(b) − t(a)| = σ(t(b) − t(a)). Using (56) and (57), we can now insert the relational solution (50) in the integrand of (47) to obtain the on-shell action:…”
Section: On-shell Action and The Hamilton-jacobi Constraintmentioning
confidence: 99%
“…When higher orders in 1 c 2 are included, S σ solves corrected Newtonian constraints, where the corrections come from the expansion of the square-root in (56). The same expansion procedure can be performed for any minisuperspace model of cosmology with a non-vanishing potential and, formally, for the field-theoretical case [50]. The corrected Newtonain constraint leads to a corrected Schrödinger equation in the quantum theory.…”
Section: Non-relativistic Limitmentioning
confidence: 99%
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