A perturbation particle method for stability studies of stellar systems

Autores
Wachlin, Felipe Carlos; Rybicki, George B.; Muzzio, Juan Carlos
Año de publicación
1993
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We discuss a numerical method for investigating the stability of stellar systems that uses an analytic distribution function to describe a stellar system in equilibrium and perturbation particles to represent departures from that equilibrium state. The particles are used only to represent the perturbation, and statistical fluctuations due to the finite number of particles are therefore much less severe than in full N-body codes. We provide a general description of the method, recipes for particular aspects of its implementation, and an example of its application to a simple model with known analytical solution.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Astronomía
Física
instabilities
methods: numerical
celestial mechanics
stellar dynamics
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:10915/137905

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network_name_str SEDICI (UNLP)
spelling A perturbation particle method for stability studies of stellar systemsWachlin, Felipe CarlosRybicki, George B.Muzzio, Juan CarlosAstronomíaFísicainstabilitiesmethods: numericalcelestial mechanicsstellar dynamicsWe discuss a numerical method for investigating the stability of stellar systems that uses an analytic distribution function to describe a stellar system in equilibrium and perturbation particles to represent departures from that equilibrium state. The particles are used only to represent the perturbation, and statistical fluctuations due to the finite number of particles are therefore much less severe than in full N-body codes. We provide a general description of the method, recipes for particular aspects of its implementation, and an example of its application to a simple model with known analytical solution.Facultad de Ciencias Astronómicas y Geofísicas1993-06-15info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf1007-1012http://sedici.unlp.edu.ar/handle/10915/137905enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/issn/1365-2966info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/262.4.1007info: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:UNLP2025-09-29T11:31:52Zoai:sedici.unlp.edu.ar:10915/137905Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:31:53.224SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv A perturbation particle method for stability studies of stellar systems
title A perturbation particle method for stability studies of stellar systems
spellingShingle A perturbation particle method for stability studies of stellar systems
Wachlin, Felipe Carlos
Astronomía
Física
instabilities
methods: numerical
celestial mechanics
stellar dynamics
title_short A perturbation particle method for stability studies of stellar systems
title_full A perturbation particle method for stability studies of stellar systems
title_fullStr A perturbation particle method for stability studies of stellar systems
title_full_unstemmed A perturbation particle method for stability studies of stellar systems
title_sort A perturbation particle method for stability studies of stellar systems
dc.creator.none.fl_str_mv Wachlin, Felipe Carlos
Rybicki, George B.
Muzzio, Juan Carlos
author Wachlin, Felipe Carlos
author_facet Wachlin, Felipe Carlos
Rybicki, George B.
Muzzio, Juan Carlos
author_role author
author2 Rybicki, George B.
Muzzio, Juan Carlos
author2_role author
author
dc.subject.none.fl_str_mv Astronomía
Física
instabilities
methods: numerical
celestial mechanics
stellar dynamics
topic Astronomía
Física
instabilities
methods: numerical
celestial mechanics
stellar dynamics
dc.description.none.fl_txt_mv We discuss a numerical method for investigating the stability of stellar systems that uses an analytic distribution function to describe a stellar system in equilibrium and perturbation particles to represent departures from that equilibrium state. The particles are used only to represent the perturbation, and statistical fluctuations due to the finite number of particles are therefore much less severe than in full N-body codes. We provide a general description of the method, recipes for particular aspects of its implementation, and an example of its application to a simple model with known analytical solution.
Facultad de Ciencias Astronómicas y Geofísicas
description We discuss a numerical method for investigating the stability of stellar systems that uses an analytic distribution function to describe a stellar system in equilibrium and perturbation particles to represent departures from that equilibrium state. The particles are used only to represent the perturbation, and statistical fluctuations due to the finite number of particles are therefore much less severe than in full N-body codes. We provide a general description of the method, recipes for particular aspects of its implementation, and an example of its application to a simple model with known analytical solution.
publishDate 1993
dc.date.none.fl_str_mv 1993-06-15
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/137905
url http://sedici.unlp.edu.ar/handle/10915/137905
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0035-8711
info:eu-repo/semantics/altIdentifier/issn/1365-2966
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/262.4.1007
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
1007-1012
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
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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