Quantum Cosmological Metroland Model
Edward Anderson, Anne Franzen

TL;DR
This paper explores a simplified quantum cosmological model called 4-stop metroland, focusing on shape dynamics of four particles on a line, providing exact solutions and insights relevant to quantum gravity and the problem of time.
Contribution
It introduces the N-stop metroland model, analyzing shape-only mechanics of four particles, and extends ideas to N-particle systems with applications to quantum cosmology.
Findings
Exact classical and quantum solutions for 4-stop metroland
Interpretation of shape operators as relative sizes and homogeneity measures
Relevance to the problem of time in quantum gravity
Abstract
Relational particle mechanics is useful for modelling whole-universe issues such as quantum cosmology or the problem of time in quantum gravity, including some aspects outside the reach of comparably complex minisuperspace models. In this article, we consider the mechanics of pure shape and not scale of 4 particles on a line, so that the only physically significant quantities are ratios of relative separations between the constituents' physical objects. Many of our ideas and workings extend to the N-particle case. As such models' configurations resemble depictions of metro lines in public transport maps, we term them `N-stop metrolands'. This 4-stop model's configuration space is a 2-sphere, from which our metroland mechanics interpretation is via the `cubic' tessellation. This model yields conserved quantities which are mathematically SO(3) objects like angular momenta but are…
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