Detection for intermediate-mass binary black holes in population III star clusters with TianQin

Open Access

Fig. 2.

Distribution of the merger numbers of IMBBHs from 168 N-body simulations. Solid lines represent f_b = 0 (orange) and f_b = 1 (blue), respectively. ${\bar{n}}_{0} \approx 0.2$ $\bar{n}_0 \approx 0.2$ and ${\bar{n}}_{1} \approx 1.2$ $\bar{n}_1 \approx 1.2$ are average numbers of IMBBH mergers for the two scenarios.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.