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Monte Carlo modelling of cometary dynamics
Authors:Claude Froeschlé  Hans Rickman
Institution:(1) Observatoire de Nice, B.P. 139, F-06003 Nice Cedex, France;(2) Astronomiska Observatoriet, Box 515, S-75120 Uppsala, Sweden
Abstract:Monte Carlo simulations can either be viewed as a numerical method for solving evolutionary equations or as a way for statistically modelling the outcome of chaotic dynamical systems. Thus they are well suited for treating many aspects of cometary dynamics. We present a critical review of past applications of Monte Carlo simulations for both long- and short-period comets indicating the strength and weaknesses of the methods with suggestions for future applications.
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