Spinodal Instabilities and the Dark Energy Problem

Details Spinodal Instabilities and the Dark Energy Problem Spinodal Instabilities and the Dark Energy Problem

2000-01-17

arxiv.org/abs/hep-ph/0001168v1

Phys.Rev.Lett. 84 (2000) 5936-5939

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 2 figures

Scientific paper

10.1103/PhysRevLett.84.5936

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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