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

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...

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Autor principal: Katsanikas, Matthaios
Formato: Objeto de conferencia
Lenguaje:Inglés
Publicado: 2011
Materias:
Ciencias Astronómicas
autonomous hamiltonian system
phase space
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/167656
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SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-167656
record_format dspace
spelling I19-R120-10915-1676562024-07-01T20:02:03Z http://sedici.unlp.edu.ar/handle/10915/167656 Simple Instability in a 3D Autonomous Hamiltonian system of galactic type Katsanikas, Matthaios 2011-07 2012 2024-07-01T17:23:33Z en Ciencias Astronómicas autonomous hamiltonian system phase space 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 Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 367-372
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
autonomous hamiltonian system
phase space
spellingShingle Ciencias Astronómicas
autonomous hamiltonian system
phase space
Katsanikas, Matthaios
Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
topic_facet Ciencias Astronómicas
autonomous hamiltonian system
phase space
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.
format Objeto de conferencia
Objeto de conferencia
author Katsanikas, Matthaios
author_facet Katsanikas, Matthaios
author_sort Katsanikas, Matthaios
title Simple Instability in a 3D Autonomous Hamiltonian system of galactic type
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
publishDate 2011
url http://sedici.unlp.edu.ar/handle/10915/167656
work_keys_str_mv AT katsanikasmatthaios simpleinstabilityina3dautonomoushamiltoniansystemofgalactictype
_version_ 1807223541215526912

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