Simple Instability in a 3D Autonomous Hamiltonian system of galactic type

Autores
Katsanikas, Matthaios
Año de publicación
2011
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
In this paper we study the orbital behavior in the neighborhood of simple unstable periodic orbits in a 3D rotating galactic potential. We use the method of color and rotation to visualize the 4D spaces of section. We found four types of structures in the 4D space of section that correspond to four types of orbits. The first three types are sticky chaotic orbits and in the last one the orbit visits all available phase space.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
autonomous hamiltonian system
phase space
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:10915/167656
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/167656
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Simple Instability in a 3D Autonomous Hamiltonian system of galactic typeKatsanikas, MatthaiosCiencias Astronómicasautonomous hamiltonian systemphase spaceIn this paper we study the orbital behavior in the neighborhood of simple unstable periodic orbits in a 3D rotating galactic potential. We use the method of color and rotation to visualize the 4D spaces of section. We found four types of structures in the 4D space of section that correspond to four types of orbits. The first three types are sticky chaotic orbits and in the last one the orbit visits all available phase space.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/pdf367-372http://sedici.unlp.edu.ar/handle/10915/167656enginfo: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:10915/167656Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:40.832SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
title Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
spellingShingle Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
Katsanikas, Matthaios
Ciencias Astronómicas
autonomous hamiltonian system
phase space
title_short Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
title_full Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
title_fullStr Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
title_full_unstemmed Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
title_sort Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
dc.creator.none.fl_str_mv Katsanikas, Matthaios
author Katsanikas, Matthaios
author_facet Katsanikas, Matthaios
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
autonomous hamiltonian system
phase space
topic Ciencias Astronómicas
autonomous hamiltonian system
phase space
dc.description.none.fl_txt_mv In this paper we study the orbital behavior in the neighborhood of simple unstable periodic orbits in a 3D rotating galactic potential. We use the method of color and rotation to visualize the 4D spaces of section. We found four types of structures in the 4D space of section that correspond to four types of orbits. The first three types are sticky chaotic orbits and in the last one the orbit visits all available phase space.
Facultad de Ciencias Astronómicas y Geofísicas
description In this paper we study the orbital behavior in the neighborhood of simple unstable periodic orbits in a 3D rotating galactic potential. We use the method of color and rotation to visualize the 4D spaces of section. We found four types of structures in the 4D space of section that correspond to four types of orbits. The first three types are sticky chaotic orbits and in the last one the orbit visits all available phase space.
publishDate 2011
dc.date.none.fl_str_mv 2011-07
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/167656
url http://sedici.unlp.edu.ar/handle/10915/167656
dc.language.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
367-372
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
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instname_str Universidad Nacional de La Plata
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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