Characterizing the Substructure of Dark Matter Halos
<p>Hierarchical structure formation in the standard Λ+cold dark matter (CDM) model produces gravitationally bound clumpy halos with abundant substructure. These subhalos are the remnants of dark matter halos that have been accreted by their host halo over cosmic time, and have survi...
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| Language: | EN |
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Yale University
2017
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| Online Access: | http://pqdtopen.proquest.com/#viewpdf?dispub=10584949 |