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Numerical Experiments on Pair Correlations and on ‘Thermodynamics’

  • R. H. Miller
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 31)

Abstract

A ‘conventional’ n-body calculation was constructed to carry out a number of numerical experiments on small stellar systems. Two of these experiments will be reported here, although something of the others will creep in. All these experiments refer to a 32-body system, in which the equations of motion were handled ‘exactly’, with the usual checks on constancy of the ten first integrals of motion. Because the emphasis was on the experiments, the calculation was constructed without particular attention to running speed or minimum storage requirements. Otherwise, the calculation was quite conventional.

Keywords

Pair Correlation Stellar System Virial Theorem Included Angle Initial Kinetic Energy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Larson, R. B.: 1970, Monthly Notices Roy. Astron. Soc. 147, 323.ADSGoogle Scholar
  2. Lynden-Bell, D. and Wood, R.: 1968, Monthly Notices Roy. Astron. Soc. 138, 495.ADSGoogle Scholar
  3. Miller, R. H.: 1966, in G. Contopoulos (ed.), ‘Theory of Orbits in the Solar System and in Stellar Systems‘, IA U Symp. 25, 137.Google Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1972

Authors and Affiliations

  • R. H. Miller
    • 1
  1. 1.University of ChicagoUSA

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