Abstract
We now contemplate dealing with frozen quantum wave equations by finding an emergent time once already at the quantum level, within semiclassical quantum cosmology’s physical regime of interest. This could be the regime in which currently observed inhomogeneities in galaxy distribution and cosmic microwave background temperatures originated. This regime is characterized by heavy–light, adiabatic slow–fast, Born–Oppenheimer, and WKB approximations. In particular, inhomogeneities are light and fast to the scalefactor of the universe and homogeneous modes being heavy and slow. At the level of a Problem of Time strategy, the WKB approximation leads to an emergent semiclassical time. We argue furthermore that this admits a Machian interpretation, in close but not identical parallel with Part II’s emergent classical Machian time, and also cast the semiclassical approach in Temporal Relationalism compatible form. One is then left with an emergent time dependent Schrödinger equation for the light fast modes. We end by discussing how using a WKB approximation is crucial for this outcome but requires further justification.
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- 1.
- 2.
These are not potentials per se, due to, firstly, overall factors of 2 and that some of the original equations having an \(\mbox{N}^{hh}(h)\) function prefactor being divided out. Secondly, due to terms going like \(\hbar^{2}\) originating from the conformal operator ordering being packaged into \(v\), by which (46.1) does not necessarily display all \(\hbar \) dependence.
- 3.
For the case in which the velocities feature solely homogeneous quadratically in the kinetic term, these are ± the same expression. However, more generally, the 2 solutions are ± in the sense of being a complex conjugate pair.
- 4.
A further argument involves constructive interference underlying classicality [897, 899]. However this amounts to imposing, rather than deducing (semi)classicality. This also applies to using (semi)classicality as a ‘final condition’ restriction on quantum-cosmological solutions. In this manner, LQC can also be argued to not address this point either, and with further issue due to the proportion of solutions rejected on such grounds being larger than is elsewise usual in Quantum Cosmology (see Sect. 43.5). Such a restriction is also akin to how Griffiths and Omnès remove by hand the superposition states which they term “grotesque universes” [390] due to their behaviour being very unlike that we experience today.
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Anderson, E. (2017). Tempus Post Quantum. ii. Semiclassical Machian Emergent Time. In: The Problem of Time. Fundamental Theories of Physics, vol 190. Springer, Cham. https://doi.org/10.1007/978-3-319-58848-3_46
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