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A hierarchical O(N log N) force-calculation algorithm
TLDR
Gravitational N-body Simulations
Gravitational N-body simulations, that is numerical solutions of the equations of motions for N particles interacting gravitationally, are widely used tools in astrophysics, with applications from…
Formation of massive black holes through runaway collisions in dense young star clusters
- S. Zwart, H. Baumgardt, P. Hut, J. Makino, S. McMillan
- PhysicsNature
- 26 February 2004
TLDR
HOP: A New group finding algorithm for N body simulations
- D. Eisenstein, P. Hut
- Computer Science
- 16 December 1997
TLDR
Dynamical Formation of Close Binary Systems in Globular Clusters
We know from observations that globular clusters are very efficient catalysts in forming unusual short-period binary systems or their offspring, such as low-mass X-ray binaries (LMXBs; neutron stars…
Star cluster ecology-IV. Dissection of an open star cluster: photometry
- S. Zwart, S. McMillan, P. Hut, J. Makino
- Physics
- 11 May 2000
The evolution of star clusters is studied using N-body simulations in which the evolution of single stars and binaries is taken self-consistently into account. Initial conditions are chosen to…
Binary-single star scattering. I: Numerical experiments for equal masses
- P. Hut, J. Bahcall
- Physics
- 1 May 1983
The Lives and Deaths of Star Clusters near the Galactic Center
- S. Zwart, J. Makino, S. McMillan, P. Hut
- Physics
- 14 February 2001
We study the evolution and observability of young, compact star clusters near the Galactic center, such as the Arches and Quintuplet systems. The clusters are modeled by integrating the equations of…
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