Understanding the Phase-space Structure of Simulated Dark Matter Halos

Details Understanding the Phase-space Structure of Simulated Dark Matter Halos Understanding the Phase-space Structure of Simulated Dark Matter Halos

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.2803b&link_type=abstract

American Astronomical Society, AAS Meeting #211, #28.03; Bulletin of the American Astronomical Society, Vol. 39, p.778

Astronomy and Astrophysics

Astronomy

Scientific paper

N-body simulations of dark matter halos present a number of characteristics that appear time and again; e.g., dual power-law density profiles. However, no explanation for these characteristics has been widely accepted. We are investigating a "thermodynamic'" approach to this issue using global properties that will shed light on the relationships observed in simulations.
This material is based upon work supported by NASA under Grant #NNX07AG86G issued through the Science Mission Directorate.

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