Abstract
Milne-like spacetimes are a class of \(k = -1\) FLRW spacetimes which admit continuous spacetime extensions through the big bang. In a previous paper Ling (Found. of Phys. 50:385–428, 2020), it was shown that the cosmological constant appears as an initial condition for Milne-like spacetimes. In this paper, we generalize this statement to spacetimes which share similar geometrical properties with Milne-like spacetimes but without the strong spatially isotropic assumption associated with them. We show how our results yield a “quasi de Sitter” expansion for the early universe which could have applications to inflationary scenarios.
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07 November 2022
A Correction to this paper has been published: https://doi.org/10.1007/s10714-022-03030-2
Notes
These extensions have been noted previously in the physics literature, see e.g. [9].
Our convention for the mean curvature H, which includes the 1/3 factor in front of \(\text {tr}(K)\), coincides with the Hubble parameter, \(a'/a\), which is also denoted by H in the physics literature.
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Acknowledgements
The author gratefully acknowledges being supported by the Harold H. Martin Postdoctoral Fellowship at Rutgers University. He thanks Greg Galloway for many helpful comments and pointing out references [10, 11]. He thanks two anonymous reviewers who greatly improved the quality of the paper. Lastly, he thanks the organizers of Singularity theorems, causality, and all that; a tribute to Roger Penrose for putting together a stimulating conference.
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Ling, E. Remarks on the cosmological constant appearing as an initial condition for Milne-like spacetimes. Gen Relativ Gravit 54, 68 (2022). https://doi.org/10.1007/s10714-022-02955-y
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DOI: https://doi.org/10.1007/s10714-022-02955-y