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 suffer from sev...

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Bibliographic Details
Main Authors: Pattabiraman, Bharath, Chatterjee, Sourav, Choudhary, Alok, Liao, Wei-keng, Morscher, Meagan, Rasio, Frederic A, Rodriguez, Carl L., Rasio, Frederic A., Rodriguez, Carl
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: Springer International Publishing 2018
Online Access:http://hdl.handle.net/1721.1/119368

Internet

http://hdl.handle.net/1721.1/119368

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