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Black Hole Coagulation: Modeling Hierarchical Mergers in Black Hole Populations

  • Authors: Z. Doctor, D. Wysocki, R. O'Shaughnessy, D. E. Holz, and B. Farr

2020 The Astrophysical Journal 893 35.

  • Provider: AAS Journals

Caption: Figure 2.

The total mass distribution of BBH mergers at three successive time steps evolving from a Salpeter natal distribution (α = 2.35) with coupling parameters a = 2 and b = 0. The smooth curves overlaid on the histograms are kernel density estimates of the Monte Carlo samples and are shown purely to guide the eye.

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