𝔖 Bobbio Scriptorium
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Direct N-body simulations

✍ Scribed by Rainer Spurzem


Book ID
104339029
Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
385 KB
Volume
109
Category
Article
ISSN
0377-0427

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✦ 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.


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