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2020

Black Hole Mergers from Hierarchical Triples in Dense Star Clusters

Martinez, Miguel A. S., Fragione, Giacomo, Kremer, Kyle et al.

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Hierarchical triples are expected to be produced by the frequent binary-mediated interactions in the cores of globular clusters.

In some of these triples, the tertiary companion can drive the inner binary to merger following large eccentricity oscillations, as a result of the eccentric Kozai-Lidov mechanism.
In this paper, we study the dynamics and merger rates of black hole (BH) hierarchical triples, formed via binary--binary encounters in the CMC Cluster Catalog, a suite of cluster simulations with present-day properties representative of the Milky Way's globular clusters.
We compare the properties of the mergers from triples to the other merger channels in dense star clusters, and show that triple systems do not produce significant differences in terms of mass and effective spin distribution.

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