NASA NTRS · 19720044254
Integration methods where force is obtained from the smoothed gravitational field.
Abstract
Discussion of the application of computer models to collisionless stellar systems. Two more recent computer models - i.e., the two-dimensional rod model, and the model for disks of stars - are described. It is shown that the dynamics of collisionless stellar systems can be studied by representing the system by large numbers of representative stars.
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Hohl, F.. 1972-01-01. Integration methods where force is obtained from the smoothed gravitational field.. https://ntrs.nasa.gov/citations/19720044254
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