On the past-completeness of inflationary spacetimes

We discuss the question of whether or not inflationary spacetimes can be geodesically complete in the infinite past. Geodesic completeness is a necessary condition for averting an initial singularity during eternal inflation. It is frequently argued that cosmological models which are expanding suffi...

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Veröffentlicht in:arXiv.org 2023-01
Hauptverfasser: Lesnefsky, J E, Easson, D A, Davies, P C W
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Sprache:eng
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Zusammenfassung:We discuss the question of whether or not inflationary spacetimes can be geodesically complete in the infinite past. Geodesic completeness is a necessary condition for averting an initial singularity during eternal inflation. It is frequently argued that cosmological models which are expanding sufficiently fast (having average Hubble expansion rate \(H_{avg}>0\)) must be incomplete in null and timelike past directions. This well-known conjecture relies on specific bounds on the integral of the Hubble parameter over a past-directed timelike or null geodesic. As stated, we show this claim is an open issue. We show that the calculation of \(H_{avg}\) yields a continuum of results for a given spacetime predicated upon the underlying topological assumptions. We present an improved definition for \(H_{avg}\) and introduce an uncountably infinite cohort of cosmological solutions which are geodesically complete despite having \(H_{avg}>0\). We discuss a standardized definition for inflationary spacetimes as well as quantum (semi-classical) cosmological concerns over physically reasonable scale factors.
ISSN:2331-8422
DOI:10.48550/arxiv.2207.00955