activity
20082023
most citedKolmogorov and Nekhoroshev theory for the problem of three bodies

57 citations · 302 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.EP2023★ 5 cited

Secular orbital dynamics of the innermost exoplanet of the -Andromedæ system

Rita Mastroianni, Ugo Locatelli

We introduce a quasi-periodic restricted Hamiltonian to describe the secular motion of a small-mass planet in a multi-planetary system. In particular, we refer to the motion of $\u…

math-ph2023★ 2 cited

Existence proof of librational invariant tori in an averaged model of HD60532 planetary system

Veronica Danesi, Ugo Locatelli, Marco Sansottera

We investigate the long-term dynamics of HD60532, an extrasolar system hosting two giant planets orbiting in a 3:1 mean motion resonance. We consider an average approximation at or…

astro-ph.EP2022★ 3 cited

A numerical criterion evaluating the robustness of planetary architectures; applications to the Andromedæ system

Ugo Locatelli, Chiara Caracciolo, Marco Sansottera +1

We revisit the problem of the existence of KAM tori in extrasolar planetary systems. Specifically, we consider the Andromedæ system, by modelling it with a three-body pr…

math-ph2022

Invariant KAM tori: from theory to applications to exoplanetary systems

Ugo Locatelli, Chiara Caracciolo, Marco Sansottera +1

We consider the classical problem of the construction of invariant tori exploiting suitable Hamiltonian normal forms. This kind of approach can be translated by means of the Lie se…

math.DS2021★ 8 cited

Librational KAM tori in the secular dynamics of the Andromedæ planetary system

Chiara Caracciolo, Ugo Locatelli, Marco Sansottera +1

We study the planetary system of ~Andromedæ, considering the three-body problem formed by the central star and the two largest planets, ~And~\emph{c} and $\upsi…

math-ph2021★ 11 cited

Computer-assisted estimates for Birkhoff normal forms

Chiara Caracciolo, Ugo Locatelli

Birkhoff normal forms are commonly used in order to ensure the so called "effective stability" in the neighborhood of elliptic equilibrium points for Hamiltonian systems. From a th…