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Towards a future singularity?

M. Gasperini
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Abstract

We discuss whether the future extrapolation of the present cosmological state may lead to a singularity even in case of "conventional" (negative) pressure of the dark energy field, namely $w=p/ρ\geq -1$. The discussion is based on an often neglected aspect of scalar-tensor models of gravity: the fact that different test particles may follow the geodesics of different metric frames, and the need for a frame-independent regularization of curvature singularities.

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M. Gasperini. 2004-05-16. Towards a future singularity?. https://doi.org/10.1142/s0218271804006310

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