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- W1548200072 abstract "The classical formulation of the gravitational N-body problem is deceptively simple. Given initial values of N masses, coordinates and velocities, the task is to calculate the future orbits. Although the motions are in principle completely determined by the underlying differential equations, accurate solutions can only be obtained by numerical methods. Self-gravitating stellar systems experience highly complicated interactions, which require efficient procedures for studying the long-term behaviour." @default.
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- W1548200072 date "2008-01-01" @default.
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- W1548200072 title "Direct N-Body Codes" @default.
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- W1548200072 doi "https://doi.org/10.1007/978-1-4020-8431-7_1" @default.
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