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20212024
most citedCoorbital homoclinic and chaotic dynamics in the Restricted 3-Body Problem

3 citations · 5 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2024

On the role of the fast oscillations in the secular dynamics of the lunar coplanar perturbation on Galileo satellites

Elisa Maria Alessi, Inmaculada Baldomá, Mar Giralt +2

Motivated by the practical interest in the third-body perturbation as a natural cleaning mechanism for high-altitude Earth orbits, we investigate the dynamics stemming from the sec…

math.DS2024

On the Arnold diffusion mechanism in Medium Earth Orbit

Elisa Maria Alessi, Inmaculada Baldomá, Mar Giralt +1

Space debris mitigation guidelines represent the most effective method to preserve the circumterrestrial environment. Among them, end-of-life disposal solutions play a key role. A…

math.DS2023★ 3 cited

Coorbital homoclinic and chaotic dynamics in the Restricted 3-Body Problem

Inmaculada Baldomá, Mar Giralt, Marcel Guardia

The description of unstable motions in the Restricted Planar Circular 3-Body Problem, modeling the dynamics of a Sun-Planet-Asteriod system, is one of the fundamental problems in C…

math.DS2023

Breakdown of homoclinic orbits to L3: Nonvanishing of the Stokes constant

Inmaculada Baldomá, Maciej J. Capiński, Mar Giralt +1

The Restricted Planar Circular 3-Body Problem models the motion of a body of negligible mass under the gravitational influence of two massive bodies, called the primaries, which pe…

math.DS2021

Breakdown of homoclinic orbits to L3 in the RPC3BP (I). Complex singularities and the inner equation

Inmaculada Baldomá, Mar Giralt, Marcel Guardia

The Restricted 3-Body Problem models the motion of a body of negligible mass under the gravitational influence of two massive bodies, called the primaries. If the primaries perform…

math.DS2021★ 2 cited

Breakdown of homoclinic orbits to L3 in the RPC3BP (II). An asymptotic formula

Inmaculada Baldomá, Mar Giralt, Marcel Guardia

The Restricted 3-Body Problem models the motion of a body of negligible mass under the gravitational influence of two massive bodies called the primaries. If one assumes that the p…