S. S. McGaugh and W. J. G. De Blok ”Testing the Hypothesis of Modified Dynamicsa with Low Surface Brightness Galaxies and other Evidence,” The Astro- physical Journal, Vol. 499, No. 1, 1998, pp. 66-81. doi:10.1086/305629

has been cited by the following article:

• TITLE: Dark Energy as a Property of Dark Matter

  AUTHORS: Jacques Leibovitz

  KEYWORDS: dark energy; dark matter.

  JOURNAL NAME: Journal of Modern Physics, Vol.2 No.12, December 7, 2011

  ABSTRACT: A novel model of dark matter (DM), elastically compressible, can contribute to the acceleration of our Universe expansion. While each galaxy compresses its own DM within its gravitation field, the DM bordering neighboring galaxies, far from their centers, is pulled apart. It is shown that, although the DM pressure tends to zero at such locations, the DM compressibility tends to infinity. This allows the DM to expand between galaxies without gravitation hindrance. The model is consistent with the coupled distributions of baryonic and dark matters, with black hole formation at the centers of large galaxies, with galactic flat rotation curves, with a Tully-Fisher relation, and with Milgrom’s MOND relation. Results are discussed.