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Introduction to the Perturbation Theory of Hamiltonian Systems (Springer Monographs in Mathematics)

معرفی کتاب «Introduction to the Perturbation Theory of Hamiltonian Systems (Springer Monographs in Mathematics)» نوشتهٔ Dmitry Treschev, Oleg Zubelevich (auth.)، منتشرشده توسط نشر Springer-Verlag Berlin Heidelberg در سال 2010. این کتاب در فرمت pdf، زبان انگلیسی ارائه شده است.

"This book presents the basic methods of regular perturbation theory of Hamiltonian systems, including KAM-theory, splitting of asymptotic manifolds, the separatrix map, averaging, anti-integrable limit, etc. in a readable way. Although concise, it discusses all main aspects of the basic modern theory of perturbed Hamiltonian systems and most results are given with complete proofs. It will be a valuable reference for Hamiltonian systems, and of special interest to researchers and graduate students of the KAM community."--Publisher's website This book is an extended version of lectures given by the ?rst author in 1995–1996 at the Department of Mechanics and Mathematics of Moscow State University. We believe that a major part of the book can be regarded as an additional material to the standard course of Hamiltonian mechanics. In comparison with the original Russian 1 version we have included new material, simpli?ed some proofs and corrected m- prints. Hamiltonian equations ?rst appeared in connection with problems of geometric optics and celestial mechanics. Later it became clear that these equations describe a large classof systemsin classical mechanics,physics,chemistry,and otherdomains. Hamiltonian systems and their discrete analogs play a basic role in such problems as rigid body dynamics, geodesics on Riemann surfaces, quasi-classic approximation in quantum mechanics, cosmological models, dynamics of particles in an accel- ator, billiards and other systems with elastic re?ections, many in?nite-dimensional models in mathematical physics, etc. In this book we study Hamiltonian systems assuming that they depend on some parameter (usually?), where for?= 0 the dynamics is in a sense simple (as a rule, integrable). Frequently such a parameter appears naturally. For example, in celestial mechanics it is accepted to take? equal to the ratio: the mass of Jupiter over the mass of the Sun. In other cases it is possible to introduce the small parameter ar- ?cially. Front Matter....Pages I-X Hamiltonian Equations....Pages 1-21 Introduction to the KAM Theory....Pages 23-58 Splitting of Asymptotic Manifolds....Pages 59-74 The Separatrix Map....Pages 75-92 Width of the Stochastic Layer....Pages 93-106 The Continuous Averaging Method....Pages 107-130 The Anti-Integrable Limit....Pages 131-142 Hill’s Formula....Pages 143-162 Appendix....Pages 163-200 Back Matter....Pages 201-211
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