Astronomy and Astrophysics – Astrophysics
Scientific paper
1995-11-20
Astronomy and Astrophysics
Astrophysics
uuencoded gzip compressed postscript file containing 14 pages, accepted for publication in MNRAS
Scientific paper
We have performed a series of high resolution N-body experiments on a Connection Machine CM-5 in order to study the stability of collisionless self-gravitating spherical systems. We interpret our results in the framework of symplectic mechanics, which provides the definition of a new class of particular perturbations: The preserving perturbations, which are a generalization of the radial ones. Using models defined by the Ossipkov-Merritt algorithm, we show that the stability of a spherical anisotropic system is directly related to the preserving or non-preserving nature of the perturbations acting on the system. We then generalize our results to all spherical systems. Since the ``isotropic component'' of the linear variation of the distribution function cannot be used to predict the stability or instability of a spherical system, we propose a more useful stability parameter which is derived from the ``anisotropic'' component of the linear variation.
Alimi Jean--Michel
Aly Jean-Jacques
Pérez Jeremy
Scholl Hans
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