Study of the influence of computational parameters on the formation of a giant gaseous planet

Detalhes bibliográficos
Autor(a) principal: Moraes, R. A. [UNESP]
Data de Publicação: 2015
Outros Autores: Neto, E. Vieira [UNESP]
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1742-6596/641/1/012012
http://hdl.handle.net/11449/168399
Resumo: Today, computational simulatios are the best method to describe the formation of our Solar System, however this kind of simulations contain numerical errors caused by boundary conditions and choises of the grid, for instance. In this paper we will present results from several hidrodynamical simulations of the formation of a planet like Jupiter able to migrate using different computational parameters. We will compare the density profile, the semimajor axis and the eccentricity of the planet for those different parameters and measure the effect of them. We will not extend our results for planets with initial eccentric orbits in this paper.
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spelling Study of the influence of computational parameters on the formation of a giant gaseous planetToday, computational simulatios are the best method to describe the formation of our Solar System, however this kind of simulations contain numerical errors caused by boundary conditions and choises of the grid, for instance. In this paper we will present results from several hidrodynamical simulations of the formation of a planet like Jupiter able to migrate using different computational parameters. We will compare the density profile, the semimajor axis and the eccentricity of the planet for those different parameters and measure the effect of them. We will not extend our results for planets with initial eccentric orbits in this paper.Universidade Estadual Paulista UNESP Campus de GuaratinguetáUniversidade Estadual Paulista UNESP Campus de GuaratinguetáUniversidade Estadual Paulista (Unesp)Moraes, R. A. [UNESP]Neto, E. Vieira [UNESP]2018-12-11T16:41:06Z2018-12-11T16:41:06Z2015-10-07info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectapplication/pdfhttp://dx.doi.org/10.1088/1742-6596/641/1/012012Journal of Physics: Conference Series, v. 641, n. 1, 2015.1742-65961742-6588http://hdl.handle.net/11449/16839910.1088/1742-6596/641/1/0120122-s2.0-849585975272-s2.0-84958597527.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of Physics: Conference Series0,2410,241info:eu-repo/semantics/openAccess2023-11-18T06:11:17Zoai:repositorio.unesp.br:11449/168399Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-11-18T06:11:17Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Study of the influence of computational parameters on the formation of a giant gaseous planet
title Study of the influence of computational parameters on the formation of a giant gaseous planet
spellingShingle Study of the influence of computational parameters on the formation of a giant gaseous planet
Moraes, R. A. [UNESP]
title_short Study of the influence of computational parameters on the formation of a giant gaseous planet
title_full Study of the influence of computational parameters on the formation of a giant gaseous planet
title_fullStr Study of the influence of computational parameters on the formation of a giant gaseous planet
title_full_unstemmed Study of the influence of computational parameters on the formation of a giant gaseous planet
title_sort Study of the influence of computational parameters on the formation of a giant gaseous planet
author Moraes, R. A. [UNESP]
author_facet Moraes, R. A. [UNESP]
Neto, E. Vieira [UNESP]
author_role author
author2 Neto, E. Vieira [UNESP]
author2_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Moraes, R. A. [UNESP]
Neto, E. Vieira [UNESP]
description Today, computational simulatios are the best method to describe the formation of our Solar System, however this kind of simulations contain numerical errors caused by boundary conditions and choises of the grid, for instance. In this paper we will present results from several hidrodynamical simulations of the formation of a planet like Jupiter able to migrate using different computational parameters. We will compare the density profile, the semimajor axis and the eccentricity of the planet for those different parameters and measure the effect of them. We will not extend our results for planets with initial eccentric orbits in this paper.
publishDate 2015
dc.date.none.fl_str_mv 2015-10-07
2018-12-11T16:41:06Z
2018-12-11T16:41:06Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/conferenceObject
format conferenceObject
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1088/1742-6596/641/1/012012
Journal of Physics: Conference Series, v. 641, n. 1, 2015.
1742-6596
1742-6588
http://hdl.handle.net/11449/168399
10.1088/1742-6596/641/1/012012
2-s2.0-84958597527
2-s2.0-84958597527.pdf
url http://dx.doi.org/10.1088/1742-6596/641/1/012012
http://hdl.handle.net/11449/168399
identifier_str_mv Journal of Physics: Conference Series, v. 641, n. 1, 2015.
1742-6596
1742-6588
10.1088/1742-6596/641/1/012012
2-s2.0-84958597527
2-s2.0-84958597527.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of Physics: Conference Series
0,241
0,241
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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