Investigation of Dynamical Chaotization in Stellar Systems with Double Massive Centers Using the Ricci Curvature Criterion

Details Investigation of Dynamical Chaotization in Stellar Systems with Double Massive Centers Using the Ricci Curvature Criterion Investigation of Dynamical Chaotization in Stellar Systems with Double Massive Centers Using the Ricci Curvature Criterion

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000astl...26..806b&link_type=abstract

Astronomy Letters, vol. 26, p. 806-808 (2000)

Astronomy and Astrophysics

Astronomy

Dynamical Instability, Gravitating Systems

Scientific paper

The Ricci curvature criterion is used to investigate the relative instability of various configurations of N-body gravitational systems. Systems with double massive centers are shown to be less stable than homogeneous systems or systems with single massive centers. In general, this is a confirmation that the Ricci curvature criterion is efficient in studying N-body systems by means of relatively simple computations.

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