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Numerical simulations have shown that black holes (BHs) can stronglyinfluence the evolution and present-day observational properties of globularclusters (GCs). Using a Monte Carlo code, we construct GC models that match theMilky Way (MW) cluster NGC 3201, the first cluster in which a stellar-mass BHwas identified through radial-velocity measurements. We predict that NGC 3201contains $\gtrsim 200$ stellar-mass BHs. Furthermore, we explore the dynamicalformation of main sequence-BH binaries and demonstrate that systems similar tothe observed BH binary in NGC 3201 are produced naturally. Additionally, ourmodels predict the existence of bright blue-straggler-BH binaries unique tocore-collapsed clusters, which otherwise retain few BHs.

How black holes shape globular clusters: Modeling NGC 3201