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Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries
Carl L. Rodriguez, Pau Amaro-Seoane, Sourav Chatterjee +5
Using state-of-the-art dynamical simulations of globular clusters, including radiation reaction during black hole encounters and a cosmological model of star cluster formation, we…
Post-Newtonian Dynamics in Dense Star Clusters: Binary Black Holes in the LISA Band
Kyle Kremer, Carl L. Rodriguez, Pau Amaro-Seoane +8
The dynamical processing of black holes in the dense cores of globular clusters (GCs), makes them efficient factories for producing binary black holes (BBHs). Here we explore the p…
How initial size governs core collapse in globular clusters
Kyle Kremer, Sourav Chatterjee, Claire S. Ye +2
Globular clusters (GCs) in the Milky Way exhibit a well-observed bimodal distribution in core radii separating the so-called "core-collapsed" and "non-core-collapsed" clusters. Her…
How black holes shape globular clusters: Modeling NGC 3201
Kyle Kremer, Claire S. Ye, Sourav Chatterjee +2
Numerical simulations have shown that black holes (BHs) can strongly influence the evolution and present-day observational properties of globular clusters (GCs). Using a Monte Carl…
Low-mass X-ray binaries ejected from globular clusters
Kyle Kremer, Sourav Chatterjee, Carl L. Rodriguez +1
We explore the population of mass-transferring binaries ejected from globular clusters (GCs) with both black hole (BH) and neutron star (NS) accretors. We use a set of 137 fully ev…
LISA sources in Milky Way globular clusters
Kyle Kremer, Sourav Chatterjee, Katelyn Breivik +3
We explore the formation of double-compact-object binaries in Milky Way (MW) globular clusters (GCs) that may be detectable by the Laser Interferometer Space Antenna (LISA). We use…