Scale invariance of dark matter clustering

Details Scale invariance of dark matter clustering Scale invariance of dark matter clustering

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..905...23g&link_type=abstract

FRONTIERS OF FUNDAMENTAL PHYSICS: Eighth International Symposium FFP8. AIP Conference Proceedings, Volume 905, pp. 23-26 (2007)

Physics

Galaxy Clusters, Systems Obeying Scaling Laws, Dark Matter, Fractals

Scientific paper

The dark matter distribution is arguably scale invariant in a range of scales, so that it has a fractal geometry, observable in the clustering of galaxies and in cosmic voids. We review evidence of fractal geometry in recent observations, which shows, in particular, that a simple fractal model is not sufficient. Therefore, we propose a multifractal model of the dark matter distribution realized on fractal halo populations, in which voids appear naturally.

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