
TL;DR
This paper explores a novel approach to resolving the Big Bang singularity by introducing a degenerate spacetime metric with a spacelike defect, potentially revealing a new 'side' of the Big Bang and related wormhole solutions.
Contribution
It proposes a new class of solutions with degenerate metrics to eliminate the Big Bang singularity and discusses the implications of a spacetime defect in cosmology.
Findings
Elimination of the Big Bang curvature singularity.
Existence of a 'pre-Big-Bang' phase alternative.
Introduction of defect wormhole solutions.
Abstract
We review the suggestion that it is possible to eliminate the Big Bang curvature singularity of the Friedmann cosmological solution by considering a particular type of degenerate spacetime metric. Specifically, we take the 4-dimensional spacetime metric to have a spacelike 3-dimensional defect with a vanishing determinant of the metric. This new solution suggests the existence of another "side" of the Big Bang (perhaps a more appropriate description than "pre-Big-Bang" phase used in our original paper). The corresponding new solution for defect wormholes is also briefly discussed.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory
