Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-20T11:46:37.508Z Has data issue: false hasContentIssue false
  • English
  • Français

The Monte Carlo Method

Published online by Cambridge University Press:  12 April 2016

M. Hénon
M. Hénon*
Affiliation:
Observatoire de Nice

Abstract

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.

We give here a detailed technical description of a Monte Carlo scheme for the dynamical evolution of spherical stellar systems. The philosophy of the method, as well as a few illustrative results, are given elsewhere (Hénon, 1971, hereafter called I).

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 10: Gravitational N-Body Problem , November 1971 , pp. 151 - 167
Copyright
Copyright © Reidel 1971

References

Chandrasekhar, S.: 1942, Principles of Stellar Dynamics, Dover Publications.Google Scholar
Contopoulos, G.: 1954, Z. Astrophys. 35, 67.Google Scholar
Coveyou, R. R. and Macpherson, R. D.: 1967, J. Ass. Comput. Mach. 14, 100.CrossRefGoogle Scholar
Hammersley, J. M. and Handscomb, D. C.: 1964, Monte Carlo Methods, Methuen, London.CrossRefGoogle Scholar
Hayli, A.: 1970, Astron. Astrophys. 7, 17.Google Scholar
Hénon, M.: 1958, Ann. Astrophys. 21, 186.Google Scholar
Hénon, M.: 1960, Ann. Astrophys. 23, 668.Google Scholar
Hénon, M. : 1966, Compt. Rend. Acad. Sci. Paris 262, 666.Google Scholar
Hénon, M.: 1971, Astrophys. Space Sci. 13, 284.CrossRefGoogle Scholar
van Albada, T. S.: 1968, Bull. Astron. Inst. Neth. 19, 479.Google Scholar
von Hoerner, S.: 1958, Z. Astrophys. 44, 221.Google Scholar