Dark Matter Properties and the Structure of Galaxy Clusters

Details Dark Matter Properties and the Structure of Galaxy Clusters Dark Matter Properties and the Structure of Galaxy Clusters

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.8908a&link_type=abstract

American Astronomical Society Meeting 203, #89.08; Bulletin of the American Astronomical Society, Vol. 35, p.1349

Astronomy and Astrophysics

Astronomy

Scientific paper

Over the past decade, laboratory experiments, large-scale computer simulations and observational cosmology have begun to constrain the non-gravitational properties of dark matter particles, specifically their cross section for baryonic and self-interaction. We use a sample of carefully-selected, highly-relaxed galaxy clusters to constrain the strength of dark matter self-interaction. We also report structural parameters for this cluster sample, and discuss the implications for our understanding of large-scale structure formation.
This work was supported by SAO Grant AR3-4016X.

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