Spectral stability, spectral flow and circular relative equilibria for the Newtonian n-body problem
نویسندگان
چکیده
For the Newtonian (gravitational) n-body problem in Euclidean d-dimensional space, d≥2, simplest possible periodic solutions are provided by circular relative equilibria, (RE) for short, namely which each body rigidly rotates about center of mass and configuration whole system is constant time central (or, more generally, balanced) configuration. d≤3, only planar, but dimension four it to get truly dimensional (RE). A classical celestial mechanics aims at relating (in-)stability properties a index generating it. In this paper, we provide sufficient conditions that imply spectral instability planar non-planar R4 generated configuration, thus answering some questions raised [14, Page 63]. As corollary, retrieve result Hu Sun [11] on linear whose non-degenerate has odd Morse index, fix gap statement [6, Theorem 1] (possibly degenerate) index. The key ingredient new formula independent interest allows compute flow path symmetric matrices having degenerate starting point, symplectic decomposition phase space linearized Hamiltonian along given inspired Meyer Schmidt's [13] us rule out uninteresting part dynamics corresponding translational (partially) rotational symmetry problem.
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ژورنال
عنوان ژورنال: Journal of Differential Equations
سال: 2022
ISSN: ['1090-2732', '0022-0396']
DOI: https://doi.org/10.1016/j.jde.2022.07.032