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• W1545806369 abstract "In this chapter, I explain how the evolution of an N-body system can be described using a formalism explicitly based on the distribution function in phase space. Such an approach can be contrasted with direct N-body simulations in which the trajectories of a large number of particles are integrated. Because trajectories with close initial conditions diverge exponentially in gravitational N-body systems (Goodman et al. 1993; Hemsendorf & Merritt 2002, and references therein), most results of N-body simulations must be interpreted statistically. It is therefore interesting to consider the simulation methods that treat the gravitational system in an explicitly statistical way." @default.
• W1545806369 created "2016-06-24" @default.
• W1545806369 creator A5022615067 @default.
• W1545806369 date "2008-01-01" @default.
• W1545806369 modified "2023-09-26" @default.
• W1545806369 title "Fokker–planck Treatment of Collisional Stellar Dynamics" @default.
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• W1545806369 doi "https://doi.org/10.1007/978-1-4020-8431-7_4" @default.
• W1545806369 hasPublicationYear "2008" @default.
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