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Million-Body Star Cluster Simulations: Comparisons between Monte Carlo and Direct -body
Carl L. Rodriguez, Meagan Morscher, Long Wang +3
We present the first detailed comparison between million-body globular cluster simulations computed with a Hénon-type Monte Carlo code, CMC, and a direct -body code, NBODY6++GPU…
A New Hybrid Technique for Modeling Dense Star Clusters
Carl L. Rodriguez, Bharath Pattabiraman, Sourav Chatterjee +4
The "gravitational million-body problem," to model the dynamical evolution of a self-gravitating, collisional N-body system with ~10^6 particles over many relaxation times, remains…
Inadequacies of the Fisher Information Matrix in gravitational-wave parameter estimation
Carl L. Rodriguez, Benjamin Farr, Will M. Farr +1
The Fisher Information Matrix (FIM) has been the standard approximation to the accuracy of parameter estimation on gravitational-wave signals from merging compact binaries due to i…