During the nineteenth century one of the main concerns in mechanics was to solve Hamiltonian systems by quadrature in terms of elliptic and hyperelliptic functions. The vein of research, abandoned for nearly a century, was entirely revived by the recent findings about the Korteweg—de Vries equation. They shed new light and perspective onto problems of finite-dimensional mechanics, which has led to effective and systematic methods for deciding about the complete integrability of Hamiltonian systems. T he problems that can be captured by these methods have the common virtue that, when run with complex time, most (complex) trajectories are dense on complex algebraic tori; such a system is called algebraically completely integrable, which is stronger than the customary notion of analytic integrability. Many old and new systems enjoy this property and, in particular, a wide variety of systems that occur in the context of orbits in Kac—Moody Lie algebras. This paper explains how the behaviour at the ‘ blow-up ’ time of the solutions to the differential equations enables one to decide about their integrability and also how to derive precise information about the invariant surfaces of the system.
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