Large-scale geometry of the Universe
Yassir Awwad, Tomislav Prokopec

TL;DR
This paper explores the large-scale geometry of the Universe, proposing it conforms to Thurston's geometrization conjecture, and discusses how different geometries evolve and can be tested through cosmological observations.
Contribution
It conjectures that the Universe's spatial section follows Thurston geometries, extending the standard cosmological models to include complex topologies and geometries.
Findings
Spatial anisotropies grow in decelerating universes
Anisotropies decay in accelerating universes
Inflation solves the anisotropy problem
Abstract
The large scale geometry of the late Universe can be decomposed as R, where R stands for cosmic time and is the three dimensional spatial manifold. We conjecture that the spatial geometry of the Universe's spatial section conforms with the Thurston-Perelman theorem, according to which the geometry of is either one of the eight geometries from the Thurston geometrization conjecture, or a combination of Thurston geometries smoothly sewn together. We assume that topology of individual geometries plays no observational role, i.e. the size of individual geometries is much larger than the Hubble radius today. We investigate the dynamics of each of the individual geometries by making use of the simplifying assumption that our local Hubble patch consists of only one such geometry, which is approximately homogeneous on very large scales,…
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Taxonomy
TopicsCosmology and Gravitation Theories
