TITLE:
Dark Energy Stars and the Cosmic Microwave Background
AUTHORS:
George F. Chapline
KEYWORDS:
Cosmology, Dark Matter, CMB
JOURNAL NAME:
Open Access Library Journal,
Vol.2 No.5,
May
21,
2015
ABSTRACT: 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.