activity
20172022
most citedEqual masses Eulerian relative equilibria on a rotating meridian of S^2

1 citations · 1 across the 2 of their papers we have counts for

collaborators

6 papers

math.CA20221 cited

Equal masses Eulerian relative equilibria on a rotating meridian of S^2

Toshiaki Fujiwara, Ernesto Pérez-Chavela

Relative equilibria on a rotating meridian on in equal-mass three-body problem under the cotangent potential are determined. We show the existence of scalene and iso…

math.DS2021

Bifurcation of closed orbits from equilibria of Newtonian systems with Coriolis forces

Anna Gołȩbiewska, Ernesto Pérez-Chavela, Sławomir Rybicki +1

We consider autonomous Newtonian systems with Coriolis forces in two and three dimensions and study the existence of branches of periodic orbits emanating from equilibria. We inves…

math.DS2020

Continuation of relative equilibria in the --body problem to spaces of constant curvature

Abimael Bengochea, Carlos García-Azpeitia, Ernesto Pérez-Chavela +1

We prove that all non-degenerate relative equilibria of the planar Newtonian --body problem can be continued to spaces of constant curvature , positive or negative, for small…

math.DS2019

Regularization of the restricted -body problem on curved spaces

Ernesto Pérez-Chavela, Juan Manuel Sánchez-Cerritos

We consider bodies moving under their mutual gravitational attraction in spaces with constant Gaussian curvature . In this system, primary bodies with equal masses f…

math.CA2018

Symmetric Liapunov center theorem for orbit with nontrivial isotropy group

Marta Kowalczyk, Ernesto Pérez-Chavela, Sławomir Rybicki

In this article we prove two versions of the Liapunov center theorem for symmetric potentials. We consider a~second order autonomous system in the pres…

math.DS2017

Stability interchanges in a curved Sitnikov problem

Luis Franco-Pérez, Marian Gidea, Mark Levi +1

We consider a curved Sitnikov problem, in which an infinitesimal particle moves on a circle under the gravitational influence of two equal masses in Keplerian motion within a plane…