Cosmological models with a large cosmological constant are unstable due
to quantum critical fluctuations at the de Sitter horizon. Due to this
instability the space-time in these models will quickly evolve into a
Friedmann-like expanding universe containing dark energy stars and radiation.
In this paper it is pointed out that this provides a simple explanation for
both the observed radiation entropy per gram of dark matter and the level of
temperature fluctuations in the cosmic microwave background. A novel prediction
is that large dark energy stars provide the seeds for the formation of
galaxies.
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