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

KEYWORDS

Cosmology, Dark Matter, CMB

Cite this paper

Chapline, G. 2015 Dark Energy Stars and the Cosmic Microwave Background. Open Access Library Journal, 2, 1-7. doi: 10.4236-oalib.1101174.





Autor: George F. Chapline

Fuente: http://www.scirp.org/



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