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Modelling ultra-fine structure in dark matter halos · Around

2008

Modelling ultra-fine structure in dark matter halos

Fantin, Daniele S. M., Merrifield, Michael R., Green, Anne M.

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Various laboratory-based experiments are underway attempting to detect dark matter directly.

The event rates and detailed signals expected in these experiments depend on the dark matter phase space distribution on sub-milliparsec scales.
These scales are many orders of magnitude smaller than those that can be resolved by conventional N-body simulations, so one cannot hope to use such tools to investigate the effect of mergers in the history of the Milky Way on the detailed phase-space structure probed by the current experiments.
In this paper we present an alternative approach to investigating the results of such mergers, by studying a simplified model for a merger of a sub-halo with a larger parent halo.

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