I performed analysis of dark matter halo data from the Millennium II simulation and
t the resulting energy and density distributions to the predictions of the DARKexp
model. For halos near virial equilibrium, I found DARKexp to t the simulated data
well, supporting it as a theoretical model for the distribution of matter in galaxies. I
also discuss the methods of data analysis and the Markov Chain Monte Carlo method
used for fitting.
Fitting DARKexp predictions to dark matter halo profiles from simulation.
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