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2018

Black hole mergers from an evolving population of globular clusters

Fragione, Giacomo, Kocsis, Bence

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The high rate of black hole (BH) mergers detected by LIGO/Virgo opened questions on their astrophysical origin.

One possibility is the dynamical channel, in which binary formation and hardening is catalyzed by dynamical encounters in globular clusters (GCs).
Previous studies have shown that the BH merger rate from the present day GC density in the Universe is lower than the observed rate.
In this \textit{Letter}, we study the BH merger rate by accounting for the first time for the evolution of GCs within their host galaxies.

Black hole mergers from an evolving population of globular clusters · Around

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