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

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004nuphs.134..121a&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 134, p. 121-123.

Physics

Nuclear Physics

Scientific paper

Laboratory experiments, large-scale computer simulations and observational cosmology have begun to make progress in the campaign to identify the particle responsible for gravitationally-inferred dark matter. We report results from an astrophysical program to measure dark matter particle properties. 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 cold dark matter cosmology.

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