c-M relation of the sub-galactic dark matter halos and the effect of the cusp-to-core transition
Approach
The Phi-4096 N-body simulation is used to measure subhalo concentrations and masses and compare their relation with established cold-dark-matter predictions.
Main result
The inferred relation agrees with a previously proposed relation spanning very small to galactic scales. The study connects it with observed halo properties from dwarf galaxies to clusters.
Scientific implications
The concentration–mass framework gives testable predictions for the density structure of Milky Way subhaloes and context for cusp-to-core transformations.
Scope and limitations
This is an IAU symposium poster paper. Its predictions concern simulated halo structure and require observational tests.