Hofer's L...-geometry: energy and stability of Hamiltonian flows, part II.
Francois Lalonde, Dusa McDuff (1995)
Inventiones mathematicae
Similarity:
Displaying similar documents to “Hofer's L...-geometry: energy and stability of Hamiltonian flows, part II (Erratum).”
Hofer's L...-geometry: energy and stability of Hamiltonian flows, part II.
Hofer's L...-geometry: energy and stability of Hamiltonian flows, part I.
Francois Lalonde, Dusa McDuff (1995)
Inventiones mathematicae
Similarity:
Dynamical systems -- past and present.
Moser, Jürgen (1998)
Documenta Mathematica
Similarity:
Modifying Lax Equations and the Second Hamiltonian Structure.
B.A. Kupershmidt, George Wilson (1980/81)
Inventiones mathematicae
Similarity:
Nekhoroshev estimates for quasi-convex hamiltonian systems.
Jürgen Pöschel (1993)
Mathematische Zeitschrift
Similarity:
On the problem of stability for near to integrable Hamiltonian systems.
Giorgilli, Antonio (1998)
Documenta Mathematica
Similarity:
On the question of stability in a Hamiltonian system
A. D. Bruno (1989)
Banach Center Publications
Similarity:
Normal Modes for Nonlinear Hamiltonian Systems.
Alan Weinstein (1973)
Inventiones mathematicae
Similarity:
Aspects of Long-time Behaviour of Solutions of Non-linear Hamiltonian Evolution Equations.
J. Bourgain (1995)
Geometric and functional analysis
Similarity:
Hamiltonian Dynamics on Pseudodifferential Symbols
Boris Khesin (1993)
Recherche Coopérative sur Programme n°25
Similarity:
Nekhoroshev stability for the D’Alembert problem of Celestial Mechanics
Luca Biasco, Luigi Chierchia (2002)
Atti della Accademia Nazionale dei Lincei. Classe di Scienze Fisiche, Matematiche e Naturali. Rendiconti Lincei. Matematica e Applicazioni
Similarity:
The classical D’Alembert Hamiltonian model for a rotational oblate planet revolving near a «day-year» resonance around a fixed star on a Keplerian ellipse is considered. Notwithstanding the strong degeneracies of the model, stability results a là Nekhoroshev (i.e. for times which are exponentially long in the perturbative parameters) for the angular momentum of the planet hold.