Fig. 3

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Contour plot of the number of BBH mergers (solid blue lines and associated labels) in the two planes summarizing the effects of the main parameter dependence: initial half-mass radius versus initial stellar mass (by assuming a primordial binary fraction of 10%; left panel), and primordial binary fraction versus average initial density within rh (by assuming an initial stellar mass of 3 × 106 M⊙; right panel). The dashed red lines and the corresponding red labels show the contour plot of the ratio between the number of dynamical to primordial BBH mergers.
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