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Simulations, Data Analysis and Algorithms

Computational Astrophysics and Cosmology Cover Image
Figure 3 | Computational Astrophysics and Cosmology

Figure 3

From: A new hybrid technique for modeling dense star clusters

Figure 3

Flowchart of the RAPID Code—After the hybridization is initialized, the BHs are transferred to the Kira process, while the remaining Monte Carlo processes sample the orbital positions of the remaining stars. The communication between the Kira process and the CMC process(es) is handled by an extension of the MPI scheme developed in CMC (Pattabiraman et al. 2013), while the N-body process can be run in serial or with OpenMP threading

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