Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy

Autores
Efthymiopoulos, Christos
Año de publicación
2011
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
This is a set of lecture notes on methods and techniques of canonical perturbation theory, as well as on the latter’s applications in the study of diffusion processes and chaos in physical systems related to dynamical astronomy. The text represents, to a considerable extent, an elaborated transcript of the lectures given by the author during the third La Plata school on Astronomy and Geophysics, in July 2011. However, the structure of the text, and in particular, the sequence of presentation of the topics, has been substantially modified with respect to the structure of the lectures. Also, the text has been enriched by a number of additional topics, reference to which was judged necessary for reasons of completeness.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
canonical perturbation theory
diffusion processes
chaos
dynamical astronomy
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/167635
Acceder
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network_name_str SEDICI (UNLP)
spelling Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomyEfthymiopoulos, ChristosCiencias Astronómicascanonical perturbation theorydiffusion processeschaosdynamical astronomyThis is a set of lecture notes on methods and techniques of canonical perturbation theory, as well as on the latter’s applications in the study of diffusion processes and chaos in physical systems related to dynamical astronomy. The text represents, to a considerable extent, an elaborated transcript of the lectures given by the author during the third La Plata school on Astronomy and Geophysics, in July 2011. However, the structure of the text, and in particular, the sequence of presentation of the topics, has been substantially modified with respect to the structure of the lectures. Also, the text has been enriched by a number of additional topics, reference to which was judged necessary for reasons of completeness.Facultad de Ciencias Astronómicas y Geofísicas2011-07info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf3-146http://sedici.unlp.edu.ar/handle/10915/167635enginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:44:40Zoai:sedici.unlp.edu.ar:10915/167635Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:40.799SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
title Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
spellingShingle Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
Efthymiopoulos, Christos
Ciencias Astronómicas
canonical perturbation theory
diffusion processes
chaos
dynamical astronomy
title_short Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
title_full Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
title_fullStr Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
title_full_unstemmed Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
title_sort Canonical perturbation theory, stability and diffusion in Hamiltonian systems: applications in dynamical astronomy
dc.creator.none.fl_str_mv Efthymiopoulos, Christos
author Efthymiopoulos, Christos
author_facet Efthymiopoulos, Christos
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
canonical perturbation theory
diffusion processes
chaos
dynamical astronomy
topic Ciencias Astronómicas
canonical perturbation theory
diffusion processes
chaos
dynamical astronomy
dc.description.none.fl_txt_mv This is a set of lecture notes on methods and techniques of canonical perturbation theory, as well as on the latter’s applications in the study of diffusion processes and chaos in physical systems related to dynamical astronomy. The text represents, to a considerable extent, an elaborated transcript of the lectures given by the author during the third La Plata school on Astronomy and Geophysics, in July 2011. However, the structure of the text, and in particular, the sequence of presentation of the topics, has been substantially modified with respect to the structure of the lectures. Also, the text has been enriched by a number of additional topics, reference to which was judged necessary for reasons of completeness.
Facultad de Ciencias Astronómicas y Geofísicas
description This is a set of lecture notes on methods and techniques of canonical perturbation theory, as well as on the latter’s applications in the study of diffusion processes and chaos in physical systems related to dynamical astronomy. The text represents, to a considerable extent, an elaborated transcript of the lectures given by the author during the third La Plata school on Astronomy and Geophysics, in July 2011. However, the structure of the text, and in particular, the sequence of presentation of the topics, has been substantially modified with respect to the structure of the lectures. Also, the text has been enriched by a number of additional topics, reference to which was judged necessary for reasons of completeness.
publishDate 2011
dc.date.none.fl_str_mv 2011-07
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dc.language.none.fl_str_mv eng
language eng
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