Exploring Properties of Dark and Visible Mass Distribution on Different Scales in the Universe

Details Exploring Properties of Dark and Visible Mass Distribution on Different Scales in the Universe Exploring Properties of Dark and Visible Mass Distribution on Different Scales in the Universe

2004-10-22

arxiv.org/abs/astro-ph/0410524v1

Int.J.Mod.Phys. A20 (2005) 3124

Astronomy and Astrophysics

Astrophysics

presented at the DPF2004 meeting in Riverside, CA; to be published in a supplement in International Journal of Modern Physics

Scientific paper

10.1142/S0217751X05025929

In this short note we discuss recent observation of linear correlation on log-log scale between distribution of dark and visible mass in gravitationally bound systems. The coefficient of such correlation appears to be essentially the same for various systems of dramatically different scales such as spiral galaxies of different luminosities and galaxy clusters. We briefly touch possible interpretations of this observation and implications for the mass of dark matter particle.

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