activity
20212026
most citedComputer-assisted estimates for Birkhoff normal forms

11 citations · 36 across the 8 of their papers we have counts for

collaborators

8 papers

math.DS2026

Improved stability estimates at elliptic equilibria of Hamiltonian systems

Massimiliano Guzzo, Chiara Caracciolo, Gabriella Pinzari

This paper deals with an improvement of the "a-priori stability bounds" on the variation of the action variables and on the stability time obtained from a given Birkhoff normal for…

math.DS2024

A parametrization algorithm to compute lower dimensional elliptic tori in Hamiltonian systems

Chiara Caracciolo, Jordi-Lluís Figueras, Alex Haro

We present an algorithm for the construction of lower dimensional elliptic tori in parametric Hamiltonian systems by means of the parametrization method with the tangent and normal…

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★ 6 cited

Normal form for lower dimensional elliptic tori in Hamiltonian systems

Chiara Caracciolo

We give a proof of the convergence of an algorithm for the construction of lower dimensional elliptic tori in nearly integrable Hamiltonian systems. The existence of such invariant…

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…