There is increasing evidence that many kilometer-sized bodies in the Solar System are piles of rubble bound together by gravity. We present results from a project to map the parameter space of collisions between kilometer-sized spherical rubble piles. The results will assist in parameterization of c
Direct N-body simulations
β Scribed by Rainer Spurzem
- Book ID
- 104339029
- Publisher
- Elsevier Science
- Year
- 1999
- Tongue
- English
- Weight
- 385 KB
- Volume
- 109
- Category
- Article
- ISSN
- 0377-0427
No coin nor oath required. For personal study only.
β¦ Synopsis
Special high-accuracy direct force summation N -body algorithms and their relevance for the simulation of the dynamical evolution of star clusters and other gravitating N -body systems in astrophysics are presented, explained and compared with other methods. Other methods means here approximate physical models based on the Fokker-Planck equation as well as other, approximate algorithms to compute the gravitational potential in N -body systems. Questions regarding the parallel implementation of direct "brute force" N -body codes are discussed. The astrophysical application of the models to the theory of relaxing rotating and non-rotating collisional star clusters is presented, brie y mentioning the questions of the validity of the Fokker-Planck approximation, the existence of gravothermal oscillations and of rotation and primordial binaries.
π SIMILAR VOLUMES
We present a qualitative diagnostic based on the continuous wavelet transform, for the detection of irregular behaviour in time series of particle simulations. We apply the method to three qualitatively different gravitational 3-body encounters. The intrinsic irregular behaviour of these encounters