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math-ph2024
Bifurcation sequences in the secular 3D planetary 3-Body problem: a geometric approach
Rita Mastroianni, Antonella Marchesiello, Christos Efthymiopoulos +1
We implement the geometric method proposed in ([9], [3], [16]) to analytically predict the sequence of bifurcations leading to a change of stability and/or the appearance of new pe…
math-ph2023
Computer-assisted proofs of existence of KAM tori in planetary dynamical models of -And
Rita Mastroianni, Ugo Locatelli
We reconsider the problem of the orbital dynamics of the innermost exoplanet of the -Andromedae system (i.e., -And ) into the framework of a Secular…
math-ph2022★ 1 cited
Kolmogorov algorithm for isochronous Hamiltonian systems
Rita Mastroianni, Christos Efthymiopoulos
We present a Kolmogorov-like algorithm for the computation of a normal form in the neighborhood of an invariant torus in `isochronous' Hamiltonian systems, i.e., systems with Hamil…