The continuous transition of Hamiltonian vector fields through manifolds of constant curvature
Abstract
We ask whether Hamiltonian vector fields defined on spaces of constant Gaussian curvature (spheres, for >0, and hyperbolic spheres, for <0), pass continuously through the value =0 if the potential functions U, ∈ R, that define them satisfy the property 0U=U0, where U0 corresponds to the Euclidean case. We prove that the answer to this question is positive, both in the 2- and 3-dimensional cases, which are of physical interest, and then apply our conclusions to the gravitational N-body problem.
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