For the 3-body problem in R^4, three families of relative equilibria are local minima of the reduced Hamiltonian when the angular momentum is close to the 3-dimensional case, implying stable bounded motions.
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Symmetry reduction of the 3-body problem in $\mathbb{R}^4$
For the 3-body problem in R^4, three families of relative equilibria are local minima of the reduced Hamiltonian when the angular momentum is close to the 3-dimensional case, implying stable bounded motions.