A new hybrid technique for modeling dense star clusters

A new hybrid technique for modeling dense star clusters

The "gravitational million-body problem," to model the dynamical evolution of a self-gravitating, collisional N-body system with ∼106 particles over many relaxation times, remains a major challenge in computational astrophysics. Unfortunately, current techniques to model such systems suffe...

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Bibliographic Details
Main Authors: Pattabiraman, Bharath (Author), Chatterjee, Sourav (Author), Choudhary, Alok (Author), Liao, Wei-keng (Author), Morscher, Meagan (Author), Rasio, Frederic A (Author), Rodriguez, Carl L. (Author), Rasio, Frederic A. (Author), Rodriguez, Carl (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Springer International Publishing, 2018-11-29T16:25:56Z.
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