Hostname: page-component-77c89778f8-fv566 Total loading time: 0 Render date: 2024-07-20T23:30:48.010Z Has data issue: false hasContentIssue false
  • English
  • Français

A Method for Solving Poisson's Equation for Systems with Axial Symmetry

Published online by Cambridge University Press:  14 August 2015

T. S. Van Albada
T. S. Van Albada*
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In computer experiments on the dynamics of stellar systems special methods are often required for the computation of the forces to keep the problem manageable. For collisionless systems a method based on solving Poisson's equation with Fourier-series expansions has been used with success (Miller et al., 1970; Hohl, 1973). The systems in these studies consist of a large number of particles moving on a rectangular grid.

Type
Part II/Flattened Systems
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 205 - 206
Copyright
Copyright © Reidel 1975 

References

Gott, J. R.: 1973. Astrophys. J. 186, 481.CrossRefGoogle Scholar
Hohl, F.: 1973, Astrophys. J. 184, 353.CrossRefGoogle Scholar
Miller, R. H., Prendergast, K. H., and Quirk, W. J.: 1970, Astrophys. J. 161, 903.CrossRefGoogle Scholar
Prendergast, K. H. and Tomer, E.: 1970, Astron. J. 75, 674.CrossRefGoogle Scholar