| http://www.w3.org/ns/prov#value | - Finally, we comment on other aspects of our simulations, such as comparisons to existing merging clusters; and the mixing of the intracluster medium due to merging, and resulting cluster entropy and cooling time profiles.Structure Formation in Braneworld CosmologyJune 12, 2009 | AAC 123 | 1:30 PM | Scott Dodelson, Angela V. OlintoFabian SchmidtWe perform cosmological N-body simulations of the Dval
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