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Seeding supermassive black holes with a nonvortical dark-matter subcomponent

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Figure

FIG. 3 (color online). The scenario proposed in this paper is one in which black holes form in the IDM component at the center of any collapsing structure, and light black holes continue to merge into a heavier one in a larger-scale overdensity
FIG. 4 (color online). Abundance of halos (mass on bottom horizontal axis) and black hole seeds (mass on top horizontal axis) in a Hubble volume ðc=H 0 Þ 3 for  I F ¼ 10 7 for various values of redshift and mass

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