A numerical experiment in the problem of N rigid gravitating bodies

Details A numerical experiment in the problem of N rigid gravitating bodies A numerical experiment in the problem of N rigid gravitating bodies

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..189c&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Mar. 1980, p. 189-192.) Soviet Astronomy Letters, vol. 6, Mar.-Apr. 1980, p. 105, 10

Astronomy and Astrophysics

Astronomy

Gravitation, Many Body Problem, Rigid Structures, Rotating Bodies, Galactic Clusters, Numerical Integration

Scientific paper

The equations of translational-rotational motion of N gravitating aspherical rigid bodies are integrated numerically in order to study the growth of their rotational energy. At the starting time the bodies are not rotating. An experiment for six-body clusters indicates that over times t longer than the relaxation time the rotational energy will rise approximately as t-squared.

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