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
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/137905
Ver los metadatos del registro completo
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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:UNLP2025-10-15T11:23:43Zoai: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:13292025-10-15 11:23:44.047SEDICI (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 |
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article |
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publishedVersion |
| dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/137905 |
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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 |
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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) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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