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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…
Survival of non-coplanar, closely-packed planetary systems after a close encounter
David R. Rice, Frederic A. Rasio, Jason H. Steffen
Planetary systems with more than two bodies will experience orbital crossings at a time related to the initial orbital separations of the planets. After a crossing, the system ente…
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…
MeerTime - the MeerKAT Key Science Program on Pulsar Timing
M. Bailes, E. Barr, N. D. R. Bhat +28
The MeerKAT telescope represents an outstanding opportunity for radio pulsar timing science with its unique combination of a large collecting area and aperture efficiency (effectiv…
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…