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- W1529538944 abstract "In this paper, we examine a flat FLRW spacetime with a scalar field potential and show by applying Osgood's criterion to the Einstein field equations that all such models, irrespective of the particular choice of potential develop finite-time singularities. That is, we show that solutions to the field equations become singular in finite time, which can have important implications for the role of inflation in cosmological models. We further point out that a possible reason for this behaviour is that the solutions to the field equations in such inflationary scenarios do not obey global existence and uniqueness properties, which is a typical characteristic of solutions that diverge in finite time." @default.
- W1529538944 created "2016-06-24" @default.
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- W1529538944 date "2015-05-28" @default.
- W1529538944 modified "2023-09-27" @default.
- W1529538944 title "On Singularities in Cosmic Inflation" @default.
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