Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-25T16:55:46.066Z Has data issue: false hasContentIssue false

Integration Methods where Force is Obtained from the Smoothed Gravitational Field

Published online by Cambridge University Press:  12 April 2016

Frank Hohl*
Affiliation:
NASA, Langley Research Center, Hampton, Va.

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.

Many problems in stellar dynamics involve phenomena occurring in inhomogeneous systems in which the interaction between the particles is fully described by a self-consistent field operating in phase space. Because the particles interact by means of the long-range Coulomb force, each particle is under the simultaneous influence of a large number of other particles. Therefore, stellar systems will respond to any perturbation in a collective manner, and a study of such systems is concerned essentially with the N-body problem.

Type
Research Article
Copyright
Copyright © Reidel 1971

References

Cooley, J. W. and Tukey, J. W.: 1965, Math. Comput. 19, 297.Google Scholar
Hockney, R. W.: 1967, Astrophys. J. 150, 797.Google Scholar
Hockney, R. W.: 1968, Publ. Astron. Soc. Pacific 80, 662.Google Scholar
Hockney, R. W. : 1970, in Methods in Computational Physics, 9, 135, Academic Press Inc., New York.Google Scholar
Hockney, R. W. and Hohl, F.: 1969, Astron. J. 74, 1102.CrossRefGoogle Scholar
Hohl, F.: 1968, Bull. Astron. 3, 227.Google Scholar
Hohl, F.: 1969, ‘Computer Simulation of a Cylindrical Galaxy’, NASA TN D-5200.Google Scholar
Hohl, F. : 1970a, in Becker, W. and Contopoulos, G. (eds.), ‘The Spiral Structure of our Galaxy’, I.A.U. Symp. 38, 368.Google Scholar
Hohl, F.: 1970b, ‘Dynamics of Disk Galaxies’, NASA TR R-343.Google Scholar
Hohl, F.: 1970c, Astron. J. 16, 202.Google Scholar
Hohl, F. and Hockney, R. W.: 1969, J. Comput. Phys. 4, 306.Google Scholar
Lindblad, P. O.: 1960, Stockholm Obser. Ann. 21, 3.Google Scholar
Miller, R. H.: 1970, J. Comput. Phys. 6, 449.Google Scholar
Miller, R. H. and Prendergast, K. H.: 1968, Astrophys. J. 151, 699.Google Scholar
Miller, R. H., Prendergast, K. H., and Quirk, W. J.: 1970, Astrophys. J. 161, 903.Google Scholar