Topological implications of inhomogeneity
Boudewijn F. Roukema (1), Vincent Blanloeil (2), Jan J. Ostrowski (1), ((1) Torun Centre for Astronomy NCU, (2) Mathematics Department U.Strasbourg)

TL;DR
This paper explores how inhomogeneity in dust models of the Universe can lead to changes in spatial topology over time, including transitions from disconnected to connected or simply connected to multiply connected spaces, within a classical framework.
Contribution
It demonstrates that Einstein equations permit solutions where cosmic topology evolves over time, influenced by non-simultaneous big bang times, highlighting a classical mechanism for topology change.
Findings
Existence of solutions with topology change from disconnected to connected
Existence of solutions with topology change from simply connected to multiply connected
Topology evolution occurs over post-quantum epochs if bang time varies significantly
Abstract
The approximate homogeneity of spatial sections of the Universe is well supported observationally, but the inhomogeneity of the spatial sections is even better supported. Here, we consider the implications of inhomogeneity in dust models for the connectedness of spatial sections at early times. We consider a non-global Lemaitre-Tolman-Bondi (LTB) model designed to match observations, a more general, heuristic model motivated by the former, and two specific, global LTB models. We propose that the generic class of solutions of the Einstein equations projected back in time from the spatial section at the present epoch includes subclasses in which the spatial section evolves (with increasing time) smoothly (i) from being disconnected to being connected, or (ii) from being simply connected to being multiply connected, where the coordinate system is comoving and synchronous. We show that (i)…
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Taxonomy
TopicsAdvanced Mathematical Modeling in Engineering
