Binary-single interactions with different mass ratios - Implications for gravitational waves from globular clusters

Open Access

Fig. 5

Left: P_cap as a function of q₂ and q₃. Right: P_cap as a function of q₂/q₃. For that, we used m₁ = 45 m_⊙, a = a_GW, and assumed a metal-poor cluster with M_cl = 5 × 10⁵ m_⊙ and r_h = 1 pc. The error bars are computed via $\sqrt{2 N_{cap}} / N_{bin}$ $\sqrt{2N_{\rm cap}}/N_{\rm bin}$ , with N_bin the number of resonant events in the bin, and N_cap the number of GW captures among them.

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