Theory of Orbits treats celestial mechanics as well as stellar
dynamics from the common point of view of orbit theory, making use
of concepts and techniques from modern geometric mechanics. It
starts with elementary Newtonian mechanics and ends with the
dynamics of chaotic motion. The two volumes are meant for students
in astronomy and physics alike. Prerequisite is a physicist's
knowledge of calculus and differential geometry.
From the reviews "The book is ... didactically written and contains topics from classical to most modern ones, treated rigorously by indicating where complete proofs are to be found." Zentralblatt für Mathematik,.
From the reviews "The book is ... didactically written and contains topics from classical to most modern ones, treated rigorously by indicating where complete proofs are to be found." Zentralblatt für Mathematik, 1999
From the reviews "The book is ... didactically written and contains topics from classical to most modern ones, treated rigorously by indicating where complete proofs are to be found." Zentralblatt für Mathematik, 1999
Dino Boccaletti, University of Rome La Sapienza, Rome, Italy / Giuseppe Pucacco, University of Rome Tor Vergata, Rome, Italy
Classical Perturbation Theory in Celestial Mechanics - Equations of Planetary Motion.- Canonical Perturbation Theory and KAM Theory.- Lie Transform Perturbation Theory.- The Theory of Adiabatic Invariants and Its Applications in Celestial Mechanics and Stellar Dynamics.- Periodic Orbits and Resonances.- Chaos.- Numerical Explorations.
Ein Marktplatz-Angebot für "Perturbative and Geometrical Methods" für EUR 49,95
