Dmitry67 said:
Lightsphere (after finite time) is always finite when curvature is finite.
The only example when it might become infinite is the final stages of the Big Rip scenario, but there curvature is infinite. Also, Goedel's solution, but it is an oodity as time is cyclical there.
What is your contre-example?
The following a an interesting article that goes into a math model that describes an infinite and eternal universe.
Inflation without a beginning: a null boundary proposal (Dated: February 7, 2008)
by Anthony Aguirre
School of Natural Sciences, Institute for Advanced Study Princeton, New Jersey 08540, USA
and Steven Gratton
Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08544, USA†
http://arxiv.org/PS_cache/gr-qc/pdf/0301/0301042v2.pdf
The following is the introduction to the article
[cite=[PLAIN]http://arxiv.org/PS_cache/gr-qc/pdf/0301/0301042v2.pdf][/PLAIN]
We develop our recent suggestion that inflation may be made past eternal, so that there is no initial cosmological singularity or “beginning of time”. Inflation with multiple vacua generically approaches a steady-state statistical distribution of regions at these vacua, and our model follows directly from making this distribution hold at all times. We find that this corresponds (at the semi-classical level) to particularly simple cosmological boundary conditions on an infinite null surface near which the spacetime looks de Sitter. The model admits an interesting arrow of time that is well-defined and consistent for all physical observers that can communicate, even while the statistical description of the entire universe admits a symmetry that includes time-reversal. Our model suggests, but does not require, the identification of antipodal points on the manifold. The resulting “elliptic” de Sitter spacetime has interesting classical and quantum properties. The proposal may be generalized to other inflationary potentials, or to boundary conditions that give semi-eternal but non-singular cosmologies.
© source where applicable
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