The N–Body Problem, Old and New

Location

San Cristobal de las Casas
,
Mexico

Dates

to

Presentation

The school aims to introduce graduate students and young re- searchers to the new trends in Hamiltonian systems and celestial mechanics. To this end, the school is articulated in five highly topical themes in the area, all sharing to a greater or lesser extent the classical N–body problem as a prototypical and paradigmatic case.

Official language of the school: English

Administrative and scientific coordinators

Renato Iturriaga (Sociedad Matem ́atica Mexicana,
Mexico
, )
Tere Seara (Universitat Politecnica de Catalunya,
Spain
, )

Scientific program

Course 1: "Central Configurations for Beginners", Eddaly Guerra Velasco (Universidad Autonoma de Chiapas, Mexico)

Course 2: "Hamilton-Jacobi Equation of N–body Problems", Ezequiel Maderna (Universidad de la Republica, Uruguay)

Course 3: "KAM Theory for a Special kind of Dissipative Systems", Renato Calleja (Universidad Nacional Autonoma de Mexico, Mexico)

Course 4: "The Anisotropic Kepler Problem ", Gian Marco Canneori (Università degli Studi di Torino, Italy)

Course 5: "Chaotic Dynamics in Celestial Mechanics", Marcel Guardia (Universitat Politecnica de Catalunya, Spain)

Website of the school

How to participate

For registration and application to a CIMPA financial support, follow the instructions given here.

Deadline for registration and application: January 30, 2022