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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 3.

Joint mass–spin distributions for three successive time steps. Top: the spin amplitudes of the more massive merger component vs. their masses. Bottom: the effective spin parameter χeff vs. the binary chirp mass. The contours represent 90% and 99.9% contour intervals for mergers at time steps T = 0 (red), T = 1 (blue), and T = 2 (black).

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