Abstract
The chaos in stellar systems is studied using the theory of dynamical systems and the Van Kampen stochastic differential equation approach. The exponential instability (chaos) of spherical N-body gravitating systems, already known previously, is confirmed. The characteristic timescale of that instability is estimated confirming the collective relaxation time obtained by means of the Maupertuis principle. © 2009 ESO.
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APA
Gurzadyan, V. G., & Kocharyan, A. A. (2009). Collective relaxation of stellar systems revisited. Astronomy and Astrophysics, 505(2), 625–627. https://doi.org/10.1051/0004-6361/200912218
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