Global properties of physically interesting Lorentzian spacetimes
Deloshan Nawarajan (Victoria University of Wellington), Matt Visser, (Victoria University of Wellington)

TL;DR
This paper explores the global topological and geometric properties of Lorentzian spacetimes, emphasizing their physical implications and advocating for a focus on structures like tetrads and complex structures over the metric alone.
Contribution
It revisits and emphasizes the importance of global properties such as orientability, parallelizability, and complex structures in Lorentzian spacetimes from an empirical physics perspective.
Findings
Spacetime should be space-, time-, and spacetime-orientable.
Spacetime should possess a globally defined tetrad or vielbein.
A globally-defined almost complex structure is nearly unavoidable.
Abstract
Under normal circumstances most members of the general relativity community focus almost exclusively on the local properties of spacetime, such as the locally Euclidean structure of the manifold and the Lorentzian signature of the metric tensor. When combined with the classical Einstein field equations this gives an extremely successful empirical model of classical gravity and classical matter --- at least as long as one does not ask too many awkward questions about global issues, (such as global topology and global causal structure). We feel however that this is a tactical error --- even without invoking full-fledged "quantum gravity" we know that the standard model of particle physics is also an extremely good representation of some parts of empirical reality; and we had better be able to carry over all the good features of the standard model of particle physics --- at least into the…
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