Abstract
The effective relaxation of one-dimensional gravitational systems towards micro-canonical equilibrium is demonstrated in a series of computer experiments, the Kolmogorov-Smirnov goodness of fit test being used to give a measure of the evolution of the distribution function. The relaxation timescalet R is shorter thanNt C, and thus much shorter than the generally accepted estimatet R∼N 2tC,N being the number of particles in the system andt C a characteristic dynamical time.
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Luwel, M., Severne, G. & Rousseeuw, P.J. Numerical study of the relaxation of one-dimensional gravitational systems. Astrophys Space Sci 100, 261–277 (1984). https://doi.org/10.1007/BF00651601
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DOI: https://doi.org/10.1007/BF00651601