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arXiv · hep-ph/0001168

Spinodal Instabilities and the Dark Energy Problem

D. Cormier·R. Holman
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Abstract

The accelerated expansion of the Universe measured by high redshift Type Ia Supernovae observations is explained using the non-equilibrium dynamics of naturally soft boson fields. Spinodal instabilities inevitably present in such systems yield a very attractive mechanism for arriving at the required equation of state at late times, while satisfying all the known constraints on models of quintessence.

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D. Cormier, R. Holman. 2000-01-17. Spinodal Instabilities and the Dark Energy Problem. https://doi.org/10.1103/physrevlett.84.5936

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