A tree code for planetesimal dynamics: Comparison with a hybrid direct code
- Autores
- Brunini, Adrian; Viturro, Hector Ruben
- Año de publicación
- 2003
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a tree code for simulations of collisional systems dominated by a central mass. We describe the implementation of the code and the results of some test runs with which the performance of the code was tested. A comparison between the behaviour of the tree code and a direct hybrid integrator is also presented. The main result is that tree codes can be useful in numerical simulations of planetary accretion, especially during intermediate stages, where possible runaway accretion and dynamical friction lead to a population with a few large bodies in low-eccentricity and low-inclination orbits embedded in a large swarm of small planetesimals in rather excited orbits. Some strategies to improve the performance of the code are also discussed.
Fil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina
Fil: Viturro, Hector Ruben. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina - Materia
-
ACCRETION, ACCRETION DISCS
CELESTIAL MECHANICS
METHODS: NUMERICAL
SOLAR SYSTEM: GENERAL - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/36894
Ver los metadatos del registro completo
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CONICET Digital (CONICET) |
spelling |
A tree code for planetesimal dynamics: Comparison with a hybrid direct codeBrunini, AdrianViturro, Hector RubenACCRETION, ACCRETION DISCSCELESTIAL MECHANICSMETHODS: NUMERICALSOLAR SYSTEM: GENERALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a tree code for simulations of collisional systems dominated by a central mass. We describe the implementation of the code and the results of some test runs with which the performance of the code was tested. A comparison between the behaviour of the tree code and a direct hybrid integrator is also presented. The main result is that tree codes can be useful in numerical simulations of planetary accretion, especially during intermediate stages, where possible runaway accretion and dynamical friction lead to a population with a few large bodies in low-eccentricity and low-inclination orbits embedded in a large swarm of small planetesimals in rather excited orbits. Some strategies to improve the performance of the code are also discussed.Fil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; ArgentinaFil: Viturro, Hector Ruben. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; ArgentinaWiley Blackwell Publishing, Inc2003-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/mswordapplication/pdfhttp://hdl.handle.net/11336/36894Brunini, Adrian; Viturro, Hector Ruben; A tree code for planetesimal dynamics: Comparison with a hybrid direct code; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 346; 3; 12-2003; 924-9320035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/346/3/924/982858info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2003.07142.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:35Zoai:ri.conicet.gov.ar:11336/36894instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:36:35.471CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
title |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
spellingShingle |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code Brunini, Adrian ACCRETION, ACCRETION DISCS CELESTIAL MECHANICS METHODS: NUMERICAL SOLAR SYSTEM: GENERAL |
title_short |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
title_full |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
title_fullStr |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
title_full_unstemmed |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
title_sort |
A tree code for planetesimal dynamics: Comparison with a hybrid direct code |
dc.creator.none.fl_str_mv |
Brunini, Adrian Viturro, Hector Ruben |
author |
Brunini, Adrian |
author_facet |
Brunini, Adrian Viturro, Hector Ruben |
author_role |
author |
author2 |
Viturro, Hector Ruben |
author2_role |
author |
dc.subject.none.fl_str_mv |
ACCRETION, ACCRETION DISCS CELESTIAL MECHANICS METHODS: NUMERICAL SOLAR SYSTEM: GENERAL |
topic |
ACCRETION, ACCRETION DISCS CELESTIAL MECHANICS METHODS: NUMERICAL SOLAR SYSTEM: GENERAL |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We present a tree code for simulations of collisional systems dominated by a central mass. We describe the implementation of the code and the results of some test runs with which the performance of the code was tested. A comparison between the behaviour of the tree code and a direct hybrid integrator is also presented. The main result is that tree codes can be useful in numerical simulations of planetary accretion, especially during intermediate stages, where possible runaway accretion and dynamical friction lead to a population with a few large bodies in low-eccentricity and low-inclination orbits embedded in a large swarm of small planetesimals in rather excited orbits. Some strategies to improve the performance of the code are also discussed. Fil: Brunini, Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina Fil: Viturro, Hector Ruben. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina |
description |
We present a tree code for simulations of collisional systems dominated by a central mass. We describe the implementation of the code and the results of some test runs with which the performance of the code was tested. A comparison between the behaviour of the tree code and a direct hybrid integrator is also presented. The main result is that tree codes can be useful in numerical simulations of planetary accretion, especially during intermediate stages, where possible runaway accretion and dynamical friction lead to a population with a few large bodies in low-eccentricity and low-inclination orbits embedded in a large swarm of small planetesimals in rather excited orbits. Some strategies to improve the performance of the code are also discussed. |
publishDate |
2003 |
dc.date.none.fl_str_mv |
2003-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/36894 Brunini, Adrian; Viturro, Hector Ruben; A tree code for planetesimal dynamics: Comparison with a hybrid direct code; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 346; 3; 12-2003; 924-932 0035-8711 1365-2966 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/36894 |
identifier_str_mv |
Brunini, Adrian; Viturro, Hector Ruben; A tree code for planetesimal dynamics: Comparison with a hybrid direct code; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 346; 3; 12-2003; 924-932 0035-8711 1365-2966 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/346/3/924/982858 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2003.07142.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/msword application/pdf |
dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613149103226880 |
score |
13.070432 |