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Khlopov, M.Y., Rubin, S.G. and Sakharov, A. (2002) Strong Primordial Inhomogeneities and Galaxy Formation. Gravitation & Cosmology, 8, 57-65.

has been cited by the following article:

• 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.