Introducing a new multi-particle collision method for the evolution of dense stellar systems

@article{Cintio2021IntroducingAN,
  title={Introducing a new multi-particle collision method for the evolution of dense stellar systems},
  author={Pierfrancesco di Cintio and Mario Pasquato and Alicia Simon-Petit and Suk-Jin Yoon},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Context. Stellar systems are broadly divided into collisional and non-collisional categories. While the latter are large-N systems with long relaxation timescales and can be simulated disregarding two-body interactions, either computationally expensive direct N-body simulations or approximate schemes are required to properly model the former. Large globular clusters and nuclear star clusters, with relaxation timescales of the order of a Hubble time, are small enough to display some collisional… 

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